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Lesson 01 Atmospheric Structure n Composition, Extent & Vertical Division
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Composition n By Volume u Nitrogen (N 2 ) 78% u Oxygen (O 2 ) 21% u Others (1%) F Carbon Dioxide (CO 2 ) 0.035% F Ozone + Others(Neon, Xenon etc) u Water Vapour (variable from 0 - 4% locally)
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Composition con’t n Analysis reveals no variation in its composition up to at least 60km H except for increasing concentrations of Ozone in the upper Stratosphere. n At higher altitudes, the force of gravity being less causes the proportions to change.
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Composition con’t n None of these gases changes its state within the normal temperature range of the atmosphere so dry air remains invisible. n Only water vapour changes its state u water gas solid
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5 The water cycle, illustrating evaporation, condensation & precipitation
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6 The 3 M’s:- X Moisture X Mass X Movement
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Properties of the Earth’s Atmosphere n The earth’s atmosphere varies both vertically and horizontally in terms of: - Pressure - Temperature - Density - Humidity
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Properties of the Earth’s Atmosphere, contd. n The atmosphere is also a poor conductor of heat and being a gas is extremely fluid and only supports life in the lower levels. Fifty percent of the atmosphere is below the 500mb pressure level (about 18,000 feet).
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Vertical Division n The atmosphere extends to about 1000 km above the earth’s surface and n consists of several layers, each with its own properties. n The layers are defined by the temperature profile as shown in the following diagram..
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Vertical Division Ionosphere
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n Layer in contact with surface n Contains 80% of atmosphere n Temperature decreases with height n Until Tropopause reached n Zone of vertical mixing by convection and turbulence n Contains most of water vapour n Zone of clouds and weather n Heated from below Troposphere
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Tropopause n Indicated by marked change in lapse rate n Upper limit of cloud and weather n Lowest tropospheric temperatures at this level n Strongest winds aloft just below it n Height varies according to season and latitude n H 2 O decreases, O 3 increases
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Typical Average Tropopause Heights and Temperatures
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Variation in Height of Tropopause n The thickness of the Troposphere will vary according to temperature. n Lower when the air is cold (i.e. polar latitudes) n Higher when air is warm (i.e. equatorial latitudes) n Height therefore depends on season and latitude n Coldest tropopause temperatures over the equator n Breaks in tropopause caused by jet streams
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Variation of Surface Pressure with Height of Tropopause n High tropopause u high air column u high surface pressure u more prevalent in summer u near equator n Low tropopause u low air column u low surface pressure u more prevalent in winter u near polar latitudes
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17 Height/temperature graph for tropopause J A, J B, J C = Jetstreams
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Layered structure defined by the temperature profile (ELR) through the atmosphere. (Radio sounding)
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19 Radio Sonde
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Stratosphere n Temperature increases with height to about 50 km. n Contains warm Ozone region in upper levels at 40-50 km. n Weather does not penetrate but some severe CB’s may penetrate several 1000’s of feet. n Nacreous clouds form at about 20-30 km
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Nacreous Clouds
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Stratopause n Marks upper limit (50 km), of the stratosphere. n Maximum temperature just below freezing.
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Mesosphere n Region of decreasing temperature n Noctilucent clouds form at approximately 80 - 85 km. n Usually visible in summer in Northern sky near midnight.
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Noctilucent Cloud North Ayrshire Scotland 1988 July 02-03 00005 UTC
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Mesopause n Marks the upper limit of the Mesosphere. n Height approximately 80-90 km. n Temperatures between -120°C (summer) & -50°C (winter) at high latitudes
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Thermosphere n Zone of increasing temperature n Upper limit undefined. n Merges into the Exosphere/Ionosphere.
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Ozone in the Stratosphere n 90% of Ozone found here. n Absorbs harmful Ultra Violet (UV) radiation. n UV Radiation u causes skin cancers. u destroys DNA molecules. n Ozone filters in aircraft n Strongly absorbs IR earth radiation n Absorbed energy re- radiated back to earth n Helps maintain the thermal balance in the atmosphere
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Ozone Production n Ozone produced by interaction of molecular O 2 and UV radiation u O 2 + UV O + O u O 2 + O O 3 n Ozone forms mainly above 25 km but drifts down producing a peak concentration at 25 km.
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Ozone Destruction n Ozone is also destroyed by UV radiation. u O 3 + UV O 2 + O u O 3 + O 2O 2 n Ozone is also destroyed by the collision between two ozone molecules. u O 3 + O 3 3O 2
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Ozone Balance n Ozone between 25 and 35 km is maintained by a delicate natural balance n Ozone can be reduced by natural events e.g. solar flares and cosmic rays. n Pollutants such as fluorocarbons also destroy ozone.
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