Published August 1985 | Version v1
Report Metadata-only

Dynamics of the penetration boundaries of solar protons during a strong magnetic storm

Creators

  • 1. Moscow State Univ., USSR

Description

The variations in the equatorial penetration boundary of solar protons with E sub p = 0.9 to 8.0 MeV during a strong magnetic storm of April 3 to 5, were analyzed. The dynamics of this boundary are compared with the dynamics of the outer trapping boundary of electrons with E sub e = - 0.3 to 0.6 MeV. The solar proton penetration and the structure of the real magnetic field are studied. The unique data on the thin structure of development of a magnetospheric substorm were obtained for the first time

Additional details

Publishing Information

Imprint Title
Ninteenth International Cosmic Ray Conference. SH sessions, volume 5
Journal Page Range
vp.
Report number
N--85-34991

Conference

Title
19. international cosmic ray conference.
Dates
11-23 Aug 1985.
Place
La Jolla, CA (USA).

INIS

Country of Publication
United States
Country of Input or Organization
United States
INIS RN
19053482
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY; S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Resource subtype / Literary indicator
Conference, Numerical Data
Descriptors DEI
BOUNDARY CONDITIONS; COSMIC ELECTRONS; EARTH MAGNETOSPHERE; EXPERIMENTAL DATA; MAGNETIC STORMS; SOLAR ATMOSPHERE; SOLAR PROTONS; STRUCTURAL MODELS
Descriptors DEC
ATMOSPHERES; BARYONS; CATIONS; CHARGED PARTICLES; COSMIC RADIATION; DATA; EARTH ATMOSPHERE; ELECTRONS; ELEMENTARY PARTICLES; FERMIONS; HADRONS; HYDROGEN IONS; HYDROGEN IONS 1 PLUS; INFORMATION; IONIZING RADIATIONS; IONS; LEPTONS; NUCLEONS; NUMERICAL DATA; PROTONS; RADIATIONS; SECONDARY COSMIC RADIATION; SOLAR PARTICLES; SOLAR RADIATION; STELLAR ATMOSPHERES; STELLAR RADIATION