Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
Department of AOSS, University of Michigan, 2455 Hayward Street, Ann Arbor, MI 48109-2143, USA - University of Michigan, 1424 Space Research Building 2455 Hayward Street, Ann Arbor, MI 48109-2143, USA for Space Environment Modeling, University of Michigan, Ann Arbor, 2455 Hayward, Ann Arbor, MI 48109-2143, USA Department of AOSS University of Michigan, 2455 Hayward Street, Ann Arbor, MI 48109-2143 for Space Environment Modeling, University of Michigan, 2455 Hayward, Ann Arbor, MI 48109, USA for Astronomy, University of Hawai'i at Manoa, Honolulu, Hawaii, USA
Institute for Astronomy, University of Hawaii at Manoa, Honolulu, HI, USA;
Institute for Astronomy, University of Hawaii, Honolulu, HI, USA;
Institute for Astronomy, Univ of Hawaii, Honolulu, HI, USA;
University of Hawaii, Institute for Astronomy, Honolulu, HI 96822, USA
Institute for Astronomy University of Hawaii, 2680 Woodlawn Drive, Honolulu, HI 96822-1897, USA
Institute for Astronomy, University of Hawaii at Manoa, 2680 Woodlawn Drive, Honolulu, HI 96822, USA
Institute for Astronomy, 2680 Woodlawn Drive, Honolulu, HI 96822
IFA, University of Hawaii
IFA, University of Hawaii, 2680 Woodlawn Drive, Honolulu, HI 96822, USA
Institute for Astronomy, University of Hawaii, 2680 Woodlawn Drive, Honolulu, HI 96822, USA for Astronomy, University of Hawaii at Manoa, Honolulu, HI 96822.
Center for Space Environment Modeling, University of Michigan at Ann Arbor, 2455 Hayward Street, Ann Arbor, MI 48109-2143 University of Michigan
University of Hawaii, Institute for Astronomy, Honolulu, USA
Institute for Astronomy - University of Hawaii, 2680 Woodlawn Dr., Honolulu, HI 9682
2D Numerical MHD Models of Solar Explosive Events
3D MHD Simulation of CME Propagation from Solar Corona to 1 AU
3D MHD Simulations of Flux Rope Driven CMEs
4D Model for MHD Wave Turbulence in the Solar Corona and Solar Wind
4D Model for the Solar Environment
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