Asymmetries in the Solar Wind from the Sun to 10 AU: Comparisons between a 3D MHD Approach and the 3D HAFv2 Kinematic Model

Details Asymmetries in the Solar Wind from the Sun to 10 AU: Comparisons between a 3D MHD Approach and the 3D HAFv2 Kinematic Model Asymmetries in the Solar Wind from the Sun to 10 AU: Comparisons between a 3D MHD Approach and the 3D HAFv2 Kinematic Model

Sep 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005esasp.592..343i&link_type=gif

"Proceedings of the Solar Wind 11 / SOHO 16, "Connecting Sun and Heliosphere" Conference (ESA SP-592). 12 - 17 June 2005 Whistl

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