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AS Course Module 3: THE ATMOSPHERE • The atmosphere is heated from BELOW 1. Solar energy hits the earth’s surface (short-wave) 2. The earth’s surface ABSORBS the short wave energy from sun via CONDUCTION 3. Also the air directly above the earth’s surface is also heated by CONDUCTION 4. The air above (30m and higher) is heated by CONVECTION (eg hot air balloon) – this forms cumulonimbus clouds. 5. As well as all this the short-wave radiation is reflected as long wave (terrestrial radiation). This is emitted from the earth’s surface and is absorbed by greenhouse gases – such as Carbon Dioxide (CO2), Methane (CH4), CO (Carbon Monoxide), Sulphur Dioxide (SO2). This process is called GLOBAL WARMING. The Structure of the Atmosphere Earth's Atmosphere The Earth is surrounded by a blanket of air, which we call the atmosphere. It reaches over 560 kilometers (348 miles) from the surface of the Earth, so we are only able to see what occurs fairly close to the ground. Early attempts at studying the nature of the atmosphere used clues from the weather, the beautiful multi-colored sunsets and sunrises, and the twinkling of stars. With the use of sensitive instruments from space, we are able to get a better view of the functioning of our atmosphere. Life on Earth is supported by the atmosphere, solar energy, and our planet's magnetic fields. The atmosphere absorbs the energy from the Sun, recycles water and other chemicals, and works with the electrical and magnetic forces to provide a moderate climate. The atmosphere also protects us from high-energy radiation and the frigid vacuum of space. The envelope of gas surrounding the Earth changes from the ground up. Four distinct layers have been identified using thermal characteristics (temperature changes), chemical composition, movement, and density. Troposphere The troposphere starts at the Earth's surface and extends 8 to 14.5 kilometers high (5 to 9 miles). This part of the atmosphere is the most dense. As you climb higher in this layer, the temperature drops from about 17 to -52 degrees Celsius. Almost all weather is in this region. The tropopause separates the troposphere from the next layer. The tropopause and the troposphere are known as the lower atmosphere. Stratosphere The stratosphere starts just above the troposphere and extends to 50 kilometers (31 miles) high. Compared to the troposphere, this part of the atmosphere is dry and less dense. The temperature in this region increases gradually to -3 degrees Celsius, due to the absorbtion of ultraviolet radiation. The ozone layer, which absorbs and scatters the solar ultraviolet radiation, is in this layer. Ninety-nine percent of "air" is located in the troposphere and stratosphere. The stratopause separates the stratosphere from the next layer. Mesosphere The mesosphere starts just above the stratosphere and extends to 85 kilometers (53 miles) high. In this region, the temperatures again fall as low as 93 degrees Celsius as you increase in altitude. The chemicals are in an excited state, as they absorb energy from the Sun. The mesopause separates the stratosphere from the next layer. The regions of the stratosphere and the mesosphere, along with the stratopause and mesopause, are called the middle atmosphere by scientists. This area has been closely studied on the ATLAS Spacelab mission series. Thermosphere The thermosphere starts just above the mesosphere and extends to 600 kilometers (372 miles) high. The temperatures go up as you increase in altitude due to the Sun's energy. Temperatures in this region can go as high as 1,727 degrees Celsius. Chemical reactions occur much faster here than on the surface of the Earth. This layer is known as the upper atmosphere. The upper and lower layers of the thermosphere will be studied more closely during the Tethered Satellite Mission (TSS-1R). Questions 1>4: 1. Why does it get colder the further you go up a mountain? • You are further away from the influence of conduction and convection at the earth’s surface – as the atmosphere is heated from BELOW • “Albedo effect” = ISR (incoming solar radiation) is reflected off lighter surfaces – eg snow • Greater windspeeds higher up because there is less friction with earths surface so any heat there is taken away • There is less pressure the higher up you go – which means that there are less molecules of air to absorb the ISR / reflected LW radiation (from earth) 2. Where would you find a higher % of water vapour? • Above trees – transpiration taking place • Over oceans – where evaporation is taking place • Clouds – where water vapour has condensed 3. In what ways are humans contributing to the greenhouse effect? • CO2 from power stations; from deforestation in Amazon; • CO from car combustion • CH4 from animals / rice fields • So2 from power stations 4. Why is the atmosphere thicker at the equator than at the poles? • The spinning effect of the earth “pulls” air into the equator away from the poles The Ozone Hole Ozone Hole Splits, Spring 2002 (total area smaller than 2001) September 25, 2003 • Solar constant • Distance from the sun • Angle of the sun in the sky • Seasonal variations The amount of energy which is received from the sun varies with sunspot activity. Its exact value is not known but is about 1380W m2 The earth’s distance from the sun varies throughout time and this