Self Inhibiting Heat-Flux I. Whistlers Quasilinear Theory
نویسنده
چکیده
Heat-transfer through weakly magnetized diffuse astrophysical plasmas excites whistlers. This leads to electron whistler resonant scattering, a reduction of the electron mean-free path, and heat-flux inhibition. However, only whistlers propagating at a finite angle to the magnetic field (off-axis) can scatter the heat-flux carrying electrons. Thus, the level of heat flux-inhibition along the magnetic field lines depends on the presence of off-axis whistlers. We obtain a solution of the Boltzmann equation with the whistler wave equation and show that if ǫthβe ≫ 10 , where ǫ is the thermal Knudsen number, and βe is the ratio of the electron pressure to the magnetic energy density, scattering of heatflux carrying electrons by off-axis whistlers, which are shown to propagate at about 65, is efficient enough to lead to heat-flux inhibition along field lines. The inhibition so obtained is proportional to (ǫthβe) .
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تاریخ انتشار 1998