Measurements of thermal electron heating and the formation of a non-Maxwellian energy distribution due to ion acoustic turbulence
Thesis/Dissertation
·
OSTI ID:5801750
The interaction of intense microwaves with an inhomogeneous plasma is studied in the U.C. Davis Prometheus III Device. P-polarized microwaves (f = 1.2 GHz, P/sub 0/ less than or equal to 5 KW) are incident on an essentially collisionless plasma with a long scale length in an oversized waveguide. For modest powers, large amplitude ion acoustic turbulence is observed on the underdense plasma shelf due to a combination of the parametric decay and the electron drift instabilities. Suprathermal and thermal electrons are strongly heated in this region with the thermal heating due to scattering with the ion turbulence. Since the cross section for interaction decreases rapidly as the electron energy increases, the low energy electrons are preferentially heated. The electron distribution function is measured and agrees with theory; the power absorption is reduced by up to a factor of two compared to a Maxwellian distribution. After the microwaves have been measured to decay, the electron distribution function is seen to relax back to its initial Maxwellian form. This occurs, as theory predicts, roughly on the electron-electron collision time scale.
- Research Organization:
- California Univ., Davis (USA)
- OSTI ID:
- 5801750
- Country of Publication:
- United States
- Language:
- English
Similar Records
Experimental observation of microwave absorption and electron heating due to the two plasmon decay instability and resonance absorption
The effects of the ion acoustic decay instability on microwave-plasma interactions
Electron heating due to resonant absorption
Thesis/Dissertation
·
Wed Dec 31 23:00:00 EST 1980
·
OSTI ID:6692566
The effects of the ion acoustic decay instability on microwave-plasma interactions
Journal Article
·
Tue Jan 31 23:00:00 EST 1989
· Journal of Geophysical Research; (USA)
·
OSTI ID:5839372
Electron heating due to resonant absorption
Conference
·
Mon Dec 31 23:00:00 EST 1979
·
OSTI ID:5516482