Evidence for a high-energy tail associated with foreshock field-aligned beams

Details Evidence for a high-energy tail associated with foreshock field-aligned beams Evidence for a high-energy tail associated with foreshock field-aligned beams

Jan 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007jgra..11201101m&link_type=abstract

Journal of Geophysical Research, Volume 112, Issue A1, CiteID A01101

Physics

Plasma Physics

3

Magnetospheric Physics: Solar Wind/Magnetosphere Interactions, Interplanetary Physics: Solar Wind Plasma, Interplanetary Physics: Interplanetary Magnetic Fields, Interplanetary Physics: Planetary Bow Shocks, Space Plasma Physics: Particle Acceleration

Scientific paper

The reduced particle distributions of field-aligned beams observed upstream of the bow shock are examined in detail using Cluster spacecraft. We find that the reduced parallel and perpendicular distribution forms can be strongly geometry-dependent. Above a certain critical value of the angle between the local shock normal and the direction of the magnetic field, $\theta$ Bn , the reduced distributions are remarkably well fit by Maxwellians. We have not found any significant changes to the spread in energies for beams at higher values of $\theta$ Bn . When the angle $\theta$ Bn decreases, leading to smaller beam velocities, a high-energy tail in the distribution appears. When the tail is present, the bulk of the distribution remains Maxwellian. The development of the high-energy tail is well correlated with decreases in the beam speed (or equivalently $\theta$ Bn ). Moreover, detailed examination of the angular distributions indicates that particles in the tails of the distributions propagate at significant pitch angles with respect to the magnetic field (are not field-aligned, as are those within the bulk of the distribution) and that these pitch angles are energy-dependent. These new observations do not fit any production mechanism expected at the shock or result from known wave-particle interactions upstream of or within the shock layer.

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