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Department of (Assistant professor) March 2017 1.Definition of Atmosphere • Atmosphere: The . The • • layer of gases that surrounds the Earth. It is a gaseous layer surrounding the earth. In other words, we can say that , called atmosphere. Yes, it is thin when compared to the size of the earth. Yet, this thin layer has its own influences on various processes that take place on earth. . In fact, it took millions of years to reach the present condition by various processes. Along with its development, life came into existence and evolved. Atmosphere extends from a However, about Most of the mass of the . All the natural processes on earth are functioning harmoniously. Atmosphere is very important . It contains in sufficiently large quantities. Constant concentration of oxygen is maintained through oxygen cycle. The oxygen cycle does not take place in isolation but it takes place along with other . These cycles connect the atmosphere with , and . The atmosphere does not function by itself, but it functions in conformity with other spheres on earth. Atmosphere is the and reaches the earth’s surface or into the water. It is a wonder, why solar radiation is mentioned as “lifesustaining” one. It is mentioned so, because, solar radiation is the , which thereby supports all other life. When solar radiation passes through the atmosphere, happen. , which is a part of our atmosphere. from reaching the earth’s surface. Earth is not heated by solar radiation uniformly due to its inclination. As a result, different weather patterns exist over the earth. In order to compensate these differences, air sets in motion resulting in winds and circulation of air. These wind currents are of global scale as well as of local scale. They are responsible for disastrous storms like cyclones, dust storms, tornadoes etc. These wind currents also influence water currents in the oceans; they in turn affect the wind currents. Consequently, understanding the atmosphere and its functions and behavior is quite complex. However, with available knowledge, scientists try to comprehend to the extent possible. Thus, understanding of the atmosphere has become very essential and important. All the above processes make the atmosphere, a dynamic atmosphere. In nutshell: • Without atmosphere:– Life would be impossible on earth and living things would be as helpless as fish without water – We would not survive for more than a few minutes (oxygen ) – there could be no clouds, winds and rains • Atmosphere acts as a great canopy /shelter/ to protect the earth’s surface from the strong sun radiation and prevent excessive loss of heat by night. • The components of atmosphere (like ozone and atomic oxygen) filter (absorb) the harmful ultra violet radiation of the sun. • It protects the earth’s surface from the direct strike of meteors that reach in the thermosphere and mesosphere burn from the heat generated by air friction 1.1.3. Composition of Atmosphere • The compositions of the atmosphere are and • The atmosphere is a mixture of and (water vapor) that surrounds the earth like a blanket. • Air is a mechanical mixture of gases, not a chemical compound. As a result of this, in the atmosphere is composed the following gases:: - Dry air, by volume, is : - They are , thereby producing the greenhouse effect. The most common greenhouse gases include:Carbon dioxide (CO2) Methane ( ) Nitrous oxide (N2O) Ozone (O3) Chlorofluorocarbons (CFCs: chiefly CFC-l3 (F-12) and CF2C-l2 (F-12)) Hydrogenated halocarbons (HFCs and HCFCs) Water vapor (H2O) A. Reactive gas species: - are produced by the cycles of sulphur, nitrogen and chlorine. These play key roles in acid precipitation and in ozone destruction. The common reactive gases include:Nitrogen species:-The reactive species of nitrogen are nitric oxide (NO) and nitrogen dioxide (NO2). Sulphur species:- species are sulphur dioxide (SO2) and is sulfur trioxide (SO3) A. Aerosols: Impurities, such as dust, ashes, smoke, salt, etc., from both natural and human sources are also present in the atmosphere. Collectively, these tiny solid or liquid suspended particles of various compositions are called aerosols. Some natural impurities found in the atmosphere are quite beneficial. Small, floating particles, for instance, act as surfaces on which water vapor condenses to form clouds. • However, most human-made impurities (and some natural ones) are a nuisance, as well as a health hazard • Permanent /uniform Gases and Variable Gases es • Permanent /Constant gases are the ones, and . • Examples of uniform gases are: (0.93%), (78.09%), (20.95%), • Ar, Ne, He, H2, Kr, Xe are called . Argon is the largest trace gases in the atmosphere. • Nitrogen and oxygen are the two major constant gases that make up 99 percent of the air. Both are important to sustain life on earth. Nitrogen constitutes 78.09% and oxygen 20.94 percent b. Variable Gases • Variable gases are . • The remaining is constituted by such as, argon, helium, krypton, xenon and also by variable gases – • Examples of variable gases are: water vapor (0-4%), CO2 (0.035%), CH4, N2O, O3, CFC. …….. [CH4, N2O, O3 and CFC are called trace gases.] In nutshell: Atmosphere has nature/characteristics:- the following ; it can’t be felt except when it is in motion; so we cannot see, smell or test air. It is It is transplant to short wave radiation but can absorb long wave (earth radiation) (infra-red) radiation. It , since it can be compressed its decreases with altitude. 