A unified picture for the gamma-ray and prompt optical emissions of GRB 990123
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小学上册英语第2单元期中试卷英语试题一、综合题(本题有100小题,每小题1分,共100分.每小题不选、错误,均不给分)1.The puppy likes to play with a ______ (toy).2.What is the bright area surrounding the sun called during an eclipse?A. HaloB. CoronaC. AuraD. Atmosphere3.What do we call the process of water turning into vapor?A. CondensationB. EvaporationC. PrecipitationD. SublimationB4.My family enjoys __________ together. (旅行)5.I have a ___ (dream).6.The _______ of sound can be measured using a sound level meter.7.The main function of nucleic acids is to store _____.8.Which animal is known for its ability to fly and has colorful feathers?A. PenguinB. SparrowC. OstrichD. BatB9. A chemical reaction can be described by a _____ equation.10. A ________ (海狮) barks and plays in the sea.11.The _______ of a substance determines its physical and chemical properties.12. A ______ is a geographical feature that can influence climate.13. A ________ (植物文化活动) enriches community life.14.I like to ___ (help) with chores.15.An electric current flows from positive to ______.16.The __________ (古代文明的成就) include advancements in writing and math.17.My favorite animal is a ___ (dog/cat).18.What is a solar system?A. A collection of starsB. A group of planets orbiting a starC. A type of galaxyD. A cloud of gas19.What do you call the process of plants making food?A. RespirationB. PhotosynthesisC. DigestionD. EvaporationB20.My best friend is my loyal _______ who always encourages me.21.The sky is ______ with stars at night. (filled)22.The tree has green ______.23. A _____ (植物活动) can raise awareness about conservation.24.I have fun playing board games with my ____.25.I admire my grandparents for ____.26.The hedgehog rolls into a _______ (球) when scared.27.The __________ can indicate areas at risk of geological hazards.28.The _______ (猫) licks its paws.29.The Kuiper Belt is home to many small icy bodies, including ______.30.The fall of Constantinople happened in _____.31.Acids and bases can neutralize each other to form ______.32.What do we call the phenomenon of water droplets falling from the sky?A. RainB. SnowC. SleetD. HailA33.What do we call the imaginary line that divides the Earth into the Northern and Southern Hemispheres?A. EquatorB. Prime MeridianC. Tropic of CancerD. Tropic of CapricornA34.Density is mass per ______.35.Which animal is known for its ability to fly at high altitudes?A. EagleB. SparrowC. PenguinD. OstrichA36.I learned how to ride my new ____ this summer. (玩具名称)37.The light is very ___ (bright).38. A turtle moves very ______ (慢).39.The __________ is a region characterized by its unique wildlife.40.Which animal is known as "man's best friend"?A. CatB. DogC. RabbitD. HorseB41.I like to watch ______ movies.42.What is the process of changing from liquid to gas called?A. MeltingB. FreezingC. EvaporationD. CondensationC43.I feel excited when I go to ________.44.The chemical symbol for palladium is _____.45.The _____ (果汁) is fresh.46.I like to pretend I'm a teacher with my toy ________ (玩具名称).47.What do we call a person who studies stars?A. BiologistB. AstronomerC. GeologistD. Chemist48.I have a toy ______ (火车) that goes around the ______ (轨道).49.I love to _______ (研究) new topics.50.We have a ________ (schedule) to stick to.51.What is the first month of the year?A. JanuaryB. FebruaryC. MarchD. AprilA52.Bees produce _______ (蜂蜜).53.The ________ was a famous declaration made in 1776.54.What is the capital of Colombia?A. BogotáB. MedellínC. CaliD. CartagenaA55.I like to ______ (玩) in the park after school.56.I love to ________ my family.57.What is the name of the fairy tale about a girl who visited a house made of candy?A. CinderellaB. Hansel and GretelC. Snow WhiteD. Little Red Riding Hood58. A __________ is formed through the action of water on rock over time.59.My mom loves to __________. (购物)60.The ____ is often seen chasing after insects and butterflies.61.What do we call a young adult?A. ChildB. TeenagerC. SeniorD. BabyB62.The ________ (dictionary) defines words.63.My dad is known for his __________ (智慧).64.The engineer, ______ (工程师), builds bridges and roads.65.The ________ is a beautiful flower that blooms in spring.66. A ______ is a part of a plant that holds seeds. (果实是植物的一部分,包含种子。
星期3 WednesdayBetter to light one candle than to curse the darkness. 与其诅咒黑暗,不如燃起蜡烛。
Text AHalf a dozen radio stations about the face of the globe crackled sparks of electricity from capital and into millions of humble homes; peace came through the air and was simultaneous over all the face of the earth. The great ceremony on the battleship Missouri in Tokyo Bay was anticlimax.The greatest fleet in the world lay amidst the greatest ruins in the world under a dark and cheerless covering of clouds. The USS Iowa was on one side of the Missouri, the USS South Dakota on the other. A tattered flag with thirty-one stars was hung on one of the turrets of the battleship —the flag of the infant republic, which Commodore Perry brought with him to the same bay almost a hundred years before. Above the mainmast fluttered the battle flag of the Union of today. The deck was crowded with the American technicians. There were a Russian with a red band about his cap and a Tass newsreel man who insisted on crawling in among the main actors to get his shots; there was a Canadian general who spoiled his part and signed on the wrong line; there was a carefully tailored Chinese general from Chungking.Half a dozen Japanese were piped over the side of the Missouri, but for the purpose of history and in every man’s memory there were only two —the general, Umezu, and the statesman, Shingemitsu. Umezu was dressed in parade uniform, all his ribbons glistening, and his eyes blank, but you could see the brown pockmarks on his cheeks swelling and falling in emotion.Shingemitsu was dressed in a tall silk hat and a formal morning coat as if he were attending a wedding or a funeral. He had a wooden leg, and he limped along the deck; when he began to climb to the veranda deck where the peace was to be signed, he clutched the ropes and struggled up with infinite pain and discomfort.Shingemitsu and Umezu were brought forward, and, after a few carefully chosen words beautifully spoken by General MacArthur, they signed their names to a document marking an end to the Japanese Empire. When they had signed, the generals and admirals of all the other nations put their signatures to the document, and peace, if peace it was, had come.1. The document was signed on[A] the USS Iowa. [B] the USS South Dakota.[C] the battleship Missouri. [D] didn’t mention.2. In the second paragraph, “A tattered flag with thirty-one stars” is of[A] USS. [B] the infant USA.[C] today’s USA. [D] the greatest fleet.3. When portraying Umezu and Shingemitsu, the author focused on all the following EXCEPT[A] facial expression. [B] appearance.[C] motions. [D] inner activity.4. By saying “and peace, if peace it was, had come”, the author implied that[A] he valued the signature ceremony.[B] he was sure of the peace coming.[C] he suspected that the signature meant the real end of war.[D] he believed the signature ceremony would bring peace.Text BLeft unfettered(无拘无束的), Anthony Konieczka, 9 years old, would happily thumb away at his Game Boy Advance or PlayStation 2 from the minute he gets up to the moment he crawls intobed, 14 bleary-eyed(睡眼惺忪的)hours later.Anthony’s basement is stocked with traditional toys — board games, puzzles, art supplies —and as far as he is concerned, they are relics of Christmases past. His sister Michaely, 6 years old, still likes dressing her Barbies. But once she starts playing Game Boy it’s hard to get her away.Play patterns like this could grab another Christmas for the toy department. Through September, toy sales were down 5% compared with the first nine months of last year, according to the NDP Group. Meanwhile, the video-game industry is heading for another record year. Thanks to hot new games like Halo 2 for the Xbox, the industry is light-years ahead of the toy business when it comes to buzz. With distractions such as instant messaging, cell phone games and iPods angling for kids’ minds and allowances, the digital revolution is making life miserable for the toy industry.While some hard-to-find toys emerge every holiday season, toymakers are heading into this one without a monster hit. Indeed, there has not been a Furby-style frenzy in years. Of 10 toy segments only two, arts and crafts and dolls, have generated sales growth over a recent 12 month period. Some of the weakest categories like construction sets and action figures are the ones aimed at boys, who suffer the most blisters from the video games. Analysts expect one of the top stocking stuffers this season to be not a traditional toy but the new generation of Nintendo’s Game Boy, the DS, which hit stores last week.The deeper issue is that shifts in play patterns are forcing toymakers to fight for shelf space in a tightening market. Boys in particular seem to be abandoning traditional toys at earlier ages in favor of consumer electronics, trendy video games, PC software and the Internet. The notion that kids are growing more sophisticated and tech-savvy (懂技术的), a trend called “age compression”, has bedeviled toy companies for at least a decade. Action figures, for instance, used to be considered healthy for boys up to age 12. Now the items are mainly marketed to boys 4 to 6. A recent study found that nearly half of the U.S children start on video games at 4 to 5 years old —and 20% at age 3 or younger.Toy companies, of course, have long seen this coming. Mattel attempted to get into educational software in the late 1990s, spending $3.6 million to buy the Learning Company. But it turned out to be a blunder and led to more than $400 million in losses. Later on Mattel got back to building basic brands like Barbie and Hot Wheels. But Bar bie’s sales slump may also be a victim of kids growing older at younger ages.Several of the toys expected to sell well this season are, in fact, those that incorporate video gaming and DVD technologies. Mattel’s Fisher-Price introduced a game system called InteracTV this year, featuring DVDs with characters like Dora the explorer. Hasbro came out with a portable color video player called VideoNow and has been putting classic games like Battleship and Yahtzee into hand-held electronic format.5. At the beginning of the passage, the author implies that[A] video games are designed only for boys.[B] girls are usually not interested in video games.[C] both Anthony and Michaely are good at playing PlayStation 2.[D] children would not like to stop playing Game Boy once they start.6. We learn from the passage that in this holiday season[A] it is hard to find traditional toys in the market.[B] toymakers are planning to design monster toys.[C] no hit toys will come onto the market.[D] Furby will become popular among children.7. The sales of construction sets are decreasing because[A] they are not healthy toys for children.[B] they are very weak and easily broken.[C] they are hard to find on shelves of toy stores.[D] they are aimed at boys who are easily attracted by the video games.8. What has been bothering toymakers for almost ten years?[A] The Internet addiction.[B] The trend of age compression.[C] The sales of action figures.[D] The new generation of Game Boy.9. It is predicted that in this season the popular toys would be[A] hot new game Halo 2 for the Xbox.[B] arts and crafts and dolls.[C] action figures designed for boys aged from 4 to 6.