Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
CSEM - University of Michigan, 1424 Space Research Building 2455 Hayward Street, Ann Arbor, MI 48109-2143, USA of Atmospheric, Oceanic, and Space Sciences, University of Michigan, Ann Arbor, Michigan, USA
University of Hawaii, Hawaii, HI, USA;
Institute for Astronomy, University of Hawaii, Honolulu, HI, USA;
Institute for Astronomy, University of Hawaii, Honululu, HI, USA;
Institute for Astronomy, Univ of Hawaii, Honolulu, HI, USA;
CSEM University of Michigan, Space Research Building 2455 Hayward Street, Ann Arbor, MI 48109-2143, USA of Michigan, 1424 Space Research Building 2455 Hayward Street, Ann Arbor, MI 48109-2143, USA for Astronomy, University of Hawaii, 2680 Woodlawn Drive, Honolulu, HI 96822, USA
University of Michigan, 2455 Hayward St., Ann Arbor, MI 48109-2143, USA of Michigan, Space Physics Research Lab. 2455 Hayward, Ann Arbor, MI 48109, USA of Hawaii, Institute for Astronomy, Honolulu, USA
Institute for Astronomy, 2680 Woodlawn Drive, Honolulu, HI 96816, USA
Institute for Astronomy - University of Hawaii, 2680 Woodlawn Dr., Honolulu, HI 96822, USA
University of Michigan
Institute for Astronomy, University of Hawaii, Honolulu, HI 96822
Institute for Astronomy-University of Hawaii, 2680 Woodlawn Dr, Honolulu, HI 96822, USA
Center for Space Environment Modeling, University of Michigan, Ann Arbor, MI
University of Michigan, 2455 Hayward Street, Ann Arbor, MI 48109, USA for Space Environment Modeling, University of Michigan, 2455 Hayward Street, Ann Arbor, MI 48109 for Space Environment Modeling, University of Michigan, 2455 Hayward Str
3D Density Structure and LOS Observations of a Model CME
A comparative study of the evolving morphology of 2.5-D simulated CMEs to Earth's magnetosphere
A Self-similar Expansion Model for Use in Solar Wind Transient Propagation Studies
Accuracy and Limitations of Fitting and Stereoscopic Methods to Determine the Direction of Coronal Mass Ejections from Heliospheric Imagers Observations
Arrival time calculation for interplanetary coronal mass ejections with circular fronts and application to STEREO observations of the 2009 February 13 eruption
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