Determining atmospheric conditions at the terminator of the hot-Jupiter HD209458b
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关于降水量与温度的模板英语作文全文共3篇示例,供读者参考篇1The Intricate Dance of Precipitation and TemperatureClimate change is one of the most pressing issues facing our planet today. As students, we are constantly reminded of the importance of understanding the complex interplay between various environmental factors and their impact on the world around us. Among these factors, precipitation and temperature stand out as pivotal players, influencing everything from agriculture to ecosystems and even human settlements. In this essay, I will delve into the intricate relationship between these two crucial elements, drawing upon scientific research andreal-world examples to illustrate their profound significance.To begin, let us first understand what precipitation and temperature are and how they are measured. Precipitation refers to the condensed moisture that falls from the atmosphere, including rain, snow, sleet, and hail. It is typically measured in units such as millimeters or inches over a specific period of time. Temperature, on the other hand, is a measure of the degree ofhotness or coldness of a substance, typically expressed in degrees Celsius or Fahrenheit. Both precipitation and temperature are monitored and recorded by various meteorological agencies around the world, providing invaluable data for scientific analysis and forecasting.The relationship between precipitation and temperature is a complex and intricate one, influenced by a myriad of factors such as atmospheric conditions, geographical features, and even human activities. One of the most evident connections lies in the water cycle, a continuous process that governs the movement of water on Earth. As temperatures rise, the rate of evaporation from bodies of water and land surfaces increases, leading to higher levels of moisture in the atmosphere. This, in turn, can result in increased precipitation in certain regions, while potentially causing droughts in others due to the uneven distribution of moisture.However, the relationship between precipitation and temperature is not always straightforward. In some cases, higher temperatures can actually lead to decreased precipitation, particularly in arid and semi-arid regions. This phenomenon is known as the "hot desert" effect, where the excessive heat causes the air to become too dry to support significant rainfall.Conversely, in certain tropical regions, warmer temperatures can fuel the formation of powerful storms and hurricanes, leading to intense and sometimes destructive precipitation events.The impact of this delicate dance between precipitation and temperature extends far beyond the confines of meteorology. Agriculture, for instance, is heavily dependent on the balance between these two factors. Farmers worldwide rely on timely and adequate precipitation to provide water for their crops, while temperature plays a crucial role in determining the growing seasons and crop yields. Extreme weather events, such as droughts or flooding, can have devastating consequences for food production, potentially leading to shortages and economic instability.Furthermore, the relationship between precipitation and temperature has significant implications for ecosystems and biodiversity. Changes in precipitation patterns can disrupt the delicate balance of water resources, affecting the survival of various plant and animal species. Alterations in temperature can also influence the distribution and behavior of these species, forcing them to adapt or migrate to more suitable habitats. The loss of biodiversity, in turn, can have far-reaching consequencesfor the entire ecosystem, impacting services such as pollination, nutrient cycling, and soil formation.Urban areas are not immune to the effects of precipitation and temperature either. Rapidly growing cities often face challenges in managing stormwater runoff, particularly during periods of intense precipitation. Inadequate drainage systems can lead to flooding, property damage, and disruptions to daily life. Additionally, extreme heat waves exacerbated by urban heat island effects can pose significant health risks to vulnerable populations, such as the elderly and those with pre-existing conditions.In light of these challenges, it is crucial for us as students to develop a comprehensive understanding of the relationship between precipitation and temperature. By studying climate science, meteorology, and environmental studies, we can gain invaluable insights into the complex mechanisms that govern these phenomena and their far-reaching impacts.Furthermore, as future leaders and decision-makers, it is our responsibility to advocate for sustainable practices and policies that address the challenges posed by climate change. This may include supporting initiatives to reduce greenhouse gas emissions, promoting renewable energy sources, andimplementing measures to adapt to the changing climate. By taking a proactive approach, we can mitigate the negative consequences of disruptions to precipitation and temperature patterns, ensuring a more resilient and sustainable future for ourselves and generations to come.In conclusion, the intricate dance between precipitation and temperature is a captivating and vital subject that deserves our utmost attention. As students, we have the opportunity to delve deep into this topic, exploring its scientific underpinnings,real-world implications, and potential solutions. By embracing this knowledge, we can better understand the intricate web of connections that bind our planet together and work towards creating a more sustainable and resilient world for all.篇2Precipitation and Temperature: The Dynamic DuoAs a student of environmental science, I've come to appreciate the intricate dance between precipitation and temperature – two key players in shaping our planet's climate and ecosystems. These meteorological partners engage in an intricate waltz, influencing each other's patterns and impacting everything from agriculture to urban planning.Let's start with precipitation, the lifeblood of our world. Whether in the form of rain, snow, sleet, or hail, precipitation is the ultimate source of freshwater, replenishing our rivers, lakes, and aquifers. Without it, life as we know it would cease to exist. And yet, the distribution of precipitation is far from uniform, with some regions experiencing torrential downpours while others suffer from relentless droughts.This uneven distribution is where temperature comes into play. Temperature plays a pivotal role in determining the phase and intensity of precipitation. Warmer air can hold more moisture, increasing the likelihood of heavy rainfall or thunderstorms. Conversely, colder temperatures can lead to snowfall or freezing rain, transforming the landscape into a winter wonderland.But the relationship between precipitation and temperature goes beyond just determining the form of precipitation. It's a delicate dance, with each partner influencing the other's movements. For instance, increased precipitation can lead to cooler temperatures through the process of evaporative cooling. As water evaporates from the Earth's surface, it absorbs heat from the surrounding air, reducing the overall temperature.Conversely, higher temperatures can intensify the water cycle, leading to increased evaporation and, consequently, more precipitation. This is particularly evident in tropical regions, where warm temperatures fuel the formation of massive thunderstorms and monsoons.The intricate interplay between precipitation and temperature has far-reaching consequences for our planet. In agricultural regions, the timing and amount of rainfall can make or break a crop season. Too little precipitation can lead to drought conditions, stunting plant growth and reducing yields. Conversely, excessive rainfall can waterlog fields, causing root rot and other problems.In urban areas, the relationship between precipitation and temperature takes on a different dimension. Heavy rainfall events can overwhelm drainage systems, leading to flooding and property damage. At the same time, prolonged periods of high temperatures can strain water resources and increase demand for cooling, putting stress on energy grids.But perhaps the most significant impact of the precipitation-temperature relationship is its role in shaping global climate patterns. The distribution of precipitation and temperature regimes across the planet determines theboundaries of different ecosystems, from lush rainforests to arid deserts. These ecosystems, in turn, influence the Earth's energy balance, albedo (reflectivity), and carbon cycles, all of which feedback into the climate system.One of the most pressing concerns in the study of precipitation and temperature is the potential impact of climate change. As global temperatures rise due to increasing greenhouse gas emissions, we are already witnessing shifts in precipitation patterns. Some regions are experiencing more frequent and intense droughts, while others are seeing an increase in heavy precipitation events, leading to flooding.These changes have far篇3The Impacts of Changing Precipitation Patterns and Temperature on the EnvironmentClimate change is one of the most pressing issues facing our world today. As greenhouse gas emissions continue to rise, we are witnessing tangible impacts on the environment through altered weather patterns, rising temperatures, and changes in precipitation levels across the globe. In this essay, I will explore the relationship between precipitation, temperature, and theirfar-reaching effects on ecosystems, agriculture, water resources, and human communities.To begin, it is crucial to understand the fundamental connection between precipitation and temperature. Precipitation, which includes rainfall, snowfall, and other forms of moisture, is driven by the Earth's water cycle. As temperatures rise due to increased greenhouse gas concentrations in the atmosphere, the rate of evaporation from oceans, lakes, and other water bodies increases. This enhanced evaporation leads to more water vapor in the air, which can potentially result in more frequent and intense precipitation events