Implications for Voyager 1 and Voyager 2 Observations From 3D Modeling and Analysis of the Interplanetary Propagation of Solar-Induced Shock Waves

Details Implications for Voyager 1 and Voyager 2 Observations From 3D Modeling and Analysis of the Interplanetary Propagation of Solar-Induced Shock Waves Implications for Voyager 1 and Voyager 2 Observations From 3D Modeling and Analysis of the Interplanetary Propagation of Solar-Induced Shock Waves

Dec 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005agufmsh51a1199i&link_type=abstract

American Geophysical Union, Fall Meeting 2005, abstract #SH51A-1199

Physics

2114 Energetic Particles (7514), 2124 Heliopause And Solar Wind Termination, 2134 Interplanetary Magnetic Fields, 2139 Interplanetary Shocks, 2164 Solar Wind Plasma

Scientific paper

We use the three dimensional HAFv2 (Hakamada-Akasofu-Fry version 2) kinematic solar wind model to study the interplanetary propagation of solar-induced shock waves from the Sun to 96 AU and over a wide range of heliolongitudes and heliolatitudes. We compare the HAFv2 model predictions at ACE (1 AU), Ulysses (5.4 AU), Voyager 2 (76 AU), and Voyager 1 (96 AU) to available data. In addition, we use the three dimensional MHD HHMS (Hybrid Heliospheric Modeling System) to further study the more detailed evolution of interplanetary magnetic field and plasma parameters to 10 AU. Statistical analyses between the data and the results from the 3D models for distances to 10 AU show high correlation coefficients. Our analyses further indicate that all of the spacecraft are observing the effects of solar events.

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