Starting from the Boltzmann equation and with some reasonable assumptions, a one-dimensional transport equation of charged
energetic particles is derived by taking account of major interactions with neutral species in the upper atmosphere, including
the processes of elastic scattering, the excitation, the ionization and the secondary electron production. The transport equation
is numerically solved, for a simplified atmosphere consisting only of nitrogen molecules (N2), to obtain the variations of incident electron fluxes as a function of altitude, energy and pitch angle. The model results
can describe fairly the transport characteristics of precipitating auroral electron spectra in the polar upper atmosphere;
meanwhile the N2 ionization rates calculated from the modeled differential flux spectra also exhibit good agreements with
existing empirical models in terms of several key parameters. Taking the energy flux spectra of precipitating electrons observed
by FAST satellite flying over EISCAT site on May 15, 1997 as model inputs, the model-calculated ionization rate profile of
neutral atmosphere consists reasonably with that reconstructed from electron density measurements by the radar.
Supported by the National Natural Science Foundation of China (Grant Nos. 40404015, 40390150), the Ministry of Science and
Technology of PRC (Grant No. 2006BAB18B06) and Key Lab of Geospace Environment and Geodesy, Ministry of Education of PRC 相似文献
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