Simulations of an IBEX Ribbon Model

Details Simulations of an IBEX Ribbon Model Simulations of an IBEX Ribbon Model

Dec 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010agufmsh21b1813h&link_type=abstract

American Geophysical Union, Fall Meeting 2010, abstract #SH21B-1813

Physics

[2126] Interplanetary Physics / Heliosphere/Interstellar Medium Interactions, [2144] Interplanetary Physics / Interstellar Gas, [2151] Interplanetary Physics / Neutral Particles

Scientific paper

The unexpected "ribbon" of enhanced ENA flux observed in the IBEX all-sky maps has generated much speculation about what could be generating this effect. Here we present our results of modeling a mechanism based on secondary ENAs created outside the heliopause from pick-up ions gyrating around the interstellar magnetic field. We will address how parameters in the solar wind and local interstellar medium affect the shape, location and intensity of the simulated ribbon.

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