๐”– Bobbio Scriptorium
โœฆ   LIBER   โœฆ

Active region mass motions observed in soft X-ray lines

โœ Scribed by J.L.R. Saba; K.T. Strong

Publisher
Elsevier Science
Year
1991
Tongue
English
Weight
877 KB
Volume
11
Category
Article
ISSN
0273-1177

No coin nor oath required. For personal study only.

๐Ÿ“œ SIMILAR VOLUMES

Preflare characteristics of active regio
Preflare characteristics of active regions observed in soft X-rays
โœ S. W. Kahler ๐Ÿ“‚ Article ๐Ÿ“… 1979 ๐Ÿ› Springer ๐ŸŒ English โš– 699 KB

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

Soft X-ray and microwave observations of
Soft X-ray and microwave observations of hot regions in solar flares
โœ H. S. Hudson; K. Ohki ๐Ÿ“‚ Article ๐Ÿ“… 1972 ๐Ÿ› Springer ๐ŸŒ English โš– 696 KB

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

The interpretation of simultaneous soft
The interpretation of simultaneous soft X-ray spectroscopic and imaging observations of an active region
โœ J. M. Davis; M. Gerassimenko; A. S. Krieger; G. S. Vaiana ๐Ÿ“‚ Article ๐Ÿ“… 1975 ๐Ÿ› Springer ๐ŸŒ English โš– 883 KB

Simultaneous soft X-ray spectroscopic and broad band imaging observations of an active region have been analyzed together to determine the parameters which describe the coronal plasma. From the spectroscopic data, models of temperature-emission measure-elemental abundance have been constructed which