Details

Autor(en) / Beteiligte

• Black, D. C.
• Mayo, R. M.
• Gerwin, R. A.
• Schoenberg, K. F.
• Scheuer, J. T.
• Hoyt, R. P.
• Henins, I.

Titel

Two‐dimensional magnetic field evolution measurements and plasma flow speed estimates from the coaxial thruster experiment

Ist Teil von

• Physics of plasmas, 1994-09, Vol.1 (9), p.3115-3131

Ort / Verlag

United States

Erscheinungsjahr

1994

Quelle

Alma/SFX Local Collection

Beschreibungen/Notizen

• Local, time‐dependent magnetic field measurements have been made in the Los Alamos coaxial thruster experiment (CTX) [C. W. Barnes et al., Phys. Fluids B 2, 1871 (1990); J. C. Fernández et al., Nucl. Fusion 28, 1555 (1988)] using a 24 coil magnetic probe array (eight spatial positions, three axis probes). The CTX is a magnetized, coaxial plasma gun presently being used to investigate the viability of high pulsed power plasma thrusters for advanced electric propulsion. Previous efforts on this device have indicated that high pulsed power plasma guns are attractive candidates for advanced propulsion that employ ideal magnetohydrodynamic (MHD) plasma stream flow through self‐formed magnetic nozzles. Indirect evidence of magnetic nozzle formation was obtained from plasma gun performance and measurements of directed axial velocities up to v z ∼107 cm/s. The purpose of this work is to make direct measurement of the time evolving magnetic field topology. The intent is to both identify that applied magnetic field distortion by the highly conductive plasma is occurring, and to provide insight into the details of discharge evolution. Data from a magnetic fluctuation probe array have been used to investigate the details of applied magnetic field deformation through the reconstruction of time‐dependent flux profiles. Experimentally observed magnetic field line distortion has been compared to that predicted by a simple one‐dimensional (1‐D) model of the discharge channel. Such a comparison is utilized to estimate the axial plasma velocity in the thruster. Velocities determined in this manner are in approximate agreement with the predicted self‐field magnetosonic speed and those measured by a time‐of‐flight spectrometer.