Computer Science
Scientific paper
Feb 1979
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979p%26ss...27..165k&link_type=abstract
Planetary and Space Science, vol. 27, Feb. 1979, p. 165-168.
Computer Science
Geomagnetic Pulsations, Ion Cyclotron Radiation, Proton Energy, Wave Packets, Earth Magnetosphere, Magnetic Field Configurations, Plasma Waves
Scientific paper
If there is a constant number of resonant particles in a magnetic flux tube, the amplitudes of excited waves reach a steady state within a time comparable to the characteristic period of nonlinear oscillations. For amplitudes in the range 10-100 milli-gamma and protons in the energy range 10-100 keV, the characteristic period is about 1-10 sec. However, observations of pearl-type geomagnetic pulsations show that the amplitudes of such pulsations increase for a much longer period; for example, pearl amplitude increases monotonically for 5-10 min up to the time of development of sideband instability. The role played by resonant-particle injection in the nonlinear evolution of pearls is emphasized.
Khabazin Iu. G.
Pokhotelov Oleg A.
Porotov A. V.
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