in certain regions.However, the relationship between temperature and precipitation is not uniform across the globe. While some areas may experience an increase in precipitation, others may face prolonged droughts and decreased rainfall. This uneven distribution of precipitation can have severe consequences for ecosystems and biodiversity. For instance, in regions experiencing reduced rainfall, plants and animals may struggle to survive, leading to potential habitat loss and species extinction. Conversely, areas with excessive precipitation may face challenges such as flooding, soil erosion, and the spread of waterborne diseases.The impacts of changing precipitation patterns and temperature are particularly significant for agriculture, which relies heavily on predictable weather conditions and adequate water supply. Farmers around the world are already grappling with the effects of climate change, including shifts in growing seasons, crop failures due to droughts or excessive rainfall, and the spread of pests and diseases favored by warmer temperatures. These challenges pose a serious threat to food security, especially in developing countries where agriculture is a primary source of livelihood and sustenance.Furthermore, changes in precipitation and temperature can have profound effects on water resources. Melting glaciers and snow packs, combined with altered precipitation patterns, can disrupt the supply of freshwater to rivers, lakes, and aquifers. This can lead to water scarcity in some regions, while others may face increased risks of flooding and water-related disasters. The availability and quality of freshwater are essential for human consumption, agriculture, industry, and ecosystem health, making the management of water resources a critical issue in the face of climate change.In addition to the direct impacts on ecosystems and human societies, changing precipitation patterns and temperature canalso contribute to feedback loops that amplify the effects of climate change. For example, as Arctic sea ice melts due to rising temperatures, the Earth's surface absorbs more heat, leading to further warming and potentially altering atmospheric circulation patterns, which can influence precipitation distribution.Addressing the challenges posed by changing precipitation patterns and temperature requires a multi-faceted approach involving mitigation efforts to reduce greenhouse gas emissions, adaptation strategies to enhance resilience, and international cooperation. Mitigation efforts can include transitioning to renewable energy sources, improving energy efficiency, and promoting sustainable land use practices. Adaptation strategies may involve developing drought-resistant crops, implementing water conservation measures, and strengthening infrastructure to withstand extreme weather events.Moreover, international cooperation is essential in tackling this global issue. Climate change does not respect national boundaries, and its impacts often transcend borders. Collaborative efforts among nations, such as the Paris Agreement, aim to coordinate actions and support vulnerable regions in adapting to and mitigating the effects of climate change.In conclusion, the relationship between precipitation, temperature, and climate change is complex and far-reaching. Altered precipitation patterns and rising temperatures pose significant challenges for ecosystems, agriculture, water resources, and human communities worldwide. As students and future leaders, it is our responsibility to understand the gravity of this issue and actively participate in efforts to mitigate and adapt to the impacts of climate change. Through collective action, scientific advancements, and a commitment to sustainability, we can work towards preserving a livable planet for present and future generations.。
龙卷风的形成原理英语作文Title: The Formation Principle of Tornadoes。
Tornadoes are one of the most awe-inspiring and destructive forces of nature. Understanding the formation principle behind these swirling vortices is crucial for predicting and mitigating their impact. In this essay, we delve into the intricate mechanisms that give rise to tornadoes, exploring the atmospheric conditions, and dynamic processes involved.Tornadoes typically form within severe thunderstorms, known as supercells, under specific atmospheric conditions. One of the key ingredients for tornado formation is wind shear, which refers to the change in wind speed and direction with height. Wind shear creates a horizontal spinning effect within the storm, known as horizontal vorticity.As the supercell evolves, updrafts within the stormtilt the horizontal vorticity into the vertical, creating a rotating column of air known as a mesocyclone. The mesocyclone serves as the precursor to tornado formation, providing the necessary rotation for the development of a tornado.Within the mesocyclone, another crucial process occurs: the formation of a rear-flank downdraft (RFD). The RFD is a region of descending air on the rear side of the mesocyclone, often associated with intense downdrafts and precipitation. As the RFD descends, it can create avertical stretching of the rotating air, further enhancing the rotation and leading to the formation of a tornado.The interaction between the updrafts, downdrafts, and rotating air within the supercell creates a dynamic environment conducive to tornado formation. However, notall supercells produce tornadoes, and the exact mechanisms behind tornado genesis remain a subject of ongoing research.Several factors influence whether a supercell will produce a tornado, including the intensity of the updrafts,the strength of the wind shear, and the presence of a strong mesocyclone. Additionally, environmental factors such as atmospheric instability and moisture content play a role in determining the likelihood of tornado formation.Once a tornado forms, its behavior can vary widely, from relatively weak and short-lived to intense and long-track tornadoes capable of causing catastrophic damage. Tornado intensity is classified on the Enhanced Fujita (EF) scale, ranging from EF0 to EF5, based on the estimated wind speeds and resulting damage.In conclusion, tornado formation is a complex interplay of atmospheric dynamics within supercell thunderstorms. Understanding the underlying principles behind tornado genesis is essential for improving tornado prediction and warning systems, ultimately reducing the loss of life and property associated with these devastating natural phenomena. Ongoing research continues to advance our knowledge of tornado formation, helping to unravel the mysteries of one of nature's most powerful forces.。
S-190 Unit 5: Atmospheric Stability, Winds, and Clouds Summary:Surface winds, temperature, and relative humidity are the most commonly considered and easy to measure elements in the fire environment. Less obvious, but equally important, is atmospheric stability, and related vertical air movements that influence fire behavior.Incident Position Description (IPD) Alignment:This unit aligns with the following FFT2 IPD specific duties(https:///positions/fft2/position-ipd):•Apply the knowledge of fuels, terrain, weather, and fire behavior to decisions and actions. Objectives:Students will be able to:•Describe atmospheric stability and discuss the effects on fire behavior.•Describe wind and its effects on fire behavior.•Explain cloud classifications and their impact on fire behavior.•Explain the similarities between smoke layers and clouds in relation to impact on fire behavior. Unit at a Glance:Topic Method Duration Unit Introduction Presentation 5 MinutesAtmospheric Stability Presentation 15 Minutes Wind Presentation 15 MinutesClouds Presentation 15 Minutes Smoke Layers Presentation 10 Minutes Total Unit Duration 60 Minutes Materials:•Incident Response Pocket Guide (IRPG), PMS 461, https:///publications/461. •NWCG Glossary of Wildland Fire, PMS 205, https:///glossary/a-z.•Fire Weather Cloud Chart, PMS 438, https:///publications/438.•Notebooks for participants.•Ability to display images and video on large screen.•White board or easel access for group breakout.S-190 Unit 5: Atmospheric Stability, Winds, and CloudsSlide 1S-190 Unit 5: Atmospheric Stability, Winds, and Clouds1S-190 Unit 5: Atmospheric Stability, Winds, and CloudsReview unit objectives.Atmospheric StabilityS-190 Unit 5: Atmospheric Stability, Winds, and Clouds3Play VideoTitle Introduction to Atmospheric StabilitySummary Introduces the way atmospheric stability can affect wildland fire.Time (00:45)AudioS-190 Unit 5: Atmospheric Stability, Winds, and Clouds 4Atmospheric StabilityThe degree to which vertical motion in the atmosphere is either enhanced or suppressed.• Environmental temperature structure of the atmosphere determines whether the atmosphere willenhance or suppress vertical motion.S-190 Unit 5: Atmospheric Stability, Winds, and Clouds5Example of Atmospheric Stability•Hot air inside the balloon is less dense than theenvironmental air outside, causing the balloon to rise.•As temperatures warm, the density of theenvironmental air rises, air in the balloon becomes less dense in comparison, and the balloon descends.Pre-Video Discussion• When heated, air parcels becomes less dense and rise in the atmosphere.• Using a hot air balloon as an example helps firefighters grasp the basic concepts of atmosphericstability. The hot air balloon can be thought of as an air parcel.❑ Play VideoTitle Hot Air BalloonsSummary The time-lapse video of hot air balloons in flight shows a stable layer of air at the surface, indicated by the low-level stratus cloud (fog) over the river. Time (00:10) No Audio❑ Inform participants the same concept applies to smoke columns, cumulus clouds, and thunderstorms, as heat from solar radiation or fires can decrease the stability in the atmosphere.S-190 Unit 5: Atmospheric Stability, Winds, and Clouds6Determining Atmospheric StabilityUnstableStableAir Parcel TempEnvironmental Temperature• Atmospheric stability is determined by comparing the temperature of an air parcel or smoke columnto the environmental temperature – the air temperature outside the parcel or smoke column.• Stable: If the parcel temperature is equal to or cooler than the environmental temperature, it will stayat its current level or sink.