Published April 1984
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Ion reflection, gyration, and dissipation at supercritical shocks
Description
This brief review emphasizes the following points: (1) Ion reflection is the dominant ion dissipation mechanism at nearly perpendicular, supercritical shocks. (2) An increasing fraction of the ions incident on a supercritical shock is reflected as the Mach number increases. The actual fraction reflected can be predicted using the Rankine-Hugoniot conservation relations. (3) The effective temperature associated with the dispersion in velocity space associated with ion reflection accounts for a large fraction of the temperature rise observed across supercritical, quasi-perpendicular shocks
Availability note (English)
MF available from INIS under the Report Number; Available from NTIS, PC A03/MF A01 as DE84011353.
Files
Additional details
Publishing Information
- Imprint Pagination
- 35 p.
- Report number
- LA-UR--84-1391
Conference
- Title
- Chapman conference on collisionless shock waves in the heliosphere.
- Dates
- 20-24 Feb 1984.
- Place
- Napa Valley, CA (USA).
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 16001896
- Subject category
- S58: GEOSCIENCES; S75: CONDENSED MATTER PHYSICS, SUPERCONDUCTIVITY AND SUPERFLUIDITY;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- COLLISIONLESS PLASMA; ION DENSITY; PLASMASPHERE; REFLECTION; SHOCK WAVES; SUPERSONIC FLOW
- Descriptors DEC
- FLUID FLOW; PLASMA
Optional Information
- Secondary number(s)
- CONF-840256--2.