EUV emission, filament activation and magnetic fields in a slow-rise flare
- 1 April 1975
- journal article
- research article
- Published by Springer Nature in Solar Physics
- Vol. 41 (2) , 397-414
- https://doi.org/10.1007/bf00154077
Abstract
No abstract availableKeywords
This publication has 17 references indexed in Scilit:
- A clue to the trigger for both the type III solar radioburst and the solar flareSolar Physics, 1974
- Ionization equilibrium in soft X-ray-emitting solar flaresSolar Physics, 1974
- Spatial distribution of soft X-ray and EUV emission associated with a chromospheric flare of importance 1B on August 2, 1972Solar Physics, 1974
- On practical representation of magnetic fieldSolar Physics, 1972
- The relations between chromospheric features and photospheric magnetic fieldsSolar Physics, 1972
- Soft X-ray and microwave observations of hot regions in solar flaresSolar Physics, 1972
- Impulsive Hard X-Ray and Ultraviolet Emission during Solar FlaresThe Astrophysical Journal, 1971
- Comparison of Solar X-Ray Line Emission with Microwave Emission during FlaresThe Astrophysical Journal, 1968
- On arch-filament systems in spotgroupsSolar Physics, 1967
- A phenomenological model for disparitions brusques followed by flarelike chromospheric brighteningsSolar Physics, 1967