• Unstable : If the air parcel temperature is warmer than the environmental temperature, it will rise.Reference Haines Index (HI) in the Incident Response Pocket Guide (IRPG), PMS 461,https:///publications/461.Stable Atmospheric IndicatorsS-190 Unit 5: Atmospheric Stability, Winds, and Clouds7•Visual indicators of stable atmospheric conditions:o Smoke layer.o Stratus clouds or fog.o Low intensity fire as a result of suppressed vertical motion and weak inflow wind to feed fire new oxygenated air.o Mountain wave clouds occur, which indicate strong winds aloft that could surface on the lee side of a mountain range that day.•Effects of stable atmospheric conditions on fire behavior:o Limited rise of smoke columns, resulting in poor smoke dispersion and visibility.o Reduced inflow of fresh air, thereby limiting fire growth, and intensity.o Lower surface wind speeds and fire spread rates, except in mountainous, and hilly terrain – refers to foehn winds.Unstable Atmospheric IndicatorsS-190 Unit 5: Atmospheric Stability, Winds, and Clouds8•Visual indicators of unstable atmospheric conditions:o Towering smoke plume.o Cumulus clouds – these are from rising air parcels.o Cumulonimbus clouds – these are from rising air parcels.o High intensity fire as a result of increased vertical motion and sufficient, sometimes intense, inflow wind feeding the fire new oxygenated air.o Gusty winds – a result from mixing of the lower atmosphere.o Good visibility.•Effects of unstable atmospheric conditions on fire behavior:o Increased likelihood of fire whirls and dust devils.o Increased likelihood for gusty and erratic surface winds.o The height and strength of convection and smoke columns often increase significantly.o Increased likelihood of fire brands being lifted to great heights.S-190 Unit 5: Atmospheric Stability, Winds, and Clouds9Determining Atmospheric StabilityUnstableStableAir Parcel TempEnvironmental Temperature• Atmospheric stability is determined by comparing the temperature of an air parcel or smoke columnto the environmental temperature – the air temperature outside the parcel or smoke column.❑ Stable: If the parcel temperature is equal to or cooler than the environmental temperature, it will stayat its current level or sink. ❑ Unstable : If the air parcel temperature is warmer than the environmental temperature, it will rise. ❑ Reference Haines Index (HI) in the Incident Response Pocket Guide (IRPG), PMS 461, https:///publications/461.S-190 Unit 5: Atmospheric Stability, Winds, and Clouds 10Atmospheric Temperature and Inversions•An inversion is a layer of very stable air.•An inversion acts like a cap or lid to severely limit the upward movement of air.Extend the discussion on atmospheric temperature and inversions using the image:o Warm layers exist at different levels of the atmosphere. Meteorologists use weather data and atmospheric models to determine the strength and level of the inversions.o Once the level and strength of the inversion is measured and analyzed, the meteorologist can determine the impacts on the fire environment.Inversion -Warm LayerS-190 Unit 5: Atmospheric Stability, Winds, and Clouds11Pre-Video Discussion❑Extend the discussion on atmospheric temperature and inversion using the video example of a low-level inversion:o The video shows an inversion that is preventing upward vertical motion, noted by the fog layer. o Surface heating or temperature changes above the inversion can erode and break the inversion. o Heat from fire activity can erode and break the low-level inversion.❑Play VideoTitle Atmospheric Temperature and InversionsSummary Time-lapse of a valley with an inversion filling the valley floor. The inversion ispreventing upward vertical motion, indicated by the fog layer.Time (00: 08)No AudioRecognizing a Developing InversionS-190 Unit 5: Atmospheric Stability, Winds, and Clouds12•Stable conditions develop.•Surface temperatures decrease.•Relative humidity increases.•Winds may become light.•Smoke flattens after limited rise (layers).•Fire behavior typically decreases.Recognizing a Dissipating InversionS-190 Unit 5: Atmospheric Stability, Winds, and Clouds13Pre-Video Discussion•Wind may increase and change direction.•Temperature increases and relative humidity decreases.•The air mass becomes unstable (changing smoke behavior).•Smoke begins to loft and develop a column.•Fire behavior increases.❑Reference Look Up, Down and Around in the Incident Response Pocket Guide (IRPG), PMS 461, https:///publications/461.❑Play VideoTitleSummary Time-lapse of a valley with an inversion leaving the valley floor.Time (00:25)No AudioS-190 Unit 5: Atmospheric Stability, Winds, and Clouds 14The horizontal movement of air relative to the surface of the earth.WindPre-Video DiscussionImportance of wind and its impact on fire behavior:• Most critical factor affecting fire behavior.• Difficult to predict, especially in complex terrain.• Most variable in time and space.• Poses safety and control problems, but can support tactics if accurately measured and forecasted. ❑ Reference Important Winds to Firefighters in the Incident Response Pocket Guide (IRPG), PMS 461, https:///publications/461.❑ Play VideoTitle Wind Summary Introduction to wind and its effect on the fire environment. Time (01:04) AudioWind DirectionCompass direction from which wind is blowing.S-190 Unit 5: Atmospheric Stability, Winds, and Clouds15 Question: A northeast wind is coming from what direction?Answer: The northeast.S-190 Unit 5: Atmospheric Stability, Winds, and Clouds16•Large scale winds caused by high- and low-pressure systems but generally influenced and modified in the lower atmosphere by terrain.Instruct participants on the concept of general winds and their characteristics:o Winds driven by large scale high- and low-pressure systems.o Winds typically found at mid- and upper-levels of the troposphere.o Winds responsible for transporting weather systems around the world.Impact of General Winds on Fire BehaviorS-190 Unit 5: Atmospheric Stability, Winds, and Clouds17Play videoTitle General WindsSummary Time-lapse of a fire and the sky above showing the impact of general winds.Time (00:16)No AudioS-190 Unit 5: Atmospheric Stability, Winds, and Clouds 18Local WindsWinds which are generated over a comparatively small area by local terrain and weather. They differ from those which would be appropriate to the general pressure pattern.Pre-Video Discussion• Winds found at lower levels of the troposphere.• Induced by small-scale differences in air temperature and pressure.• Influenced by terrain; the more varied the terrain, the greater the influence.• Influenced by the difference in sea and land surface temperatures.• Local winds may be the only wind impacting a fire, or it could be a combination of general and local winds.Play VideoTitle Local Winds Summary Time-lapse of fire on a mountain side and the effects of local winds on the fire. Time (00:16) No AudioS-190 Unit 5: Atmospheric Stability, Winds, and Clouds 19Downslope and Down-Valley Winds Downslope wind speeds range from 2-5 mph.Down-valley wind speeds range from 5-10 mph.Pre-Video Discussion• Small-scale convective winds that occur due to local heating and cooling of a natural incline of the ground.• A result of slopes or valleys cooling at night. The cooler air will sink down a slope or valley. Play VideoTitle Downslope and Down-Valley Winds Summary Animation of a valley at night with a fire on a nearby slope and arrows showing the movement of air. Time (00:21) No AudioS-190 Unit 5: Atmospheric Stability, Winds, and Clouds 20Land and Sea Breezes• Land and sea breezes are common winds in coastal regions. Firefighters should anticipate wind shifts when working near large bodies of water (lake or ocean).• Land Breeze: During the evening and overnight hours, the land mass becomes cooler than the air over the large body of water. Air over the land becomes stable and the air over the body of water becomes unstable. The rising air over the water is replaced by the air over the land.• Sea Breeze: During the late morning and early afternoon, the land mass becomes warmer than the air over the large body of water. Air over the land becomes unstable and rises (low pressure). The rising air over the land is replaced by the air over the body of water.S-190 Unit 5: Atmospheric Stability, Winds, and Clouds 21Mid-Flame WindFlame HeightReference Beaufort Scale in the Incident Response Pocket Guide (IRPG)https:///publications/461.• General or local winds, or components of both, contribute to wind speed and direction, including 20-foot and mid-flame winds.• Mid-flame wind is the wind that acts directly on the flaming fire front at the level of half the flame height. An excellent approximation of the mid-flame wind is the eye-level wind.• Eye-level wind can be measured by the firefighter with the Belt Weather Kit wind meter or a handheld electronic weather meter.Wind Effects on Fire BehaviorS-190 Unit 5: Atmospheric Stability, Winds, and Clouds22Pre-Video Discussion•Wind carries away moisture-laden air and hastens the drying of wildland fuels.•Once a fire ignites, wind aids combustion by increasing the supply of oxygen.•Wind increases fire spread by carrying heat and burning embers to new fuels (spotting). •Wind bends the flames closer to the unburned fuels, pre-heating the fuels ahead of the fire front. •Changes in wind direction and speed can rapidly change fire behavior from inactive to active. •The direction of the fire spread and smoke transport are determined mostly by wind direction. Play VideoTitle Wind Effects on Fire BehaviorSummary Time-lapse of wildfires on varying landscapes and the effects of wind on firebehavior.Time (00:17)No AudioCloudsS-190 Unit 5: Atmospheric Stability, Winds, and Clouds23Pre-Video Discussion❑Reference Look Up, Down and Around in the Incident Response Pocket Guide (IRPG), PMS 461, https:///publications/461.❑Play VideoTitle CloudsSummary Introduction to how clouds can change fire behavior.Time (00:39)AudioS-190 Unit 5: Atmospheric Stability, Winds, and Clouds 24CloudsStableUnstable A visible collection of moisture suspended in the atmosphere.• Clouds form under stable or unstable atmospheric conditions, and not all clouds produce precipitation.