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The Solar corona : proceedings /
The Solar Corona covers the proceedings of the International Astronomical Union Symposium No. 16 held at Cloudcroft, New Mexico, U.S.A. on August 28-30, 1961. The book focuses on the characteristics, reactions, and analysis of the solar corona. The selection first offers information on the local phy...
| Clasificación: | Libro Electrónico |
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| Autor Corporativo: | |
| Otros Autores: | |
| Formato: | Electrónico eBook |
| Idioma: | Inglés Francés |
| Publicado: |
New York :
Academic Press,
1963.
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| Temas: | |
| Acceso en línea: | Texto completo |
Tabla de Contenidos:
- Front Cover; The Solar Corona; Copyright Page; Contributors; Preface; Table of Contents; SESSION I: LOCAL PHYSICS OF THE CORONA; Introductory Review Paper; Chapter 1. Local Physics of the Corona; Density; Temperature; Excitation and Ionization; Energy Balance; References; Chapter 2. Comments on Coronal Heating; Electrostatic Ejection of Light Ions; References; Chapter 3. Remarks About the Temperature of the Solar Corona; Introduction; The Energy Balance of the Electrons; The Influence of Shock Waves on the Scale Height and on the Widths of Spectral Lines; References.
- Chapter 4. Relative Populations of Fe in the CoronaChapter 5. Excitation of the Red and Green Coronal Lines; Chapter 6. On the Filamentary Structure of the Solar Corona; References; Chapter 7. Prominences and the Solar Corona; References; Chapter 8. Solar X-Ray Emission; Chapter 9. Prediction of Solar Emission Lines in the Short-Wave Region of the Spectrum; References; Chapter 10. Solar Corona in Active Regions from Pulkovo Observations of the Green and Red Lines; References; AFTERNOON SESSION I; Chapter 11. Corona-Chromosphere Interface, and the Heating of the Corona.
- Description of the InterfaceThe Heating of the Corona; Chapter 12. Study of the Corona by Radar, Rockets, and Satellites; Rocket and Satellite Work; Discussion of X-Ray Events; Radar Technique; Chapter 13. Magnetic Fields and Coronal Condensations; Stability of Coronal Structures; SESSION II: CORONAL PHENOMENA; Introductory Review Paper; Chapter 14. Fast Phenomena in the Solar Corona; General Remarks on Flares; Coronal Observations; References; Introductory Review Paper; Chapter 15. Slow Variations of the Solar Corona; The Three Components of the Corona; The F-Component.
- The Total Brightness of the CoronaThe Electron Density; The Temperature; Shape and Ellipticity of the Corona; Emission-Regions; The East-West Asymmetry; Coronal Condensations; References; Chapter 16. The Influence of Flares on the Associated Permanent Coronal Condensation; References; Chapter 17. Photometry of the Solar Corona at the Eclipse of February 15, 1961; References; Chapter 18. A Thermal Origin of the Postburst Increases of Solar Microwave Radiation; Acknowledgments; References; Chapter 19. Some Features of AS Prominences; References; Chapter 20. The Evolution of Solar Prominences.