[D] toys that integrate video gaming with DVD technologies.Text CSpace is a dangerous place, not only because of meteors(流星) but also because of rays from the Sun and other stars.Radiation is the greatest known danger to explorers in space. Doses of radiation are measured in units called “rem”. We all receive radiation here on the Earth from the Sun, f rom cosmic rays and from radioactive minerals. The “normal” dose of radiation that we receive each year is about 100 millirem; it varies according to where you live, and this is a very rough estimate. Scientists have reason to think that a man can put up with far more radiation than this without being damaged; the figure of 60 rem has been agreed on. The trouble is that it is extremely difficult to be sure about radiation damage — a person may feel perfectly well, but the cells of his or her sex organs may be damaged, and this will not be discovered until the birth of children or even grandchildren.Early space probes showed that radiation varies in different parts of space around the Earth. It also varies in time because, when great spurts of gas shoot out of the Sun, they are accompanied by a lot of extra radiation. Some estimates of the amount of radiation in space, based on various measurements and calculations, are as low as 10 rem per year, while others are as high as 5 remper hour! Mission to the Moon have had to cross the Van Allen belts of high radiation and, during the outward and return journeys, the Apollo 8 crew accumulated a total dose of about 200 millirem per man. It was hoped that there would not be any large solar flares during the times of Apollo moon walks because the walls of the lunar excursion modules (LEMs) were not thick enough to protect the men inside, though the command modules did give reasonable protection. So far, no dangerous doses of radiation have been reported, but the Gemini(双子座)orbits and the Apollo missions have been quite short. We simply do not know yet how men are going to get on when they spend weeks and months outside the protection of the atmosphere, working in a space laboratory or in a base on the Moon. Drugs might help to decrease the damage done by radiation, but no really effective ones have been found so far. At present, radiation seems to be the greatest physical hazard to space travelers, but it is impossible to say just how serious the hazard will turn out to be in the future.10. What make space a dangerous place?[A] The radioactive meteors.[B] The Sun and other stars.[C] Rays from the earth.[D] Rem.11. According to the passage, which of the following is NOT true?[A] The “normal” dose of radiation we rec eive is generally accepted as safe.[B] Scientists are certain that 60 rem of radiation won’t damage man.[C] Harm of radiation is not likely to be seen immediately.[D] We don’t know exactly the seriousness of radiation damage.12. Missions to the moon are dangerous to the explorers because[A] they have to cross the high radioactive area.[B] solar flares may damage the LEMs.[C] they have to stay in space for a long time.[D] they will probably run into meteors.13. How will men effectively protect themselves when they spend long periods in space?[A] By taking special drugs.[B] By wearing special suits.[C] By using a protective blanket.[D] No effective solution has been found yet.14. The example of Apollo is to show[A] the Apollo mission was very successful.[B] protection from space radiation is no easy job.[C] astronauts don’t care about radiation damage.[D] radiation is not a threat to well-protected space explorers.15. The best title for this passage would be[A] The Atmosphere and Our Environment[B] Research on Radiation[C] Effects of Space Radiation[D] Important Protection against RadiationText DA simple computer program that teaches children to distinguish between sounds can dramatically boost their listening skills. It can allow them to progress by the equivalent of two years in just a few weeks, the game’s creator claims.The game, called Phonomena, was devised by David Moore of the University of Oxford, U.K., as an aid for children with language problems, but he says his latest trials also show that it can help any child. Other experts, however, are reserving judgment until independent tests are carried out.Phonomena is designed to improve children’s ability to distinguish between differentphonemes(音素), the basic sounds that form the building blocks of language. Up to a fifth of all children are thought to have problems hearing the differences between some sounds, says Moore, who heads the U.K. Medical Research Council’s Institute of Hearing Research.In the game, children have to distinguish between pairs of phonemes such as the “i” sound from the word “bit” and the “e” from “bet”. They are played one phoneme followed by two more examples, and asked which one matches the first sound. As the game progresses, the phonemes are gradual ly “morphed”(改变) to make them more and more similar, making it increasingly difficult to distinguish between them.With 44 phonemes in English, there are potentially more than 1,000 different pairs, but the game concentrates on just 22 pairs of the commonest and most similar-sounding phonemes.In the latest trials, 18 children aged between eight and ten played the game three times a week for four weeks. Their language abilities were compared before and after exposure to the game using a standard listening test.The team found a dramatic improvement in their language abilities, with listening ages up by an average 2.4 years compared with 12 children who did not play the game. In earlier trials on children with learning difficulties, the speech and language therapists who tested the game reported similar improvements.But Ted Wragg, an expert in education at the U.K’s University of Exeter, warns that such trials can produce misleading results. The improvements could be due to the efforts and attention of teachers and therapists, rather than the game itself. There is a history in education of people and companies making claims about learning products that do not stand up to scrutiny, he says.It is a bit like teaching someone to catch a ball, Moore adds. “Sensor y performance is no different from motor performance. As far as we know, the neural processes driving them both are the same.” And just as playing catch improves hand-eye coordination in other tasks, Moore thinks the phoneme training boosts children’s gene ral language skills.The advantage of using computers, he says, is each game can be tailored to a child’s abilities.An oxford-based company called MindWeavers has been set up to commercialize the game.Similar computer0based language tools already exist, such as those developed by Scientific Learning of Oakland, California. But these are geared exclusively towards children with speech and language problems and involve intensive training.“We don’t believe you need to do this Draconian(严酷的) amount of training for it to do good,” says Moore. He is also exploring the use of phoneme training as an aid to adults learning a foreign language.16. At first, the Phonomena game is designed for[A] adults.[B] disabled children.[C] children with language problems.[D] all children.17. We can infer from the passage that in the game[A] one fifth of the children have difficult distinguishing between sounds.[B] children are asked to tell the differences between similar sounds.[C] the phonemes are becoming increasingly difficult to distinguish.[D] 44 phonemes in English are involved.18. In Ted Wrag g’s opinion,[A] the trial results are not reliable and reasonable.[B] the game is helpful to children with language problems.[C] the trial results are accurate.[D] the trial results show that the game is useless.19. What is the advantage of using computers in Phonomena game?[A] It can provide customized service.[B] It can provide multimedia service.[C] Children can play the game at home.[D] It can improve child’s ability.20. What’s the limitation of the existing computer-based language tools?[A] They are designed exclusively for children.[B] They require too much training.[C] They are too harsh.[D] They do nothing good to language skills.语境词汇Text A1. crackle sparks of electricity <喻>通过电波传递2. anticlimax n.令人扫兴的结尾3. tatter v.扯碎,使变破烂:a tattered flag 一面破旧的国旗4.mainmast n.主桅5. pipe v.召集,召唤6. the veranda deck 舰艇上的游廊7. clutch v.抓住,抓紧Text B1. thumb v.以拇指摆弄n. 大拇指2. blister n.水泡,气泡v.使起水泡3. angle v.谋取;垂钓n.角;角度,观点4. hit n.成功的尝试;击中v.打(击)5. frenzy n.狂乱;极度的激动6. trendy a.时髦的,流行的n.新潮人物,穿着时髦的人7. bedevil vt.使苦恼;折磨8. slump n.经济衰退;消沉v.倒下,陷落;下跌Text C1. radiation n.放射,辐射;放射物,放射线2. cosmic n.宇宙的;广大的,无限的3. probe n.太空探测器;探查v.查究,调查4. spurt n.喷射;忽然的加速、增强vi.喷出,涌出5. accumulate v.积累,聚集;增长6. excursion n.郊游,远足,游览Text D1. distinguish vt.&vi.区分,辨别2. phoneme n.音素,音位2. exposure n.暴露,揭露;曝光,曝光时间3. scrutiny n.细察,详审4. sensory a.知觉的,感觉的,感觉器官的5. tailor vt.使合适,修改n.裁缝6. exclusively ad.仅仅,专门地;排他地,独占地难句突破Text A1. There were a Russian with a red band about his cap and a Tass newsreel man who insisted on crawling in among the main actors to get his shots; there was a Canadian general who flubbed his part and signed on the wrong line; there was a carefully tailored Chinese general from Chungking. 【分析】并列复合句。
小学下册英语第4单元测验卷[有答案]英语试题一、综合题(本题有50小题,每小题1分,共100分.每小题不选、错误,均不给分)1 The _____ (giraffe) is very tall.2 I can ______ (提升) my creativity through art.3 We eat _____ (breakfast/lunch) in the morning.4 The _____ (海豹) often basks in the sun on the rocks.5 A _____ (森林) is full of many different kinds of plants.6 My _____ (妹妹) has a dollhouse where she plays with her dolls. 我妹妹有一个洋娃娃屋,和她的洋娃娃一起玩。
7 I feel _______ when I play sports.8 His favorite book is about a ________.9 The ocean is a source of ______ for many organisms.10 The __________ (气候研究) informs policy decisions.11 What is 50 25?A. 15B. 25C. 35D. 4512 What is the scientific study of the atmosphere and weather called?A. GeologyB. MeteorologyC. AstronomyD. Biology答案:B13 What do you call the time it takes for the Earth to go around the Sun?A. DayB. MonthC. YearD. Century答案:C14 The _______ (Japanese internment camps) were established during World War II in the US.15 The __________ is known for its stunning beaches.16 A chemical change may involve a change in _____ (color, temperature, or odor).17 Parrots can ______ human speech.18 The __________ can show the effects of erosion and sedimentation.19 What do we call the act of working together toward a common goal?A. CollaborationB. TeamworkC. CooperationD. All of the Above答案:D20 The __________ (历史的情感) connects us to the past.21 What do you call a person who fixes broken machines?A. MechanicB. ElectricianC. PlumberD. Engineer22 What do you call the person who teaches students?A. StudentB. TeacherC. PrincipalD. Janitor答案: B23 小海豚) jumps out of the water. The ___24 She calls her friend _____ (朋友).25 A ______ is a natural barrier formed by geographical features.26 The rabbit has big _________ (耳朵).27 I have _____ (three/four) pets.28 The book is on the _______ (shelf).29 We are visiting the ___. (art gallery)30 An indicator changes color in the presence of an ______.31 What is the name of the famous explorer who sailed around the world?A. Ferdinand MagellanB. Christopher ColumbusC. Vasco da GamaD. Marco Polo32 The frog jumps ______ (高) to catch flies.33 The __________ is a famous mountain in Japan.34 The __________ (历史的解释) evolves over time.35 The sun is _______ (温暖的).36 My cousin is a ______. She loves to write stories.37 I like to _____ my lunch at school. (eat)38 The _____ (海鸥) flies over the beach, looking for fish. 海鸥在海滩上空飞翔,寻找鱼。
