Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Solar and Stellar Astrophysics
Scientist
W.W. Hansen Experimental Physics Laboratory, Stanford University
Hansen Experimental Physics Laboratory, Stanford University, Stanford, CA, USA
HEPL, 455 via Palou, Stanford University, CA 94305-4085.
W. W. Hansen Experimental Physics Laboratory, Stanford University, Stanford, CA 94305-4085.
W.W. Hansen. E. P. L., Stanford University, Stanford, CA 94305, USA
Service d'astrophysique, CEA / DSM / DAPNIA, CE Saclay, 91191 Gif-sur-Yvette, France
Service d'Astrophysique, CEA / DSM / DAPNIA, CE Saclay, 91191 Gif sur Yvette, France
W. W. Hansen Experimental Physics Laboratory, Stanford University, Stanford, CA 94305 University
HEPL, Stanford University
W. W. Hansen Experimental Physics Laboratory, Stanford University, Stanford, CA 94305-4085
Stanford Univ. Hansen Exp. Physics Lab., 455 Via Palou, Stanford, CA 94305-4085, USA of Physics and Astronomy, University of Birmingham, Edgbaston, Birmingham B15 2TT, UK
W.W.Hansen Experimental Physics Laboratory, Stanford University, Stanford, CA 94305-4085, USA
CEA / DSM / DAPNIA, CE Saclay, 91191 Gif sur Yvette, France; W. W. Hansen Experimental Physics Laboratory, Stanford University, Stanford, CA 94305-4085. Hansen Experimental Physics Laboratory, Stanford University, 455 Via Palou Stanford University, Stanford, CA 94305-4085
W.W. Hansen Experimental Physics Laboratory, Stanford University, 455 Via Palou, Stanford, CA 94305-4085, USA
CEA / DAPNIA / Service d'Astrophysique, 91191 Gif-sur-Yvette, France
Stanford University, Stanford, CA
About the rotation of the solar radiative interior
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
Comparison of Line-of-Sight Magnetograms Taken by the Solar Dynamics Observatory/Helioseismic and Magnetic Imager and Solar and Heliospheric Observatory/Michelson Doppler Imager
Contamination by Surface Effects of Time-distance Helioseismic Inversions for Sound Speed Beneath Sunspots
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