Autor: |
Quon, B. H., Dandl, R. A., DiVergilio, W., Guest, G. E., Lao, L. L., Lazar, N. H., Samec, T. K., Wuerker, R. F. |
Předmět: |
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Zdroj: |
Physics of Fluids (00319171); May85, Vol. 28 Issue 5, p1503, 13p |
Abstrakt: |
High-beta, hot-electron plasmas have been produced by electron-cyclotron heating in the SM-1 axisymmetric mirror using closely-spaced multiple frequencies. The relativistic electrons produce annular distributions (ELMO rings) with as much as ten times more stored energy than with single-frequency heating. While larger frequency separations (Δf/f∼0.1) provide some control of the ring size, the dominant effects are associated with an improvement in heating efficiency which persists to very small frequency separations (Δf/f∼10-3). Details of the reconstruction of the ring distribution (both in steady state and during build-up), the influence of multiple frequency heating on fluctuations, axial electron losses, and a scaling of these effects with power are presented. [ABSTRACT FROM AUTHOR] |
Databáze: |
Complementary Index |
Externí odkaz: |
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