Structure and Development of Solar Active Regions
K. O. KIEPENHEUER ( Fraunhofer Institut, Freiburg i. Br., Germany) The present symposium, to my knowledge the largest ever held in the field of solar research (170 astronomers from 21 countries) was held in the building of the Hun garian Academy of Sciences in Budapest from September 4 to 8, 1967....
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Format: | eBook |
Language: | English |
Published: |
Dordrecht
Springer Netherlands
1968, 1968
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Edition: | 1st ed. 1968 |
Series: | International Astronomical Union Symposia
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Online Access: | |
Collection: | Springer Book Archives -2004 - Collection details see MPG.ReNa |
Table of Contents:
- Welcome by the Hungarian Academy of Sciences
- Preface and introduction
- I General Development of an Active Region
- II Theoretical Aspects
- III Optical Structure of an Active Region
- IV Cooperative Study of Solar Active Regions (CSSAR)
- Evolution of Ca plages of the CSSAR active regions
- Correlation between Ca plages and longitudinal magnetic fields of the CSSAR active regions
- Évolution des émissions coronales au cours de la vie d’un centre actif
- V Coronal and Interplanetary Structure of an Active Region
- VI Transient Phenomena
- VII Proton Flare Project (PFP)
- VIII Radio Structure of an Active Region
- Summarizing Review