Published 1988 | Version v1
Journal article

Long-decay soft X-ray flares. 3

  • 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