An improved X-ray polarimeter is briefly described and preliminary results of the measurements carried out on the satellite 'Intercosmos-7' are presented. One flare with considerable polarization (P~> 16%) was observed on 1972 August 4. Two other flares with rather low polarization (P ~ 4 %; P/> 2 %
Simultaneous measurements of EUV and soft X-ray solar flare emission
โ Scribed by D. M. Horan; R. W. Kreplin
- Publisher
- Springer
- Year
- 1981
- Tongue
- English
- Weight
- 354 KB
- Volume
- 74
- Category
- Article
- ISSN
- 0038-0938
No coin nor oath required. For personal study only.
โฆ Synopsis
Broadband sensors aboard the Naval Research Laboratory's SOLRAD 11 satellites measured solar emission in the 0.5 to 3 ~, 1 to 8/~, 8 to 20 ~, 100 to 500/~, 500 to 800 ~, and 700 to 1030 bands between March 1976 and October 1979. Measurements of EUV and soft X-ray emission from a large number of solar flares were obtained. Although solar flare measurements in the soft X-ray bands are continuously made and used as a standard of a flare's geophysical significance, direct measurements of flare EUV emission are quite rare. We present measurements of the X-ray and EUV emission from several flares with special emphasis on the relative EUV response associated with flares in different categories determined by 1 to 8/~ soft X-ray flux. An example of a flare exhibiting an impulsive (nonthermal) phase is included. * Proceedings of the 14th ESLAB Symposium on Physics o[Solar Variations, 16-19 Semptember 1980, Scheveningen, The Netherlands.
๐ SIMILAR VOLUMES
A study is made of several ATM flares, to investigate the effect of soft X-ray heating at chromospheric levels. It is shown that the amount of energy released in Lya and Lyman continuum emissions, and their spatial and temporal behavior, in compact flares correspond to what is expected from model ca
X-ray emission from seventeen X-ray flares was analyzed to obtain electron temperatures and emission measures associated with the source region in the solar corona. The source region was assumed to be isothermal with a Maxwellian electron velocity distribution. Flares which were characterized by a