Anisotropy observation of diffuse ions (greater than 30 keV/e) upstream of the earth's bow shock

Physics

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Anisotropy, Bow Waves, Earth Atmosphere, Ionic Diffusion, Shock Waves, Solar Wind, Energy Spectra, Protons, Space Density

Scientific paper

A detailed study was performed of the temporal development of field-aligned anisotropies and density gradient anisotropies during several diffuse ion events observed upstream of the earth's bow shock. A clear anticorrelation between the field-aligned anisotropy and the particle intensity is found; in the solar wind frame this anisotropy, which is directed away from the bow shock, decreases as the particle flux increases. Furthermore, the field-aligned anisotropy increases with increasing particle energy. In the strong scattering limit the one-dimensional diffusion-convection formalism predicts a decrease of the anisotropy with increasing energy. It is concluded that upstream escape is significant for higher energy particles and leads to the deviation from the prediction of the diffusion-convection formalism. Quantitatively, the diffusion-convection formalism predicts a field-aligned anisotropy which is larger than measured for the lowest energy particles (about 30 keV/e).

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