The Effects of Magnetic Field Fluctuations on the IBEX Ribbon

Details The Effects of Magnetic Field Fluctuations on the IBEX Ribbon The Effects of Magnetic Field Fluctuations on the IBEX Ribbon

Dec 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011agufmsh23b1963k&link_type=abstract

American Geophysical Union, Fall Meeting 2011, abstract #SH23B-1963

Physics

Plasma Physics

[7524] Solar Physics, Astrophysics, And Astronomy / Magnetic Fields, [7837] Space Plasma Physics / Neutral Particles, [7863] Space Plasma Physics / Turbulence

Scientific paper

The IBEX ENA ribbon is most likely formed secondary ENAs. They are essentially (neutralized, then re-ionized and again neutralized solar wind ions reflected from the magnetic field around our Heliosphere (Heerikhuisen et al 2010). The fluctuation of the interstellar field may result in a broadening of the ribbon as well as in the formation of local structures. We carry out a time-reversed backward tracing simulation to investigate the effects caused by the field fluctuations. In particular, we shall study the possible time dependence and lifetime of the local structures introduced by the magnetic field fluctuations.

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