Published April 1984 | Version v1
Report Restricted

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

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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.