can cause a 6% variation in the solar constant. It has been argued that this has been enough to cause the ice ages. The curvature of the earth means that there is TWICE as much incoming solar radiation reaching the earth's surface at the equator (during the autumn and spring equinox’s) than there is at 600N or S It is clear in this diagram how much more land area the same “bundle” of solar radiation has to cover than that at the equator EARTH Equator During theNorthern summerHemisphere months when thethe Northern is tilted During the winter, angle at Hemisphere which the incoming The are short during winter there is little time for the The days towards time the of year sun, makes the angle an enormous at which the difference incoming to solar the amount radiation of solar radiation reaches thethe surface isand very low and each bundle of incoming radiation The N Hemisphere summer days are long which means there is solar radiation to aheat the ground after the long nights. Noteover that the North is having to heat far larger area of land. The is directly overhead the radiation strikes the which earth’s reaches surface the isearth’s high. The surface sunsun is directly the Tropic more time for the ground to be heated by incoming solar radiation 0 SOUTH Pole receives no insolation at23.5 all during this time Tropic of Capricorn, ofequator. the equator. of Cancer, which iswhich 23.50is NORTH of the Consequently the summers in the N Hemisphere areare hot. Consequently N Hemisphere winters cold. 600N. This is the latitude of northern Scotland Equator Earth’s axis is on a 23.50 tilt SUN December 21st Midwinter's day in the Northern Hemisphere June 21st Midsummer's day in the Northern Hemisphere September 21st Autumn equinox Twice during the The sun is year the sun is “sideways on” to directly overhead the earth and as at the equator a result the tilt is and the N and S negated Hemispheres receive equal amounts of I S R March 21st Spring equinox SUN Consequently there is 12 hour night and 12 hour day across the entire globe, give or take 15 minutes Earth’s axis is on a 23.50 tilt For an excellent graphical explanation of the seasons go to; www.usatoday.com/weather As a result of ISRblanket never Consequently Stratus cloudsdesert on clouds, theenvironments other 23% hand of (Grey have the greatest cloud) are Cumulus clouds (the “fluffy” ones) reflect a lot of ISR dueitto Based on this information can you explain why The During However As apicture result the atthe summer is it NIGHT is complicated warmer all months the at heat night further it is on when warmer the asequatorial itground there depends during isescapes heavy the what day reaches earth's surface. dark. diurnal (day and night) variation and rainforests their light clearly colour. reduce the amount ISRitduring the SORT ifClouds into cloud there space OF cover. is CLOUDS no as there are are as in all no the the clouds sky ISRthe can toof hold reach in…... the earths is warmer incloud, the day during winter when have the least These day, prevent butreflected this longwave doesn’t necessarily radiation leaving mean itthe will lower bethe colder! 20% and 3% is absorbed by surface………. This isis due to the ALBEDO effect, which we will look at later. there is cloud? atmosphere and can keep the environment WARMER water droplets themselves 6% reflected / absorbed by atmosphere Earth’s albedo 30% 20% reflected by clouds 4% reflected from earth’s surface 16% absorbed by dust and gases 3% absorbed by clouds •The 6% is either absorbed •Much It is remaining themore absorption (over 20%) and scattering incoming of by stratospheric ozoneby(O) or reflected byand the • different 16%is absorbed atmospheric gases radiation wavelengths is “scattered” of by ISR the bygases gases and atmosphere. The by and dust. is proportion radiated longwave dust. dust which ThisThis incoming cause theradiation sky as toabsorbed be isblue thenduring ozone is as UV radiation, which isthe extremely radiation which in turn warms known the day. “diffuse radiation”. harmful to human skin and eyes (known to be atmosphere. carcinogenic) as well as harmful to plants Aurora borealis / australis The northern / southern lights Thermosphere and uppermost Mesosphere – solar wind (clouds of electrically charged particles) – Earth’s magnetic field directs them towards poles – excite oxygen (O) and nitrogen (N2) ions in ionosphere emit light 4% is reflected from the earth’s surface without being absorbed. This is due to the ALBEDO effect which was mentioned earlier……. Different surfaces absorb and reflect varying amounts of ISR. This is known as their albedo. Place the following surfaces in order, based on the amount of ISR they reflect. Have a guess at the amount of ISR they reflect •Oceans •Light coloured and darkdeserts soils <10% •Coniferous •Coniferousforest forest 15% •Grassland •Fresh snow and deciduous forest 25% • •Oceans Light coloured and dark deserts soils 40% •Fresh •Grassland snow and deciduous forest 85% and landterms are twothen, clear examples these InWater layman's it takesoftwice Being a body of therefore has a by Thenear situation is water further complicated variations. asthe much energy to heat water, BUT noticeable effect on the climate of a landmass as the different ways in which the earth’s It requires 4.2kj of energy to heat 1kg of water by following slides demonstrate. ALSO it needs to