Coronal changes associated with a disappearing filament
Authors:
- 1 December 1975
- journal article
- research article
- Published by Springer Nature in Solar Physics
- Vol. 45 (2) , 377-392
Abstract
No abstract availableKeywords
This publication has 18 references indexed in Scilit:
- French Communism, 1920-1972Telos, 1975
- The reconnection of magnetic field lines in the solar coronaThe Astrophysical Journal, 1975
- XUV observations of coronal magnetic fieldsSolar Physics, 1975
- On the Fe XXIV emission in the solar flare of 1973 June 15The Astrophysical Journal, 1974
- Observing programs in solar physics during the 1973 ATM Skylab programSolar Physics, 1972
- Results from OSO-IV: The long term behavior of X-ray emitting regionsSolar Physics, 1972
- Radiation from a High-Temperature Low-Density Plasma: the X-Ray Spectrum of the Solar CoronaThe Astrophysical Journal, 1971
- On the Association Between Loop Prominences and Flares.The Astrophysical Journal, 1964
- The Solar Corona in Active Regions and the Thermal Origin of the Slowly Varying Component of Solar Radio Radiation.The Astrophysical Journal, 1961
- On the Interpretation of Prominence Spectra. III. The Line and Continuous Spectrum of a Loop Prominence and Limb Flare.The Astrophysical Journal, 1961