Initial Results From the 3D Hybrid Heliospheric Modeling System With Pickup Protons

Details Initial Results From the 3D Hybrid Heliospheric Modeling System With Pickup Protons Initial Results From the 3D Hybrid Heliospheric Modeling System With Pickup Protons

Dec 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008agufmsh21b1611d&link_type=abstract

American Geophysical Union, Fall Meeting 2008, abstract #SH21B-1611

Physics

7837 Neutral Particles (2151), 7851 Shock Waves (4455), 7959 Models

Scientific paper

Interstellar neutral hydrogen flows into the heliosphere and becomes ionized by photoionization and by charge exchange with solar wind protons. These "pickup" protons cause a slowing and heating of the solar wind flow in the outer heliosphere. We are adding the physics of these processes to our time-dependent 3D Hybrid Heliospheric Modeling System. We plan to present initial results for the "Halloween" 2003 events, and to show comparisons with both ACE and Ulysses observations and with our previous results (without pickup protons). This work is sponsored by NASA Grant NNX08AE40G and by Carmel Research Center. Detman et al., 2006, A hybrid heliospheric modeling system: Background solar wind, J. Geophys. Res., V 111, doi:10.1029/2005JA011340

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