LOSE twice as much 0 surfaces heat and cool. This is obviously 1 C. toacool downwhen by the sameatamount. key factor looking climate as it In comparison it takes only 2.1kj to heat 1kg of is essentially the ground which heats the soil. As a result the oceans are cooler in the atmosphere. Sand requires 0.84kj. in the winter and summer but only warmer The way inas which materials absorb and are known THERMAL RESERVOIRS release heat energy is known as their SPECIFIC HEAT CAPACITY. It is the amount of energy required to raise 1kg of a substance by 1C. Inland areas are far from the sea and Note thefrom warm away the and the cold areas. warming influence Anyofideas as to why this is? the Caribbean Keeps inland areas warm in winter Warm Caribbean 400 North 400 North Note how much farther north the UK is compared to the latitude line. Any ideas as to why it isn’t extremely cold? (We are the same latitude in Bedford as Calgary in Canada) 400 North 400North GCM The World January 29th 2002 The World January 29th 2002 Equatorial Low Pressure Trough: Clouds and Rain The Intertropical Convergence Zone (ITCZ) Doldrums L ITCZ Subtropical High-Pressure Cells: Hot Desert Air The Horse Latitudes Broad Cells of High Pressure H AIR MASSES Unstable Air Instability is caused by an air mass rising off the ground. This can be caused for example, by a body of cold air (in this case polar Maritime air) getting warmer as it moves further south – ie Towards the equator. As the air rises it COOLS. As it cools down it’s capacity to hold moisture decreases. Another way of saying this is that it increases in humidity. When the humidity reaches 100% - the air is said to be saturated – or reaches its “DEW POINT TEMPERATURE”. At this point air held as water vapour condenses and water droplets or CLOUDS FORM. At the same time LATENT HEAT OF CONDENSATION is released which gives the rising air more upward momentum (like a hot air balloon). This forms cumulonimbus rain clouds. Polar Maritime Air Mass North Pole UK Cold air begins to warm as It travels further south therefore Rises off the ground – leading To UNSTABLE AIR Equator DEPRESSIONS Atmospheric Pressure Pressure can be thought of as the weight of all overlying air (though, in reality, pressure exerts force in all directions). Average Sea Level Atmospheric Pressure: 29.92” of Mercury 76 cm of Mercury 1013 millibars (mb) Mercury Barometer - Invented by Toricelli, 1643 Warm Front Cold Front Cold Air Warm air Cold Polar Maritime Air Warm Tropical Maritime air WEATHER ASSOCIATED WITH THE PASSAGE OF A CLASSIC DEPRESSION Ahead of the warm front Passage of the warm front Warm sector Passage of the cold front Cold sector Pressure starts to fall steadily continues to fall steadies starts to rise continues to rise Temperature quite cold, starts to rise continues to rise quite mild sudden drop remains cold Cloud cover cloud base drops and thickens (cirrus and altostratus) cloud base is low and thick (nimbostratus) cloud may thin and break clouds thicken (sometimes with large cumulonimbus) clouds thin with some cumulus Wind speed and direction speeds increase and direction backs veers and becomes blustery with strong gusts remain steady, backs slightly speeds increase, sometimes to gale force, sharp veer winds are squally Precipitation none at first, rain closer to front, sometimes snow on leading edge continues, and sometimes heavy rainfall rain turns to drizzle or stops heavy rain, sometimes with hail, thunder or sleet showers ANTICYCLONES Air Pressure Force exerted by air molecules per unit area (Result of compression of the air by gravity). This pressure force is omnidirectional. LOCAL ENERGY BUDGETS Mountain-Valley Breezes Land and Sea Breezes L H x 5x Temperature Inversions An upside-down situation The ‘Normal’ Situation 105’ 38°F 105’ 38°F 64’ 40°F 64’ 40°F 32’ 40°F 32’ 40°F 16’ 41°F 8’ 41°F 16’ 41°F 8’ 41°F Temperature Inversions These are when the ‘normal’ situations are reversed ie when warmer air overlies colder air. This can be at low level Temperature Inversions These are when the ‘normal’ situations are reversed ie when warmer air overlies colder air. This can be at low level or at high level Temperature Inversions There is a natural inversion in our atmosphere as the stratosphere is the layer that absorbs most of the ultraviolet radiation (high level) Temperature Inversions High level inversions are also found in depressions, when the warm sector overlies the cold sector (occlusion) Temperature Inversions Low level or ground inversions occur in anticyclonic conditions when there is a rapid loss of energy at night. The air near the surface is cooled by conduction of heat to the cold ground. The lower layer is therefore colder than Temperature Inversions Low level or ground inversions occur in anticyclonic conditions when there is a rapid loss of energy at night. The air near the surface is cooled by conduction of heat to the cold ground. The lower layer is therefore colder than Temperature Inversions A classic inversion is where the hot emissions given off by industrial chimneys trap in the colder air below Signs of a surface inversion in the early morning Lack of heavy cloud cover Windless or light variable wind Ground Fog Frost (or dew) HOT AIR – more able to carry moisture Cold Air descends and condenses forming fog Smoke from a chimney forming a layer Surface inversion - early morning