1.1.4. Origin of atmosphere • The origin of our earth’s atmosphere is • The solar system is . • As there are no human then, any explanations about the solar system are simply theories based on the observation we make now. • The • The . • Such clouds are common between the stars in our galaxy even today and astronomers now identified them and think all stars, including the sun have formed from them. • Evidence from these clouds, especially cosmic gas suggests that first atmosphere probably consisted mainly of Hydrogen (71%), Helium (27%) as well as trace amounts of Ammonia and Methane. This is called primordial atmosphere. • However, the gaseous elements that comprised this original atmosphere of the earth under went much evolution. • In the early stage of planet formation from interstellar clouds, solar and gravitational effects probably resulted in accretion of some gases and the subsequent escape of others. • When the earth was formed some 4.6 billion years ago, it was probably too hot to retain any of the atmospheres it had to begin with. • Hydrogen and Helium escaped from the earth’s atmosphere. In addition, the lower gravitational force of the earths is unable to retain light gases such as hydrogen and helium. • Continuous out gassing, a process that expelled gases and other materials form the earth’s interior, took place 4.6 billion years ago by volcanism and plate tectonics. Volcanoes particularly emitted water vapor and carbon dioxide with a little bit of nitrogen. It produced the earth’s secondary atmosphere. The vast amounts of water vapor formed clouds, which in turn produced rain. At this time, the surface temperature was cool enough for water vapor to condense in to water. Over a period of thousands of years, the rain accumulated as rivers, lakes, basins and oceans. • These water reservoirs acted as sinks for large amounts of carbon dioxide and through chemical process become locked up in the sedimentary rocks such as limestone. The nitrogen, which is not chemically active continued to accumulate in the atmosphere. The earth’s atmosphere is unique among the planets of the solar system since O2 have been added in the atmosphere over time. Oxygen is the byproduct of photosynthesis. Evolutionist Theory • This is the most widely • According to this theory • The first atmosphere is . • When the Earth was formed , Earth’s atmosphere was probably mostly (H) and (He) plus , such as methane ( ) and ammonia ( ). • The earth originated from • The first atmosphere consists of • But these gases ( ) are very light gases. • Over billions of year, and (energetic particles). and simply they are light, hence they are diffused to the atmosphere. • Volcanic emission – The release of gases from rock through volcanic eruption (so-called outgassing) was the . – The primeval (ancient) atmosphere produced by the out-gassing was mostly carbon dioxide (CO2) with some Nitrogen (N2) and water vapour (H2O), and trace amounts of other gases. • Hot springs • Emission of water vapor, CO2, N2 – The first atmosphere would have consisted of gases in the solar nebula, primarily hydrogen. – As the solar nebula dissipated these gases would have escaped, partly driven off by the solar wind. – The next atmosphere, consisting largely of plus and , was produced by out gassing from volcanism, supplemented by gases produced during the late heavy bombardment of Earth by huge asteroids. – A major part of emissions were soon dissolved in water and built up carbonate sediments. • Third atmosphere: The constant re-arrangement of continents by plate tectonics influences the long-term evolution of the atmosphere by transferring carbon dioxide to and from large continental carbonate stores. – Free oxygen did not exist in the atmosphere until about during the Great Oxygenation Event and its appearance is indicated by the end of the banded iron formations. – Before this time, any oxygen produced by photosynthesis was consumed by oxidation of reduced materials, notably iron. • The earth is surrounded by a thin layer of air, called, atmosphere. The atmosphere, from the surface of earth extends up to 60,000 km. • You may wonder how such a thickness would be called a thin layer. Where, most of the mass of the atmosphere is found near the planetary surface. • It is near the earth’s surface from surface to about . This is due to the earth’s gravity, which pulls the atmospheric constituents, towards its center. . • It is the thin layer, in which most of the atmospheric processes take place. According to the concentration of the gases, atmosphere is divided into: : the lower region, extending from the surface of the earth to a height of 80 to 100 km above the earth. In this layer, gases are more or less uniform in their chemical composition. 