Physical parameters in long-decay coronal enhancements
- 1 February 1979
- journal article
- Published by Springer Nature in Solar Physics
- Vol. 61 (1) , 69-88
- https://doi.org/10.1007/bf00155447
Abstract
No abstract availableKeywords
This publication has 33 references indexed in Scilit:
- The morphological and statistical properties of solar X-ray events with long decay timesThe Astrophysical Journal, 1977
- Coronal plasma parameters in a long-duration X-ray event observed by SKYLABThe Astrophysical Journal, 1977
- Interpretation of broad-band polarimetry of solar coronal transients - Importance of H-alpha emissionThe Astrophysical Journal, 1976
- Radiation from a High-Temperature Low-Density Plasma: the X-Ray Spectrum of the Solar CoronaThe Astrophysical Journal, 1971
- Solar Loop Prominences: a Theoretical ModelThe Astrophysical Journal, 1967
- Spectrographic Observations of the Flare of July 20, 1961The Astrophysical Journal, 1967
- Loop Prominences and Coronal Condensations. II. The Source of Mass and Energy and a Model of the Loop Prominence Mechanism.The Astrophysical Journal, 1965
- On the Association Between Loop Prominences and Flares.The Astrophysical Journal, 1964
- On the Interpretation of Prominence Spectra. III. The Line and Continuous Spectrum of a Loop Prominence and Limb Flare.The Astrophysical Journal, 1961
- Physical Conditions in Limb Flares and Active Prominence. I. The Loop Prominence of November 12 and 22, 1956.The Astrophysical Journal, 1959