Published October 1987
| Version v1
Journal article
Geomagnetic indication of solar flares with γ-line emission and search fo solar neutrons
Description
The problem of the pulse component of geomagnetic effects of solar flares (ESF) which is observed close to the point of local half-day synchronously with the burst of gamma-lines 22.2 MeV is studied. The duration of pulse component is 30-100 s. The results of research prove that pulse component of ESF proves the possibility of searching solar neutrons of flare origin
Additional details
Additional titles
- Original title (Russian)
- Geomagnitnyj priznak solnechnykh vspyshek s ehmissiej γ-linij i poiski solnechnykh nejtronov
Publishing Information
- Journal Title
- Izv. Akad. Nauk SSSR, Ser. Fiz.
- Journal Volume
- 51
- Journal Issue
- 10
- Series
- Izv. Akad. Nauk SSSR, Ser. Fiz.
- Journal Page Range
- 1851-1853
- ISSN
- 0367-6765
- CODEN
- IANFA
Conference
- Title
- All-union conference on cosmic rays.
- Dates
- 23-25 Apr 1986.
- Place
- Tbilisi (USSR).
INIS
- Country of Publication
- Russian Federation
- Country of Input or Organization
- USSR
- INIS RN
- 19102522
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY; S58: GEOSCIENCES;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- GAMMA RADIATION; GEOMAGNETIC FIELD; MEV RANGE 01-10; SOLAR FLARES; SOLAR NEUTRONS; TIME DEPENDENCE
- Descriptors DEC
- BARYONS; ELECTROMAGNETIC RADIATION; ELEMENTARY PARTICLES; ENERGY RANGE; FERMIONS; HADRONS; IONIZING RADIATIONS; MAGNETIC FIELDS; MEV RANGE; NEUTRONS; NUCLEONS; RADIATIONS; SOLAR ACTIVITY; SOLAR PARTICLES; SOLAR RADIATION; STELLAR ACTIVITY; STELLAR FLARES; STELLAR RADIATION