1. Chapter 1 Introduction to the Atmosphere ATMO 1300 Spring 2010

2. “Weather” vs. “Climate” Weather – Short-term variations in the sensible state of the atmosphere (e.g., hot today, rain over the weekend, etc…) METEOROLOGY – The study of weather Climate – Long-term state of the atmosphere (e.g., global warming) CLIMATOLOGY – The study of climate The link between meteorology and climatology…

3. The source of energy for our atmosphere is the sun! -Drives existence and motion of weather systems

4. General Characteristics of the Atmosphere The atmosphere is a 3-dimensional fluid

5. General Characteristics of the Atmosphere Very shallow depth (relative sense) Figure from www.met.tamu.edu/class/metr452/models/2001/global.gif

6. General Characteristics of the Atmosphere No defined top Has mass, therefore weight, due to gravity Mainly composed of invisible gas molecules and aerosols

7. Q: Which scenario is correct upon combining air masses of different densities? LESS DENSE (WARM) HEIGHT MORE DENSE (COLD) This is a STABLE situation (something has to happen externally to overturn it) That something is WEATHER! Example: Think of a pot of water on the stove… why do hot air balloons fly?

8. COLD COLD HOT UNSTABLE situation, air is less dense underneath more dense air. Atmosphere always wants to achieve stability. To do, so which way must cold/warm air move? WEATHER exists to remove the imbalance. In this case, thermal imbalance leads to a thunderstorm. (Much) more later… just wait COLD

9. Permanent Atmospheric Gases Nitrogen (N 2 ) – 78% Oxygen (O 2 ) – 21% Argon (Ar) – 1%

10. Variable Gases Water Vapor (H 2 O) (varies from ~ 0-4%) Carbon Dioxide (CO 2 ) Ozone (O 3 )

12. Mainly found in the Stratosphere (a beneficial shield), but can often be found in the Troposphere (a harmful pollutant). Ozone absorbs UV radiation from the sun Photochemical reactions determine development and destruction of ozone: Creation: O 2 → O + O O 2 + O + M = O 3 + M Depletion (need ChloroFluoroCarbons, CFCs): CFCl 3 + UV radiation = CFCl 2 + Cl Cl + O 3 = ClO + O 2 ClO + O = Cl + O 2

13. Fig. 1-8, p. 10

14. Fig. 1-9, p. 11

15. Carbon Dioxide Controlling factor on temperature (greenhouse gas) Increase since 1950s (intense debate regarding link to global warming) Sources include: animal respiration and combustion.

16. Fig. 1-3, p. 6

17. Fig. 1-4, p. 7

18. Important Facts About Water Vapor

19. Water Vapor – the “other” greenhouse gas An invisible gas Gaseous phase of water If you can see it, it’s not water vapor!

20. Water Vapor An invisible gas Gaseous phase of water If you can see it, it’s not water vapor! Referred to as atmospheric moisture Greatest concentration in lower atmosphere (near surface of the Earth) WHY?

21. Water Vapor How does water vapor get into the atmosphere? By a process called EVAPORATION Liquid water to water vapor Called a change of phase

22. Gas vs. Liquid Gas Liquid

23. Fig. 1-5, p. 8

24. Sources of Water Vapor left photo from webworld98.com; right photo from killamfarms.com EVAPORATIONTRANSPIRATION

25. Importance of Water Vapor Necessary for clouds to form (clouds are composed of LIQUID water droplets – CONDENSATION necessary!) Controlling factor on temperature (greenhouse gas) Phase transformations are a huge source of energy in the atmosphere –Energy from latent heat release (condensation) in a thunderstorm is on the order of a 1 kiloton nuclear bomb!

26. Aerosols Small (microscopic) solid particles (e.g., clay, silver iodide, organic material) Combustion by-products, sea spray, dust Act as condensation nuclei –the beginning of the precipitation process Affects health, visibility, optical effects

27. Blowing Dust in Lubbock Welcome to Lubbock, those of you who are new to the area…

28. Fig. 1-11, p. 12

29. Vertical Structure of the Atmosphere Vertical Distribution of Mass Vertical Distribution of Temperature

30. Vertical Distribution of Mass Density = mass per unit volume Density decreases with increasing altitude Figure from apollo.lsc.vsc.edu/classes/met130

31. Atmospheric Pressure Pressure = Force per unit Area Related to Density Its how much “stuff” is above you Stuff= atmosphere

32. Pressure Change with Height Like density, pressure decreases with increasing altitude. It does so at a greater rate in the lower atmosphere Here in Lubbock…we are at about 3300 ft (about 1 km) elevation

33. Fig. 1-13, p. 15 Hurricane Katrina at its peak: 902 mb Hurricane Wilma at its peak: 882 mb – all time record low for Atlantic

34. Ideal Gas Law Part of the Physics that governs the atmosphere… Atmosphere or air can be thought of as an “ideal” or “perfect” gas and follows a simple relation Pressure x Volume = constant x Temperature Or Pressure = R x Density x Temperature R=287.05 J/kg K

35. Vertical Distribution of Temperature Average temperature distribution FOUR layers Temperature trend determines atmospheric layers – NOT A FIXED DEPTH!

36. Troposphere Where most “weather” occurs

37. Troposphere Figure from www.atmos.ucla.edu/AS3 Temperature decreases with height Amount of temperature decrease with height (e.g., -10 deg C / km) called a Lapse Rate Strong cooling with height VERY important for development of thunderstorms!

38. Troposphere Depth varies with latitude (greatest over tropics) and season (greatest in summer)

39. Stratosphere Temperature increases with height – called an Inversion Contains Ozone (i.e., the “ozone layer”) Not much “weather” occurs

40. Tropopause Boundary between the Troposphere and Stratosphere

41. Mesosphere/Thermosphere Mesosphere – cooling with height Thermosphere – warming with height (inversion)

42. The Ionosphere Upper Mesosphere into Thermosphere Contains electrically charged particles called IONS Figure from apollo.lsc.vsc.edu/classes.met130

43. The Ionosphere Affects radio transmissions D layer absorbs AM radio waves D layer disappears at night, E,F layers reflect AM radio waves back to earth Figure from apollo.lac.vsc.edu/classes/met130

44. The Ionosphere Where Aurora Borealis (northern lights) occurs Photo from climate.gi.alaska.edu/Curtis

45. End of Chapter 1