Long-decay soft X-ray flares. 3
Creators
- 1. Slovenska Akademia Vied, Skalnate Pleso (Czechoslovakia). Astronomicky Ustav
- 2. AN SSSR, Crimea. Krymskaya Astrofizicheskaya Observatoriya
Description
Twenty cases of LDE flares were analyzed with regard to the development of their morphology in the H-alpha line. It was found that LDE flares may be classed as: a) ''one-ribbon'' flares, in which the long-lasting H-alpha emission loops are arranged along the axis of the filament, or along its channel; b) two-ribbon flares, and c) three-ribbon flares which are a combination of the first two types. The system of central loops (SCL) of the three-ribbon flares is situated along the axis of the interribbon space and is a dynamic formation which cannot be mistaken for flare-loop tops. The repeated energy release which occurs in the lower part of the interribbon space indicates that the accumulation of energy, required for the formation of SCL and also for the trigger mechanism of the flare, is concentrated in the low structures (lower than 3.5-7.0 thousand kilometres). (author). 5 figs., 3 tabs., 46 refs
Additional details
Additional titles
- Subtitle (English)
- H-alpha activity in the interribbon space of the LDE flares
Publishing Information
- Journal Title
- Bulletin of the Astronomical Institutes of Czechoslovakia
- Journal Volume
- 39
- Journal Issue
- 2
- Series
- Bull. Astron. Inst. Czech.
- Journal Page Range
- 97-105
- ISSN
- 0004-6248
- CODEN
- BAICA
INIS
- Country of Publication
- Czech Republic
- Country of Input or Organization
- Serbia and Montenegro
- INIS RN
- 20017455
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Is Lead record
- Yes
- Descriptors DEI
- BALMER LINES; IMAGES; SOLAR FLARES; SOLAR X-RAY BURSTS; VELOCITY
- Descriptors DEC
- SOLAR ACTIVITY; STELLAR ACTIVITY; STELLAR FLARES