Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
UCLA
UCLA, Los Angeles, CA, US
AFRL, Albuquerque, NM, USA;
National Solar Observatory, 950 North Cherry Avenue, Tucson, AZ 85726-6732, USA
National Solar Observatory, USA
Air Force Research Laboratory / Space Vehicles Directorate
Astronomy Department, University of California
NSO
National Solar Observatory, P.O. Box 26732, 950 North Cherry Avenue, Tucson, AZ 85726-6732, USA of Physics and Astronomy, UCLA, Los Angeles, CA 90095-1562
National Solar Observatory, 950 N. Cherry Avenue, Tucson, AZ 85719, USA Solar Observatory, 950 North Cherry Avenue, Tucson, AZ 85719, USA Solar Observatory, BOX 2732 950 N. Cherry Ave., Tuscon, AZ 85726, USA Solar Observatory, PO Box 26732, Tucson, AZ 85726-6732, USA of Physics and Astronomy, UCLA, Los Angeles, CA 90095-1562, USA
Institut d'Astrophysique Spatiale, Université Paris XI, 91405 Orsay, France
AFRL, Albuquerque, NM, USA
National Solar Observatory, 950 North Cherry Avenue, Tucson, AZ 85719 Solar Observatory, 950 N Cherry Av, Tucson, AZ 85719 Solar Observatory, 950 N. Cherry Ave., Tucson, Az 85719, USA
National Solar Observatory, PO Box 26732, Tucson, AZ 86726, USA Solar Observatory, 950 N. Cherry Ave., Tucson, AZ 85719 Solar Observatory, 950 N. Cherry Ave., Tucson, AZ 85719, USA Solar Observatory
Department of Physics and Astronomy, Division of Astronomy, University of California, Los Angeles, CA 90095-1562
Air Force Research Laboratory, Kirtland AFB, NM, USA;
Institute for Scientific Research, Boston College, Chestnut Hill, Massachusetts; National Solar Observatory, Tucson, Arizona
AFRL / Space Vehicles Directorate, Kirtland AFB, NM, USA; Institute for Scientific Research, Bo
A global SOLIS vector spectromagnetograph (VSM) network
About the rotation of the solar radiative interior
Air Force Data Assimilative Photospheric Flux Transport (ADAPT) Model
Analysis of low frequency signal with the GOLF experiment: methodology and results
Analysis of rotational frequency splittings sensitive to the rotation rate of the solar core
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