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Effects of strong magnetic field on flow characteristics of MHD seawater propulsion system

Conference ·
OSTI ID:5256281
 [1];  [2]
  1. Argonne National Lab., IL (USA)
  2. Office of Naval Research, Arlington, VA (USA)
A three-dimensional MHD fluid flow computer model has been developed and applied to study the concept of MHD seawater propulsion. The effects of strong magnetic fields on the current and electrical fields inside the MHD duct and their interaction with the flow fields, particularly those in the boundary layers have been investigated. Results of parametric studies for variables influencing the flow field characteristics and the overall performance of the propulsion systems are discussed. Such parameters include the magnetic field, and electrical loading of the MHD thruster. The results of the calculations performed indicate the sensitivity of the thrust performance to the load factor. The distribution of J{sub y} current density in the Hartmann layers of the insulating sidewalls caused the flattening of the velocity particles of sidewall boundary layers relative to the velocity profiles over the electrode walls. These nonuniformities in the flow field give rise to nonuniform distribution of the skin friction, along the walls of the thrusters where higher values are predicted over the sidewalls relative to those over the electrode walls. The extent of such nonuniformities of the flow fields and the corresponding differences in the skin friction between the sidewalls and electrode walls diminishes as the magnetic field or load factor decreases. Careful considerations should be given to the calculation and magnitude of frictional losses because of their impact on the efficiency of MHD thrusters. 10 refs., 8 figs., 2 tabs.
Research Organization:
Argonne National Lab., IL (USA)
Sponsoring Organization:
DOD
DOE Contract Number:
W-31109-ENG-38
OSTI ID:
5256281
Report Number(s):
CONF-891226-2; ON: DE90004877; CNN: NOOO14-89-F-0064
Country of Publication:
United States
Language:
English