aboard the SMM satellite imaged extensive coronal structures after occurrences of two-ribbon flares. The archlike structures extended along the neutral line of the longitudinal magnetic field to altitudes of 1 x 105 to 2 • 105 km. The first arch observed by HXIS on 6-7 November appeared after the f
✦ LIBER ✦
X-ray observations of limb flare loops and post-flare coronal arch
✍ Scribed by Zdenék Švestka; Kermit L. Smith; Keith T. Strong
- Publisher
- Springer
- Year
- 1992
- Tongue
- English
- Weight
- 374 KB
- Volume
- 139
- Category
- Article
- ISSN
- 0038-0938
No coin nor oath required. For personal study only.
✦ Synopsis
We present observations of another post-flare arch following an eruptive flare, detected in X-ray lines above the western solar limb on 2 May 1985.
📜 SIMILAR VOLUMES
Images of post-flare coronal structures
✍
Zdeněk Švestka; Paul Hick
📂
Article
📅
1986
🏛
Springer
🌐
English
⚖ 196 KB
Hydrodynamics of coronal loops: A compar
✍
E. Antonucci; M.A. Dodero; G. Peres; S. Serio
📂
Article
📅
1986
🏛
Elsevier Science
🌐
English
⚖ 383 KB
Structure and evolution of post-flare lo
✍
B Schmieder; P Heinzel; J.E Wiik; J Lemen; E Hiei
📂
Article
📅
1996
🏛
Elsevier Science
🌐
English
⚖ 276 KB
X-ray and gamma-ray observations of a wh
✍
H.S. Hudson
📂
Article
📅
1981
🏛
Elsevier Science
🌐
English
⚖ 272 KB
Estimation of equivalent flaring loop ge
✍
J. Sylwester; B. Sylwester; J. Jakimiec; H.A. Garcia; S. Serio; F. Reale
📂
Article
📅
1993
🏛
Elsevier Science
🌐
English
⚖ 400 KB
X-ray observations of stellar coronae an
✍
Robert A. Stern
📂
Article
📅
1987
🏛
Springer
🌐
English
⚖ 198 KB
It is now more than ten years since the first x-ray emitting stellar corona was discovered (Catura, Acton, and Johnson 1975). Since then, rapid progress has been made in cataloging the incidence and range of stellar x-ray emission, most notably with the Einstein Observatory (see, eg., reviews by Ste