2. : it starts from the and – In this layer, Concentration of . and hence, . • The atmosphere is composed of a series of , and . • These layers vary in altitude and temperature, and they do not mix together. • The name is derived from the Greek word “tropos” meaning to turn or mix because it has a great deal of vertical mixing due to solar heating at the surface (describes the layer’s convective and mixing characteristics). Major characteristics of the Troposphere: The lowest layer of the atmosphere which surrounds the earth like It is the layer of atmosphere Within the troposphere, air circulates in great vertical and horizontal convection currents, constantly redistributing heat and moisture around the globe. It is the zone where The composition are N2, O2, CO2, Ar, O3 (small amount), aerosols and water vapour. The average depth of the troposphere is about 12km. Because holds most air molecules close to the earth’s surface, the troposphere is much denser than the other layers: Throughout this layer, there is a general decrease of temperature with increasing height at a mean rate of about 6.5°C/1km (6.5°C/1000m). This is called So lapse rate is a characteristics of Troposphere The main reasons are:• The lower atmosphere in the troposphere is heated by terrestrial re-radiation that is heat rising from the surface of the earth not directly from the sun. – So in the troposphere, the higher we go from the lower atmosphere, the further we go from the source of(terrestrial) heat • The density of the atmosphere (air) decreases with altitude. • The troposphere is capped in most places by a temperature inversion level (i.e., a layer of relatively warm air above a colder layer) and in others by a zone that is isothermal with height. • A sudden reversal of this temperature gradient creates a sharp boundary called the tropopause, which limits mixing between the troposphere and upper zones. Tropopause • It is an isothermal layer (equal temperature) • It is a zone of perfect calm (constant) • It forms a boundary layer (transition zone) between trop • In some regions troposphere is broken down so there is mixing between the two zones. Because it is mixed (marked) by jet streams (very fast and high level wind). • There are marked variations in the altitude of the tropopause with latitude, from about 16km at the equator, where there is strong heating and vertical convective turbulence, to only 8km at the poles. • So 12km is an average height (16 + 8 /2=12). 2. The Stratosphere (stratified sphere) The name is derived from the Latin ‘stratum’ meaning a layer – this describes its state of non - convective nature. Major characteristics of the Stratosphere:• It is the next layer of atmosphere above the troposphere. • It extends from the • In the stratosphere, there is a • Thus, unlike the troposphere, the relatively calm; so, commercial jets fly here. is There is so little mixing in the stratosphere that volcanic ash or human-caused contaminants can remain in suspension there for many years. The composition are the same with stratosphere (N2, O2, CO2, Ar, O3 (small amount), aerosols and water vapour) but the exception is maximum ozone (O3) and little water vapour. There is no visible weather condition. That means temperature increases with altitude. This is called So temperature inversion is the characteristics of stratosphere. Can you suggest the reason why temperature increases with increase altitude in the stratosphere? o The reason for the increased temperature with altitude in the stratosphere is due . o This absorbed energy makes the atmosphere warmer toward the top of the stratosphere. o Because UV radiation damages living tissues, causing skin cancer, genetic mutations, crop failures, this UV absorption in the stratosphere also protects life on the earth’s surface. • Ozone gas is largely concentrated at about 30 kmcalled (a place where there is maximum ozone). • Its upper part is called (boundary b/n stratosphere and mesosphere) • The name is derived from the Greek word ‘ ’ meaning ‘ ’ • It is the layer of atmosphere directly • Extending from km above Earth’s surface. • The boundary near 50 km, which separates stratosphere and mesosphere, is called the . • The air at this level is , which means that only one-thousandth of all the atmosphere’s molecules is above this level and 99.9% of the atmosphere’s mass is located below it. • Temperature falls rapidly with increasing altitude as there is no (or little) water vapour, dust or Ozone to absorb the incoming