Published March 1989
| Version v1
Journal article
Three-dimensional configuration and damping effect of flare coronal transients
Creators
- 1. AN SSSR, Moscow (USSR). Inst. Zemnogo Magnetizma, Ionosfery i Rasprostraneniya Radiovoln
Description
Inverse problem of searching for three - dimensional configuration of coronal mass outburst (CMO) in the class of flattened spheroids was solved on the basis of solving primal problem of projecting CMO of the given configuration on celestial plane, using experimental data of white light coronograph. It was obtained that CMO, as interplanetary shock waves, were oblate with ∼ 1.25 ratio of axes to the plane of great circle, passing through the flare, parallel to magnetic axis of the nearest bipolar group
Additional details
Additional titles
- Original title (Russian)
- Трехмерная конфигурация и эффекты угасания вспышечных корональных транзиентов
Publishing Information
- Journal Title
- Geomagnetizm i Aeronomiya
- Journal Volume
- 29
- Journal Issue
- 2
- Series
- Geomagn. Aeron.
- Journal Page Range
- 216-221
- ISSN
- 0016-7940
- CODEN
- GEAEA
INIS
- Country of Publication
- Russian Federation
- Country of Input or Organization
- USSR
- INIS RN
- 21000631
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Resource subtype / Literary indicator
- Numerical Data
- Descriptors DEI
- COORDINATES; DISTURBANCES; EXPERIMENTAL DATA; PLASMA JETS; SHOCK WAVES; SOLAR CORONA; SOLAR FLARES; SOLAR RADIO BURSTS; SPATIAL DISTRIBUTION; SPHEROIDS; THREE-DIMENSIONAL CALCULATIONS; TIME DEPENDENCE
- Descriptors DEC
- ATMOSPHERES; DATA; DISTRIBUTION; ELECTROMAGNETIC RADIATION; INFORMATION; NUMERICAL DATA; RADIATIONS; RADIOWAVE RADIATION; SOLAR ACTIVITY; SOLAR ATMOSPHERE; STELLAR ACTIVITY; STELLAR ATMOSPHERES; STELLAR CORONAE; STELLAR FLARES