Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Solar and Stellar Astrophysics
Scientist
NorthWest Research Associates, CoRA Division
Colorado Research Associates Division, NorthWest Research Associates Inc., Boulder, USA
CoRA, Boulder
Northwest Research Associates, 3380 Mitchell Lane, Boulder, CO 80301, USA
NWRA, CoRA Division Boulder CO 80301 USA
Colorado Research Associates, NorthWest Research Associates, Inc., 3380 Mitchell Lane, Boulder, CO 80301.
Colorado Research Associates, Boulder, CO, USA;
CoRA, NWRA, Boulder, CO, USA;
W. W. Hansen Experimental Laboratory, Stanford University, Stanford, CA 94305
W. W. Hansen Experimental Physics Laboratory, Stanford University, Stanford, CA 94305
Colorado Research Associates Division, NorthWest Research Associates Inc.
Department of Physics, Stanford University, Stanford, CA 94305, USA
W.W. Hansen Experimental Physics Lab, Stanford University
W.W. Hansen Experimental Laboratory, Stanford University
Stanford University
NWRA / CoRA
CORA / NWRA
Stanford University.
NorthWest Research Associates, CoRA Division, 3380 Mitchell Lane, Boulder, CO 80301 Research Associates, Colorado Research Associates Division, Boulder, CO 80301
NWRA, CoRA Division, 3380 Mitchell Lane, Boulder, CO 80301, USA
NorthWest Res. Assoc., CoRA DIv.
W. W. Hansen Experimental Physics Laboratory, Stanford University, Stanford, CA 94305-4085 of Physics, Stanford University, Stanford, CA 94309 University, W.W. Hansen Experimental Physics Laboratory, Stanford, CA 94305-4085, USA of Physics, Stanford University, Stanford, CA 94309, USA Hansen Experimental Physics Laboratory, Stanford University, Stanford, CA 94305-4085, USA
Colorado Research Associates, NWRA
Department of Physics, Stanford University, Stanford, CA 94309 Hansen Experimental Laboratory, Stanford Univ
"Hare and Hounds" Tests of Helioseismic Holography
A Nonlinear Model for Solar Spicules
A procedure for the inversion of f-mode travel times for solar flows
A Wave-Theory Approach to Time-Distance Helioseismology
Absorption of p Modes by Magnetic Plage
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