Published March 1985 | Version v1
Journal article Metadata-only

On a viscons interaction of solar wind streams

Creators

Description

Conditions of instability excitation deteriorate with heliocentric distance and the role of turbulent viscosity in evolution of SW stream fronst decreases due to geometry of stream motion. The efficiency of competing mechanism of fore-front swire grows on the contrary with the distance, so the reversal of fore-fronts and formation of shock waves must take place behind the Earth orbit

Additional details

Additional titles

Original title (Russian)
О вязком взаимодействии потоков солнечного ветра

Publishing Information

Journal Title
Astron. Zh.
Journal Volume
62
Journal Issue
2
Series
Astron. Zh.
Journal Page Range
371-376
ISSN
0004-6299
CODEN
ASZHA

INIS

Country of Publication
Russian Federation
Country of Input or Organization
USSR
INIS RN
17020534
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY; S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Descriptors DEI
HELMHOLTZ INSTABILITY; INTERPLANETARY MAGNETIC FIELDS; PLASMA; SOLAR WIND; TURBULENCE; VELOCITY; VISCOSITY
Descriptors DEC
INSTABILITY; MAGNETIC FIELDS; PLASMA INSTABILITY; PLASMA MACROINSTABILITIES; SOLAR ACTIVITY; STELLAR ACTIVITY; STELLAR WINDS

Optional Information

Notes
For English translation see the journal Soviet Astronomy (USA).