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Air B

Air B. Radiation and Climate. Solar Radiation. The sun (Sol) is a huge fusion reactor - combines two nuclei of H to a He atom. The produces a tremendous amount of energy Stars are the “birthplace” of all elements in the universe through the process of fusion. Solar Radiation.

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Air B

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  1. Air B Radiation and Climate

  2. Solar Radiation • The sun (Sol) is a huge fusion reactor - combines two nuclei of H to a He atom. • The produces a tremendous amount of energy • Stars are the “birthplace” of all elements in the universe through the process of fusion.

  3. Solar Radiation • Some of the energy from the sun is in the form of electromagnetic radiation - low to high types of energy. • All electromagnetic radiation is part of the electromagnetic spectrum

  4. Electromagnetic Spectrum

  5. Electromagnetic Radiation • Electromagnetic Radiation is composed of photons • Photons are small bundles of energy • Photons travel as waves - at the speed of light • Photons can travel through a vacuum - they don’t need a medium to travel on (like sound)

  6. Properties of Waves • Frequency - how many times a waves passes per amount of time. • Wavelength - the distance between two adjacent waves. • Must be the same “part” of the wave. • The wavelength and frequency along with the size of the photon determine the type of wave and its energy.

  7. Parts of a wave

  8. The sun and the ER • The sun’s radiant energy • 9% of it is UV rays • 46% is visible light • 45% is infrared light

  9. Infrared Radiation • Infrared Radiation is the portion of light just below red on the electromagnetic spectrum. • Causes molecules to vibrate this cause friction and the molecules heat up. • Most IR does not reach Earth’s surface. It is absorbed by CO2. • Some higher level radiation does hit Earth and is absorbed and reradiated back as IR. • This lead to the heating of the Earth’s atmosphere.

  10. Visible Light • Clear Day = 90% of visible light reaches the earth’s surface. • It is blocked by dust, clouds, pollution etc. • It can energize electrons in some biochemicals = photosynthesis. • It can excite cells in our eyes causing us to see.

  11. Ultraviolet Radiation • Stronger energy than visible light. • Three categories of UV radiation: • UV-A: • Longest wavelength, lowest energy • UV-B: • Shorter wavelength, higher energy - causes cancer. • UV-C: • Shortest wavelength, highest energy - used for sterilization • UV-A, UV-B, UV-C are mostly blocked by the ozone layer. • UV-C is absorbed by the atmosphere. • Mostly UV-A gets through to us.

  12. UV radiation • If all UV radiation reached the Earth’s surface - the Earth would be destroyed. • However, we need some UV radiation - it helps us produce vitamin D when exposed to our skin.

  13. The Carbon Cycle • The carbon cycle is the movement of carbon throughout the Earth’s ecosystem. • 100 yrs ago it was predicted that the level of carbon dioxide in the atmosphere due to the increase in burning of fossil fuels would be detrimental • The law of conservation of matter states that the matter can’t be created or destroyed so the amount of carbon would just keep changing forms (physical states)

  14. The Carbon Cycle • Atmospheric “reservoirs” of Carbon: • Carbon dioxide in the air • Calcium Carbonate (CaCO3) in limestone • Natural gas (CH4) • Petroleum

  15. The Carbon Cycle

  16. The Carbon Cycle

  17. The Carbon Cycle • 71% of Carbon is in the form of CO2 in ocean. • 22% is in the form of fossil fuels • The rest is in the rocks.

  18. The Carbon Cycle - Burning Fossil Fuels • Coal: C + O2 CO2 • Natural Gas: CH4+2O2 CO2+2H2O • Gasoline: 2C8H18+25O216CO2+18H2O

  19. Greenhouse gases and global change • The greenhouse effect is a natural and necessary phenomenon. • Carbon dioxide and water vapor are the two principle greenhouse gases. • These gases have been constant for millions of years…….until human came along.

  20. Global warming • There are 12 trillion tons of water vapor in the atmosphere. • Human activity can effect the temp. of atmosphere. • This causes more water vapor to evaporate. • More water vapor (greenhouse gas) means more warming. • More warming means more evaporating. • More evaporating mean more warming etc. • However, increase water vapor increases cloud cover so the temperature increase is not as dramatic.

  21. Global Warming • Carbon dioxide is similar. • If too much CO2 is added to atmosphere then stored CO2 in ice and soil could be released and the warm up continues. • Two other greenhouse gases: N2O and CH4 (methane).

  22. Global Warming • The last ten years have been the warmest to date. • If nothing done, temp. will inc. .3C per year. • By 2100 temp will inc. by 1C per year.

  23. Global Warming • Most scientists agree that the Earth will increase in temperature by 3-5C over the next century. • However, new data shows that the lower atmosphere is not warming as fast as the Earth’s surface. So there must be other factors affecting the warming. • El Nino • La Nina

  24. Effects of Global Warming. • The oceans (melting polar ice caps) will rise 5 cm (about 2 in.) per decade over the next century. • Flooding in several major cities: brings disease, pestilence, wastewater. • Rain cycle and growing season would be affected • Possibility of big storms with long droughts in between. • Short winters with severe blizzards.

  25. Preventing Global Warming • Kyoto Protocol • Developing energy efficient technologies • Focus on renewable energies.

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