Kinetic growth (decay) of whistlers in the solar corona

Details Kinetic growth (decay) of whistlers in the solar corona Kinetic growth (decay) of whistlers in the solar corona

Dec 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989kfnt....5...44m&link_type=abstract

Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 5, Nov.-Dec. 1989, p. 44-54. In Russian.

Physics

6

Electron Decay Rate, Solar Corona, Whistlers, Electron Distribution, High Energy Electrons, Solar Magnetic Field, Wave Propagation

Scientific paper

Under conditions of solar corona plasma, the local kinetic increments and integral growth coefficients of whistlers propagating at an arbitrary angle with respect to the magnetic field are calculated. The calculations are carried out using the linear adiabatic approach to the distribution function of high-energy electrons including a beam with loss-cone and temperature anisotropy. Cerenkov, normal cyclotron, and anomalous cyclotron resonances during growth and decay are considered.

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