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The Earth and Its Atmosphere: 1. Vertical structure 2. Weather and climate

The Earth and Its Atmosphere: 1. Vertical structure 2. Weather and climate. Mass,Weight, Density, Pressure. Mass M : property of matter, SI unit: kg. Other units: 1kg=1000 g, 1 lb=450 g Weight : a force, has a magnitude and direction (vector).

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The Earth and Its Atmosphere: 1. Vertical structure 2. Weather and climate

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  1. The Earth and Its Atmosphere:1. Vertical structure2. Weather and climate

  2. Mass,Weight, Density, Pressure • Mass M: • property of matter, • SI unit: kg. Other units: 1kg=1000 g, 1 lb=450 g • Weight : • a force, has a magnitude and direction (vector). • weight = mass x gravity g(Earth)= 9.78 m/s2 • SI unit: kg m/s2 -> N g(Mars)= 3.7 m/s2 • Density r: • mass per unit volume: density = mass / volume • SI unit: kg/m3, Other: g/cm3 • Pressure p: • p= force/area • SI units: Pa=N/m2, Other: 1bar=100 Pa

  3. Atmospheric pressure and air density Atmospheric pressure and density decrease with altitude exponentially!!!

  4. RECAP • Atmospheric composition: • Permanent gases: N2, O2, Ar, Xe, Ne, H2, He • Variable gases: CO2,H2O,O3,CH4 • Greenhouse gases: H2O, CO2, NO,CH4 • Mass. • Weight. • Density. • Pressure. • The atmospheric pressure and density decrease with altitude.

  5. Mid-chapter brief review(s) • The earth’s atmosphere is a mixture of many gases. In a volume of dry air near the surface, nitrogen (N2) occupies about 78 percent and oxygen (O2) about 21 percent. • Water vapor, which normally occupies less than 4 percent in a volume of air near the surface, can condense into liquid cloud droplets or transform into delicate ice crystals. Water is the only substance in our atmosphere that is found naturally as a gas (water vapor), as a liquid (water) and as a solid (ice). • Both water vapor and carbon dioxide (CO2) are important greenhouse gases. • Ozone (O3) in the stratosphere protects life from harmful ultraviolet (UV) radiation. At the surface, ozone is the main ingredient of photochemical smog. • The majority of water on our planet is believed to have come from its hot interior through outgassing. • Atmospheric pressure at any level represents the total mass of air above that level, and atmospheric pressure always decreases with increasing height above the surface. ? ?

  6. Vertical Structure of the Earth’s Atmosphere 99.9% 90% Lapse rate

  7. Atmospheric layers(according to the temperature) • Troposphere: • The temperature T decreases with height at a rate of 6.5 K/km. • Well mixed as a result of turbulence and convection • Weather phenomena • Tropopause: • Isothermal (T constant) • Located 8-15 km above the ground. • Stratosphere: • The temperature T increases with height • O3 layer at 25 km altitude • The atmosphere is very stable • Stratopause: T=const • Mesosphere: • T is decreasing with height: effective cooling through IR emission • Very unhealthy region: hypoxia (oxygen deprivation), UV burns, blood begins to boil • Mesopause: the coldest region on Earth. • Thermosphere: fast T increase. Diffusive separation of gases.

  8. Atmospheric layers: other classifications • Mixing: • Homosphere: • well mixed, • the chemical composition is constant. • Heterosphere: • no turbulence and mixing, • diffusive separation of gases • Ionization: • Ionosphere: part of the atmospheric gas is ionized through photo ionization or impact ionization. • (talk about the atom)

  9. The Terrestrial Planets 1 0.39 0.72 1.5 39.4 1 0.055 0.815 0.1 0.0025 1 0.38 0.95 0.53 0.176 5.5 5.43 5.24 3.94 2 9.78 3.62 8.57 3.7 0.3 23.4 0 2.7 25 62 1 0.24 0.6 1.88 247 24 1407 5832 24.6 153 Mercury Venus Earth Mars Pluto Distance AU. 260 -235 Mass ME. 480 T=15 C Radius RE. -60 Density -110 Gravity -190 Obliquity Orbital period. Rotationalperiod -225 -215 Main components - N2, O2 CO2 CH4 CO2

  10. The Giant Planets 1 5.2 9.5 19.2 30 1 318 94.5 14.5 17 1 11 9.5 4 3.9 5.5 1.31 0.69 1.29 1.64 9.78 22.9 9 8.7 11 23.4 3 27 98 30 1 11.9 29.5 84 165 24 10 10 18 19 Earth Jupiter Saturn Uranus Neptune Distance AU Mass ME Radius RE Density Gravity Obliquity Orbital period Rotationalperiod Main components H2, He N2, O2 H2, He H2,He,CH4 H2, He

  11. Weather/ Climate • Weather elements: • Air temperature: thermometer (C, F, K) • Air pressure: barometer (bar, mbar) • Humidity: hygrometer (%) • Wind: (m/s , km/h, mi/h) • Clouds • Precipitation • Visibility • Weather: the daily variations of the atmospheric conditions. “It is partly cloudy today, with a 50% chance of rain” • Climate: average weather. “The average maximum temperature for the month of January is 35 F.”

  12. Weather Forecasting Using Satellites isobar streamline isotherm

  13. The World

  14. Jupiter as seen from Cassini

  15. Jupiter

  16. Meteorology – a brief history • Meteorology is the study of the atmosphere and its phenomena • In “Meteorologica” (340 B.C.) Aristotle discussed • meteors (things which fall from the sky) • weather and climate, astronomy, geography… • clouds, rain, snow, wind, hail, thunder, hurricanes… • Invention of weather instruments in the Middle Ages • Pressure: barometer (1643, E. Torricelli) • Humidity: hygrometer (1783, H. de Saussure) • Rapid exchange of weather information (telegraph, 1843) • Crude weather maps (1869) • Norwegian model of storm development (1920’s) • Air balloon and high-flying aircraft observations (1940) • High-speed computers and numerical predictions (1950-) • Weather satellites (1960-) Aristotle de Saussure

  17. Simplified surface weather map

  18. Weather phenomena: a preview Clouds and thunderstorms Ice storm Tornadoes Flooding

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