Astronomy and Astrophysics – Astronomy
Scientist
Astronomy and Astrophysics
Astronomy
Scientist
NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA
High Altitude Observatory, National Center for Atmospheric Research, Boulder, CO 80307-3000 Altitude Observatory, National Center for Atmospheric Research, Boulder, CO 80307-3000
High Altitude Observatory, National Center for Atmospheric Research, Boulder, CO 80307-3000 Altitude Observatory, National Center for Atmospheric Research, Boulder, CO 80307-3000 Physics and Astronomy, Rice University, 6100 Main Street, Houston TX 77005 of Physics and Astronomy, Rice University, Houston, TX 77005 of Physics and Astronomy, Rice University, Houston, TX 77005 / GSFC, Greenbelt, MD, USA; Science Division, NASA Goddard Space Flight Ctr, Greenbelt, MD, USA; Goddard Space Flight Center, Greenbelt, MD, USA; University
HAO / NCAR
High Altitde Observatory / NCAR
High Altitude Observatory, National Center for Atmospheric Research, Boulder, CO 80301
NCAR / High Altitude Obs., 3450 Mitchell Lane, Boulder, CO 80301, USA Altitude Observatory, P.O. Box 3000, Boulder, CO 80307-3000, USA
Sterrekundig Instituut Utrecht
NCAR / HAO, P.O. Box 3000, Boulder, CO 80307-3000, USA
Rice University, 6100 Main St., Houston, TX 77005, USA Altitude Observatory / NCAR, P.O. Box 3000, Boulder, CO 80307-3000, USA
High Altitude Observatory / NCAR, P.O. Box 3000 3450 Mitchell Lane, Boulder, CO 80307-3000, USA
NCAR / High Altitude Observatory, 3450 Mitchell Lane, Boulder, CO 80301, USA
National Center for Atmospheric Research / HAO, 3450 Mitchell Lane, Boulder, CO 80301, USA
NCAR / HAO, 3450 Mitchel
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 New Method of Determining Line-of-Sight Velocity Using MLSO/CHIP He I 1083 nm Observations
A New Technique for Deriving Prominence Mass from SOHO/EIT Fe XII (19.5 Nanometers) Absorption Features
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