Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Solar and Stellar Astrophysics
Scientist
Birmingham, University, England
Astronomy Unit, School of Mathematical Sciences, Queen Mary and Westfield College, Mile End Road, London E1 4NS, UK Solar Observatory, P.O. Box 26732, Tucson, AZ 85726-6732 National Solar Observatory, Tucson, AZ, USA; Solar Observatory, 950 North Cherry Avenue, Tucson, AZ 85719 Solar Observatory, PO Box 26732, Tucson, AZ 85726-6732, USA
National Solar Observatory, Tucson, AZ 85719
National Solar Observatory
University of Birmingham, Edgbaston, Birmingham, UK
National Solar Obs.
National Solar Observatory, 950 North Cherry Avenue, Tucson, AZ 85719.
National Solar Observatory, National Optical Astronomy Observatoires, 950 North Cherry Avenue, Tucson, AZ 85719
NSO Tucson
National Solar Observatory, GONG Program
University of Birmingham, United Kingdom
School of Physics and Space Research, University of Birmingham, Edgbaston, Birmingham B15 2TT
National Solar Observatory, P.O. Box 26732, Tucson, AZ 85726-6732, USA 950 N. Cherry Ave., Tucson, AZ 85726, USA Solar Observatory, 950 N. Cherry Ave., Tucson, AZ 85719, USA Solar Observatory, 950 N. Cherry Ave. P.O. Box 26732, Tucson, AZ 85726-6732, USA Solar Observatory, P.O. Box 26732, Tucson, AZ 85726, USA Solar Observatory, P.O. Box 26732, Tucson, AZ 86732-6732, USA University
School of Physics and Space Research, University of Birmingham, Edgbaston, Birmingham B15 2TT, UK
National Solar Observatory, Tucson, AZ of Physics and Astronomy, University of Birmingham, Edgbaston, Birmingham B15 2TT, UK; National Solar Observatory, 950 North Cherry Avenue, Tucson, AZ 85719.
National Solar Observatory, 950 N. Cherry Ave, Tucson, AZ 85719, USA Solar Observatory, 950 N. Cherry Avenue, Tucson, AZ 85719, USA Solar Observatory, P.O. Box 267
2 Years of Meridional Circulation from GONG Ring Diagrams
A Comparison of Low-Degree Solar p-Mode Parameters from BiSON and GONG: Underlying Values and Temporal Variations
A Comparison of Solar p-Mode Parameters from MDI and GONG: Mode Frequencies and Structure Inversions
A Comparison of Solar p-Mode Parameters from the Michelson Doppler Imager and the Global Oscillation Network Group: Splitting Coefficients and Rotation Inversions
A Helioseismic Comparison of the Solar Minima Preceding Cycles 23 and 24
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