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Today Earth’s Atmosphere ( chp 1 cont’d) Geography 101 Warming the Atmosphere ( chp 2)

Mon. Sep 8. Today Earth’s Atmosphere ( chp 1 cont’d) Geography 101 Warming the Atmosphere ( chp 2) Wednesday (9/10) Air Temperatures ( chp 3). Weather Review. Weather Review. Weather Review. Monsoon Haboob. Weather Review. 5?/7?. 79. 59/79. 57/76. 58/76.

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Today Earth’s Atmosphere ( chp 1 cont’d) Geography 101 Warming the Atmosphere ( chp 2)

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  1. Mon. Sep 8 • Today • Earth’s Atmosphere (chp 1 cont’d) • Geography 101 • Warming the Atmosphere (chp 2) • Wednesday (9/10) • Air Temperatures (chp 3)

  2. Weather Review

  3. Weather Review

  4. Weather Review Monsoon Haboob

  5. Weather Review 5?/7? 79 59/79 57/76 58/76 Was this a good forecast?

  6. CO2 Cycle

  7. CO2 Time Series

  8. CO2 Time Series

  9. OZONE (O3) • Two types • “Good” ozone - Stratosphere (40-50K ft.) • Absorbs ultraviolet (UV) radiation • “Bad” ozone – Near the earth’s surface • Main ingredient of photochemical smog. • 3rd most potent greenhouse gas

  10. Ozone Formation • Surface Ozone

  11. Ozone Destruction • Stratospheric Ozone • UV radiation has enough energy to naturally break up the molecule. • Accelerated by CFCs’ • Hairspray, freon etc. • Catalyst • Accelerate Breakdown

  12. Ozone Hole 1978

  13. Ozone Hole 1988

  14. Ozone Destruction 1989MontrealProtocol

  15. Ozone Hole 1998

  16. Ozone Hole 2008

  17. Ozone Hole 2012

  18. Ozone Hole

  19. Meteorology Conventions Meteorological Directions(Cardinal Directions) N = 0 W = 270 E = 90 S = 180 Example: 225 degrees = Southwest

  20. Meteorology Conventions • Plotted Data • Altitude is represented on charts as increasing upward (y-axis) • Temperature increases to the right (x-axis) Altitude Temperature

  21. Meteorology Conventions • Greenwich Mean Time • GMT • UTC (Coordinate Universal Time) • Zulu (Z) • PST = UTC – 8 hours • PDT = UTC – 7 hours • 0000 UTC = 1700 PDT = 5 PM PDT • 1200 UTC = 0500 PDT = 5 AM PDT

  22. Map Classwork (HW#2 - 10 pts)

  23. Map Classwork

  24. Map Classwork

  25. 71 % covered by water • N. Hemi = 61% • S. Hemi = 81% 3 5 4 Map Classwork 1 6 2 9 7 1. Gulf of Mexico 2. Caribbean Sea 3. Bering Sea 4. Mediterranean 5. North Sea 6. Arabian Sea 7. Bay of Bengal 8. Tasman Sea 9. S. China Sea 8

  26. Map Classwork

  27. Cascades NewEngland GreatLakes Map Classwork SierraNevada Rocky Mountains GreatBasin Midwest AtlanticSeaboard Great Plains MississippiValley PACIFICOCEAN ATLANTICOCEAN Gulf Coast Gulf of Mexico

  28. WARMING THE EARTH AND THE ATMOSPHERE

  29. ENERGY AND HEAT TRANSFER • What is Energy? It’s the capacity to do work on some form of matter • Potential energy: The total amount of stored energy • Kinetic energy: Energy of motion

  30. HEAT CONDUCTIVITY

  31. Cold Air vs. Warm Air Slower and closer together | Faster and farther apart

  32. ENERGY AND HEAT TRANSFER • Atoms and molecules have kinetic energy due to their motion (heat energy) • Sun’s radiant energy most important • Air temperature is a measure of the average kinetic energy of its molecules

  33. ENERGY AND HEAT TRANSFER • Heat = energy transferred because of a temperature difference • After heat is transferred, it is stored as internal energy • Heat is transferred in the atmosphere by • Conduction • Convection • Radiation

  34. ENERGY AND HEAT TRANSFER • Latent heat: energy required to change a substance, such as water, from one state to another • Evaporation = cooling process, absorption of latent heat from the environment • Condensation = warming process, release of latent heat to the environment

  35. Changes of State

  36. ENERGY AND HEAT TRANSFER • Conduction: the transfer of heat from molecule to molecule • Always flows from warmer to colder • Air is an extremely poor conductor of heat

  37. ENERGY AND HEAT TRANSFER • Convection = heat transfer by the mass movement of a fluid (water or air) • Example • Pan of boiling water • Rising air currents • Convection circulation • Warm air expands • Rises • Cools and sinks

  38. Thermal Circulations

  39. ENERGY AND HEAT TRANSFER • Radiation = Energy transfer via electromagnetic waves • Radiative Properties • Hotter objects • Emit shorter wavelengths • Emit radiation at a greater rate or intensity

  40. Electromagnetic Radiation Fig. 2.7, p. 41

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