Observation of soft X-ray emission from a region near Per X-1
β Scribed by P. C. Agrawal; K. Long; G. P. Garmire
- Publisher
- Springer Netherlands
- Year
- 1974
- Tongue
- English
- Weight
- 372 KB
- Volume
- 28
- Category
- Article
- ISSN
- 0004-640X
No coin nor oath required. For personal study only.
π SIMILAR VOLUMES
Thermal bremsstrahlung from the X-ray observed plasma accounts for most of the observed 9.1 cm emission from McMath 12336, an old, spotless active region, on June 2, 1973. This implies that only a small fraction of the emission measure within the active region is in the range around 106 K and below.
X-ray images from the AS&E telescope on Skylab are used to investigate coronal conditions in solar active regions during the 20-min periods preceding the X-ray onsets of small flares. The preflare or precursor phase is defined as a phase with a characteristic length or time scale significantly diffe