Presented by: Dave McComas Southwest Research Institute San Antonio, Texas on Behalf of the IBEX Science Team. PI: Dave McComas
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Southwest Research InstituteSan Antonio, Texas
on Behalf of the IBEX Science Team
PI: Dave McComas
Co-Is: Peter Bochsler Maciej Bzowski Hans Fahr Horst Fichtner Priscilla Frisch Herb Funsten Steve Fuselier Mike Gruntman Vlad Izmodenov Paul Knappenberger Marty Lee Stefano Livi Don Mitchell Eberhard Möbius Tom Moore Ed Roelof Nathan Schwadron Peter Wurz Gary Zank
Collaborators: Frederic Allegrini Mike Collier George Gloeckler David Hollenbach Dan Reisenfeld Martin Wieser Manfred Witte
Image courtesy of L. Huff/P. Frisch
Predicted ENA distributions near HSp nose for strong (black) and weak (green) TS [Gruntman et al., 2001]. ENAs >1 keV are accelerated inner heliosheath protons based on projecting observed distributions beyond TS.
Extremes of differential ENA fluxes from 0.3-0.6 keV predicted for a strong gas-dynamical TS (top) and a TS weakened by a large pickup ion pressure (bottom) [Gruntman et al., 2001].
IBEX-HiIntegration of IBEX Payload
Various Institutions: Science Team
Adler Planetarium: E/PO
LMATC: IBEX Lo
LANL: IBEX Hi
ATK: Solid Rocket Motor
OSC: MOCLead Institutional Responsibilities
Interstellar Boundary Explorer – IBEX
It is time for IBEX’s breakthrough mission of exploration and discovery beyond the planets!
Imaging the Edge of Our Solar System and Beyond