• There are numerous cloud types. This course only covers some of the basic, important clouds to firefighters.S-190 Unit 5: Atmospheric Stability, Winds, and Clouds 25Cloud Impacts on Fire Environment•Temperature•Relative Humidity•Atmospheric Stability•Wind•Fuel Temperature•Fuel Moisture•Fire BehaviorClouds can modify the fire environment by changing:Pre-Video Discussion• Clouds can reflect incoming solar radiation and, therefore, affect fire weather conditions by: o Creating cooler temperatures. o Increasing relative humidity. o Changing wind and stability.• Changes in fire weather conditions directly impact:o Fuel moisture. o Decreases in fire behavior.• Once clouds move away from the environment, fire behavior can increase.Play VideoTitle Campfire Summary An animation of a campfire burning and clouds moving in, creating cooler temperatures. Time (00:17) No AudioCloud ClassificationS-190 Unit 5: Atmospheric Stability, Winds, and Clouds26❑Refer participants to the The Fire Weather Cloud Chart, PMS 438,https:///publications/438, printout that each participant was provided.❑Lead participants in a discussion of basic cloud classification:o Clouds are classified by height.o High: 6,000-50,000 feet. Usually pure white in color and made up of ice crystals.o Middle: 6,500-23,000 feet. Usually a combination of white and gray in color and made of water droplets and ice crystals.o Low: 0-6,500 feet. Usually gray in color and made of water droplets.❑Task participants with locating the clouds of critical concern for firefighters outlined in red boxes. ❑Lead participants in a discussion on the information provided for the following clouds of critical concern:o Altocumulus castellanus / altocumulus floccuso Cumulonimbuso Mature thunderstormVertically Developed CloudsS-190 Unit 5: Atmospheric Stability, Winds, and Clouds27Pre-Video Discussion•Made up of water and ice and indicate unstable atmospheric conditions.•An unstable atmosphere can result in an increase in fire behavior. Identifying this type of cloud is important when predicting changes to the fire environment.•Cumulus clouds could result in cumulonimbus clouds (thunderstorms), which could result in gusty and erratic winds.•Bases can range from 1,500 to 10,000 feet, depending on air mass conditions in different parts of the country.•For example, cumulus clouds or thunderstorms typically have higher bases compared to the same cloud types in southern and eastern sections of the United States.Play VideoTitle Vertically Developed CloudsSummary Time-lapse of cumulus cloud being formed over land.Time (00:14)No AudioS-190 Unit 5: Atmospheric Stability, Winds, and Clouds 28Smoke layers mimic clouds in modifying the fire environment by changing:•Temperature •Relative Humidity •Atmospheric Stability •Wind •Fuel Temperature •Fuel Moisture •Fire BehaviorSmoke LayersInform participants of the similarities between smoke layers and clouds on the fire environment.S-190 Unit 5: Atmospheric Stability, Winds, and Clouds 29Stable or Unstable?1. Clouds or smoke columns that grow vertically indicate a(n) ________ atmosphere.2. A smoke column that spreads out after limited rise indicates a(n)______ atmosphere.unstable stableEvaluate instruction using the knowledge check.Instructor can choose to have questions answered by individuals or in groups.Question 1: Clouds or smoke columns that grow vertically indicate a(n) _________ atmosphere.Answer: UnstableQuestion 2: A smoke column that spreads out after limited rise indicates a(n) _______ atmosphere.Answer: StableS-190 Unit 5: Atmospheric Stability, Winds, and Clouds 30Fill in the blanks.1.Wind direction is the direction _______which the wind isblowing.2.General wind is a _______ scale wind associated with high andlow pressure.3.Local wind is a _______ scale wind.4.(True or False). Wind is the most critical factor affecting firebehavior.5.The direction of the fire spread and smoke transport are mostly determined by _______________.from large small Truedirection of windEvaluate instruction by using the knowledge check.Instructor can choose to have questions answered by individuals or in groups.Question 1: Wind direction is the direction _______ which the wind is blowing.Answer: fromQuestion 2: General wind is a ______ scale wind associated with high and low pressure.Answer: largeQuestion 3: Local wind is a ______ scale wind.Answer: smallQuestion 4: True or False. Wind is the most critical factor affecting fire behavior.Answer: TrueQuestion 5: The direction of the fire spread and smoke transport are mostly determined by.Answer: direction of windS-190 Unit 5: Atmospheric Stability, Winds, and Clouds 31The smoke column in the image indicates _______.A.Stable AtmosphereB. Unstable AtmosphereC. NeitherProvide explanations for the answer, if required.Question: The smoke column in the image indicates_______.Answer: Unstable AtmosphereThe cloud in this image is a towering cumulus.Does this type of cloud indicate a stable or unstable atmosphere?Unstable atmosphere.What fire behavior can be anticipated?Increase in fire behavior.S-190 Unit 5: Atmospheric Stability, Winds, and Clouds32Provide explanations for the answers if required.Question: Does this type of cloud indicate a stable or unstable atmosphere?Answer: Unstable atmosphere.Question: What fire behavior can be anticipated?Answer: Increase in fire behavior.Review unit objectives.。
西北大学继续教育学院学位英语考试真题Northwestern University School of Continuing Education Degree English Exam QuestionsPart 1: Reading Comprehension (30 points) Read the following passage and answer the questions below:Climate change refers to long-term changes in the temperature, precipitation, and other atmospheric conditions on Earth. The most significant cause of climate change is human activities, particularly the burning of fossil fuels such as coal, oil, and natural gas. These activities release greenhouse gases into the atmosphere, which trap heat and cause the Earth's temperature to rise.Questions:1. What is the main cause of climate change?2. How do human activities contribute to climate change?3. What are greenhouse gases, and how do they affect the Earth's temperature?Part 2: Vocabulary and Grammar (40 points) Fill in the blanks with the correct word or phrase:1. The ___________ of plastic bags is harmful to the environment.2. The government has implemented ___________ to reduce carbon emissions.3. It is important to ___________ renewable energy sources to combat climate change.4. ___________ is a key factor in determining the Earth's climate.Part 3: Writing (30 points)Write an essay of at least 300 words on the following topic: "The Impact of Climate Change on Global Food Security." In your essay, discuss how climate change affects food production and access to food, and propose solutions to mitigate these impacts.Part 4: Listening Comprehension (20 points)Listen to the audio recording and answer the questions below:1. What are the main causes of deforestation?2. How does deforestation contribute to climate change?Good luck on your exam! Remember to review your notes and practice your English skills before the test.。
---------------------------------------------------------------最新资料推荐------------------------------------------------------外文翻译---高程测量方法附录:高程测量方法高程是高于或低于一个参考基准的一个垂直距离。
虽然垂直距离可以参考任何一个基准,但是在测量上,这个参考基准一般使用的是平均海平面(MSL)。
MSL被赋予一个 0. 000 英尺或 0. 000 米的高程,地球上所有其它点可以用高于或低于0 的高程来描述。
高程精确测出的永久点(水准点)被用于大多数区域的测量工作. 在中国,利用青岛验潮站从 1950 年到 1956 年 7 年的观测数据处理】和平差,建立了 56 黄海高程系统。
1987 年,在依照了验潮站 1952 到 1979 年的观测资料后,这个基准被进一步精确反映长时期海潮变化的 85 国家高程基准建立起来。
虽然,严格说来,国家高程基准在特殊的点上与 MSL 并不恰好吻合,术语MSL 一般还是用来描述它。
MSL 高程的赋值为 0. 000 英尺或米,高程的差异【高差】可以由下列方法测得:1. 水准测量,直接测得垂直距离,水准测量是高程测量方法中精度最高、使用最普遍的方法2. 三角高程测量,利用测量竖直角和水平或斜距来测高程3. 视距高程测量,利用视距测量,使用1 / 10工程经纬仪和水准尺;平板仪和照准仪和水准尺;或者自处理视距仪和水准尺测得垂直距离 4. 气压水准测量,通过使用气压计测量不同站点大气压力的差值来测高程 5. 重力水准测量,通过使用重力计测量不同站点的重力值差值来测高程,用于大地测量学的目的6. 惯性定位系统,含有一个惯性平台,具有三个互相垂直轴,其中一个是向上的,所以这个系统产生的输出其中一个就是高程。
各自地,据相关报告,在 60和 100km 的距离上,其精度能达到 15 到 50cm,这种装置成本极高,只限于非常大的项目,这些项目地质、气象、授时、以及施特殊限制在传统方法上 7. GPS 高程测量,它的参考面是地球椭球面,但是如果在测区有充分的高程点,可以修正至高程基准上来,在这种情况下,其高差的标准差能够达到 0. 053 到0. 094 米。
大自然和天气的作文英语Title: The Majesty of Nature and Weather。
Nature is an enigmatic force that surrounds us, encompassing the vast expanse of the earth and reaching beyond into the depths of the cosmos. Within its realm lies the ever-changing spectacle of weather, a dynamic interplay of atmospheric conditions that shapes our world in profound ways. In this essay, we delve into the intricate tapestry of nature and weather, exploring their magnificence and significance.First and foremost, nature embodies a breathtaking beauty that transcends human comprehension. From the towering peaks of majestic mountains to the tranquil serenity of meandering rivers, nature's splendor is evident in every corner of the globe. The verdant forests teeming with life, the azure depths of the oceans brimming with mystery, and the vibrant hues of a sunset painting the sky – all testify to the awe-inspiring grandeur of the naturalworld.At the heart of nature's majesty lies the phenomenon of weather, an ever-shifting mosaic of elements that dictates the rhythms of life on earth. The sun, the primary source of energy, casts its golden rays upon the earth, warming the land and stirring the atmosphere. Winds whisper secrets as they dance through the trees, carrying with them the breath of distant lands. Clouds gather in silent congregation, heralding the arrival of rain, snow, or storms that shape the landscape with their gentle caress or fierce embrace.Indeed, weather is more than just a fleeting spectacle – it is a powerful force that influences every aspect of our existence. Agriculture and farming, for instance, are intrinsically linked to the whims of weather, with rainfall and temperature patterns determining crop yields and harvests. Likewise, industries such as transportation and energy are deeply impacted by weather conditions, from the efficiency of air travel to the generation of renewable energy sources like wind and solar power.Moreover, the study of weather holds profound implications for our understanding of climate change and environmental sustainability. As human activities continue to alter the delicate balance of the earth's ecosystems, the repercussions are felt in the form of extreme weather events, rising temperatures, and changing precipitation patterns. It is imperative that we heed the warnings of science and take proactive measures to mitigate the effects of climate change, lest we face catastrophic consequences for future generations.Yet, amidst the challenges and uncertainties, there is also resilience and hope to be found in the embrace of nature. In the face of adversity, life finds a way to endure and thrive, adapting to the ever-changing conditions of its environment. Just as a seedling perseveres through the harshness of winter to bloom in the warmth of spring, so too can humanity draw strength from the resilience of the natural world.In conclusion, the majesty of nature and weather is atestament to the wonders of our planet and the interconnectedness of all life forms. From the gentlecaress of a breeze to the fury of a tempest, nature'sbeauty and power inspire awe and reverence in equal measure. As stewards of the earth, it is our responsibility to cherish and protect the precious gift of nature, ensuring that its splendor endures for generations to come.。