你校将以四月十二日世界航天日英语作文全文共3篇示例,供读者参考篇1The Infinite Frontier: Celebrating World Space DayAs students of the modern age, we stand at the precipice of an era defined by unprecedented technological advancements and an insatiable thirst for exploration. It is with great pride and excitement that our school commemorates World Space Day on April 12th, a celebration that transcends mere boundaries and unites us in our shared fascination with the vast expanse of the cosmos.From the moment our ancestors first gazed up at the twinkling stars, the allure of the heavens has captivated the human spirit. Today, we find ourselves living in an era where that primal curiosity has blossomed into a vibrant reality, with humanity's footprints etched upon the lunar surface and our robotic emissaries venturing ever deeper into the unknown.On this momentous occasion, we pause to reflect on the remarkable journey that has brought us to this point. The history of space exploration is a tapestry woven with tales ofunparalleled bravery, unwavering determination, and groundbreaking scientific discoveries. From the pioneering work of visionaries like Galileo Galilei and Isaac Newton, whose theories laid the foundation for our understanding of the cosmos, to the audacious dreamers who dared to reach for the stars, each chapter in this epic saga has propelled us forward, fueling our collective drive to unlock the secrets of the universe.As we gaze upon the night sky, our minds are transported to the pivotal moments that have shaped our understanding of the cosmos. We remember the awe-inspiring sight of Neil Armstrong taking that first small step onto the lunar surface, forever etching humanity's mark on another celestial body. We recall the breathtaking images beamed back from the Hubble Space Telescope, revealing the intricate beauty and complexity of distant galaxies. And we marvel at the astonishing achievements of robotic explorers like the Curiosity rover, which has unveiled invaluable insights into the enigmatic landscapes of Mars.Yet, as we bask in the glory of these accomplishments, we must also acknowledge that space exploration is not merely a pursuit of scientific knowledge but a testament to the indomitable spirit of human endeavor. It serves as a powerfulreminder of what we can achieve when we set our sights on the seemingly impossible and harness the collective genius of our species.The exploration of space has transcended borders, uniting nations in a shared quest to unravel the mysteries of the cosmos. It has fostered international cooperation and inspired generations of young minds to pursue careers in science, technology, engineering, and mathematics (STEM). The profound impact of space exploration extends far beyond the confines of the Earth's atmosphere, influencing virtually every aspect of our lives, from advanced communication systems to cutting-edge medical technologies.As students, we are the torchbearers of this incredible legacy, inheriting the mantle of a generation that dared to dream and challenged the boundaries of human potential. It is our responsibility to carry forth this spirit of exploration, to nurture the flames of curiosity that burn within us, and to push the frontiers of knowledge ever further.On World Space Day, we celebrate not only the achievements of the past but also the boundless possibilities that lie ahead. As we stand in awe of the celestial wonders that adorn the night sky, we are reminded of the vast expanse thatawaits our exploration. Perhaps one day, our footsteps will grace the rusty dunes of Mars, or our robotic ambassadors will venture beyond the confines of our solar system, unlocking the secrets of exoplanets and unveiling the enigmas that have captivated humanity for eons.This is a call to action, a rallying cry for the dreamers, the visionaries, and the pioneers of tomorrow. Let us embrace the spirit of exploration that has guided humanity thus far, and let us pledge to push the boundaries of what is possible. For in the vast expanse of the cosmos, there lie infinite frontiers waiting to be conquered, mysteries yearning to be unraveled, and wonders beyond our wildest imaginations.Today, as we honor World Space Day, let us raise our gaze to the heavens and allow our minds to soar among the stars. Let us revel in the accomplishments of those who came before us while casting our sights towards the boundless horizons that beckon. For it is in the pursuit of knowledge, in the relentless quest to unlock the secrets of the universe, that we truly embody the essence of what it means to be human.The cosmos is our canvas, and we are the artists, painting the narrative of humanity's journey through the vast expanse of space. Let us embrace this opportunity to leave an indelible mark,to inspire generations to come, and to forge a legacy that will echo throughout the ages.篇2The Infinite Frontier: Celebrating World Space DayAs students of the 21st century, we stand at the precipice of a new era of exploration and discovery. The vast expanse of space, once an unyielding mystery, has become our canvas upon which we paint the boldest dreams of humanity. On April 12th, we celebrate World Space Day, a date that carries profound significance for all those who dare to gaze upwards and ponder the infinite wonders that lie beyond our terrestrial confines.From the moment our ancestors first glimpsed the twinkling lights in the night sky, an insatiable curiosity has burned within the human spirit. What secrets do those celestial bodies hold? What lies beyond the veil of our atmosphere? These questions have ignited the imaginations of generations, fueling a relentless pursuit of knowledge that has propelled our species to remarkable heights.The journey into the cosmos began with baby steps, as our primitive understanding of the universe gradually gave way to scientific breakthroughs. From Galileo's pioneering use of thetelescope to Newton's laws of motion, each revelation ushered in a paradigm shift, redefining our perception of the cosmos. Yet, it was the dawn of the Space Age that truly shattered the boundaries of what we believed possible.On that fateful day in 1961, when Yuri Gagarin became the first human to venture into space, the world watched in awe as he orbited our planet, defying the shackles of gravity. This momentous achievement not only symbolized the triumph of human ingenuity but also ignited a fervent race to conquer the final frontier. Nations rallied their resources, pouring their collective determination into reaching for the stars, and the ensuing decades witnessed a flurry of milestones etched into the annals of space exploration.From the awe-inspiring footprints left on the lunar surface by Neil Armstrong and Buzz Aldrin to the breathtaking images captured by the Hubble Space Telescope, each achievement has broadened our horizons and deepened our reverence for the cosmos. We have witnessed the birth of stars and the death throes of ancient galaxies, unraveling the intricate tapestry of our universe thread by thread.Yet, our journey into the unknown is far from over. As we celebrate World Space Day, we are reminded of the boundlesspotential that lies ahead. The exploration of Mars, once a distant dream, is now within our grasp, with robotic emissaries paving the way for future human expeditions. The uncharted mysteries of exoplanets beckon, tantalizing us with the possibility of discovering life beyond our solar system.Moreover, the realm of space has transcended mere scientific curiosity, becoming an integral part of our daily lives. Satellite technology has revolutionized communication, navigation, and our understanding of our planet's intricate systems. Space-based observations have unveiled the intricate dynamics of climate change, prompting us to take action and safeguard our fragile world.As we stand in awe of these achievements, we must also acknowledge the collaborative spirit that has propelled us forward. Space exploration has served as a unifying force, transcending borders and ideologies, bringing nations together in pursuit of a common goal. It has ignited the imaginations of countless young minds, inspiring them to pursue careers in science, technology, engineering, and mathematics, shaping the innovators and explorers of tomorrow.On this World Space Day, let us pause and reflect on the incredible journey we have undertaken thus far. Let us honor thepioneers who dared to dream and the visionaries who turned those dreams into reality. But let us also look ahead, for the infinite expanse of space holds secrets yet to be uncovered, challenges yet to be surmounted, and wonders yet to be revealed.To the young minds of today, the baton is passed to you. Embrace the boundless curiosity that resides within you, for it is the fuel that will propel humanity towards new frontiers. Dare to dream of distant worlds, to unravel the mysteries of black holes, and to push the boundaries of what we thought possible. The cosmos beckons, and the limitless potential of space exploration awaits your inquisitive minds and unwavering determination.As we celebrate this momentous occasion, let us raise our eyes to the heavens and revel in the magnificence of the universe that surrounds us. For in the vast tapestry of stars and galaxies, we find not only the answers to our deepest questions but also a humbling reminder of our place in the grand scheme of existence.The infinite frontier lies before us, and with each step we take, we etch our names into the cosmic tapestry, forever intertwined with the boundless wonders of space. On World Space Day, let us embrace the spirit of exploration, for it isthrough this unwavering pursuit that we unlock the secrets of the universe and fulfill our destiny as custodians of knowledge, pioneers of discovery, and ambassadors of the infinite.篇3A Voyage Among the Stars: Celebrating World Space DayAs I gaze up at the twinkling celestial tapestry that adorns the night sky, my mind is consumed by a profound sense of wonder and curiosity. The vast expanse of the cosmos, once an impenetrable enigma, has gradually unveiled its secrets to the relentless pursuit of human ingenuity and exploration. It is with great anticipation that our school eagerly awaits the arrival of World Space Day on April 12th, a momentous occasion that commemorates the triumphs and aspirations of space exploration.From the moment our ancestors first cast their gaze upon the heavens, a primal yearning to unravel the mysteries of the universe has been etched into the human psyche. The ancients, while lacking the technological advancements of today, wove intricate mythologies and cosmologies in an attempt to make sense of the celestial bodies that danced across the night sky. Little did they know that their celestial musings would one daypave the way for the extraordinary feats of space exploration that have reshaped our understanding of the cosmos.It was not until the 20th century that humanity's dreams of venturing into the great unknown began to crystallize. The pioneering work of visionaries like Konstantin Tsiolkovsky, Robert Goddard, and Wernher von Braun laid the foundations for the development of rocket technology, propelling us into the realms of space travel. The launch of Sputnik 1 in 1957 marked a watershed moment, igniting the Space Race between the United States and the Soviet Union, and forever altering the course of human history.Yet, it was the Apollo program that truly captured the world's imagination and solidified our place among the stars. On July 20, 1969, the world held its collective breath as Neil Armstrong became the first human to set foot on the lunar surface, uttering those immortal words: "That's one small step for man, one giant leap for mankind." This momentous achievement not only demonstrated the boundless potential of human ingenuity but also served as a poignant reminder that even the most audacious dreams can be realized through unwavering perseverance and determination.Since those pioneering days, space exploration has undergone a remarkable transformation, transcending the boundaries of nations and evolving into a collaborative endeavor that unites humanity in its quest for knowledge and discovery. The International Space Station stands as a shining example of this global cooperation, a celestial outpost where astronauts from diverse backgrounds work in harmony to advance our understanding of the universe and the intricacies of life in space.As we celebrate World Space Day, we are reminded of the countless contributions that space exploration has made to our daily lives. From weather forecasting and global communication networks to advancements in medical technology and materials science, the ripple effects of our cosmic endeavors have profoundly enriched our terrestrial existence. Furthermore, the study of celestial bodies and phenomena has shed light on the origins of our universe and our place within it, prompting us to ponder existential questions that have captivated philosophers and stargazers alike throughout the ages.Yet, our journey among the stars is far from over. As we stand on the precipice of new frontiers, our insatiable curiosity and thirst for knowledge propel us ever forward. The exploration of Mars, once a distant dream, is now a tangible reality, withrobotic rovers and future human missions poised to unravel the secrets of the Red Planet. Beyond our celestial neighborhood, the quest to detect and study exoplanets – worlds beyond our solar system – has opened up a universe of possibilities, igniting speculation about the existence of extraterrestrial life and the potential for future interstellar travel.Moreover, the advent of commercial space enterprises and the democratization of space exploration have ushered in a new era of accessibility and innovation. Private companies are now developing reusable launch vehicles, making space travel more affordable and sustainable, while also pushing the boundaries of what was once thought impossible. This burgeoning industry holds the promise of ushering in a new age of space tourism, where ordinary citizens can experience the wonders of the cosmos firsthand, forever altering their perspective on our fragile yet awe-inspiring planet.As we gather to celebrate World Space Day, let us embrace the spirit of exploration that has propelled humanity to the stars. Let us honor the courageous men and women who have risked their lives in the pursuit of knowledge, and let us inspire the next generation of explorers, scientists, and dreamers to carry the torch of discovery into the vast unknown.For it is through our insatiable curiosity and unwavering determination that we will continue to push the boundaries of what is possible, unlocking the secrets of the universe one celestial body at a time. As we gaze upon the stars, let us remember that our journey among them has only just begun, and that the limitless expanse of the cosmos beckons us to embrace the unknown, to dare greatly, and to never cease in our quest to understand the wonders that lie beyond our terrestrial abode.。
