Содержание
- 2. Some particularities of the solar atmosphere Solar atmosphere is non-homogeneous and very unstable. Phenomena in the
- 3. Two successive photos of a solar flare phenomenon evolving on the sun. The solar disk was
- 4. Solar spots Some relatively cold formations (4599 – 4600 K) of irregular shape appearing in the
- 5. http://en.wikipedia.org/wiki/File:Solar-cycle-data.png
- 6. Total spectrum of the solar radiation Gamma rays Visible wavelengths (μ) X-rays Violet 0,39 – 0,455
- 8. http://en.wikipedia.org/wiki/File:Atmospheric_Transmission.png
- 9. Notion of OPTICAL WINDOW Emittance of the Sun is close to the emittance of the a.
- 10. Solar constant The amount of SR (radiation flux) coming to the upper boundary of the Earth
- 11. Temperature of the Sun emitting surface Average distance between the Sun and the Earth And the
- 13. Difference between the insolation in Northern and southern hemispheres is explained by the eccentricity of the
- 14. Distribution of the Sun energy in various areas of the spectrum UV ( ) – 9%
- 15. Solar radiation distribution over the globe We’ll consider the distribution over the upper “boundary of the
- 16. Insolation The flux of solar radiation falling on a horizontal surface is called INSOLATION denotes altitude
- 17. Denotes time of sunrise Denotes time of sunset At
- 18. Calculation made from this formula allowed obtaining following distribution of the insolation over the globe.
- 20. The Q values in summer of the Southern hemisphere are bigger than corresponding values for the
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