Physics
Scientific paper
Oct 2003
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003pobeo..75..101g&link_type=abstract
Publications of the Astronomical Observatory of Belgrade (ISSN 0373-3742), No. 75, p. 101 - 104 (2003). In: Proceedings of the X
Physics
Physics Of Stars, Stellar Systems, Cyclotron Radiation
Scientific paper
The process of spontaneous excitation of quasi-perpendicular electrostatic ion-cyclotron (QPESIC) waves by an electron drift of sufficient magnitude, parallel to the external magnetic field, in a weakly ionized Maxwellian plasma containing one species of light positive ions and one species of heavy negative ones is analyzed from the standpoint of kinetic theory combined with the linear theory of perturbation. Attention is focused on the mode with the modal frequency close to the first ion-cyclotron harmonic of the negative (heavy) ions. It is found that the increase in the light-ions (not resonant to the wave analyzed) number density lowers both the maximum deviation of modal frequency from that of the ion-cyclotron harmonic and the threshold drift for spontaneous excitation of the mode.
Gajić D.
Milić B. S.
Novaković N.
No associations
LandOfFree
Kinetic theory of QPESIC waves in isothermal ionospheric plasmas with resonant negative ions does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Kinetic theory of QPESIC waves in isothermal ionospheric plasmas with resonant negative ions, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Kinetic theory of QPESIC waves in isothermal ionospheric plasmas with resonant negative ions will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1035076