Physics – Plasma Physics
Scientific paper
Dec 2010
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010agufmsm51b1806k&link_type=abstract
American Geophysical Union, Fall Meeting 2010, abstract #SM51B-1806
Physics
Plasma Physics
[7845] Space Plasma Physics / Particle Acceleration, [7851] Space Plasma Physics / Shock Waves, [7867] Space Plasma Physics / Wave/Particle Interactions
Scientific paper
We analyze simultaneous multipoint observations of several diffuse ion events observed upstream of Earth’s quasi-parallel bow shock. Each upstream ion event is treated individually in order to determine the similarities and differences of the physical process of energetic ion scattering as a function of interplanetary magnetic field and plasma conditions. The data were provided by the CIS and the FGM instruments onboard Cluster SC1 and SC3 at times of large (i.e., 1-1.5 Re) interspacecraft separation distance. The diffuse ion partial density gradients were determined at different distances from the quasi-parallel bow shock along the magnetic field lines and the e-folding distances (and the diffusion coefficients) were calculated. Our results show that during times of quiet interplanetary magnetic field (IMF) conditions (i.e., when the IMF presents a substantial directional stability) the field aligned beam (FAB) intensity is high which has an impact on the diffuse ion scattering process. We demonstrate that high intensity FAB generated waves are convected deep in the foreshock region and scatter especially the lower energy (i.e., 10-18 keV) diffuse ions efficiently which results in unusually low e-folding distance (and diffusion coefficient). These new results reveal the complexity of the energetic ion scattering process in the foreschock region and help to understand the process of ion acceleration at Earth’s bow shock.
Kis A.
Klecker Berndt
Lemperger I.
Lucek Elisabeth A.
Reme Henri
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