Published 1987 | Version v1
Journal article

Dm-spikes and their relation to other flare phenomena in October 14, 1983 event

  • 1. Ceskoslovenska Akademie Ved, Ondrejov. Astronomicky Ustav
  • 2. Trieste Astronomical Observatory (Italy)
  • 3. Hvar Observatory (Yugoslavia)
  • 4. Helsinki Univ. of Technology, Otaniemi (Finland). Radio Lab.
  • 5. NFRA, Radio Observatory, Dwingeloo (Netherlands)

Description

Using the observations in H-alpha and radio frequencies between 169 MHz and 37 GHz on October 14, 1983 a two-ribbon flare was analyzed. A coherent picture of the event is given using the standard topology for two-ribbon flares and describing the dm-spikes as manifestations of electron acceleration in a reconnection process (with a stationary shock wave). The drifting chains of these spikes are explained by the movement of this ''stationary'' shock wave. It is shown that the behavior with time of the number density of the spikes is in agreement with that of the 37 GHz flux and hence the same population of accelerated electrons that gave rise to the spikes also produced the 37 GHz radiation. (author). 4 figs., 14 refs

Additional details

Publishing Information

Journal Title
Bull. Astron. Inst. Czech.
Journal Volume
38
Journal Issue
1
Series
Bull. Astron. Inst. Czech.
Journal Page Range
42-46
ISSN
0004-6248
CODEN
BAICA

INIS

Country of Publication
Czech Republic
Country of Input or Organization
Serbia and Montenegro
INIS RN
19020257
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Descriptors DEI
GHZ RANGE 01-100; MHZ RANGE 100-1000; RADIATION DETECTION; SOLAR FLARES; SOLAR RADIO BURSTS
Descriptors DEC
DETECTION; ELECTROMAGNETIC RADIATION; FREQUENCY RANGE; GHZ RANGE; MHZ RANGE; RADIATIONS; RADIOWAVE RADIATION; SOLAR ACTIVITY; STELLAR ACTIVITY; STELLAR FLARES