Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Solar and Stellar Astrophysics
Scientist
Department of Physics, Stanford University, Stanford, CA, 94305, USA
National Solar Observatory, 950 N Cherry Av, Tucson AZ 85719, USA
California State-Northridge
National Solar Observatory, Sunspot, NM, US
National Solar Observatory
NSO
National Solar Observatory, 950 North Cherry Avenue, Tucson, AZ 85718
NSO / KP, NOAO
National Optical Astronomy Observatoires, Sunspot, NM, US
National Solar Observatory / Sacramento Peak, National Optical Astronomy Observatoires
Department of Physics, Stanford University, Stanford, California 94305
Cal State Univ Northridge
NSO / NOAO
California State University, Northridge, Department of Physics and Astronomy, and San Fernando Observatory, 18111 Nordhoff Street, Northridge, CA 91330-8268, USA
National Solar Observatory, 950 N Cherry Ave., Tucson, AZ 85719
National Solar Observatory, POBox: 26732, Tucson, AZ 85726, USA
California Institute of Technology, Pasadena
National Solar Observatory, P.O. Box 26732, Tucson, AZ 85726
CSUN / SFO
National Solar Observatory, 950 N. Cherry Ave., Tucson, AZ 85719, USA Solar Observatory, 950 N. Cherry Ave., Tucson, AZ 85719
National Solar Observatory, Tucson, AZ 85718
National Solar Observatory, 950 N. Cherry Avenue, Tucson, AZ 85719, USA
Department of Physics, Stanford University, Stanford, CA 94305, USA
San Fernando Observatory and California State University Northridge, Department of Physics and Astronomy, 18111 Nordhoff Street, Northridge, CA 91330-8268, USA
National Solar Observatory, 950 N Cherry Av, Tucson, AZ 85726, USA Solar Observatory, 950 N Cherry Av, Tucson, AZ 85719
National Solar Observatory, 950 N. Cherry Ave., Tucson, Az 85719, USA
An Erupting Active Region Filament: Three-Dimensional Trajectory and Hydrogen Column Density
An Erupting Active Region Filament: Three-Dimensional Trajectory and Hydrogen Column Density
Background-Induced Measurement Errors of the Coronal Intensity, Density, Velocity, and Magnetic Field
Capabilities of the MCCD System at Mees Solar Observatory
Comparison of NSO/KPVT 1083 NM and SOHO/CDS/SUMER Observations of a Coronal Hole.
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Profile ID: LFWR-SCP-P-210804