Physical mechanisms of subcritical collisionless shock-wave formation
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--.