英语四级词汇复习天气类天气是我们日常生活中不可忽视的一个因素,它直接影响到我们的衣食住行。
在英语四级考试中,天气类的词汇也是一个非常重要且常见的话题。
下面将为大家系统地复习英语四级中与天气相关的词汇。
1. Climate (气候)Climate refers to the long-term weather conditions of a particular region. It is determined by various factors such as temperature, precipitation, humidity, and wind patterns. For example, the climate in tropical countries is generally hot and humid, while the climate in polar regions is extremely cold.2. Weather forecast (天气预报)A weather forecast is a prediction of the weather conditions for a specific area and time period. It is usually provided by meteorological agencies or broadcasted on TV and radio. People rely on weather forecasts to plan their activities and make appropriate clothing choices.3. Temperature (温度)Temperature measures the degree of hotness or coldness of the atmosphere. It is usually measured in degrees Celsius or Fahrenheit. In different seasons and regions, the temperature can vary greatly. For instance, during the summer, the temperature in some areas can reach over 30 degrees Celsius, while in winter, it can drop below freezing point.4. Humidity (湿度)Humidity refers to the amount of moisture or water vapor present in the air. It is an important factor affecting people's comfort level. High humidity makes the air feel sticky and uncomfortable, while low humidity can cause dryness in the skin and respiratory system.5. Precipitation (降水)Precipitation includes all forms of water that fall from the atmosphere to the Earth's surface, such as rain, snow, sleet, or hail. The amount and type of precipitation are influenced by temperature, humidity, and atmospheric conditions. Rainfall is the most common form of precipitation, while snow is more common in colder regions.6. Wind (风)Wind is the movement of air in the atmosphere. It is caused by differences in air pressure and is classified into various categories based on speed, such as breeze, gale, or hurricane. Wind plays a crucial role in determining the weather patterns and can affect temperature, humidity, and precipitation.7. Season (季节)Seasons refer to the four main divisions of the year: spring, summer, autumn (fall), and winter. Each season has distinct weather characteristics. Spring is often associated with blooming flowers and mild temperatures, while summer is known for its heat and longer days. Autumn is characterized by falling leaves and cooler weather, and winter brings cold temperatures and possible snowfall.8. Sunny (晴朗的)Sunny describes a weather condition with clear skies and abundant sunlight. It is often associated with good weather and is a preferred condition for outdoor activities. People often feel uplifted and cheerful on sunny days.9. Cloudy (多云的)Cloudy describes a weather condition with a significant amount of clouds covering the sky. It often indicates the absence of direct sunlight and may be associated with lower temperatures. Some people find cloudy weather gloomy, while others enjoy the cooler temperatures it brings.10. Rainy (多雨的)Rainy describes a weather condition with continuous or intermittent rainfall. It is often associated with lower temperatures and increased humidity. Rainy weather may affect people's moods and activities, but it is essential for the growth of plants and agriculture.11. Snowy (多雪的)Snowy describes a weather condition with falling or accumulated snow. It is common in regions with cold winters and is often associated with winter sports and activities. Snowy weather can create beautiful scenery but may also cause travel disruptions and safety hazards.12. Stormy (暴风雨的)Stormy describes a weather condition characterized by strong winds, heavy rainfall, and sometimes thunder and lightning. Stormy weather can bedangerous and may cause damage to buildings and infrastructure. It is important to take precautions and stay indoors during storms.以上是对英语四级考试中与天气相关的词汇的系统复习。
为什么下雨的英语作文英文回答:Why does it rain? Rain is a natural phenomenon that occurs when water vapor in the atmosphere condenses into droplets and falls to the ground. There are several factors that contribute to rainfall.Firstly, one of the main factors that causes rain is the water cycle. The water cycle involves the continuous movement of water between the Earth's surface and the atmosphere. When the sun heats up the Earth's surface, water evaporates and rises into the atmosphere as water vapor. As the water vapor cools, it condenses into clouds. When the clouds become saturated with water droplets, they release the excess moisture in the form of rain.Secondly, another factor that leads to rain is the presence of moisture in the atmosphere. Moisture can come from various sources such as oceans, lakes, and rivers.When warm air comes into contact with this moisture-laden air, it rises and cools, causing the water vapor to condense and form raindrops.Furthermore, the topography of an area can also affect rainfall patterns. Mountains, for example, can act as barriers to the movement of air masses. When moist air is forced to rise over a mountain range, it cools and condenses, resulting in rainfall on the windward side ofthe mountain. On the leeward side, however, the air descends and warms, leading to drier conditions.In addition, atmospheric conditions such as temperature, humidity, and air pressure play a role in determining whether rain will occur. Low-pressure systems often bring about unstable atmospheric conditions, which can lead tothe formation of rain clouds. Conversely, high-pressure systems tend to bring clear skies and dry weather.To sum up, rain is a result of the water cycle, the presence of moisture in the atmosphere, topography, and atmospheric conditions. It is a natural process that helpsto maintain the Earth's water balance and is essential for the survival of plants, animals, and humans.中文回答:为什么会下雨?下雨是一种自然现象,当大气中的水蒸气凝结成水滴并降落到地面时就会发生。
2024年高中地理考试题目和解答英文版2024 High School Geography Exam Questions and Answers1. What is the main cause of earthquakes?- Earthquakes are mainly caused by the movement of tectonic plates along fault lines.2. Describe the process of erosion.- Erosion is the gradual wearing away of land by natural elements such as water, wind, and ice.3. Explain the difference between weather and climate.- Weather refers to the short-term atmospheric conditions in a specific area, while climate is the long-term average of weather patterns.4. What is the significance of the Amazon Rainforest?- The Amazon Rainforest is important for its biodiversity, as it is home to a wide variety of plant and animal species.5. How do glaciers form?- Glaciers form when snow accumulates over time and compresses into ice, flowing slowly downhill under the force of gravity.6. What is the Ring of Fire and why is it significant?- The Ring of Fire is a horseshoe-shaped area in the Pacific Ocean known for its high levels of volcanic and seismic activity.7. Discuss the impact of deforestation on the environment.- Deforestation leads to loss of habitat, soil erosion, and contributes to climate change by releasing carbon dioxide into the atmosphere.8. What is the difference between renewable and non-renewable resources?- Renewable resources can be replenished naturally over time, while non-renewable resources are finite and cannot be easily replaced.9. Explain the concept of urbanization.- Urbanization is the process by which an increasing proportion of a population lives in cities and urban areas.10. How does latitude affect climate?- Latitude plays a significant role in determining climate, with regions closer to the equator generally experiencing warmer temperatures.11. Describe the formation of a desert.- Deserts form in areas with low precipitation, where evaporation exceeds rainfall, leading to arid conditions.12. Why are rivers important for human civilization?- Rivers provide water for drinking, agriculture, transportation, and energy production, making them vital for human survival and development.13. Discuss the impact of climate change on sea levels.- Climate change is causing sea levels to rise due to the melting of glaciers and ice caps, posing a threat to coastal communities.14. What is the difference between a tsunami and a hurricane?- Tsunamis are giant sea waves caused by underwater earthquakes, while hurricanes are powerful tropical storms with high winds and heavy rainfall.15. Explain the concept of sustainable development.- Sustainable development aims to meet the needs of the present without compromising the ability of future generations to meet their own needs.。
