TY - JOUR
T1 - Electron Cooling in a Magnetically Expanding Plasma
AU - Little, J. M.
AU - Choueiri, E. Y.
N1 - Publisher Copyright:
© 2016 American Physical Society.
PY - 2016/11/23
Y1 - 2016/11/23
N2 - Electron cooling in a magnetically expanding plasma, which is a fundamental process for plasma flow and detachment in magnetic nozzles, is experimentally investigated using a radio frequency plasma source and magnetic nozzle (MN). Probe measurements of the plasma density, potential, and electron temperature along the center line of the MN indicate that the expansion follows a polytropic law with exponent γe=1.15±0.03. This value contradicts isothermal electron expansion, γe=1, which is commonly assumed in MN models. The axial variation of the measured quantities can be described by a simple quasi-1D fluid model with classical electron thermal conduction, for which it has been previously shown that a value of γe≈1.19 is expected in the weakly collisional limit. A new criterion, derived from the model, ensures efficient ion acceleration when a critical value for the ratio of convected to conducted power is exceeded.
AB - Electron cooling in a magnetically expanding plasma, which is a fundamental process for plasma flow and detachment in magnetic nozzles, is experimentally investigated using a radio frequency plasma source and magnetic nozzle (MN). Probe measurements of the plasma density, potential, and electron temperature along the center line of the MN indicate that the expansion follows a polytropic law with exponent γe=1.15±0.03. This value contradicts isothermal electron expansion, γe=1, which is commonly assumed in MN models. The axial variation of the measured quantities can be described by a simple quasi-1D fluid model with classical electron thermal conduction, for which it has been previously shown that a value of γe≈1.19 is expected in the weakly collisional limit. A new criterion, derived from the model, ensures efficient ion acceleration when a critical value for the ratio of convected to conducted power is exceeded.
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U2 - 10.1103/PhysRevLett.117.225003
DO - 10.1103/PhysRevLett.117.225003
M3 - Article
C2 - 27925736
AN - SCOPUS:84999808938
SN - 0031-9007
VL - 117
JO - Physical review letters
JF - Physical review letters
IS - 22
M1 - 225003
ER -