目录1997—2015历年真题中重复考的词汇 (2)1997年同等学力人员申请硕士学位英语水平全国统一考试 (10)1998年同等学力人员申请硕士学位英语水平全国统一考试 (13)1999年同等学力人员申请硕士学位英语水平全国统一考试 (16)2000年同等学力人员申请硕士学位英语水平全国统一考试 (20)2001年同等学力人员申请硕士学位英语水平全国统一考试 (24)2002年同等学力人员申请硕士学位英语水平全国统一考试 (29)2003年同等学力人员申请硕士学位英语水平全国统一考试 (34)2004年同等学力人员申请硕士学位英语水平全国统一考试 (40)2005年同等学力人员申请硕士学位英语水平全国统一考试 (44)2006年同等学力人员申请硕士学位英语水平全国统一考试 (48)2007年同等学力人员申请硕士学位英语水平全国统一考试 (53)2008年同等学力人员申请硕士学位外国语水平全国统一考试 (57)2009年同等学力英语人员申请硕士学位外国语水平全国统一考试 (60)2010年同等学力英语人员申请硕士学位外国语水平全国统一考试 (63)2011同等学力全国统一考试英语试卷(A卷) (66)2012年在职申硕同等学力英语真题一真题与答案超详解 (71)2013年在职申硕同等学力英语真题一真题与答案超详解 (74)2014年在职申硕同等学力英语真题一真题与答案超详解 (75)2015年在职申硕同等学力英语真题一真题与答案超详解 (76)1997—2015历年真题中重复考的词汇2000年2011年1997年同等学力人员申请硕士学位英语水平全国统一考试PartⅡVocabulary(10 minutes,10 points)Section A16. The recent findings are also applicable to other areas of design engineering.可适用的,可应用的A) practical B) relevant C) convenient D) comparable 实用的,现实的有关的,相应的方便得,便利的可比较的,比得上的7.The century-old hostilities敌对between the two tribes eventually terminated through the persistent efforts of the local government. 部落停止,结束A) diminished B) shrunk C) vanished D) worsened减少,变小收缩,缩短消失,突然不见变得更坏,恶化18. The leaders of the two countries are planning their summit meeting with a pledge to maintainand develop good ties. 首脑会议、峰会誓言,承诺A) strategy B) standpoint C) priority D promise策略,战术立场,观点优先,优先权允诺,答应19. Computers will flourish繁荣兴旺because they enable us to accomplish tasks that could neverbefore have been undertaken. 实现,完成A) implement B) render C) assign D) complete贯彻,实行给予,补偿分配,指派完成,使完善20. Herman's success is due to his hard work and his ability to formulate plans which will get workdone efficiently. 规划,设计A) fulfill B) approve C) conceive D) conduct履行,实现批准, 通过设想,构思传导21. The farm ministers scheduled an emergency meeting in Luxembourg in hopes of easing theA) crisis C) hazard D) peril紧要关头,危机期警钟;惊恐, 忧虑危险,冒险危险22).The young man asked his parents not to worry because he was full of optimism about his career.乐观主义A) confidence B) motivation C) imagination D) resolution自信动机,动力想象决心,坚定23. One's awareness, both conscious and unconscious, of what happened in the past has a stronginfluence on one's behavior.觉悟,意识A) storage B) impression C) memory D) perception存储,储藏量印象,感想记忆,回忆理解,感知24. On hearing of the case some time later, Conan Doyle was convinced that the man was not guilty,and immediately went to work to ascertain the truth.确定,探知(重音在后面)A) explore B) obtain C) verify D) search探测,探究获得,得到检验,查证搜查25. All the staff members of the department made zealous efforts to clean up the hall for the Christmas party. 热心的A) enthusiastic B) concerted C) gigantic D) dedicated热情的,热心的商定的,协定的巨大的专注的,献身的Section B26. I ________ a letter to an internet service that distributes journalists' questions to more than 750 institutions.A) assigned B) detached C) attached D) dispatched分配,指派分开,派遣贴上,隶属派遣,发送27. All experts agree that the most important consideration with diet drugs is carefully________ therisks and benefits.A) weighing B) valuing C) evaluating D) distinguishing考虑,权衡估价,评价评价,估计区别,辨别28 More international trend for business and pleasure brings greater _______to other societies.A) exchange B) exposure C expansion D contribution交换,兑换暴露,常与to搭配膨胀,扩张贡献,捐献29. Shortage of land and funding are blamed for the city's_______ green space.A) inefficient B) inaccurate C) inadequate D) indispensable效率低的,无能的错误的,不准确的不充分的,缺乏的不可缺少的30 If English is not our first language you can often be puzzled by ways of expression that thenative speaker of English does not even have to_______.A) think out B)think about C) think over D) think for熟思,想出考虑,回想仔细考虑,重新考虑预料31.Retail sales volume in local urban and rural areas rose 57,8 per cent and 46.8 per cent, _______,over February 1995.A) individually B) accordingly C) correspondingly D)respectively个别地,单独地从而,因此;相应地相对地各个地,分别地32.This book is a _______ of radio scripts, in which we seek to explain how the words and expressions become part of our language.A) collection B) publication C) volume D)stack收藏,收集出版,出版物卷,册堆,叠33. A man's ________is best when he can forget himself and any reputation he may have requiredand can concentrate wholly on making the right decisions.A) anticipation B)acknowledgment C) expectation D)judgment预期,预料感谢,承认期待,指望判断,判断力34.Does brain power _______ as we get older? Scientists now have some surprising answers.A)decline B)descend C)deduce D)collapse下降,衰落下降,落下推论,演绎出倒塌,瓦解35.The largest system serving e-mail messengers is the internet, a _______ of millions of computerslinked worldwide.A) unity B)combination C)network D) connection团结,联合结合,联合网络连接,关系1998年同等学力人员申请硕士学位英语水平全国统一考试Part ⅡVocabulary(10 minutes,10 points)Section A16. People of diverse backgrounds now fly to distant places for pleasure,business or education.A. differentB. distinctiveC. similarD. separate【正确答案】A【句子翻译】不同背景的人们乘飞机到遥远的地方去寻找快乐、商机或教育。
UNIT 1 SCIENCE FICTION一、阅读词汇——在词块中明义1.science fiction科幻小说2.annual bonus年终红利3.a ridiculous rumour 荒谬的谣言4.a man of integrity一个诚恳正直的人5.with grace and dignity文静而庄重6.an absurd idea 一个荒唐的想法7.bus fares公交车车费8.excuse for inaction不实行措施的理由9.alien forces in the region 该地区的外国军队10.grip the rope 抓紧绳子11.be filled with hazy frost 充溢着朦胧的雾霭12.the maximum height 最高高度13.pay a huge salary付一大笔薪水14.fall backwards仰面摔倒15.fetch some books 拿来一些书二、表达词汇——在语境中活用(一)在括号内写出蓝体词汇在语境中的汉语意思1.Some of the studies show positive results, whereas others do not.(conj.然而)2.We go and do the weekly shopping every Thursday.(adj.每周的)3.The company wants to keep down labour costs.(n.劳动)4.Many people were not satisfied with the pace of change.(n.速度)(二)写出蓝体词汇的语境之义及拓展形式1.She made an appointment for her son to see the doctor.(n.预约)拓展:appoint v.任命;委任;支配→appointed adj.指定的;约定的2.His guilty expression confirmed my suspicions.(adj.内疚的)拓展:guilt n.内疚;懊悔;犯罪3.The population explodes to 40,000 during the tourist season.(vi.激增) 拓展:explosion n.爆炸;爆发;激增4.I dismissed the problem from my mind.(vt.消退)拓展:dismissal n.解雇;撤职5.He declared he would not run for a second term as president.(vt.宣称) 拓展:declaration n.申报(单);宣布;公告6.From this you can calculate the total mass in the Galaxy.(vt.计算)拓展:calculation n.计算→calculator n.计算器7.We have a relationship infinitely superior to those of many of our friends.(adj.更好的)拓展:superiority n.优越感;优势;优越(性)8.I taught my daughter how to do division at the age of six.(n.除法)拓展:divide v.(使)分开9.They urged Congress to approve plans for their reform programme.(vt.力劝) 拓展:urgency n.紧迫;急事→urgent adj.紧急的;迫切的→urgently adv.迫切地;紧急地10.The survey used a random sample of two thousand people across the Midwest.(adj.随机的)拓展:randomly adv.随机;随意;未加支配地三、词块短语——在语境中辨义活用写出或选出加蓝部分在语境中的汉语意思1.The new product had been tested out before it was put on the market.检验2.The organization encourages members to meet on a regular basis as well as provides them with financial support.定期3.Although she is my teacher, Ms Wang and I are more like friends. 更像是4.Do you know what this product is? Or rather,what it does?更准确地说5.After his defeat, many of his supporters fell away.消逝6.Their opinion on the accident conflicted with ours.与……冲突或抵触7.This model of 5G mobile phone is far superior to any others.比……更好8.We have an urge to give advice immediately to make the person feel better and try to fix the problem.有剧烈的欲望9.Miss Smith is leaving to get married and Miss Jones will take over the class.A A.接手B.汲取C.呈现D.占据10.You can't expect everything to turn out as you wish.DA.关掉B.熄灭 C.在场D.结果是四、经典句式——在佳句背诵中品悟规则用法2.3.4.教材原句Night came as if a lamp was being turned out, and in another moment came the day.(as if引导方式状语从句)夜幕驾临了,仿佛一盏灯正在熄灭,转瞬间,白昼就来临了。
丙种球蛋白联合甲基强的松龙治疗小儿重症病毒性脑炎的效果观察发布时间:2023-03-01T09:25:35.739Z 来源:《医师在线》2022年34期作者:陆丽娟[导读] 目的:对小儿重症病毒性脑炎患儿开展丙种球蛋白与甲基强的松龙合用治疗,对联用药物方案的效果加以科学评定陆丽娟常州市儿童医院 213000摘要:目的:对小儿重症病毒性脑炎患儿开展丙种球蛋白与甲基强的松龙合用治疗,对联用药物方案的效果加以科学评定。
方法:自2018年1月起,直至2022年9月份,于本院确诊并接受科学治疗的重症病毒性脑炎患儿有60例,结合患儿入院时间,把30例优先入院患儿统一作为对照组,常规疗法下,予以甲基强的松龙治疗,而对于后入院患儿30例,统一纳入观察组,予以常规治疗+甲基强的松龙+丙种球蛋白治疗方案。
从临床治疗有效情况、症状改善时间、用药副作用、后遗症、细胞免疫指标以及生活质量多个方面,详细对照临床疗效。
结果:观察组治疗总有效率高达90.00%,相比于对照组63.33%显著更高(P<0.05);对比各项症状改善时间,提示观察组抽搐(2.24±0.85)d、发热(4.21±0.80)d、意识障碍(5.05±0.92)d、颅内刺激征(3.71±0.12)d发作时间均较对照组(5.77±2.10)d、(6.60±1.48)d、(8.46±1.62)d、(5.47±1.60)d更短(P<0.05);两组用药副作用发生率差异不明显,但后遗症发生率方面,观察组3.33%相比对照组26.67%低(P<0.05);未治疗前,观察组免疫指标IgA水平(0.66±0.22)g/L低,IgE(1.41±0.09)g/L、IgG(8.20±1.76)g/L与对照组(0.64±0.23)g/L、(1.40±0.12)g/L、(8.17±1.80)g/L无统计学差异(P>0.05),但治疗后均有所改善,且观察组免疫指标IgA水平(0.37±0.09)g/L低,IgE(1.68±0.34)g/L、IgG(17.36±3.12)g/L指标水平高于对照组(0.46±0.16)g/L、(1.50±0.20)g/L、(11.36±2.55)g/L,差异十分显著(P<0.05);在生活质量方面,观察组社会功能评分为(84.59±4.55)分,躯体功能评分为(84.92±3.27)分、心理功能评分为(85.02±3.41)分、精神功能评分为(85.01±2.68)分,均高于对照组(78.29±3.22)分、(77.59±2.75)分、(78.03±4.01)分、(77.56±3.71)分,差异有统计学意义(P<0.05)。
小学上册英语第2单元测验试卷(含答案)英语试题一、综合题(本题有100小题,每小题1分,共100分.每小题不选、错误,均不给分)1.I love to eat ________ in the fall.2.The spider spins its web to catch _________ (猎物).3.The ancient civilization of Egypt is known for its ________.4.My toy robot can _____ and dance.5.Which season is the coldest?A. SpringB. SummerC. FallD. Winter答案:D6.How many letters are in the word 'elephant'?A. 6B. 7C. 8D. 9答案:B7.The __________ is a famous area known for its folklore.8.The famous singer I like is _______ (名字). 她的歌很 _______ (形容词).9.Reading is one of my favorite activities. I enjoy books about __________ and__________. They take me on adventures and teach me new things.10.Heat makes molecules move ______.11.She is learning to ________.12.She is a _____ (历史学家) documenting significant events.13.What is the name of the common game played with marbles?A. JacksB. MarblesC. Snakes and LaddersD. Chess答案: B14.I think it’s fun to try ________ (新食物).15.What is the name of the famous American holiday celebrated on the fourth Thursday in November?A. ThanksgivingB. ChristmasC. New Year'sD. Independence Day 答案:A16.My ________ (玩具名称) is made of soft material.17.The dog is ________ at the door.18.I enjoy visiting ______ during summer break.19.__________ is the process of separating a mixture into its components.20.His favorite sport is ______ (basketball).21. A ______ is a type of energy related to heat.22.The _______ of an object can be demonstrated with an experiment.23. A precipitate is a solid that forms during a ________ reaction.24.The sun is ______ (rising) in the morning.25. A diatomic molecule consists of two _______ atoms.26.The butterfly emerges from its _____ chrysalis.27. f Enlightenment emphasized reason and ________ (科学). The Age28.Sedimentary rocks can be formed from ______ materials.29.I love to sing ______ songs with my friends.30.What is the name of the famous American national park known for its waterfalls?A. YosemiteB. Grand CanyonC. YellowstoneD. Zion答案:A31.In _____ (南非), you can see the Big Five animals.32.The first man to circumnavigate the globe was ______ (麦哲伦).33.Ancient Greece is often called the birthplace of _____.34.Which country is known for sushi?A. ChinaB. JapanC. ThailandD. India答案: B35.An electric generator converts mechanical energy into ______ energy.36.Chemical reactions can be classified as ________ or endothermic.37.What do we call the process of planting seeds?A. HarvestingB. SowingC. GrowingD. Watering答案:B38.My brother is a great ________.39.The ______ (绿色建筑) incorporates plants for sustainability.40.My favorite color is ______ (purple).41.My mom likes to ______ (种植) vegetables.42.I have a ______ of toys in my room. (collection)43.The main product of the light-dependent reactions of photosynthesis is ______.44. A __________ (化学药品) is used for medical treatments and research.45.The __________ (北极) is melting due to climate change.46.The ice cream is _____ melting. (slowly)47.In a redox reaction, oxidation refers to the loss of _____ by a substance.48. A cat can see better in ______ than humans.49.The _______ can produce seeds for future planting.50.The chemical symbol for barium is ______.51.The ancient Egyptians used ________ to document their history.52.ers are cultivated for their ability to reduce ______ and promote healing. (某些花因其减压和促进愈合的能力而被种植。