radiation. • The top part (mesopause) has the lowest temperature close to 100oC; this layer is the of the atmosphere. • Has the . • Pressure is very low due to the lower density of the atmospheric molecules. • Is the darkest part of the atmosphere due to the scarcity of the air molecules to reflect or scatter radiation • Most meteorites which enter the mesosphere from space burn and disintegrate as they experience increasing friction. Therefore, this layer has meteoritic dust particles • Extends upw • • • • and temperature continuously rises with increasing altitude throughout this layer called . The increase of temperature in the thermosphere is due to the reaction between ultra-violet radiation with atomic oxygen (O) and molecular nitrogen (N2). These gases absorb a few solar energy raises temperature into a greater degree. The thermosphere is important in long-distance communication because it reflects outgoing radio waves back to Earth without the aid of satellites. The warmest layer of the atmosphere • It is electrically charged zone • Nitrogen (N2) and (O) are abundant in the lower part of thermosphere (the ionosphere). • These are the capacity to absorb the incoming very short ultra-violet radiation (below 0.2 micro meters in wave length). • When these gases absorb the rays of the sun, they lose their electrons and the ionosphere becomes full of electrically charged particles. • The loss of electrons from an atom is called the ionization process. • As the electrons move in the thermosphere, they cause an inversion of temperature. • Important in reflecting radio waves: B.B.C. • The electrons of the ionosphere are also used for communication because they can reflect radio-waves back to the earth’s surface (known as ionospheric reflection of radio waves). • • • • • Exo- means external, outer layer Temperature reaches up to 1100oC Light gases are exist Gravity reaches to (0) In the upper layer of the thermosphere (exosphere), negatively charged electrons increasingly separated from neutron and proton atoms by high energy radiation from the sun. • In the magnetosphere (the outer most layer of the thermosphere) there are only electrons (negative) and protons (positive) derived from solar wind-plasma of electrically conducting gas. Gas Permanent % By volume Nitrogen Oxygen 78.09 20.95 Variable Gases Carbon dioxide 0.03 Water Vapor 0.2-4 Ozone 0.00006 Inert Gases Argon (Inactive gases) Helium, Neon, krypton 0.93 Trace Non gaseous Dust particles Trace Pollutants Sulfur dioxide, Trace Nitrogen oxide, Methane, etc Importance for weather & Other function ( Source ) Climate Needs for plant growth Produced by photosynthesis, reduced by deforestation. Absorbs long wave radiation Used by plants for photo from earth keeps synthesis; temperature steady; Increased by burning fossil has greenhouse effect fuels and by deforestation Source of cloud formation& perception, reflects (absorbs) incoming radiation Absorbs incoming UVradiation Can reach 4 %, can be stored as ice/snow Absorbs / reflects incoming radiation, forms condensation nuclei necessary for cloud formation Affects radiation, causes acid rain Volcanic dust, meteoritic dust, soil erosion by wind Reduced / destroyed by chlorofluorocarbon CFCs From industry, power stations and car exhausts • The word “weather” is used to denote the • It shows short term variability in terms of: • Is the day-to-day state of atmosphere and pertains to shortterm changes in conditions of • Is constantly . • It results fundamentally from processes that attempt to equalize differences in the distribution of net radiant energy received from the sun. • The weather is made up of different elements, which are measured either by special instruments or are observed by a meteorologist. • These measurements are then recorded and used in the making of climate graphs and weather forecasts. Temperature is a physical quantity that is a measure of It is a measure of the local thermal energy of matter or radiation; it is measured by a , which may be calibrated in any of various temperature scales, etc., etc. Many things depend on temperature, such as: physical properties of materials including the phase (solid, liquid, gaseous or plasma), density, sol ubility, vapor pressure, electrical conductivity. rate and extent to which chemical reactions occur the amount and properties of thermal radiation emitted from the surface of an object speed of sound is a function of the square root of the absolute temperature Temperature scales • Much of the world uses the Celsius scale (°C) for most temperature measurements. It has the same incremental scaling as the Kelvin scale used by scientists, but fixes its null point, at 0°C = 273.15K, approximately the freezing point of water (at one atmosphere of pressure). The United States uses the Fahrenheit scale for common purposes, a scale on which water freezes at 32 °F and boils at 212 °F (at one atmosphere of pressure). • 