a r X i v :0803.1054v 2 [a s t r o -p h ] 7 M a y 2008Accepted to Ap.J May 6,2008Preprint typeset using L A T E X style emulateapj v.10/09/06DETERMINING ATMOSPHERIC CONDITIONS AT THE TERMINATOR OF THE HOT-JUPITER HD209458bDavid K.Sing 1,A.Vidal-Madjar 1,A.Lecavelier des Etangs 1,J.-M.D ´e sert 1,G.Ballester 2,and D.Ehrenreich 3Accepted to Ap.J May 6,2008ABSTRACTWe present a theoretical model fit to the HST /STIS optical transit transmission spectrum of HD209458b.In our fit,we use the sodium absorption line profile along with the Rayleigh scat-tering by H 2to help determine the average temperature-pressure profile at the planetary terminator,and infer the abundances of atomic and molecular species.The observed sodium line profile spans an altitude range of ∼3,500km,corresponding to pressures between ∼0.001and 50mbar in our atmo-spheric models.We find that the sodium line profile requires either condensation into sodium sulfide or ionization,necessary to deplete atomic sodium only at high altitudes below pressures of ∼3mbar.The depletion of sodium is supported by an observed sudden abundance change,from 2times solar abundance in the lower atmosphere to 0.2solar or lower in the upper atmosphere.Our findings also indicate the presence of a hot atmosphere near stratospheric altitudes corresponding to pressures of 33mbar,consistent with that of the observed dayside temperature inversion.In addition,we find a separate higher altitude temperature rise is necessary within both the condensation and ionization models,corresponding to pressures below ∼0.01mbar.This hot higher altitude temperature indi-cates that absorption by atomic sodium can potentially probe the bottom of the thermosphere,and is possibly sensitive to the temperature rise linked to atmospheric escape.Subject headings:planetary systems -radiative transfer -stars:individual(HD209458)1.INTRODUCTIONEarly theoretical transit models of hot-Jupiter exo-planetary atmospheres (Seager &Sasselov 2000;Brown 2001;Hubbard et al.2001)contained strong sodium ab-sorption signatures,predicted to be as high as 0.2%for clear cloudless atmospheres.The original measured Na absorption signature in HD209458b from medium reso-lution HST data Charbonneau et al.(2002)was,how-ever,∼3×smaller than initial predictions.Addition-ally,Barman (2007)has also identified a potential broad band Na signature from photometry of low resolution STIS data in the same planet,taken several years later (Knutson et al.2007).These observations have lead to multiple theories to explain the small Na signa-ture.The most widely cited explanations of reduced Na absorption include:high clouds or hazes,ionization,low global Na abundance,rainout,as well as non-local thermal equilibrium effects (Charbonneau et al.2002;Barman et al.2002;Barman 2007;Fortney et al.2003).High opaque clouds could potentially mask absorption features by effectively cutting transit information for al-titudes lower than the cloud deck (Seager &Sasselov 2000;Fortney et al.2003).The small atmospheric sig-nature has made detection from ground-based telescopes difficult,with no Na detection currently reported for HD209458b after multiple attempts (Narita et al.2005;Arribas et al.2006).In the grazing line of sight of transit geometry,the mea-sured effective altitude depends upon the wavelength de-1Institut d’Astrophysique de Paris,CNRS;Universit´e Pierre et Marie Curie,98bis bv Arago,F-75014Paris,France;sing@iap.fr 2Lunar and Planetary Laboratory,University of Arizona,Sonett Space Science Building,Tucson,AZ 85721-0063,USA 3Laboratoire d’astrophysique de Grenoble,Universit´e Joseph-Fourier,CNRS (UMR 5571),BP 53F-38041Grenoble cedex,Francependant opacities of the atmospheric constituents giving a transit transmission spectrum its altitude sensitivity (see relevant equations in Lecavelier et al.2008a).The effective altitude is also dependant upon the abundance of absorbing atmospheric particles,as well as the atmo-spheric pressure.As the abundances are not in general a priori known,this leads to atmospheric models which have degenerate solutions between modeled abundance and pressure,where an atmospheric transit model with increased abundance is identical to models with lower abundances and higher pressures.Here we interpret the optical HST STIS transmission spectra of HD209458b of Sing et al.(2008).The spectra consists of STIS data obtained during planetary tran-sit at low and medium spectral resolutions.The two datasets are combined to extend the measurements over the entire optical regime,providing a way to simulta-neously measure,in the case of atomic Na,both the narrow line core and wide line wing absorption as well as other absorbing or scattering species.Since the Na line core and wings are optically thick at different at-mospheric heights,a detailed analysis of the Na line profile in conjunction with other observed species can potentially break the model degeneracies and reveal at-mospheric structure such as the altitude-temperature-pressure (z-T-P)relation,abundance,and the possible presence and height of planetary clouds.In this paper,we focus mainly on the resulting temperature pressure profile,as well as the Na line itself.We briefly describe the observations and resulting spectra in §2,present our transit model fits in §3,report on an observed tempera-ture inversion in §3.3,and discuss our results in §4&5.In addition to this work,Lecavelier et al.(2008b)provides a detailed description of H 2Rayleigh scatter-ing while D´e sert et al.(2008)goes into modeling details of TiO,VO,and other molecular species.22.OBSERVATIONSThe data reduction,procedures,and various tests re-sulting in the transmission spectra used in this analy-sis are covered in detail by Sing et al.(2008),though we briefly describe them here for completeness.The HST/STIS optical transit data for HD209458b consist of data at low resolution covering∼3,000-10,000˚A with the G430L and G750L gratings and medium resolution data from the G750M grating covering5,813-6,382˚A. With the medium resolution data,Sing et al.(2008) measured the Na absorption using the double differen-tial photometric method of Charbonneau et al.(2002), as well as a double differential spectroscopic evaluation. For the differential photometric measurement,Sing et al. (2008)selected23wavelength bands from4to100˚A cen-tered on the Na D lines,Charbonneau et al.(2002)used three different wavelength bands,and compared the ab-sorption to that of regions red-ward and blue-ward of the Na D line region.The resulting photometric Na absorp-tion profile(see Sing et al.2008,Fig.3)matches the original results of Charbonneau et al.(2002)and,in ad-dition,reveals the strong absorption from the Na D line centers.To analyze the low and medium resolution HST spec-tra together,Sing et al.(2008)used a limb-darkened cor-rected transit spectral ratio to probe the full wavelength dependence of atmospheric absorption features(see Fig. 1&Fig.2).From this analysis,the Na D wavelength region shows an absorption plateau between∼5600-6700˚A,which is∼0.045%above the minimum absorption level observed(see Fig.1).Note that the wavelength range of the medium resolution data,originally used to detect at-mospheric Na(Charbonneau et al.2002),is entirely con-tained within this broad plateau absorption region.The total absorption seen in the Na D line cores,therefore, is the result from the medium resolution data,which is the absorption above the plateau region measured to be ∼0.065%,plus the absorption level of the plateau region itself.This total Na core absorption level is∼0.11%, within a4.4˚A band,and is much closer to the original predictions(Seager&Sasselov2000;Brown2001),indi-cating that a large extent of the atmosphere is being probed during transit.Additionally,the Na D doublet is resolved in our resulting spectra which shows two strong narrow absorption lines(see Fig.2).2.1.Observed Na line profileThe observed Na D transit line profile(Fig.1), with it’s narrow absorption core and broader plateau-like shape,is in stark contrast to cloudless theoretical mod-els of HD209458b(Seager&Sasselov2000;Brown2001; Fortney et al.2003;Barman2007)which have smoothly decaying Lorentzian“Eiffel Tower”shaped line wings. This more complicated observed line profile suggests a very low quantity of Na is present in the middle at-mosphere and much larger quantity in the lower atmo-sphere,pointing to either high altitude Na condensation into Na2S or alternatively,depletion via ionization. Previous studies have predicted models of HD209458b which included Na2S clouds(Iro,B´e zard,&Guillot 2005),as high altitude temperatures on the night side reach levels cool enough for condensation of atomic Na (Lodders1999;Showman&Guillot2002).Sodium sul-fide would effectively decrease the amount of atomic sodium at altitudes above the condensation tempera-ture,creating a stratified-like atmospheric profile de-pleted of atomic Na only at those high altitudes.The transit signature with such a layered Na profile produces a broad plateau shaped line wing along with narrow ab-sorption cores rising above the plateau to higher levels (Iro,B´e zard,&Guillot2005).Na2S would have to be transparent,since they are not observed in absorption during transit at the limb.If Na2S or other clouds/hazes were opaque in absorption during transit at the conden-sation altitude,significant absorption would extend over a very broad wavelength range(Fortney2005),masking the low resolution absorption features we observe.Such a flat,largely featureless transmission spectra has recently been observed in HD189733b,the result of high altitude haze(Pont et al.2008;Lecavelier et al.2008a).An alternative method to deplete neutral atomic sodium is by ionization(Fortney et al.2003).In this scenario,UV photons between wavelengths of1,107and 2,412˚A(corresponding to11.2and5.14eV respectively) photoionize sodium along the transit line of sight until recombination matches ionization.Fortney et al.(2003) found a sharp boundary at the limb between higher at-mospheric regions of complete ionization and lower re-gions with no ionization.Such a model could explain the observed Na line shape,with a narrow Na absorption core rising above broad line wings,if the atmosphere suddenly becomes ionized above a certain altitude.3.MODEL FITS TO THE TRANSIT TRANSMISSIONSPECTRA OF HD209458BWe modeled the atmospheric transmission spectra cal-culating the transit signature based on a theoretical model(Ehrenreich et al.2006)containing absorption by Na,H2Rayleigh scattering,TiO and VO.The model out-put absorption spectrum can then be directly compared to our limb-darkened corrected transit absorption spec-trum.We calculated the optical depth along a grazing line of sight through the planet’s atmosphere,and calcu-lated the absorption depth at a given wavelength using equations given in Lecavelier et al.