专利名称:Gamma-ray detector and gamma-ray imagepick-up apparatus发明人:Gono, Yasuyuki,Motomura, Shinji,Enomoto,Shuichi,Yano, Yasushige申请号:EP04090513.5申请日:20041223公开号:EP1548465A1公开日:20050629专利内容由知识产权出版社提供专利附图:摘要:Disclosed is a gamma-ray image pickup apparatus having high energy resolution and high position resolution. A Compton camera is constructed by arranging twoelectrode split planar germanium semiconductor detectors in front and behind. This Compton camera processes a detection signal obtained from an anode and a cathode of the planar electrode split germanium detector, and can measure at how deep position from the detector surface the interaction of a gamma ray occurs. Moreover, with regard to the direction parallel to the electrode surface of the detector, the interaction position of the gamma ray was able to be measured with high accuracy. Accordingly, spatial resolution is improved by resolving a formula for the kinematics of Compton scattering with excellent accuracy.申请人:Riken地址:2-1, Hirosawa Wako-shi, Saitama 351-0198 JP国籍:JP代理机构:Ziebig, Marlene, Dr. Dipl.-Chem.更多信息请下载全文后查看。
Mediterranean Journal of MathematicsVol. 10, No. 4(2013), pages 1609-2028ContentsS. Capparelli and P. MarosciaOn Two Sequences of Orthogonal Polynomials Relatedto Jordan Blocks ….…………………………………………………………………….1609-1630 G. Aranda Pino and L. VašNoetherian Leavitt Path Algebras and Their Regular Algebras………………………..1631-1654 S. Ali, A. Fošner, M. Fošner and M. S. KhanOn Generalized Jordan Triple ( α,β )*- Derivations and related Mappings……….…..1655-1666 H. LarkiLeavitt Path Algebras of Edge-Colored Graphs……………….…..…… . …………….1667-1682 F. Qi and C. BergComplete Monotonicity of a Difference Between the Exponential and TrigammaFunctions and Properties Related to a Modified Bessel Function ……………………..1683-1694 M. Krnić, J. Pečarić and P. VukovićA Unified Treatment of Half-Discrete Hilbert-Type Inequalities witha Homogeneous Kernel…………………………………………………………………..1695-1714 B. LisenaAsymptotic Properties in a Delay Differential Inequality withPeriodic Coefficients…………………………………………………………………….1715-1728 Y. Jalilian and R. JalilianExistence of Solution for Delay Fractional Differential Equations…………………….1729-1746 J. Llibre and C. VallsGeneralized Weierstrass Integrability of the Abel Differential Equations………………1747-1758 P. Álvarez-Caudevilla, J. D. Evans and V. A. GalaktionovThe Cauchy problem for a tenth-order thin film equation I. Bifurcationof oscillatory fundamental solutions…………………………………………..…………1759-1790 A. BoughammouraHomogenization of a Highly Heterogeneous Elastic-ViscoelaticComposite Materials……………………………………………………………………...1791-1810M. StojanovicWave Equation Driven by Fractional Generalized Stochastic Processes………..………1811-1829 C. Bardaro and I. MantelliniOn Linear Combinations of Multivariate Generalized Sampling Type Series……………1831-1850 C. Ferreira, J. L. López and E.Pérez SinusíaThe Second Appell Function for one Large Variable…………………………….……….1851-1864 B. WróbelLaplace Type Multipliers for Laguerre Expansions of Hermite Type…………………….1865-1879 A. OsękowskiSharp Logarithmic Bounds for Beurling-Ahlfors Operator Restrictedto the Class of Radial Functions……………………………………………………..……1881-1892 M. Baronti and P. L. PapiniOn Some Types of Rigid Sets in Banach Spaces…………………………………………..1893-1901 Y. Yagoub-ZidiSome Isometric Properties of Subspaces of Function Spaces…………………………….1903-1913 S. Lambert, K. Lee and A. LuttmanOn the Generality of Assuming that a Family of ContinuousFunctions Separates Points…………………………………………………………..……1915-1933 I. Akbarbaglu and S. MaghsoudiBanach-Orlicz Algebras on a Locally Compact Group…………………………………...1935-1945 M. Abel and R. M. Pérez-TiscareñoLocally Pseudoconvex Inductive Limit of Topological Algebras………………….………1947-1961 P. Aiena, J. R. Guillén and P. PeñaLocalized SVEP, property (b) and property (ab)………………………………………….1963-1974 I. K. Erken and C. MurathanA Class of 3-Dimensional Contact Metric Manifolds…………………………………..…1975-1991 D. E. Dobbs and J. ShapiroOn the Strong (A)-Rings of Mahdou and Hassani…………………………………………1993-1995 M. De Falco, F. de Giovanni and C. MusellaGroups whose Proper Subgroups of Infinite Rank Have a TransitiveNormality Relation…………………………………………………………………………………. 1997-2004 S. SamkoVariable Exponent Herz Spaces………………………………………………………..….2005-2023S. SamkoErratum to “Variable exponent Herz spaces”, Mediterr. J. Math.DOI: 10.1007/s00009-013-0285-x, 2013………………………………………………….2025-2028。
高三英语艺术批评方法科学严谨运用单选题30题及答案1. The painting is truly _____.A.magnificentB.insignificantC.ordinaryD.trivial答案:A。
“magnificent”表示壮丽的、宏伟的;“insignificant”表示不重要的、微不足道的;“ordinary”表示普通的;“trivial”表示琐碎的。
这幅画被描述为“truly”,那应该是积极的评价,所以选“magnificent”。
2. The artist's style is very _____.A.uniquemonC.familiarD.similar答案:A。
“unique”表示独特的;“common”表示常见的;“familiar”表示熟悉的;“similar”表示相似的。
艺术家的风格通常是独特的,所以选“unique”。
3. The sculpture is _____ in design.A.simpleplexC.elaborateD.plain答案:C。
“simple”表示简单的;“complex”表示复杂的;“elaborate”表示精心制作的;“plain”表示朴素的。
雕塑通常会有精美的设计,所以选“elaborate”。
4. The performance was _____ and moving.A.powerfulB.weakC.lightD.faint答案:A。
“powerful”表示有力的;“weak”表示虚弱的;“light”表示轻的;“faint”表示微弱的。
表演通常是有力且动人的,所以选“powerful”。
5. The art work is full of _____.A.creativityzinessC.boredomD.dullness答案:A。
“creativity”表示创造力;“laziness”表示懒惰;“boredom”表示无聊;“dullness”表示枯燥。
小学上册英语第3单元期末试卷英语试题一、综合题(本题有100小题,每小题1分,共100分.每小题不选、错误,均不给分)1.The _____ (卡车) carries goods.2.The ____ has a long tail and is often seen playing.3.The ________ (生态系统保护) ensures biodiversity.4.The __________ (历史的契机) can lead to breakthroughs.5. A __________ is formed during a chemical reaction.6.What is the name of the famous ancient city in Italy?A. PompeiiB. RomeC. HerculaneumD. All of the above7. A mixture that appears different throughout is called a _______ mixture.8.The __________ is a region known for its deserts and dry climate.9.My favorite fruit is _______ (西瓜).10.What is the main topic of a story called?A. SettingB. PlotC. ThemeD. CharacterC11.They are going to ________ a picnic.12.What is the primary ingredient in salsa?A. TomatoB. OnionC. PepperD. Cilantro13. A _______ describes how easily an element can lose electrons.14.What is the capital of Kenya?A. NairobiB. MombasaC. KisumuD. NakuruA15.I have a blue _______ (我有一个蓝色的_______).16.I like to color pictures of _____.17. A ______ is a type of animal that can glide from tree to tree.18.I see a __ in the garden. (worm)19.The ________ was a prominent advocate for children’s rights.20.我的朋友喜欢 _______ (活动). 她觉得这很 _______ (形容词)21.The flamingo gets its pink color from the food it _______ (吃).22.The process of crystallization separates solids from ______.23.What is the primary color of grass?A. BlueB. GreenC. YellowD. RedB24. A rabbit can produce multiple litters of ________________ (幼崽) a year.25.The _____ (小牛) grazes in the field.26. A ______ is a systematic collection of data for analysis.27.The ______ (青蛙) croaks loudly in the evening.28.The ______ (果肉) of fruits is often sweet and nutritious.29.The chemical symbol for mercury is _______.30.I enjoy _______ (听音乐)在晚上.31.The clock is ________ on the wall.32.The tree is very ___. (tall)33.The story is very ________.34.I want to travel to ________ (意大利) one day.35.Greenland is the world's largest ________ (格林兰是世界上最大的________).36.I like to ___ (ride) my scooter.37.What is the primary color of a green pepper?A. GreenB. RedC. YellowD. Orange38. A __________ can help scientists learn about past climates.39.The _____ (养殖技术) improve plant health.40.The girl sings very ________.41.The first African American to serve as President was _______. (奥巴马)42.We have _______ for breakfast.43.The __________ is a famous coastal region.44.What do you call a story that is made up and not real?A. BiographyB. FictionC. HistoryD. Non-fiction答案:B45.What do you call a young bat?A. PupB. KitC. CubD. FawnA46.The cat is _____ (small).47.The sun is ___ in the sky. (high)48.The chemical symbol for cerium is ____.49.The process of oxidation involves the addition of ______.50. A ________ (植物文化活动) enriches community life.51.My birthday is in ___. (April)52.What is the capital city of Georgia?A. TbilisiB. BatumiC. KutaisiD. Rustavi53.The __________ is the main organ for breathing in humans.54.I enjoy making videos about my daily life to share with __________.55.I have a ______ of stuffed animals. (collection)56.What is the capital city of China?A. ShanghaiB. BeijingC. Hong KongD. GuangzhouB57.The chemical symbol for zirconium is ______.58.What do you call the imaginary line that divides the Earth into Northern and Southern Hemispheres?A. EquatorB. Prime MeridianC. Tropic of CancerD. Tropic of Capricorn59.What is the name of the famous American holiday celebrated on the fourth Thursday in November?A. ChristmasB. ThanksgivingC. New Year's DayD. Independence DayB60.I like to play ______ (soccer) with my friends.61.The Great Barrier Reef is found off the coast of __________.62.ts can ______ (繁殖) quickly and cover large areas. Some pla63.The ______ is known for her support of local artists.64.They are ________ a picnic today.65. A _____ (草坪) is perfect for picnics in the park.66.What is the name of the fairy tale character who had a long braid?A. CinderellaB. RapunzelC. Snow WhiteD. Belle67.Chemical reactions often involve the _______ of energy.68.What do you call a piece of furniture to sit on?A. TableB. ChairC. CouchD. BenchB69.The ancient Chinese invented _______ paper.70.My friend loves __________ (帮助他人).71. Wall was built over many _______. (世纪) The Grea72.Basalt is an example of a ______ rock that forms from lava.73.I want to be a ________.74.My favorite snack is ________ (巧克力) after school.75.Acids react with bases to form _____ and water.76.We should respect all ______ (生物).77.The seal can _________ fast in the water. (游泳)78.The chemical symbol for vanadium is _______.79.The _____ (door) is open.80.The first animal in space was a dog named ______ (莱卡).81. A ______ is a summary of experimental findings.82.I enjoy participating in online classes to learn more about __________.83.What is the currency used in the USA?A. YenB. DollarC. EuroD. Peso84.My cousin loves to __________ (与家人共度时光).85.I have a _____ (有趣的事情) to share.86.What do we call the frozen form of water?A. IceB. SteamC. LiquidD. Gas87.What is the opposite of "big"?A. HugeB. SmallC. TallD. Large88.The main component of natural gas is ______.89. A ____ enjoys playing fetch with its owner.90.The ________ (小溪) flows through the forest and is very peaceful.91.Which of these is a cold drink?A. TeaB. CoffeeC. LemonadeD. Soup92.His favorite sport is ________.93.The _____ (dragonfly) is colorful.94.What do you call a young horse?A. CalfB. FoalC. KidD. Puppy95.What do we call the layer of gases surrounding the Earth?A. AtmosphereB. LithosphereC. HydrosphereD. BiosphereA96.The invention of the printing press helped spread __________ (知识).97.What do we call the central part of a cell?A. NucleusB. CytoplasmC. MembraneD. OrganismA98.What do you call a person who studies the weather?A. MeteorologistB. BiologistC. GeologistD. ChemistA99.What do you call a person who repairs shoes?A. TailorB. CobblerC. SeamstressD. BlacksmithB100. A _____ (生态系统保护) is essential for future generations.。
