The filament-corona transition region from OSO-VI EUV observations
Abstract
The transition region between filament and corona is investigated measuring the intensity of six EUV lines above two filaments on the disk observed on September 1 and 2, 1969by OSO-VI. The comparison between these intensities and those observed on quiet regions shows that there is no difference between the two transition regions
- Publication:
-
Solar Physics
- Pub Date:
- November 1977
- DOI:
- 10.1007/BF00150883
- Bibcode:
- 1977SoPh...55..177D
- Keywords:
-
- Electron Density (Concentration);
- Far Ultraviolet Radiation;
- Solar Corona;
- Spaceborne Astronomy;
- Temperature Distribution;
- H Alpha Line;
- Oso-6;
- Solar Physics;
- Transition Layers;
- Ultraviolet Astronomy;
- Ultraviolet Spectra;
- Solar Physics