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Cosmic Ray Anisotropy Workshop 2013

26–28 Sept 2013
Union South, UW-Madison
US/Central timezone

Session

Modeling the Lyman-alpha backscatter observed by Voyager 1 and 2 in the outer heliosphere and the structure of the heliospheric bow shock - Gary Zank, U of Alabama-Huntsville

28 Sept 2013, 10:45
Union South, UW-Madison

Union South, UW-Madison

1308 West Dayton Street, Madison, WI 53706

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  1. 15. Modeling the Lyman-alpha backscatter observed by Voyager 1 and 2 in the outer heliosphere and the structure of the heliospheric bow shock
    Dr Gary Zank (University of Alabama in Huntsville)
    28/09/2013, 10:45
    Gary Zank
    1) Observations made by ultraviolet (UV) detectors on board Pioneer 10 , Voyager 1 , and Voyager 2 can be used to analyze the distribution of neutral hydrogen throughout the heliosphere, including the interaction regions of the solar wind and local interstellar medium. We use state-of-the art three-dimensional (3D) magnetohydrodynamic (MHD) – kinetic neutral H models to simulate Lyman-alpha...
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