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The Sun's Atmosphere. Photosphere - the 5800 K layer we see. Chromosphere
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1. Outer Layers of the Sun Photosphere
Limb darkening
Sun spots
Chromosphere
Corona
Prominences, flares, coronal mass ejections
Reading 18.5-18.10
2. The Sun’s Atmosphere Photosphere - the 5800 K layer we see.
Chromosphere – a thin layer, a few 1000 km thick, at a temperature of about 10,000 K. Can be seen during solar eclipse.
Corona – Outermost layer, 1,000,000 km thick, at a temperature of about 1,000,000 K.
3. Outer layers of sun
4. Photosphere
5. Chromosphere
6. Corona
7. Corona
8. Limb darkening
9. Limb darkening
10. Sunspots are low temperature regions in the photosphere
11. Particles spiral around magnetic field lines
12. Sunspots are low temperature regions in the photosphere
13. Sunspot cycle
14. Sunspots can be used to measure the rotation of the Sun
15. Sunspot cycle
16. Granulation
17. What direct observational evidence supports the model of thermonuclear reactions in the Sun’s core? Neutrinos
Gamma rays
Sun spot counts
WMD inspections
18. Solar magnetic fields also create other phenomena Prominences
Flares
Solar wind
Coronal mass ejections
19. Particles spiral around magnetic field lines
20. Prominences -Cooler than photosphere.
21. Solar flares -Hotter, up to 40,000,000 KMore energetic
22. Coronal mass ejections -eruption of gas, can reach Earth and affect aurora, satellites
23. Coronal mass ejection
24. Which statement is not correct? The solar coronal temperature is about 106 K.
Sunspots are very cool and dark, with temperatures of about 300 K.
The Sun’s core has a temperature about 107 K.
The chromosphere is hotter than the photosphere.
25. Review Questions Since the Sun is so bright, how is it possible to see its dim outer atmosphere (corona)?
Where does the solar wind come from?
What are sunspots? Why do they appear dark?
What is the connection between sunspots and the Sun’s magnetic field?
What is the sunspot cycle?