The Avengers, super hero group is one of the world's most famous.With more and more under the cartoon characters, the Marvel Super Heroes of thesecompanies make a group, this can not only bring fire a numberof popular his second tier figures, but also create many opportunitiesfor Super Heroes made a guest appearance. For business purpose, the avenger was born. Avenger initially by the iron man, Thor, ant man and theWasp Woman, USA captain et al. With the continuous development, more and morecartoon characters to join, has become a composed of hundreds of superhero team hero.They have a unified plan and PR measures.On weekdays, the super heroes each busy each, each have their own careerand friends sike.Wait until the occurrence of some event, when one or several super hero cannot handleevents when the Avengers assembled together, for the maintenance of the world and their own reasons to fight.The Avengers, a super hero group, is one of the best-known across the world.The Avengers was initially built by Iron Man, Thor, Ant Man, Wasp Woman, and Captain America. With the continuous development, more and more cartooncharacters join, making it a league of hundreds of superheroes. They havea unified strategy and PR measures.On weekdays, the super heroes are busy dealing with their own things, and each of them has their own career, friends and enemies. When the occurrence of a certain event, which one or several super heroes cannot handle, the Avengers assemble together, fighting for the only world they live in and some special reasons.Tony Stark/Iron ManHe is the complete playboy who also happens to be an engineering genius.He creates an armored suit and become a super hero---Iron Man.Odin (The king of the gods) 's eldest son .Only he can use a hammer named Mjolnir which is a symbol of Thor’s power. Due to his overconfidence, h e has to learn compassion on earth. And he makes some good friends when he is fighting in the Avengers. He has a strong body, strength and bravery, knows the importance of responsibility and loves his people, so he will become a good king.Bruce Banner/HulkA scientist and researcher .Once he was wounded by radiation for a experiment about gamma ray. Then he can become hulk when he is angry or fear. Hulk is much more powerful than an army.Black widow/ Natalia RomanovaShe was trained into an agent by Soviet, but she betrayed them and escaped under the help of Clint. Then she joined the Avengers just like Clint.Hawkeye/ Clint BartonSteve Rogers/Captain AmericaHe took part in the "super soldiers plan" in World war 2.And he become the first and only survivor ,as Captain America.。
九江2024年统编版小学6年级上册英语第1单元真题试卷[有答案]考试时间:100分钟(总分:110)A卷考试人:_________题号一二三四五总分得分一、综合题(共计100题共100分)1. 选择题:What do you call a baby pig?A. PigletB. CalfC. KidD. Foal答案: A2. 填空题:In summer, I enjoy going to the ______ (海滩) to build ______ (沙堡) and swim in the ______ (海水).3. 选择题:What do you call the first book in the Bible?A. ExodusB. GenesisC. RevelationD. Psalms答案:B4. 听力题:Gamma-ray bursts are among the most energetic events in the ______.5. 听力题:A liquid that can dissolve a solute is called a ________.6. 填空题:My sister is very _______ (有趣).7. 选择题:What is the color of a typical tomato?A. YellowB. GreenC. RedD. Blue8. 听力题:The clock ticks _____ (slowly/quickly).9. 选择题:What is the chemical symbol for sodium?A. NaB. SC. SoD. Sd答案: A10. 填空题:I enjoy learning about animals and their habitats. It’s important to protect our ______ (环境).11. 听力题:Mixtures can be homogeneous or _____.12. 听力题:A solvent is the substance that dissolves the ______.13. 选择题:What is the shape of a stop sign?A. CircleB. TriangleC. SquareD. Octagon14. 听力题:My brother loves to build with ____ (Legos).15. 填空题:I want to _______ (去参加) the festival.16. 选择题:Which of these is a fruit?A. CarrotB. PotatoC. AppleD. LettuceWhat is the capital of China?A. BeijingB. ShanghaiC. Hong KongD. Guangzhou答案: A18. 选择题:What is the term for the light emitted by a star as it fuses hydrogen into helium?A. Stellar RadiationB. Nuclear FusionC. Solar EmissionD. Cosmic Light19. 填空题:The _____ (火龙果) is a unique fruit that looks very interesting.火龙果是一种外形非常独特的水果。
合肥2024年07版小学四年级上册英语第四单元真题(含答案)考试时间:90分钟(总分:100)A卷考试人:_________题号一二三四五总分得分一、综合题(共计100题)1、What is the term for a tree that loses its leaves in the winter?A. EvergreenB. DeciduousC. ConiferousD. Tropical答案:B2、听力题:The candy is very ___. (colorful)3、填空题:The _____ (花束) is a gift for special occasions.4、填空题:The ancient Greeks believed in many ________.5、听力题:A _______ is a substance that can donate hydrogen ions in a solution.6、听力题:The ancient Egyptians had a complex system of ________.7、听力题:The chemical formula for bismuth sulfide is ______.8、填空题:The _______ (小驱鸟) hunts insects in the air.9、听力题:The Milky Way is just one of many ______ in the universe.10、听力题:The main component of natural gas is _______.11、填空题:The tarantula is often feared for its ______ (外表).12、听力题:A _______ is a measure of how much mass is contained in a given volume.13、听力题:The main product of photosynthesis is _______.14、听力题:The chemical symbol for iron is __________.15、听力题:The __________ of a solution can affect how fast a reaction occurs.16、填空题:The _____ (袋鼠) jumps high.17、填空题:I love to ______ (与朋友分享) my interests.18、听力题:I like to ___ (listen/sing) to music.19、填空题:I feel ______ when I am with my friends.20、听力题:The substance that is dissolved in a solution is called the _______.21、填空题:In spring, flowers begin to ______.22、填空题:The __________ (历史的启发) ignites passion.23、听力题:My favorite animal is a ______ (dolphin).24、What is the opposite of 'full'?A. EmptyB. HalfC. CompleteD. Packed答案:A25、听力题:A _______ can convert mechanical energy into electrical energy.26、填空题:The _______ (Armistice) ending World War I was signed on November 11, 1918.27、填空题:My cousin, ______ (我的表弟), loves to dance hip hop.28、填空题:The first successful airplane flight took place in ________.29、填空题:The _______ (The Japanese Internment Camps) were established during WWII.30、听力题:I can ______ (jump) high on the trampoline.31、填空题:The ______ (小鸡) pecks at the ground, looking for seeds and ______ (虫子).32、填空题:The sheep grazes on _______ (草地).33、What is the term for a collection of stars, gas, and dust bound together by gravity?A. GalaxyB. NebulaC. Star ClusterD. Solar System答案:A34、听力题:The chemical formula for sodium acetate is ______.35、What is the name of the giant panda’s main food?A. BambooB. GrassC. LeavesD. Fruits答案:A36、听力题:The capital of Cuba is __________.37、填空题:The ancient Greeks made many contributions to ________ (科学).38、What do we use to cut paper?A. GlueB. TapeC. ScissorsD. Ruler答案:C39、Which animal hops?A. ElephantB. FrogC. FishD. Snake40、填空题:在古代,________ (scripts) 用于记录重要事件。
科技英语阅读理解目录Contents1.Mae Jemison (2)2.Can a Computer Think?……………………………………………………………………(4)3. BlackHoles (6)cation May Protect against Effects of Shrinking Brain (9)5.Radioactivity ……………………………………………………………………………(11)6. Uses of Ultrasound (14)7.Challenges for a Webbed Society (16)8.The World of Robots (19)9.The Scientific Exploration of Space…………………………………………………(21) 10. Improving IndustrialEfficiency through Robotics (24)11. Heat Loss from the Human Body ...............................................................(26) 12. Energy and Public Safety (28)13.Earth Resources Technology Satellites (32)14.Can Stress Make You Sick? (35)15.Can It Really Happen? (37)16.An Ultrasonic Torch ……………………………………………………………………(40) 17. Miracle of theBrain (42)18.All Over in a Flash (45)19.Control Earthquakes……………………………………………………………………(48) 20. Smoking and Cancer (51)21.How Well Do You See? (54)22. A Killer Is Born (56)23.It May Be Easy To Live Longer--Just Stop Eating (59)24.Study: T. Rex No Speedster (62)25.Modern Examination (64)26.Ecology (68)27.Appearances Can Be Important (70)28.Animal Senses (74)29.Telecommunications Satellite Spins Out of Control (76)30.Building Better Ultralight Computers (78)31.NASA Oks Second Space Tourist (81)32.Drink to - and for - Your Health (84)33.Three Things That Will Change Your Life (86)34.Bye-bye Credit Cards & Hello Digital Money (88)35.Gender Detector (90)1. Mae JemisonImagine you are lying on your back, strapped into a chair, with your knees bent in front of you. You feel your heart beating with excitement as you hear a voice on the earphone inside your helmet counting down slowly,” Three, two, one,” Then, beneath you, a deep rumble start as rocket fuel ignites in the huge engines. You① feel a lurch as the docking mechanisms let go, and your rocket begins to rise. This is the moment Mae Jemison has been waiting and working for since 1987. The firstAfrican-American female astronaut-in-training at the National Aeronautics and Space②Administration (NASA) , Jemison is scheduled to “fly” in September 1992. She is to serve as a specialist on Spacelab—J, a joint Japanese—American research project.Mae Jemison was thirty-three when she was selected for NASA’s astronaut training program. Astronaut candidates must have science degree. They must be fit and healthy with normal blood pressure and good eyesight. They must stand between five feet and six feet four inches tall. They must complete a one-year training program that includes water-survival lessons and weightless walks in a huge antigravity tank. On the 1991 mission, astronaut Jemison says that her “responsibility are to be familiar with the shuttle and how it operates, to do the experiments once you get③ into orbit, to help launch the payloads or satellites, and also to do extra-vehicular activities, or space walks.”How did Mae Jemison grow up to become such a special person? Science —especially astronomy—fascinated her from childhood.She also had a strong desire to help other people. Born in Alabama, but raised in Chicago, she studied chemical engineering and African—American culture and history at Stanford University. To help others, she decided to become a doctor. While still a medical student, she went to Cuba and Kenya on study trips, then worked in④a refugee camp in Thailand. She spent three years in West Africa as a doctor with the Peace Corps. When Dr. Jemison finally returned to the United States, she settled in California to practice medicine. And it was then that she decided to reach for the stars.Mae Jemison’s first application to NASA was not successful. Then, in 1986, the⑤Challenger space shuttle exploded, killing all aboard . NASA did not take in any new astronauts for about a year. When it finally reopened its application process, Mae Jemison was ready, and so was NASA. After being selected as a minority astronaut, Mae Jemison received a good deal of attention from newspaper and television. She explained to reporters that the space program and other fields in high technology offer promising careers for African-Americans and other minorities who study hard⑥and make the most of their opportunities .1.The first paragraph is about ______.A.how excited Mae Jemison was when she became an astronautB. how Mae Jemisonbecame an astronautC.how the people usually feel when the rocket they take begins to riseD.what Mae Jemison did after she was able to fly a rocket2.Which of the following statements is true?A.Mae Jemison had a strong desire to become famous.B.Mae Jemison was brought up in Alabama.C.Mae Jemison studied astronomy at Stanford University.D.Mae Jemison studied medicine.3.When did the Challenger space shuttle explode? A. Before Mae Jemison became a doctor.B.Shortly after Mae Jemison graduated from Stanford University.C.About a year before Mae Jemison was selected as an astronaut.D.About a year after Mae Jemison became famous all over the world.4.Mae Jemison believed that _______.A.men and women were not equalB.women were better paid than men wereC.American blacks were unable to find satisfactory jobs no matter how hard they studiedD.American blacks were able to find satisfactory jobs if they studied hard and made gooduse of their chance5.What is the attitude of the writer towards Mae Jemison’s achievements?A.JealousB.UpsetC. NegativeD. PositiveNotes:①lurch v. : To roll or pitch suddenly or erratically. 突然倾斜,突然地或者无规则地倾斜或坠落。
At the zoo,one is immediately enveloped by the cacophony of animal sounds,a symphony of nature that is both enchanting and intriguing.The first thing that catches your eye is the variety of enclosures,each designed to replicate the natural habitat of the animals it houses.The zoo is a place where one can observe a wide array of species,from the majestic lions with their impressive manes to the playful antics of the monkeys swinging from branch to branch.The elephants,with their immense size and gentle demeanor,are a sight to behold as they use their trunks to spray water or pick up food.The aviary is another highlight,housing a multitude of birds from around the world.The vibrant colors of the macaws and parrots contrast sharply with the sleek elegance of the eagles and hawks.The melodic songs of the birds fill the air,creating a soothing ambiance.Visitors can also marvel at the agility of the cheetahs as they sprint across their enclosure, demonstrating their incredible speed.The grace of the giraffes,with their long necks and legs,is captivating as they move gracefully,reaching for leaves high up in the trees. The zoo provides educational opportunities as well,with informative signs and displays that offer insights into the animals behaviors,diets,and conservation status.Interactive exhibits and feeding sessions allow visitors to engage more closely with the animals, fostering a deeper appreciation for wildlife.Children are particularly delighted by the petting zoo,where they can interact with more docile animals such as goats,sheep,and rabbits.This handson experience can be a memorable part of their visit,teaching them about the importance of gentleness and respect towards animals.The zoo also plays a crucial role in conservation efforts,often breeding endangered species in captivity to increase their numbers in the wild.This aspect of the zoos work is vital in preserving biodiversity and ensuring the survival of species that are at risk.In conclusion,a visit to the zoo is not only an entertaining experience but also an educational one.It offers a glimpse into the lives of various animal species,promoting awareness and appreciation for the natural world.The zoo serves as a reminder of our responsibility to protect and preserve the environment and its inhabitants for future generations.。
