Hydromagnetic structure of interplanetary stream from powerful flare of August 4, 1972
Creators
- 1. AN SSSR, Moscow. Inst. Zemnogo Magnetizma, Ionosfery i Rasprostraneniya Radiovoln
Description
The magnetic measurements of the interplanetary flux from the solar flare on the 2.8.1972 carried out on the ''Prognoz-2'' and ''Prognoz'' satellites have been analyzed. A characteristic structure of the flux has been revealed: the head shock layer, ''magnetic'' region and the region of the flare plasma. The head shock layer has been detected according to the magnetic field jump from approximately 30 to approximately 130 Oe on the ''Prognoz'' at 20 hr 53 min +- 1 min of IT. The ''magnetic'' region has been detected on the ''Prognoz''-2 in the periods from 23 hr 08 min +- 1 min to 3 hr 12 min +-1 min of IT and from 4 hr 41 min and further along the region. In the range of 3 hr 12 min- 4 hr 41 min of IT the ''Prognoz-2'' crossed twice the front of the flare plasma region
Additional details
Additional titles
- Original title (Russian)
- Гидромагнитная структура межпланетного потока от мощной вспышки 4.8 1972 г
Publishing Information
- Journal Title
- Geomagn. Aeron.
- Journal Volume
- 16
- Journal Issue
- 6
- Series
- Geomagn. Aeron.
- Journal Page Range
- 970-975
INIS
- Country of Publication
- USSR
- Country of Input or Organization
- USSR
- INIS RN
- 9396849
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- INTERPLANETARY MAGNETIC FIELDS; INTERPLANETARY SPACE; MAGNETIC FLUX; PLASMA; PROGNOZ SATELLITES; SHOCK WAVES; SOLAR FLARES
- Descriptors DEC
- MAGNETIC FIELDS; SATELLITES; SOLAR ACTIVITY; SPACE
Optional Information
- Notes
- For English translation see the journal Geomagn. Aeron.