A Relation of Optical and x-ray Emissions in Hale-Bopp
✍ Scribed by R. Schulz; A. Owens; G. P. Tozzi; J. A. Stüwe
- Book ID
- 110233081
- Publisher
- Springer Netherlands
- Year
- 1997
- Tongue
- English
- Weight
- 13 KB
- Volume
- 77
- Category
- Article
- ISSN
- 1573-0794
No coin nor oath required. For personal study only.
📜 SIMILAR VOLUMES
We evaluate the possibility that the short-lived Balmer line emission at H9 A3835 A. of the 1972, August 2 (1839 UT) solar flare is due to heating of the chromosphere by bombarding electrons. We point out some of the problems of comparing the time behavior and spatial distribution of simultaneous ha
Our observation of postperihelion Hale-Bopp on November 17-23, 1997, revealed the comet soft X-ray luminosity of (3.7 ± 1.2) × 10 24 photons s -1 in an aperture of 6 × 10 5 km and in the EUVE range of 97-165 eV. We also analyzed observations of three comets from the EUVE archive. The X-ray luminosit