0°C = 273.15K = 32 °F & 1°C = 274.15K = 33.8 °F • Insolation is a measure of solar radiation energy received on a given surface area and recorded during a given time. • It is also called and expressed as " " if recorded during an hour or " " if recorded . • The unit recommended by the is (MJ/m2) or (J/mm2). Sunlight is a portion of the electromagnetic radiation given off by the Sun, particularly infrared, visible, and ultraviolet light. On Earth, sunlight is filtered through the Earth's atmosphere, and is obvious as daylight when the Sun is above the horizon. When the direct solar radiation is not blocked by clouds, it is experienced as sunshine, a combination of bright light and radiant heat. When it is blocked by the clouds or reflects off other objects, it is experienced as diffused light. The World Meteorological Organization uses the term "sunshine duration" to mean the cumulative time during which an area receives direct irradiance from the Sun of at least 120 watts per square meter. Precipitation is any product of the condensation of atmospheric water vapour that falls under gravity. The main forms of precipitation include drizzle, rain, sleet, snow, and hail. Precipitation occurs when a Fog and mist are not precipitation but suspensions, because the water vapour does not condense sufficiently to precipitate. • Two processes, possibly acting together, can lead to air becoming saturated: cooling the air or adding water vapor to the air. • Precipitation is a major component of the water cycle, and is responsible for depositing the fresh water on the planet. • Approximately 505,000 cubic kilometers of water falls as precipitation each year; 398,000 cubic kilometers) of it over the oceans and 107,000 cubic kilometers over land. • Given the Earth's surface area, that means the globally averaged annual precipitation is 990 millimeters (39 in), but over land it is only 715 millimeters (28.1 in). The table below shows the weather element details. SN Element Description How it is measured Units of measurement 1 Temperature How hot or cold it is By Thermometers, found inside a Stevenson Screen Degrees Celsius ( c) 2 Insolation Incoming solar radiation 3 Sunshine The hours of sunshine By a Sunshine Mega joules per square metre (MJ/m2) Recorder Hours and minutes 4 Precipitation By a Rain Gauge Millimetres (mm.) 5 Humidity Moisture from the sky e.g. rain, snow etc. The amount of water vapour in the air 6 Cloud Cover Relative Humidity (% of water vapour that can be held by the air at the actual temperature) Oktas − eighths of the sky 7 Visibility 8 Air Pressure By a Hygrometer (wet and Dry Bulb Thermometers) It is observed by a meteorologist It is observed by a meteorologist By a Barometer 9 Wind Speed By an Anemometer Knots, or by the Beaufort Scale 10 Wind Direction By a Wind Vane Points of the compass (north, north−west etc), or bearing in degrees The amount of cloud in the sky How far you can see The "weight" of the air pushing on the surface of the Earth How fast the wind is blowing Where the wind is blowing from Kilometers Hectopascals (although most people know it as millibars) • Is described as (heat, moisture, and air movement) of an area over a long period of time. • It is the • The It is a condition in the atmosphere at any time or short period of time. Weather conditions can change suddenly. Today may be warm and sunny, tomorrow may be cool and cloudy. Weather conditions include rain, snow, sleet, hail, fog, mist, sunshine, wind, temperature and thunderstorms. Describes surface and atmospheric conditions over a longer period or over a large geographical area. Climate changes slowly, usually over decades, centuries and thousands of years. • In the study of climate and weather, the same elements temperature, moisture, pressure and wind are used. Scope of Weather and Climate • Scope of weather: The study of what causes • Scope of climate: The study of Significance of (studying) weather and climate • The weather affects us in many different ways. The study of weather and climate is important for determined: • Clothing type: the type of clothes that people wear varies from season and season, and from climate of one region to another. • Housing condition: People construct houses that suit the type of climate in which they are living. • Food crops: the kinds of food crops grown vary according to the variation in climate. Climate affects the type of economic activity. • Animal and plant life: the kinds of animals and plants that live in certain environment are the result of climate. Controls of Weather and Climate • Both weather and climate differs from place to place and form time to time due to the variation in the amount, intensity and areal distribution of various climate elements. • The factors that cause for such variation are termed as controls of climate and weather. Some of the controls of climate and weather are:• Latitude: is the position of place either north ward or south ward of the equator that determines the length of the day, intensity & duration of sunlight. • As a result, places at lower latitude (around equator) receive high angle of the sun which increases intensity &vice versa. • Altitude: Is the height of places asl. It has effect on temperature (Alt.