Physics
Scientist
High Altitude Observatory, Boulder, Colo.
Department of Applied Physics and Information Science, University of California
High Altitude Observatory, Boulder, CO
University of Colorado, Boulder, CO, US
NCAR / HAO
High Altitude Observatory, National Center for Atmospheric Research, Boulder, CO 80302; The National Center for Atmospheric Research is sponsored by the National Science Foundation. Altitude Observatory, National Center for Atmospheric Research
High Altitude Observatory, National Center for Atmospheric Research, Boulder, CO 80301
National Center for Atmospheric Research, Boulder, CO, US
NCAR / High Altitude Obs., 3450 Mitchell Lane, Boulder, CO 80301, USA
High Altitude Observatory, P.O. Box 3000, Boulder, CO 80307-3000, USA / UCAR
Sterrekundig Instituut Utrecht
NCAR / HAO, P.O. Box 3000, Boulder, CO 80307-3000, USA Altitude Observatory / NCAR, P.O. Box 3000, Boulder, CO 80307-3000, USA Altitude Observatory / NCAR, P.O. Box 3000 3450 Mitchell Lane, Boulder, CO 80307-3000, USA / High Altitude Observatory, 3450 Mitchell Lane, Boulder, CO 80301, USA / HAO, 3450 Mitchell Lane, Boulder, CO 80301, USA Center for Atmospheric Research, Boulder, Colo.
HAO / NCAR
NCAR HAO, 3450 Mitchell Lane, Boulder, CO 80301, USA
HAO, NCAR, Boulder, CO
High Altitude Observatory, National Center for Atmospheric Research, Boulder, Colorado
NCAR / High Altitude Observatory; Boulder, CO 80307
High Altitude Observatory, National Center for Atmospheric Research, Boulder, CO 80307-3000 Altitude Observatory, National Center for Atmospheric Research, Boulder, CO 80307-3000
2D MHD Models of the Large Scale Solar Corona
A Comparison of CME-associated atmospheric waves observed in coronal (19.5 nm) and chromospheric (He I 1083 nm and H-alpha 656 nm) lines
A Comparison of CME-associated Atmospheric Waves Observed in Coronal (Fe XII 19.5 nm) and Chromospheric (He I 1083 nm) Lines
A Comparison of CME-Associated Atmospheric Waves Observed in Coronal (Fe XII 195 Å) and Chromospheric (He I 10830 Å) Lines
A comparison of the reduced and approximate systems for the time dependent computation of the polar wind and multiconstituent stellar winds
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