1 / 111

Geology 1001/1101

Geology 1001/1101. Sec 003 Chris Paola Class 12: climate and glaciation. Chapter 10. THE CLIMATE SYSTEM AND GLACIATION. Key ideas about climate & glaciation. Much of Minnesota’s landscape has been sculpted by glaciers

omar
Télécharger la présentation

Geology 1001/1101

An Image/Link below is provided (as is) to download presentation Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author. Content is provided to you AS IS for your information and personal use only. Download presentation by click this link. While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server. During download, if you can't get a presentation, the file might be deleted by the publisher.

E N D

Presentation Transcript


  1. Geology 1001/1101 Sec 003 Chris Paola Class 12: climate and glaciation

  2. Chapter 10 THE CLIMATE SYSTEM AND GLACIATION

  3. Key ideas about climate & glaciation • Much of Minnesota’s landscape has been sculpted by glaciers • Glacial cycles are controlled by variation in Earth’s orbit on time scales of 10,000 – 100,000 yr • Climate  weather; climate is long-term average of weather

  4. Climate: planetary controls • Distance from Sun • Albedo (reflectivity or “whiteness”) • Atmosphere (greenhouse effect) • Orbital properties • Plate configuration (mainly due to effect on ocean circulation)

  5. Climate: geographic controls • Distance from equator • Average air flow & pressure • Distance to the ocean • Prevailing wind relative to mountains & ocean

  6. Cold Hot NOT distance to Sun! 92,900,000 miles 3,900 miles

  7. all sunlight that hits Earth’s surface

  8. 10% of sunlight spread across 6.5% of sunlit surface at equator, Earth’s surface is almost perpendicular to sunlight, so energy is concentrated in small area

  9. 10% of sunlight spread across 6.5% of sunlit surface ~ 150% of average intensity at equator, Earth’s surface is almost perpendicular to sunlight, so energy is concentrated in small area

  10. 10% of sunlight spread across 20.5% of sunlit surface 10% of sunlight spread across 6.5% of sunlit surface ~ 150% of average intensity at poles, Earth’s surface slopes away from sunlight, so energy is spread across a greater area

  11. 10% of sunlight spread across 20.5% of sunlit surface < 50% of average intensity 10% of sunlight spread across 6.5% of sunlit surface ~ 150% of average intensity at poles, Earth’s surface slopes away from sunlight, so energy is spread across a greater area

  12. Cold Hot due to the angle of the Earth’s surface

  13. Global air flow determines large-scale rainfall patterns Mars: one cell per hemisphere

  14. dry wet dry Earth: 3 cells per hemisphere

  15. Energy and power • Energy (work) • Joules • BTUs: 1 BTU = 1055 J • Kilowatt-hour: 1 KWH = 3600000 J • Calorie (food): 1 Cal = 4187 J • Power: energy per time (energy rate) • 1 Joule/sec = 1 Watt • 1 HP = 746 Watt • US energy consumption (power), per capita: 11.4 kW (11,400 Watt)

  16. 99% of air mass

  17. Importance of the ocean in climate • Heat storage (heat capacity of water >> that of air) • Heat and moisture transport

  18. Ocean currents

  19. Importance of the ocean in climate • Heat storage (heat capacity of water >> that of air) • Heat and moisture transport now onto the cryosphere…

  20. A side note: Ice and sea level

  21. El Niño Warm, rising air here  lo pressure  helps maintain the wind pattern

  22. El Niño movie

  23. Part II: glaciation

  24. Movies

More Related