↑To↓), pressure (Alt.↑P↓) & precipitation (Alt.↑ PPT↑). • Distance from the sea (nearness to water bodies): water bodies have warming and cooling effect on the surrounding land masses. – This has a greater effect on temperature and rainfall distribution. As a result, places far away from water bodies have high temperature and less amount of rainfall. e.g. the Sahara desert. • Ocean currents: Are horizontal movements of ocean waters that are caused by winds and difference in temperature. There are two major types of ocean currents which we call warm and cold ocean currents. Warm ocean currents that move from tropics towards the poles have warming effect while cold ocean currents that move from poles towards the tropics have cooling effect. • Cloud cover: the presence of cloud cover in an area has a significant influence on the temperature condition of a place. With clear skies, temperature increases due to direct reach of incoming solar radiation to the earth’s surface without any reduction or absorption and reflection of it through clouds. • Mountain barriers: landform barriers, particularly high mountain ranges, influence the temperature of a place by blocking the movements of moisture bearing winds which finally control the weather and climate condition of a locality. • Aspect: In the northern hemisphere north facing slope will have cold condition due to polar cold winds and sheltered from insolation. – In the southern hemisphere north facing slope has high temperature (warming condition) due to north warming conditions and exposure to the sun. type of climate data • max,/min, range ppt, temp, humidity, wind speed sources of climate data how to get climate data and import it to excel sheet (CSV) how to fill data gaps – interpolation? Or? • analysis in Excel environment – basic analysis like mean, median, max/min, range, • For what purpose and how we use Regression • Data to ArcGIS environment – major statistical method in climate studies Climate graphs are line graph, bar graph or a combination of both a bar graph and a line graph (climograph). Temperature is shown on a line graph. Rainfall is shown by a bar graph. Temperature and Rainfall together may be shown with climograph. A line chart or line graph is a type of chart which displays information as a series of data points connected by straight line segments. It is a basic type of chart common in many fields. A line chart is often used to – a time series – thus the line is often drawn chronologically. Structure • A line chart is typically drawn bordered by two perpendicular lines, called axes. • The horizontal axis is called the x-axis and the vertical axis is called the y-axis. • Each axis represents one of the data quantities to be plotted. • Typically the y-axis represents the dependent variable and the x-axis (sometimes called the abscissa) represents the independent variable. • The chart can then be referred to as a graph of ``Quantity one versus quantity two, plotting quantity one up the y-axis and quantity two along the x-axis. B. Bar chart • A bar chart or bar graph is a chart with rectangular bars with lengths proportional to the values that they represent. The bars can be plotted vertically or horizontally. A vertical bar chart is sometimes called a column bar chart. • One axis of the chart shows the specific categories being compared, and the other axis represents a discrete value. Some bar graphs present bars clustered in groups of more than one (grouped bar graphs), and others show the bars divided into subparts to show cumulate effect (stacked bar graphs). C. A climograph is a graphical representation of basic climatic parameters, which is monthly average temperature and Precipitation, at a certain location. It is used for a quick-view of the climate of a location. One form of representation uses an overlapped combination of a bar and line chart used to show the climate of a place over a 12 month period. • Use following table to make A. Line Graph For Maximum temperature For Minimum Temperature For Maximum and Minimum Temperature both B. Bar Graph to show Precipitation C. Climograph to show Max. Temperature and Precipitation / Min. Cambridge 1971–2000 averages Month Jan Feb Mar Apr May Jun Jul Aug Sep Oct Nov Dec Max Temp [°C] 7.0 7.4 10.2 12.6 16.5 19.4 22.2 22.3 18.9 14.6 9.9 7.8 Min Temp [°C] 1.3 1.1 2.9 4.0 6.7 9.8 12.0 11.9 10.1 7.1 3.7 2.3 Days of Air Frost [days] 9.7 9.5 4.9 3.2 0.5 0.0 0.0 0.0 0.0 1.2 4.8 8.0 Sunshine [hours] 55.5 72.6 107.0 145.8 189.7 180.0 191.3 186.9 141.6 115.0 68.1 47.7 Rainfall [mm] 45.0 32.7 41.5 43.1 44.5 53.8 38.2 48.8 51.0 53.8 51.1 50.0