Solar and Stellar Physics Proceedings of the 5th European Solar Meeting Held in Titisee/Schwarzwald, Germany, April 27-30, 1987
These proceedings bring together ideas from solar and stellar physics. The sun is near enough for rather detailed observations and one chapter is devoted to the more recent experimental data from observations from space. On the other hand the multitude of stars provides a wide range of physical para...
| Other Authors: | , |
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| Format: | eBook |
| Language: | English |
| Published: |
Berlin, Heidelberg
Springer Berlin Heidelberg
1987, 1987
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| Edition: | 1st ed. 1987 |
| Series: | Lecture Notes in Physics
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| Subjects: | |
| Online Access: | |
| Collection: | Springer Book Archives -2004 - Collection details see MPG.ReNa |
Table of Contents:
- What can the sun tell us about stellar activity?
- On the origin of stellar magnetism
- Stellar activity and rotation
- Solar and stellar convection
- Photospheric structure in solar-type stars
- Solar and stellar chromospheres
- Solar an stellar coronae
- Stellar vs. solar activity: The case of pre-main sequence stars
- Winds in late type stars and the solar wind
- Observations from space vs. ground based observations: Advantages and disadvantages
- New ideas about granulation based on data from the solar optical universal polarimeter instrument on spacelab 2 and magnetic data from big bear solar observatory
- Future prospects of stellar and solar physics from space