Published February 1973
| Version v1
Journal article
MHD acceleration in the unsteady expansion of a shock tube driver
Description
The isentropic unsteady expansion of the driver gas in a shock tube is made to pass through an MHD interaction. The interaction is tailored so as to produce a new isentropic unsteady expansion downstream with greater energy than the original, which will drive a new shock of greater but constant velocity. Illustrative examples are calculated.
Additional details
Identifiers
- DOI
- 10.1071/ph730061;
Publishing Information
- Journal Title
- Australian Journal of Physics
- Journal Volume
- 26
- Journal Issue
- 1
- Series
- Aust. J. Phys.
- Journal Page Range
- 61-78
- ISSN
- 0004-9506
INIS
- Country of Publication
- Australia
- Country of Input or Organization
- Australia
- INIS RN
- 4072360
- Subject category
- S75: CONDENSED MATTER PHYSICS, SUPERCONDUCTIVITY AND SUPERFLUIDITY;
- Descriptors DEI
- ACCELERATION; ARGON; CROSSED FIELDS; ELECTRIC FIELDS; ELECTRODES; ENTROPY; EXPANSION; IONIZED GASES; MAGNETIC FIELDS; MAGNETOHYDRODYNAMICS; SHOCK TUBES; SHOCK WAVES; VELOCITY; WAVE PROPAGATION
- Descriptors DEC
- ELEMENTS; FLUID MECHANICS; FLUIDS; GASES; HYDRODYNAMICS; MECHANICS; NONMETALS; PHYSICAL PROPERTIES; RARE GASES; THERMODYNAMIC PROPERTIES
Optional Information
- Notes
- Updated automatically by Metadata and Full-Text Enrichment Agent