TY - JOUR
T1 - Obliquely Propagating Unstable Whistler Waves
T2 - A Computer Simulation
AU - Cuperman, S.
AU - Sternlieb, A.
N1 - Funding Information:
Many thanks are due to W. Bernstein and L. R. Lyons for reading the manuscript critically. Useful discussions with Y. Salu are also acknowledged. The authors are thankful to T. B. Gray and Wilbur M. L. Spangler for computer advice. Acknowledgement is made to the National Center for Atmospheric Research, which is sponsored by the National Science Foundation, for the computer time used in this research.
PY - 1974/4
Y1 - 1974/4
N2 - Obliquely propagating unstable electron cyclotron electromagnetic (whistler) waves have been studied with the aid of an especially designed computer simulation experiment. The plasma-wave system considered is homogeneous and infinite, and the plasma is taken to be a mixture of warm (bi-maxwellian) and cold populations. With no cold plasma, the rates of growth of the low k modes maximize for the case of parallel propagation (θ = 0°) and decrease as θ increases; for higher k modes, the opposite occurs. Changing from k space to ωspace the above results indicate that off-angle propagation tends to stabilize the low-frequency whistlers but to destabilize the higher-frequency ones. These results are consistent with linear predictions. In all cases, however, the total electromagnetic energy generated in the system decreases with increasing θ. When cold plasma is added to the system, the total generated electromagnetic energy can maximize for a non-zero propagation angle.
AB - Obliquely propagating unstable electron cyclotron electromagnetic (whistler) waves have been studied with the aid of an especially designed computer simulation experiment. The plasma-wave system considered is homogeneous and infinite, and the plasma is taken to be a mixture of warm (bi-maxwellian) and cold populations. With no cold plasma, the rates of growth of the low k modes maximize for the case of parallel propagation (θ = 0°) and decrease as θ increases; for higher k modes, the opposite occurs. Changing from k space to ωspace the above results indicate that off-angle propagation tends to stabilize the low-frequency whistlers but to destabilize the higher-frequency ones. These results are consistent with linear predictions. In all cases, however, the total electromagnetic energy generated in the system decreases with increasing θ. When cold plasma is added to the system, the total generated electromagnetic energy can maximize for a non-zero propagation angle.
UR - http://www.scopus.com/inward/record.url?scp=84976155196&partnerID=8YFLogxK
U2 - 10.1017/S0022377800024594
DO - 10.1017/S0022377800024594
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AN - SCOPUS:84976155196
SN - 0022-3778
VL - 11
SP - 175
EP - 188
JO - Journal of Plasma Physics
JF - Journal of Plasma Physics
IS - 2
ER -