Published November 1984 | Version v1
Journal article Metadata-only

Interaction of cosmic rays with anisotropic turbulence of a magnetic field

Creators

  • 1. AN Ukrainskoj SSR, Kiev. Inst. Geofiziki

Description

Process of propagation of cosmic rays (CR) in a turbulent statistically anisotropic plasma of solar wind is considered on the base of the collisionless kinetic equation. It is shown that effective mechanism of particle acceleration occurs in magnetized cosmic plasma with reflectory non-invariant turbulence of magnetic field. The mechanism of particle acceleration is connected with the presence of mean electric field of fluctuations directed along regular magnetic field

Additional details

Additional titles

Original title (Russian)
Взаимодействие космических лучей с анизотропной турбулентностью магнитного поля

Publishing Information

Journal Title
Izv. Akad. Nauk SSSR, Ser. Fiz.
Journal Volume
48
Journal Issue
11
Series
Izv. Akad. Nauk SSSR, Ser. Fiz.
Journal Page Range
2120-2122
ISSN
0367-6765

Conference

Title
All-union conference on cosmic rays.
Dates
Jul 1984.
Place
Yakutsk (USSR).

INIS

Country of Publication
Russian Federation
Country of Input or Organization
USSR
INIS RN
16056085
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Resource subtype / Literary indicator
Conference
Descriptors DEI
ACCELERATION; ANISOTROPY; COSMIC RADIATION; COSMIC RAY PROPAGATION; INTERPLANETARY MAGNETIC FIELDS; KINETIC EQUATIONS; MAGNETOHYDRODYNAMICS; SOLAR WIND; TURBULENCE
Descriptors DEC
EQUATIONS; FLUID MECHANICS; HYDRODYNAMICS; IONIZING RADIATIONS; MAGNETIC FIELDS; MECHANICS; RADIATIONS; SOLAR ACTIVITY; STELLAR ACTIVITY; STELLAR WINDS

Optional Information

Notes
For English translation see the journal Bulletin of the Academy of Sciences of the USSR, Physical Series (USA).