Characteristics of the linear polarization observed in the 16 May 1991 solar flare
β Scribed by N. M. Firstova; A. V. Boulatov
- Book ID
- 104641197
- Publisher
- Springer
- Year
- 1996
- Tongue
- English
- Weight
- 873 KB
- Volume
- 164
- Category
- Article
- ISSN
- 0038-0938
No coin nor oath required. For personal study only.
π SIMILAR VOLUMES
## Abstract Large solar telescopes built at places with a quite excellent seeing, equipped with a sophisticated optics and control system are too expensive and unique to be used currently in hunting of sudden and shortβlasting activity events, e.g. flares and eruptive prominences. For a systematic
It is known that mode coupling may occur in quasi-transverse magnetic field regions of the solar corona, which produces linear polarization at microwave frequencies. A microwave polarimeter measuring all 4 Stokes parameters at 8.918 GHz simultaneously at three different highfrequency bandwidths (40