A comparison of Hα and soft X-ray characteristics of spotless and spot group flares
✍ Scribed by V. Ruždjak; B. Vršnak; A. Schroll; R. Brajša
- Book ID
- 104642657
- Publisher
- Springer
- Year
- 1989
- Tongue
- English
- Weight
- 396 KB
- Volume
- 123
- Category
- Article
- ISSN
- 0038-0938
No coin nor oath required. For personal study only.
✦ Synopsis
A comparative analysis of spotless and spot group flares recorded at Hvar and Kanzelh6he Observatories during the 21st cycle of solar activity is presented. The rate of occurrence of two-ribbon flares was found to be significantly higher for the spotless flares. In comparison with spot group flares of corresponding Hot importance, the soft X-ray peak values have been systematically lower for the spotless flares. The highest peak values and the energy released in soft X-rays was found for flares with a He ribbon protruding over a major spot umbra. It was found that the effective plasma temperatures in spotless flares have been considerably lower than the temperatures in spot group flares.
📜 SIMILAR VOLUMES
Hot regions in solar flares produce X-radiation and microwaves by thermal processes. Recent X-ray data make it possible to specify the temperature and emission measure of the soft X-ray source, by using, for instance, a combination of the 1-8 A (peak response at about 2 keV) and the 0.5-3 ]k (peak r