order… the sun mercury venus earth the moon mars phobos jupiter europa saturn titan uranus oberon...
TRANSCRIPT
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Order…The SunMercuryVenusEarthThe MoonMarsPhobosJupiterEuropaSaturnTitanUranusOberonNeptunePluto
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Atmospheric Processes
The structure of the atmosphere
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• 8th June 1898 – French scientist Léon Teisserenc de Bort used balloons carrying thermometers to record temperature variations within the atmosphere
• Temperature decreased with height to 11.8 km above sea level (ASL), then remained constant to 13 km ASL
• 206 further balloon ascents over next 4 years showed that temperature begins to increase above 13 km ASL
• Teisserenc De Bort had discovered the stratosphere
The structure of the atmosphere
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Atmosphere can be divided into four layers:
Thermosphere
Mesosphere
Stratosphere
Troposphere
Layers reflect differences in ability to absorb solar radiation
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Atmospheric pressure
• Rapid fall in air density and pressure with increasing height above Earth’s surface
• 50% of atmospheric mass lies within lowest 5.6 km
• >99% of atmospheric mass lies within lowest 40 km
• Atmospheric pressure units = millibars (mb or mbar)
• Normal pressure at sea-level = 1013.2 mb
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Troposphere
• Derived from the Greek word ‘tropos’ meaning ‘turn’ – referring to the layer’s convective and mixing characteristics
• Lowest layer of atmosphere – contains 75% of atmospheric mass
• Pressure decreases with altitude
• Approximately uniform decrease in temperature with height of c.6.5°C per 1000 m – environmental lapse rate
• Contains virtually all the atmosphere’s water vapour, clouds and pollution
• Contains the weather
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Tropopause
Troposphere
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Tropopause • Temperature inversion that acts as a ‘ceiling’ to air rising within the troposphere
• Latitudinal variations in height of tropopause ASL:
– Equator = 16-18 km (11 miles)
– Poles = 8-9 km (5 miles)
• Distortions in tropopause occur above mid-latitude jetstreams & tropical cyclones
– Dust and water vapour may penetrate up into stratosphere
– Dry ozone-rich air drawn down from stratosphere into troposphere
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Stratosphere
• Derived from the Greek word ‘stratum’ meaning ‘layer’ – referring to the layer’s stratified, non-convective nature
• Located above troposphere – between c. 10 and 50 km (30 miles) ASL
• Temperature increases with height from c. –60OC (lower stratosphere) to c.0°C at c.50 km ASL (stratopause)
• Contains small amounts of ozone (Ozone Layer) – absorbs ultraviolet (UV) solar radiation, causing warming of stratosphere
• Extremely dry layer with no weather (stable conditions due to cold air below)
• Most meteorites entering the atmosphere burn out above the stratosphere
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Ozone Layer• Discovered by Charles Fabry and
Henri Buisson, 1913
• From the Greek – “to smell”
• Absorbs 93-99% of the sun’s UV light which could be damaging to life on Earth
• Approximately 11-50 km in altitude
• Approximately 90% of Ozone in our atmosphere is found here
• Created by the Ozone-oxygen cycle
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Nacreous clouds
• Also known as ‘mother of pearl’ or polar stratospheric clouds
• Form at c.15-25 km (9-16 miles) ASL during polar winter when lower stratosphere temperatures fall to c. –80OC
• Consist of droplets / ice crystals of water, nitric acid and / or sulphuric acid
• Only visible before dawn / after dusk as clouds receive sunlight from below horizon and reflect it to ground surface
Nacreous clouds
Nacreous clouds
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Mesosphere
• Derived from the Greek word ‘meso’ meaning ‘middle’
• Located above stratosphere – between c.50 and 85 km (50 miles) ASL
• Temperature again decreases with height from c.0OC (at stratopause) to c.–90OC at c.80 km ASL (mesopause) (lowest value within layers)
• There are no gases, particles or water vapour to absorb UV radiation
Thermosphere
• Derived from the Greek words ‘thermos’ meaning ‘heat’
• Located above mesosphere – between c.85 and 500 km ASL
• Temperature increases with height to c.1200OC at 350 km ASL – due to oxygen molecules absorbing ultraviolet (UV) solar radiation
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Ionosphere - upper mesosphere and thermosphere (above 80km)
• Contains many ions (electrically charged particles)
• Absorbs UV radiation
• Can reflect radio signals
• Give rise to the northern and southern lights
There is no clearly defined boundary which marks the end of the atmosphere – gases are continuously lost into space (Exosphere) which is mainly made up of Helium and Hydrogen
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Noctilucent clouds
• Polar mesospheric clouds
• Form at c.85 km (50 miles) ASL – highest clouds in atmosphere
• Formation not fully understood – mainly composed of water ice
• Most commonly observed between 50O and 60O north during summer months
• Only visible before dawn / after dusk when lower atmosphere is in Earth’s shadow – otherwise too faint to be seen
• First reported in 1885 – shortly after eruption of Krakatoa
Noctilucent clouds
Noctilucent clouds
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Aurora borealis
Aurora borealis
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Fly through - NASA
• http://svs.gsfc.nasa.gov/vis/a010000/a010000/a010014/
What can I expect in the exam?