Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Solar and Stellar Astrophysics
Scientist
Bartol Research Institute
Institute for Astronomy, 4761 Lower Kula Road, P.O. Box 209, Kula, HI 96790, USA
Maui Scientific Research Center, University of New Mexico, 590 Lipoa Parkway, Suite 262, Kihei, HI 96753 for Astronomy, University of Hawai'i, 4761 Lower Kula Road, Kula, Hawaii 96790, USA of Deleware, Newark, DE, US
University of Hawaii
Bartol Research Institute, Newark, DE
University of Delaware, Newark, DE, US
Bartol Research Inst.
Institute for Astronomy, University of Hawaii
National Solar Observatory
Franklin Institute, Bartol Research Foundation, Newark, DE
Maui High Performance Computing Center, University of New Mexico, 550 Lipoa Parkway, Kihei, HI 96753 Scientific Research Center / University of New Mexico
Bartol Research Inst., Newark, DE
Institute for Astronomy, University of Hawaii, 34 Ohia Ku, Pukalani, HI 96768, USA Solar Observatory, P.O. Box 26732, Tucson, AZ 85726, USA
Bartol Research Institute, University of Delaware, Newark, DE 19716, USA
Birmingham, University, England
Maui Scientific Research Center / University of New Mexico, 590 Lipoa Pkwy, Ste 262, Kihei, HI 96753, USA
Maui Scientific Research Center, University of New Mexico, 590 Lipoa Parkway, Ste 262, Kihei, HI 96753, USA
Consejo Superior de Investigaciones Cientificas, Tenerife, Spain
National Solar Observatory, Tucson, AZ.
Institute for Astronomy, University of Hawaii, Kula, USA
Institute for Astronomy, University of Hawaii, HI 96768-8288, USA Scientific Research Center, University of New Mexico, 590 Lipoa Parkway, Suite 272, Kihei, HI 96753; Steward Observatory, University of Arizona, 933 North Cherry
A Calcium-Based Magneto-Optical Filter
A comparison of acoustic mode parameters using multi-spectral data
A new Instrument for High-cadence, Multi-height Observations of the Velocity and Magnetic Fields of the Full Solar Disk
A new instrument for sounding the solar atmosphere
A New Way to Model the Solar Oscillation ℓ-ν Power Spectrum
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Profile ID: LFWR-SCP-P-97957