a r X i v :a s t r o -p h /0612504v 1 18 D e c 2006to appear in MNRASA unified picture for the γ-ray and prompt optical emissions of GRB 990123A.Panaitescu 1&P.Kumar 21Space Science and Applications,Los Alamos National Laboratory,Los Alamos,NM 87545,USA 2Department of Astronomy,University of Texas,Austin,TX 78712ABSTRACTThe prompt optical emission of GRB 990123was uncorrelated to the γ-ray light-curve and exhibited temporal properties similar to those of the steeply-decaying,early X-ray emission observed by Swift at the end of many bursts.These facts suggest that the optical counterpart of GRB 990123was the large-angle emission released during (the second pulse of)the burst.If the optical and γ-ray emissions of GRB 990123have,indeed,the same origin then their properties require that (i)the optical counterpart was synchrotron emission and γ-rays arose from inverse-Compton scatterings (the ”synchrotron self-Compton model”),(ii)the peak-energy of the optical-synchrotron component was at ∼20eV,and (iii)the burst emission was produced by a relativistic outflow moving at Lorentzfactor >∼450and at a radius >∼1015cm,which is comparable to the outflow deceleration radius.Because the spectrum of GRB 990123was optically thin above 2keV,the magnetic field behind the shock must have decayed on a length-scale of <∼1%of the thickness of the shocked gas,whichcorresponds to 106−107plasma skin-depths.Consistency of the optical counterpart decay rate andits spectral slope (or that of the burst,if they represent different spectral components)with the expectations for the large-angle burst emission represents the most direct test of the unifying picture proposed here for GRB 990123.Key words:gamma-rays:bursts -radiation mechanisms:non-thermal -shock waves1INTRODUCTIONThe Swift satellite has evidenced the existence (in a major-ity of bursts)of a fast-decaying phase after the end of γ-ray emission (e .g .O’Brien et al .2006),during which the 0.3–10keV flux falls-offas F x ∝t −(1.5−4).The emission of the opti-cal counterpart of GRB 990123,measured by ROTSE (Ak-erlof et al .1999),has a similarly steep decay,F o ∝t −(1.5−2.5)at about the same time (50–400s after trigger)as the fast-decaying phase of Swift X-ray afterglows.This similarity suggests that the optical counterpart of GRB 990123and the fast decay phase of Swift X-ray afterglows originate from the same shock of the GRB relativistic outflow.In Swift bursts,the transition from the prompt emission to the fast X-ray de-cay is continuous,which indicates that the γ-ray and X-ray emissions also have a common origin.This leads to the con-jecture that the optical and γ-ray emissions of GRB 990123arise from the same shock.As shown in figure 2of Galama et al .(1999),the prompt optical emission of GRB 990123is well above the extrap-olation of the burst continuum to lower energies.Then,if the optical and burst emission originate from the same part of the outflow,they must represent different spec-tral components,i .e .optical must be synchrotron emission and γ-ray must be inverse-Compton scatterings.This is the ”synchrotron self-Compton model”which has been used byPanaitescu &M´e sz´a ros (2000)and Stern &Poutanen (2004)to explain the hard low-energy spectra observed for some BATSE bursts (Preece et al .1998).Kumar et al .(2006)have shown that the temporal and spectral properties of GRBs 050126and 050219A favour this model for the γ-ray emission.As discussed by Nousek et al .(2006)and Zhang et al .(2006),the fast-decay phase of Swift afterglows can be iden-tified with the ”large-angle emission”released during the burst,i .e .the emission from the fluid moving at an angle θlarger than the inverse of the outflow’s Lorentz factor Γ,with θmeasured relative to the outflow center –observer axis.Any radiating GRB outflow whose opening is larger than Γ−1yields a large-angle emission,irrespective of the type of shock (internal,reverse-external,or forward-external)and radiative process.As shown by Kumar &Panaitescu (2000),relativistic effects lead to a simple relation between the spec-tral slope and decay index of the fast-decaying X-ray af-terglow,which is generally found to be consistent with the observations.If,as argued above,the prompt optical emission of GRB 990123and the fast-decay phase of Swift X-ray afterglows have the same origin,then the former could also be identi-fied with the large-angle emission produced during the burst.This conjecture can explain why the optical emission of GRB 990123appears uncorrelated with that at γ-rays.As shown2Panaitescu &Kumartime (s)101011021031040.01C γ (c t s /s ) F R (m J y )Figure 1.The BATSE 25–1000keV count-rate for GRB 990123,with 1s time resolution,and the ROTSE R -band light-curve of its optical counterpart.in Figure 1,the optical emission of GRB 990123is weaker during the first pulse,exhibits a maximum during the tail of the second pulse (which peaks at 38s),and then decays monotonically throughout the third GRB pulse and after the burst end.The decoupling of the optical and γ-ray emissions of GRB 990123can be explained if the optical counterpart is identified with the large-angle emission released during the second GRB pulse (when the optical counterpart peaks)and if the optical emission of other pulses is weaker than that of the second GRB pulse.Given the simple structure of GRB 990123light-curve and the sparse sampling of the optical counterpart,the lack of an optical-γ-ray temporal correlation could also be the result of fluctuations in the optical-to-γ-ray output ratio from pulse to pulse.Thus,the large-angle emission is not a unique explanation for the un-correlated optical and burst emissions of GRB 990123;it just represents a possible reason and a working assumption for the calculations below.Based on the above arguments,in this work we at-tribute the optical prompt emission of GRB 990123to the large-angle synchrotron emission produced during the sec-ond GRB pulse and identify the prompt γ-ray emission with up-scatterings of the synchrotron photons.The obser-vational constraints imposed on this scenario are presented in §2and used in §3to determine the outflow parameters which accommodate them.In §4,we discuss some impli-cations of the large-angle emission scenario for the optical counterpart and a possible shortcoming of the synchrotron self-Compton model,which can be circumvented if the mag-netic field decays and does not fill the entire GRB outflow.We emphasize two aspects of the following treatment of the unification of the γ-ray and prompt optical emissions of GRB 990123.First,we do not assume a certain mechanism for the dissipation of the relativistic outflow energy.This mecha-nism could be (i )internal shocks in an unsteady wind,as proposed by M´e sz´a ros &Rees (1999),or (ii )the external reverse-shock,as proposed by Sari &Piran (1999)(fig.1of Panaitescu &M´e sz´a ros 1998also shows that a 10–16th mag-nitude optical emission could arise from the reverse-shock),and further investigated by Kobayashi &Sari (2000),Soder-berg &Ramirez-Ruiz (2002),Fan et al .(2002),Panaitescu &Kumar (2004),Nakar &Piran (2005),and McMahon,Kumar &Piran (2006).Thus,the scenario proposed here does not represent a new theoretical framework for the GRB emission.Second,the calculations below address primarily the im-plications of the proposed unifying scenario and represent a test of that scenario only to the extent that the resulting physical parameters are plausible.Otherwise,the proposed scenario for the optical counterpart of GRB 991023is mo-tivated by (i )the similarity between its temporal proper-ties and those of the X-ray emission following Swift bursts,and (ii )the identification of the latter with the large-angle burst emission.The only observational test for the proposed scenario is the consistency between the decay of the opti-cal emission of GRB 990123and the expectation from the large-angle emission for the measured low-energy slope of the burst spectrum (§2).2OPTICAL AND GAMMA-RAY EMISSIONSOF GRB 990123The optical measurements of GRB 990123,shown in figure 1,are too sparse to pinpoint when the flux peaked,but suf-ficient to show that a substantial fraction of the post-peak optical flux arose during the second GRB pulse.As burst emission episodes may be dynamically independent,the de-cay of the ROTSE optical emission should be timed from the onset of the second GRB pulse,which occurred at ∼30s after the GRB trigger,as shown in Figure 2.The optical counterpart emission decays as a power in time F (t )∝t −α,with index α≃1.5.The available optical coverage of Swift afterglows in-dicates that,quite often,the optical emission decays as a power-law from the first observations,at only 100–200s after trigger (see figure 1of Panaitescu et al .2006).This suggests that the forward-shock contributes to the optical emission just at the end of the burst and motivates us to back-extrapolate the 0.1–2day optical emission of GRB af-terglow 990123to the epoch of the ROTSE observations and subtract it to determine the optical emission at that time which is excess of the forward-shock contribution.As shown in Figure 2,the ROTSE excess emission has a decay index α=1.8±0.1,but the power-law fit is not that good,having χ2=6.4for 4degrees of freedom.The reason is that the ex-cess emission exhibits a steepening decay,from α=1.3±0.3for the first two measurements after the second GRB pulse to α=2.0±0.2during the last four measurements (figure 2).If the decay of the ROTSE optical flux is indeed the large-angle emission produced during the burst and if this emission switches-offsufficiently fast,then the slope βo of the optical spectral energy distribution (SED),F ν∝νβo ,must be βo =2−α(1)(Kumar &Panaitescu 2000).Thus,the above possible de-cay indices αof the ROTSE optical emission imply that 0<βo <0.7.The consistency of βo with the burst SEDGRB9901233time (s)Figure2.The0.1–2day optical light-curve of GRB afterglow 990123(red symbols),fit with a power-law decay(thick,solid line),extrapolated to the epoch of ROTSE observations(blue symbols)and subtracted to isolate the early optical emission in excess of that from the forward-shock(black symbols).This excess emission exhibits an increasing decay rate after50s.Time is measured from30s after trigger,which is when the second GRB pulse starts(this pulse peaks about8s after its beginning and12 s before the largest opticalflux measured by ROTSE).The excess optical emission can arise in the same mechanism that generated the burst,its continuation after the end of the burst(which is at 60s)being due to the large-angle prompt emission.slope at low-energy(20–300keV),which Briggs et al.(1999) report to beβLE=0.4±0.1,supports the synchrotron self-Compton interpretation for the optical andγ-ray emissions of GRB990123because,in this model,the SED of syn-chrotron and inverse-Compton components must have the same spectral slopes at frequencies above self-absorption. Therefore,the SED of the emission of GRB990123’s optical counterpart should beFǫ∝ ν1/3ǫ<ǫp,syν−βHEǫ>ǫp,sy(2)as the only expected spectral slope consistent withβo and βLE is1/3.βo=1/3corresponds to the optical range being above the self-absorption energy,ǫa,sy,but below the peak-energy of the synchrotron spectrum,ǫp,sy.βLE=1/3implies that the20–300keV range is betweenǫa,ic=γ2pǫa,sy andǫp,ic=γ2pǫp,sy,whereγp is the peak Lorentz factor of the electron distribution with energy in the shockedfluid andǫp,ic is the peak-energy of the burst spectrum.The low-energy spectrum of GRB990123,Fν∝ν−βLE peaks at an energy which is a fractionβLE/(βLE+1)of the peak-energy E p of theνFνspectrum.According to Briggs et al.