Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
W.W. Hansen Experimental Physics Laboratory, Stanford University, Palo Alto, USA
STANFORD
Hansen Experimental Physics Laboratory, Stanford University, 455 via Palou, Stanford, CA 94305-4085, USA
Stanford University, 455 Via Palou, Stanford, CA 94305, USA Astrofizicheskaia Observatoriia, Nauchny, Ukrainian SSR
Stanford University.
Institute of Astronomy, Cambridge, UK
W. W. Hansen Experimental Physics Laboratory, Stanford University, Stanford, CA 94305-4085.
Stanford University, Stanford, CA, USA;
HEPL, Stanford Univ-Geophysics Dept, Stanford, CA, USA;
HEPL, Stanford University, Stanford, CA, USA;
Hansen Exp. Physics Laboratory, Stanford Univ-Solar Projects, Stanford, CA, USA;
W. W. Hansen Experimental Laboratory, Stanford University, Stanford, CA 94305
W. W. Hansen Experimental Physics Laboratory, Stanford University, Stanford, CA 94305, USA
W.W. Hansen Experimental Physics Laboratory, Stanford University, Stanford, CA 94305, USA
W. W. Hansen Experimental Physics Laboratory, Stanford University, Stanford, CA 94305, Stanford University, Stanford, CA 94305-4085, USA
W. W. Hansen Experimental Physics Laboratory, Stanford University, Stanford, CA Hansen Experimental Laboratory, Stanford University, Stanford, CA 94305, USA
W.W. Hansen Experimental Physics Lab, Stanford University
W. W. Hansen Experimental Physics Laboratory, Stanford University
W.W. Hansen Experimental Phyiscs Laboratory, Stanford University
W.W. Hansen Experimental Laboratory, Stanford University
W.W. Hansen Experimental Physics Lab., Stanford University.
W. W. Hansen Experimental Physics Laboratory, Stanford University, 455 via Palou, Stanford, CA 94305-4085
W. W. Hansen Experimental Physics Laboratory, Stanford University, Stanford, CA 94305-4085
"Hare and Hounds" Tests of Helioseismic Holography
A brief history of the solar oblateness. A review
A Functional Analytic Approach to Fréchet Traveltime Kernels
A Mechanism of the Solar Acoustic Emission
A new estimate of the solar core rotation from IPHIR
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