Article contents
The Coronal Responses to the Large-Scale and Long-Term Phenomena of the Lower Layers of the Sun
Published online by Cambridge University Press: 14 August 2015
Extract
Based on the assumption, generally accepted over the past decade, that all the forms of solar and interplanetary activity are responses to the magnetic fields generated initially in the subphotosphere, some characteristics of the large-scale and long-term behaviour of the solar corona during the last three solar cycles are presented.
- Type
- Part II. Coronal and Interplanetary Responses to Long Time Scale Phenomena
- Information
- Symposium - International Astronomical Union , Volume 91: Solar and Interplanetary Dynamics , 1980 , pp. 87 - 104
- Copyright
- Copyright © Reidel 1980
References
- 1
- Cited by