The Solar Spectrum Proceedings of the Symposium held at the University of Utrecht 26–31 August 1963
A good deal of our information on solar physics and on solar phenomena is derived from the solar spectrum. A quantitative interpretation of this spectrum was only possible after 1920, after the establishment of Bohr's atomic model, the discovery of Saha's law, and the development of spectr...
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| Format: | eBook |
| Language: | English |
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Dordrecht
Springer Netherlands
1965, 1965
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| Edition: | 1st ed. 1965 |
| Series: | Astrophysics and Space Science Library
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| Subjects: | |
| Online Access: | |
| Collection: | Springer Book Archives -2004 - Collection details see MPG.ReNa |
Table of Contents:
- Opening Address
- Fourty Years of Solar Spectroscopy
- Session I The Photosphere
- La Structure de la Photosphère
- The Current Revision of the Solar Spectrum Table ? 2935 Å to ? 8770 Å
- Discussion on Line Formation and Photospheric Structure
- Discussion on New Instrumental Techniques
- Discussion on Photospheric Motions
- Session II The Quiet Chromosphere
- The Theory of the Chromospheric Spectrum
- The Chromospheric Spectrum at Eclipse
- Rocket Spectra of the Chromosphere
- Discussion on the Quiet Chromosphere
- Session III The Active Photosphere and Chromosphere Spots, Plages, Flares and Prominences
- Spectra of Solar Activity Regions
- About the Flare Problem
- Discussion on the Active Chromosphere
- Session IV The Corona
- The Theory of the Coronal Spectrum
- The Coronal Spectrum
- Discussion on tne Corona
- Session V Particle and Radio Emission From The Sun
- Particle and Radio Emission from the Sun
- The Variable Solar Radio Spectrum
- Non-Thermal Sources and Amplified Emission in Solar Radio Bursts
- Some Aspects of the Type-IV Continuum Radiation on Decimeter Wavelengths
- Discussion on Radio and Particle Emission from the Sun