Physics
Scientific paper
Dec 2004
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004agufmsh34a..06s&link_type=abstract
American Geophysical Union, Fall Meeting 2004, abstract #SH34A-06
Physics
7851 Shock Waves, 7867 Wave/Particle Interactions, 2154 Planetary Bow Shocks
Scientific paper
We investigate quasi-linear theory of ion acceleration at Earth's quasi-parallel bow shock using Cluster magnetic field and particle measurements during an upstream diffuse ion event (February 18, 2003). Simultaneous magnetic field power spectra far upstream obtained by ACE show that the interplanetary fluctution level in the region of resonant frequencies was orders of magneitude lower than near the bow shock, so that the fluctuations near the bow shock were excited by backstreaming ions. In particular, we determine the energetic ion spatial profile, the dependence of the upstream ion scalelength upon energy, the behavior of the energetic ion anisotropy upstream and downstream of the shock, the spatial scale lenghts of the low frequency upstream waves that resonate with them, and the dependence of the integrated wave energy density upon the ion energy density at the shock.
Bosqued Jean Michel
Kis A.
Kistler Lynn M.
Klecker Berndt
Kucharek Harald
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