Published 1984 | Version v1
Journal article

Physical mechanisms of subcritical collisionless shock-wave formation

Creators

  • 1. Iowa Univ., Iowa City

Description

The key process in shock wave formation is related to energy dissipation, and the nature of the operative dissipation mechanism determines the basic character of the resulting shock. In the case of collisionless plasmas, the primary problem consists in the identification of the processes which can provide the necessary dissipation in relatively short spatial scale lengths. The present investigation is concerned with the various collisionless dissipation mechanisms which can operate in weak shocks, taking into account the effects of different mechanisms on shock structure. Particular attention is given to a restricted class of quasi-perpendicular low beta low Mach number shocks. Such shocks are traditionally called laminar shocks. Resistive shocks are considered along with subcritical shocks observed with the aid of the ISEE spacecraft. 39 references

Additional details

Publishing Information

Journal Title
Adv. Space Res.
Journal Volume
4
Series
Adv. Space Res.
Journal Page Range
245-253
ISSN
0273-1177
CODEN
ASRSD

Conference

Title
25. plenary session of COSPAR.
Dates
25 Jun - 7 Jul 1984.
Place
Graz (Austria).

INIS

Country of Publication
United States
Country of Input or Organization
United States
INIS RN
17000550
Subject category
S70: PLASMA PHYSICS AND FUSION TECHNOLOGY;
Resource subtype / Literary indicator
Conference
Descriptors DEI
COLLISIONLESS PLASMA; ENERGY LOSSES; MACH NUMBER; PLASMA HEATING; SHOCK WAVES; SOLAR WIND; WAVE PROPAGATION
Descriptors DEC
HEATING; PLASMA; SOLAR ACTIVITY; STELLAR ACTIVITY; STELLAR WINDS; VELOCITY

Optional Information

Secondary number(s)
CONF-8406167--.