The Absence of Flares in λ 3835 and the Heating of the Chromosphere
Abstract
Simultaneous observations of flares in Hα and a band 15 Å wide centered on 3835 Å show no change whatever in 3835 Å at the time of several flares, although the chromospheric network is easily visible. Flares are therefore transparent in this wavelength.
- Publication:
-
Solar Physics
- Pub Date:
- October 1972
- DOI:
- 10.1007/BF00165281
- Bibcode:
- 1972SoPh...26..393Z
- Keywords:
-
- Convection;
- Flare;
- Heat Input;
- Simultaneous Observation;
- Test Heat