(2008a).For the Na D lines,we used collision-broadened line-shapes calculated using Equations of Iro,B´e zard,&Guillot(2005).Con-cerning atomic sodium,ultimately the free parameters tofit in the transit calculation include the atmospheric temperature profile as a function of altitude,and the mixing ratios of Na below and above the condensation or ionization level(see Fig.3).We found two families of solutions,with each giving similarly goodfits to the data.In one model,Na is allowed to condense into sodium sulfide at the chemi-cal equilibrium temperature,while in the other model neutral Na is depleted at high altitudes,presumably by ionization,below an arbitrary pressure.3.1.Condensation model3.1.1.Temperature-Pressure profileFor the calculation,wefit various simplified T-P pro-files in which the temperature is taken as a linear func-tion of the altitude and pressure is calculated using hy-drostatic equilibrium.Note that it is not specifically the T-P profile shape itself which is important in ourfitting of the data,but rather the different temperature and3pressure regimes imposed by the observations.At our signal-to-noise levels,the general variation of the T-P profile in between the different atmospheric regimes we find (hot at high pressure,cool at middle pressures,and hot at low pressures)is only loosely constrained.A more complicated T-P profile would add undesired additional parameters into the fit,leading us to choose as simple a T-P profile as possible.We found it necessary to have a minimum of three variable points in the T-P profile.The temperature as a function of the altitude,T (z ),is thus composed of two linear functions below and above the altitude z m ,where z m is the altitude of the minimum temperature,T m .We took the lower reference altitude,z s ,for the altitude cor-responding to the mean planetary radius (Knutson et al.2007),and the altitude z th is the fixed position,at high altitude,needed to define the second part of the T (z )lin-ear function.We used z th corresponding to the altitude of the absorption depth of 1.55%,which corresponds to the mean absorption depth in the core of the sodium doublet.The temperature and pressure at the altitude z s ,the altitude z m of minimum temperature T m ,and T th are the five free parameters defining the T-P pro-file.The sodium abundance in the lower and the upper atmosphere are the two other free parameters in the fit.In our condensation fit we found:(1)a high tempera-ture of 2,200±260K at 33±5mbar (∼500km)mainly constrained by Rayleigh scattering (Lecavelier et al.2008b)seen at wavelengths shorter than ∼5,000˚A ,(2)a low temperature of 420±190K at 0.63±0.27mbar needed to explain the plateau at 0.045%(∼1,500km)above the minimum absorption level as a Na abundance change due to condensation,and finally (3)a high altitude (∼3,500km)high temperature of 1,770+500−570K at 0.0063±0.003mbar needed to fit the strong peak and narrow width of the cores of the Na I doublet.The pressure-temperature gradient we find when im-posing condensation is close to and consistent (within 1σ)of an adiabatic gradient.A temperature gradient which is adiabatic or less is needed to be stable against convection,and solutions imposing adiabatic variations give acceptable fits to the data (an adiabatic fit is shown in Fig.3).We ultimately,however,choose to quote val-ues found from the more general solution,as the linear temperature-altitude relation we assume includes adia-batic gradients and the general fit is located at a well behaved minimum χ2.Although the best fit solution is slightly superadiabatic,the relatively low quality of the data still allows for a wide range of T-P gradients and the adiabatic-like profile found from our general fit indicates that an adiabatic behavior is likely at those altitudes.3.1.2.Atmospheric Na Condensation,TiO &VOOur model contained two different amounts of atomic Na having separate variable parameters for the mixing ratios of the middle and lower atmospheres.The pressure boundaries (or condensation pressure)where the quan-tity changes occur is taken to be at an altitude where the temperature profile crosses the Na 2S condensation curve.In our fits,we found a Na mixing ratio of 3.5+2.9−1.9×10−7in the middle atmosphere and 4.3+2.1−1.9×10−6in the lower atmosphere,corresponding to 0.2and 2times solar abun-dance.Fortney (2005)estimated that the optical depth of Na 2S condensates in transit geometry could be optically thick for HD209458b (τ∼0.73)for an atmosphere of so-lar composition and cloud base at 30mbar.Given the fit T-P profile,we find a Na 2S cloud base of ∼3mbar.Lower pressures or larger particle sizes would provide a natural explanation for transparent clouds,as the con-densate optical depth is proportional to the pressure and inversely proportional to the particle size (Marley 2000).Given our determined Na abundances,the mixing ratio of Na 2S we find is (2±1)×10−6,which matches the as-sumed value of Fortney (2005).Scaling the estimated optical depth of Fortney (2005),a cloud base at 3mbar gives τ∼0.073,indicating that transparent Na 2S con-densates are plausible.The continuum blue-ward of the Na D lines,between ∼4,000and 5,500˚A ,shows a slightly lower absorption than the red-ward region,7,000-8,000˚A ,and a signifi-cant absorption ‘bump’around ∼6,250˚A which appears in both resolutions.Our fits indicate that the red-ward absorption levels (7,000-8,000˚A )are likely due to TiO and VO at stratospheric heights,being largely confined to altitudes below our Na condensation level (also see D´e sert et al.2008).The TiO and VO features mask part of the long wavelength Na line wing,though not the short wavelength side,providing strong constraints on the abundance and altitude of TiO and VO.The hot low altitude temperatures we find from Rayleigh scatter-ing are consistent with the presence of TiO and VO,as both species begin to condense out of the atmosphere at temperatures below ∼1,800K.The low-altitude pressure assumed here is dependent on the detection of Rayleigh scattering (Lecavelier et al.2008b),though multiple interpretations of the absorption rise at those wavelengths exist (Lecavelier et al.2008b;Ballester,Sing,&Herbert 2007;Barman 2007).Ulti-mately,it may be difficult without Rayleigh scattering to assign an absolute pressure scale to these measurements which are inherently differential.The effective planetary radius seen during transit is sensitive to the quantity of the atmospheric pressure times the abundance of ab-sorbing species (see equations of Lecavelier et al.2008a),making an atmospheric fit at higher altitude possible by simply increasing the absorbers abundance.The advan-tage of detecting Rayleigh scattering by H 2when in-terpreting these models is that the abundance of H 2is known,constituting the bulk of the atmosphere,which thereby fixes the pressure,and defines the pressure scale for the rest of the transmission spectrum.Our adoption of Rayleigh scattering here is based on the goodness of fit to the data and the necessity to probe a large pressure range,given the total Na profile observed.Since the low-altitude pressure is an upper limit con-strained by Rayleigh scattering,a lower pressure would have an effect on the lower temperature profile,increase the lower Na mixing ratio,and decrease the condensate pressure determined in our transit fit.Whatever the true pressure P s or additional absorption sources,however,the basic atmospheric characteristics of Na determined here would remain the ly,the middle at-mosphere has a greatly reduced amount of Na with a temperature below Na 2S condensation,while the lower and higher atmospheres are warmer than the condensa-tion temperature with the lower atmosphere containing4a solar-like Na abundance and higher one a significantly reduced Na abundance.3.2.Photoionization modelGiven the large uncertainties modeling hot-Jupiter Na photoionization,we choose not to employ a com-plex ionization model,but rather follow the results of Fortney et al.(2003)and assume in our model that neu-tral Na can be suddenly ionized above a given altitude leading to the observed Na depletion.The ionization depth found by Fortney et al.(2003)is around 1.7mbar,close to the pressure we find for a Na abundance change in the condensation model,indicating the effects could be important at those pressures and such a model is viable.A model with Na ionization effectively lifts the con-straint of the temperature profile dropping below the Na condensation curve,which the condensation model uses to deplete atomic Na.Effectively,a model with Na ion-ization leaves a wide range of temperatures possible in the middle atmosphere (corresponding in our model to T m )as the collisional broadened Na profile at those al-titudes (1,000-2,000km)contains no temperature in-formation.The corresponding H 2Rayleigh scattering slope (below ∼3,400˚A )is at the edge of the spectrum and also provides no useful middle atmospheric temper-ature constraints.Within the framework of equilibrium chemistry,the temperature T m is likely below that of the TiO/VO condensation curve and above that of the Na 2S condensation curve.However,Rayleigh scattering still implies a high temperature of 2,200±260K at 33±5mbar and the deep narrow Na cores suggest high altitude temperatures of around 1,770+500−570K.Without a strong constraint on the middle atmosphere temperature,T-P profile fits are dominated by these upper and lower at-mospheric constrains,leading to anomalously high tem-perature T-P profiles fit to be everywhere above 2,000K.Though technically good fits to the data,such pro-files can be ruled out as the temperatures would be ev-erywhere higher than the dayside temperature inversion seen with Spitzer (Knutson et al.2008;Burrows et al.2007a).Additionally,the lack of observed Ca I at λ4,227˚A in the low resolution data further suggests tempera-tures reach values lower than that required for Ca-Ti and Ca-Al-bearing condensates (Loders &Fegley 2006).Though the current data lacks enough constraints for a unique T-P profile solution in the photoionization model,the ionization pressure,P ion ,can be estimated given the likely range of temperatures.We fit various isothermal models fitting P ion as free parameter along with the Na abundances (taken to be constant)above and below that pressure.The resulting ionization pressure varies from 0.5mbar to 5mbar for temperatures of 1,100and 2,000K respectively.Higher temperature fits result in smaller upper-atmospheric Na abundances and larger Na abun-dance contrasts.The abundances found in the lower tem-perature fits are in general agreement with those found in the Na condensation model,while the upper temper-ature fits find much smaller upper-abundances,with the 2,000K model giving an upper Na abundance 180times less than solar.Thus,a Na abundance drop by a factor of ten can be considered as a lower limit,and may be much larger depending on the depletion mechanism.3.3.High altitude temperature inversionA ∼0.11%absorption of Na indicates that our trans-mission spectra probes an altitude range of ∼3,500km.Such a large altitude range with our slant transit ge-ometry indicates we are sensitive to pressures between 10’s of mbar and ∼0.001mbar.These limb pressures are in agreement with those found from Fortney et al.