(1999),E p≃720keV for the second GRB pulse,therefore ǫp,ic(t p)=210keV.(3) The burst SED at high-energy(1–10MeV)is a power-law of slopeβHE=−2.1±0.1(Briggs et al.1999).This shows that theγp-electrons at the peak of the power-law electron distribution with energy,dN2r(θ2+Γ−2)(6) whereΓis the bulk Lorentz factor of the GRB-emitting source,and is Doppler-boosted by a factorD=2Γt(8) on virtue of equations(6)and(7).Therefore,the large-angle emission arriving atfixed observer frequency corresponds to an ever-increasing comoving-frame frequency.Then,the above conclusion that, for GRB990123,optical is below the peak-energy of the synchrotron spectrum(ǫp,sy)implies that the synchrotron light-curve should steepen at t+whenǫp,sy crosses the op-tical domain:2eV=ǫ′p,sy D(t+)=ǫ′p,sy D(t p)t p t+(9) where prime denotes a quantity in the comoving-frame.The ROTSE emission with the forward-shock contribution sub-tracted(Figure2)shows such a steepening at about45s, the subsequent decay index,α≃2,implying an optical SED slopeβo≃0,as expected at the peak of synchrotron spec-trum.For now,we parameterize the time when t+relative to the epoch of the second GRB pulse peak:t+=x t p.There-fore,the observer-frame synchrotron peak-energy isǫp,sy(t p)=2x eV x>1.(10) The extrapolation of the power-lawfit to the ROTSE4Panaitescu &Kumar10101010101010photon energy (eV)10−210−110101102103104F ν (m J y )εa,sy =0.17εp,sy εc,sy =7εp,sySYICx=10 η=10Figure 3.Synchrotron (optical)and inverse-Compton (γ-ray)components for GRB 990123.The synchrotron SED is the sim-plified spectrum given in equation (2)and has the peak fre-quency and flux given in equations (10)and (11)for x =10.The inverse-Compton spectrum is calculated by integrating the scattered emissivity per electron over the electron distribution (equation 4).Dotted curves show the effect of self-absorption for ǫa,sy =0.17ǫp,sy ,(equation 49).Dashed line shows the effect of electron cooling for ǫc,sy =7ǫp,sy (equation 5).For comparison,the dot-dashed curve shows the inverse-Compton spectrum for monoenergetic electrons with γp given in equation (16).light-curve to t p ,predicts an optical flux of F R (t p )=4Jy.The extrapolation of the forward-shock (FS)emission to the same time is F F S (t p )=0.93Jy,therefore the peak of the ex-cess optical emission (which we attribute to the same mecha-nism as the burst itself)is F sy (t p )=F R (t p )−F F S (t p )=3.07Jy (the forward-shock emission may have started later than the optical peak time,in which case the F sy (t p )above un-derestimates the true synchrotron flux by 25%).Taking into account that the slope of the optical SED is βo =1/3,it fol-lows that the flux at the peak of the synchrotron spectrum isF p,sy (t p )=F sy (t p )ǫp,syǫc,syβHEǫc,syǫp,icβLE(13)which leads to x <14for ǫc,sy =7ǫp,sy ,which is the lowest value of the cooling energy (see equation 5),and to x <9for ǫc,sy >2keV.Therefore,under the assumption that the synchrotron spectrum extends up keV energies,the peak-energy of the synchrotron spectrum should satisfy x <∼7−14(14)and should cross the optical at t +=x t p <115s after the peak of the second GRB pulse (145s after trigger).If ROTSE emission is mostly the large-angle emission of the second GRB pulse then the optical light-curve should exhibit a break at t +,which is consistent with observations (see Figure 2).Based on the constraint above,we normalize x to 10.3SYNCHROTRON ANDINVERSE-COMPTON EMISSIONSIntegrating the scattering photon spectrum per electron (e .g .equation 2.48of Blumenthal &Gould 1970)over the syn-chrotron spectrum (equation 2)and over the electron distri-bution (equation 4),we obtain thatǫp,ic =0.82γ2p ǫp,sy .(15)Therefore,the typical electron Lorentz factor in the shocked fluid is γp =ǫp,ic3Γǫ′p,sy4πehGRB9901235 The receivedflux at the peak of the synchrotron spec-trum isF p,sy=z+13φ(p)e3ǫp,sy F p,sy =2.4x−4/31=0.82γ2pF p,ic3γ2dτe3p−1F p,sy =7.1×10−5x−1/31(27)using the synchrotron and peakfluxes of GRB990123.Theelectron optical thickness is set by the electron column den-sity:τe=σTr2(28)whereσT is the Thomson cross-section.The last two equa-tions allow the determination of the radius a which the burstand prompt optical emissions are released:rγ=6.3×1014x−2/31η−1/21cm.(29)The last observational constraint to be used is equation(5).The radiative cooling timescale of theγp-electrons ist c(γp)=z+1σT1cΓ=5.7×104x−2/31η−1/21Γ−2s(32)for a shell at the GRB radius rγgiven equation(29).Then,the condition t c(γc)>t∆leads to a lower limit on theLorentz factor of the shockedfluid:Γ≥1660x1/21η−1/61.(33)Substituting in equation(20),wefind a lower limit onthe magneticfieldB≤290x3/21η1/61G(34)while equation(32)yields an upper limit on the sub-pulseduration:δt≤20x−5/31η−1/61ms.(35)Note that r,Γ,B andδt have a weak dependence on thesomewhat uncertain numberηof overlapping sub-pulseswithin a GRB pulse.and that the timescale for the sourceintrinsicfluctuations,δt,is smaller than the temporal reso-lution(256ms)of GRB990123light-curve shown infigure1of Briggs et al.(1999),i.e.the source intrinsicfluctuationsare averaged over10times thefluctuation timescale.The comoving-frame peak-energy of the inverse-Compton spectrum isǫ′p,ic=(z+1)ǫp,ic/Γ<∼7×10−4m e c2,henceγpǫ′p,ic<∼0.07m e c2.This means thatthe second inverse-Compton scattering occurs around the⋆The origin of the burst emission from a shell with this thicknessis the only non-trivial assumption made in this section6Panaitescu &KumarKlein-Nishina reduction in the scatteringtegrating the Compton parameter given in over the burst spectrum and electron ing the Klein-Nishina scattering that the Compton parameter for the second ˜Y >∼0.89γ2p τe =0.82x −4/31,i .e .a factor <∼Y for the first scattering.Therefore,the Compton model implies the existence of a ponent,whose F νspectrum peaks at γ2p ǫe,ic and having a fluence ΦGeV =˜Y Φγ>∼3×10−44IMPLICATIONS OF SELF-COMPTON MODEL FOR 4.1Jet edgeIf the optical counterpart of GRB 990123is indeed the large-angle emission produced during the second GRB pulse (i .e .if there is little contribution to the ROTSE optical emission from subsequent GRB pulses)then the optical light-curve should exhibit a sharp break when photons emitted from the edge of the jet (θ=θjet )arrive at the observer.From equation (6),this break should be seen at t edge =(z +1)r γθ2jet˜Γ(t jet )(37)where ˜Γis the Lorentz factor of the circumburst medium swept-up by the forward-shock,which can be calculated from the isotropic-equivalent kinetic energy E of the shock and the density of the circumburst medium:E =4πr A m p c 2˜Γ2.(38)The above equation applies for a circumburst medium witha radial proton density distribution n (r )=Ar −2,character-istic for the wind ejected by a massive star as the GRB pro-genitor,and results from that the comoving-frame energy-per-particle in the shocked medium is ˜Γ.For the above the dynamics of the shocked medium,˜Γ∝r −1/2,integration of the equation for photon arrival t =3(z +1)˜Γ2(r ′)(39)where the factor 3relates ˜Γto the arrival time of photons emitted from θ=˜Γ−1(as most of the afterglow emission arises from this location),leads to ˜Γ(t )=3Ez +1−1/4.(40)Taking the GRB output E γ=3×1054ergs as an estima-tion of the forward-shock kinetic energy and parameterizing the wind medium density to that of a massive star ejecting 10−5M ⊙yr −1at 103km s −1,i .e .A =3×1035A ∗cm −1,we obtaintime (s)Figure 4.Same as in Figure 2,but using a steeper fit,F F S ∝t −1.23instead of F F S ∝t −1.23.The ROTSE light-curve with the forward-shock emission subtracted exhibits now a sharp decline at t >∼50s.˜Γ(t d )=25E 1/454.5A −1/4∗t −1/4d (41)where t d is observer time measured in days.From equations (37)and (41),the jet opening corre-sponding to a light-curve break at t jet <∼3d isθjet <∼0.052E −1/454.5A 1/4∗rad .(42)Then,from equation (36)and (29),the large-angle emission should end att edge <∼74x −2/31η−1/21E −1/254.5A 1/2∗s .(43)Coincidentally,this is about the same as the time t +=xt p =80x 1s when the peak energy of the synchrotron spectrum crosses the optical,i .e .there are two independent factors which imply the existence of a steeper decay of the large-angle emission after 80s from the beginning of the second GRB pulse (110s after trigger).This conclusion is at odds with the ROTSE light-curve shown in Figure 2but is consis-tent with the optical counterpart emission after subtracting a slightly more steeply-decaying forward-shock contribution,as illustrated in Figure 4.The power-law fit to the 0.1–2day optical light-curve shown in Figure 4is statistically accept-able (χ2=13/17dof)and has a decay index αlarger than that of the best-fit shown in Figure 2by 1σ.4.2Self-absorption photon energyFor the power-law electron distribution given in equation(4),the self-absorption linear coefficient at frequency νis αν=p +2(γp m ec )2ν−2∞γpdγP ν(γ)γ3πm e c 2Fν16eGRB9901237 the modified Bessel function of index5/3)andνc the syn-chrotron characteristic frequency for electrons of energyγm e c2.Atν≪νc(γp),the synchrotron function isF(y)≃2.15y1/3(46)and the integral in equation(44)can be calculated ana-lytically,leading to the following optical thickness to syn-chrotron self-absorption,τa(ν)=(αντe)/(n eσT),τa(ν)=3.3p+2σT Bγ5p νǫp,sy −5/3.(48)Therefore,the self-absorption energy of the synchrotron spectrum,defined byτa(ǫa,sy)=1,isǫa,sy>∼0.17x2/51η−1/101ǫp,sy=3.3x7/51η−1/101eV.(49)Ifǫa,sy were above the optical,thenβo=2and the large-angle emission would beflat(from equation1).That the ROTSE optical light-curve decays,implies thatǫa,sy is below the optical domain.Then equation(49)leads tox<∼10η1/141.(50) which is close to the upper limit obtained by requiring that the synchrotronflux does not overshine the inverse-Compton emission at2keV(equation14).The synchrotron self-absorption energy given in equation(49)implies that the up-scattered self-absorption energy isǫa,ic>∼48Panaitescu &KumarThe sub-pulse duration of equation (32)is now t ∆≤0.25x −5/31η−1/62b −5/6−1.5s,therefore the source intrinsic fluc-tuations are marginally resolved and the observed fluctua-tion amplitude of about 10%requires that η≃100,which is the canonical value chosen in the above equations.Requiring that the sub-pulse duration t ∆does not exceed the FWHM duration of a GRB pulse,which is t γ≃10s,leads tob >6×10−4x −21η−1/5(56)with η>∼1because,for t ∆≃t γ,the GRB pulse should be a single emission episode.The comoving-frame electron density of the shocked fluid isn ′=N eΓ′n ′m p c 2≃0.27x 13/61(Γ′−1)−1ζ−1b −1−1.5(58)of the energy density in the shocked fluid,where Γ′is theLorentz factor of the shock energizing the GRB-emitting fluid measured in the frame of the yet unshocked plasma.If the GRB ejecta were not initially highly magnetized then a sub-equipartition magnetic field (εB <0.5)requires thatb >0.03x 13/61(Γ′−1)−1ζ−1.For a relativistic shock with Γ′∼few and ζ=4Γ′,this condition becomesb >∼10−4x 13/61(59)which is close to that obtained by requiring that t ∆<∼10s (equation 56).Thus,we find that the magnetic field length-scale is a fraction b =10−3.5−10−1.5of the thickness of the shocked gas.For the comoving-frame density given in equation (57),the plasma skin-depth in the shocked gas is λ=cπγp m eGRB9901239 due to the large computational effort required to follow theevolution of magneticfields over such long scales.We notethat other researchers have obtained similar constraints onthe magneticfield decay length-scale:from energetic argu-ments related to the outflow parameters obtained throughafterglow modelling,Rossi&Rees(2003)have set a lowlimit of10−2on the fraction of shellfilled by magneticfield,while Pe’er&Zhang(2006)have inferred a decay length-scale smaller by a factor10than our value,from the con-dition that,in internal-shocks synchrotron-emission GRBs,electrons do not cool significantly during the burst.There are two other bursts whose accompanying opti-cal emission has been measured.The optical andγ-ray light-curves of GRB041219A(Vestrand et al.2005)are correlatedand the post-burst decay of the optical counterpart exhibitsvariability(Blake et al.2005),both indicating that the coun-terpart is not the large-angle emission released during theburst.The optical andγ-ray emissions of GRB050820A(Vestrand et al.2006,Cenko et 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