(2003),who analyzed the original Charbonneau et al.(2002)medium resolution Na measurements.At pres-sures higher than 30-50mbar,our transmission spectra is optically thick to Rayleigh scattering by the abundant molecule H 2,providing a firm upper pressure limit.Such pressure restrictions,in addition to the strong narrow Na line cores,facilitate the necessity of a hot high-altitude temperature (above ∼1,500),which then naturally pro-vides the observed altitude range due to an increased scale height.Our high altitude high limb temperature may point toward the atmospheric escape mechanism being felt,which necessitates large temperature rises to perhaps 10,000or 15,000K in the exosphere (Yelle 2004;Vidal-Madjar et al.2003,2004).The highest altitudes probed here are dependent on the Na core,however,and thus have a correspond-ingly larger associated error.The large error coupled with the possible Na depletion mechanisms leaves open a wide range of possible upper atmospheric tempera-ture profiles.However,a high altitude temperature rise can be seen when analyzing the narrowest Na wave-length bands alone,sensitive to high altitudes well above the condensation/ionization altitude,making the high-altitude temperature measurement independent of the depletion mechanism.The hot high-altitude tempera-ture is illustrated in Fig.4,which shows photomet-ric Na measurements from Charbonneau et al.(2002)and Sing et al.(2008)overplotted with various constant abundance isothermal models.A single isothermal model fits through the 12and 17˚A bands,indicating that the temperature and Na abundance do not change signif-icantly between those altitudes (∼2,000to 2,200km).However,the absorptions measured in the 4.4and 8.8˚A bands,which probe higher in altitude (∼2,700to 3,700km),rise much faster than the isothermal model fitting the lower altitudes of the 12and 17˚A bands,indicating that warmer temperatures are needed.In the ionization Na depletion scenario,there are less temperature constraints for the middle atmosphere com-pared to the Na condensation model.However,limb temperatures everywhere above ∼1,500K are unlikely,and in contradiction with Spitzer measurements of in-frared brightness temperature.T-P profiles applicable to Na ionization models have less severe temperature rises compared to the condensation model,though a hot high-altitude temperature is still necessary and at least a modest temperature rise probable.A similar high altitude temperature rise will also be likely necessary to explain recent measurements of an-other hot-Jupiter,HD189733b.The Na core in that hot-Jupiter reaches ∼4,950km above the average optical transit altitude (Redfield et al.2008;Pont et al.2007).As the atmospheric scale height of HD189733b is smaller than HD209458b at the same temperature,a more ex-treme high altitude temperature rise is likely necessary,however,to fully explain the existing measurements.5parison with Spitzer anti-transit dataA stratospheric temperature inversion has been used to interpret Spitzer infrared secondary eclipse measure-ments of HD209458b(Knutson et al.2008),thought to be caused by an absorber at optical wavelengths on the day-side of the planet(Burrows et al.2007a; Fortney et al.2007).This optical absorber has been postulated to be clouds or molecules TiO and VO(Hubeny,Burrows&Sudarsky2003;Burrows et al. 2007a;Fortney et al.2007),with a low albedo ruling out some species,though not TiO or VO(Rowe et al.2006; Burrows et al.2007a).Comparing our limb T-P profile to the day-side pro-file from Burrows et al.(2007a)(see Fig.3),the at-mospheric pressures probed are similar,between0.01 and30mbar,despite our slant transit viewing geome-try(Fortney2005).The atmosphere in the infrared has a higher opacity,due to strong molecular transitions from species such as water(Burrows et al.2007a),placing the infrared surface of the planet viewed at normal angles at similar altitudes as those probed in slant geometry in the optical at the limb.The high altitude temperature inversion we observe at the limb below pressures of∼1mbar is separate from that of the dayside and occurs at a much higher altitude. However,the altitude of TiO and VO wefind from both models,largely confined to pressures above∼10mbar, closely matches the model presented by Burrows et al. (2007a),who placed the stratospheric absorber at pres-sures of∼25mbar and imposed heat redistribution be-tween pressures of10and100mbar.The probable pres-ence of TiO and VO in our spectrum along with the alti-tude similarity implies TiO and VO are indeed likely to be the stratospheric day-side temperature inversion insti-gators(Fortney et al.2007).As ourfit of TiO and VO is based largely on low resolution data,a more robust de-tection and interpretation of TiO/VO will likely require higher resolution HST spectra than those used here,such that multiple specific molecular bandheads could be ob-served.Some form of heat redistribution at or near our low-altitude pressure(∼30mbar)would likely be needed to explain the high temperature wefind there,as the tem-peratures there are significantly above that predicted by radiative equilibrium(Showman et al.2008).Ini-tial Spitzer mid-infrared measurements of the bright-ness temperature as a function of orbital phase have re-vealed that at least30%of the energy from the stel-larflux must be redistributed to the night side to ex-plain their null results,implying efficient heat redistri-bution(Cowan,Agol,&Charbonneau2007).Compar-ing with models by Burrows et al.(2007a,b)with higher P n s(>0.35),night side temperatures in the region of imposed heat distribution(corresponding to our pres-sure at z s)can have larger temperatures than the day side,perhaps explaining our high temperature at z s.Al-ternatively,systematic pressure scale differences between the two studies may indicate that our transmission spec-tra instead probes the top of the stratospheric tempera-ture inversion,giving a potential explanation of the high temperature at z s as those altitudes could already be warm.The minimum temperature wefind,however,is in general agreement with radiative equilibrium,perhaps implying the approximation is valid at those pressures around1mbar.Such scenarios can be further distin-guished in future studies,with tighter constraints on the average infrared and optical opacities,additional in-frared observations,along with improved global circula-tion models.The presence of a temperature inversion, TiO and VO along with heat redistribution would seem to currently place HD209458b in a intermediate hot-Jupiter class between the pM and pL classes as proposed by Fortney et al.(2007).4.DISCUSSIONThe atmospheric temperatures wefind,within the con-densation scenario,and presence of TiO and VO can also explain other HD209458b observational features.For in-stance,the low middle atmospheric temperature and the presence of TiO and VO would also explain the lack of observed potassium(K),originally predicted to be a ma-jor contributor to the optical opacity.At the lower tem-peratures of the middle atmosphere,K condenses into potassium chloride allowing KCl to become a dominant K-bearing gas.Condensed K would then naturally de-plete the atmosphere of atomic K,as seen here with Na, leading to reduced signatures.In the lower warmer at-mosphere,where wide atomic K line wings would be ob-servable even at low resolution,TiO and VO likely make up the surrounding continuum further masking the sig-nature.If Na is instead ionized,the minimum limb tem-perature is higher and ionization of K,which is easier than Na to ionize,likely depletes neutral K.If present in the atmosphere,a positive detection of atomic K in HD209458b will probably require high resolution ground-based or medium resolution space-based data to detect the K line core.Further detections or upper-limits of other atomic species which have different ionization po-tentials and condensation temperatures can offer clues in future studies when distinguishing between the two depletion scenarios.The Na mixing ratio wefind for the lower atmosphere is about two times solar while the abundance in the mid-dle and upper atmosphere is found to be0.2times solar or less,thus our models have decreased Na abundance without the need for a global deficiency of Na.In chem-ical equilibrium,Na2S condensation effectively removes all the Na below the condensation temperature,since the protosolar Na abundance is∼13%that of S,limit-ing the amount of Na2S which can condense directly to the amount of Na.Our condensation model T-P pro-file crosses the condensation curve again at higher alti-tude,making the altitudes of our minimum temperature a“cold trap”for Na.It is currently unclear how the2nd crossing of the condensation curve could affect the Na abundance,as the S/N limits us tofit only a single value for the whole upper Na abundance.Assuming equilibrium chemistry,our temperature pro-file would also result in less CO in the middle atmosphere, as our temperature profile at that level is closer to the CO =CH4curve which would result in an enhancement of CH4and H2O over that of CO and H2(see Fig.2).This is consistent with the lack of CO detection in HD209458b during transit(Deming et al.2005),although deviations from equilibrium have been shown to push the CH4/CO ratio to small values for the pressures probed here of less than1bar Cooper&Showman(2006).。