Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
Institut fuer Astrophysik, Georg-August-Universitaet Goettingen, Germany
Max-Planck-Institut fuer Sonnensystemforschung, Katlenburg-Lindau, Germany
Max-Planck-Institut für Sonnensystemforschung, 37191 Katlenburg-Lindau, Germany
W. W. Hansen Experimental Physics Laboratory, Stanford University, Stanford, CA 94305-4085.
W.W. Hansen Experimental Physics Laboratory, Stanford University, Stanford CA 94305, USA
Max-Planck-Institut für Sonnensystemforschung, Germany
Max-Planck-Institut für Sonnensystemforschung, 37191 Katlenburg-Lindau, Germany Hansen Experimental Physics Laboratory, Stanford University, Stanford, CA 94305-4085, USA
Hansen Experimental Physics Laboratory, 455 Via Palou, Stanford, CA 94305, USA für Sonnensystemforschung, Max-Planck-Strasse 2, 37191 Katlenburg-Lindau, Germany
W.W.Hansen Experimental Physics Laboratory, Stanford University, Stanford, CA 94305, USA
Max Planck Institute for Solar System Research, Katlenburg-Lindau, Germany
W. W. Hansen Experimental Physics Laboratory, Stanford University, 455 Via Palou, Stanford, CA 94305-4085 für Sonnensystemforschung, Max-Planck-Str. 2, Katlenburg-Lindau, 37191 Germany University, Hansen Experimental Physics Laboratory, Stanford, CA 94305-4085, USA Experimental Physics Laboratory, Stanford University, 455 via Palou, Stanford, CA 94305-4085, USA; MPI Sonnensystemforschung, Max-Planck-Str. 2, Katlenburg-Lindau, 37191 Germany
W. W. Hansen Experimental Physics Laboratory, Stanford University, Stanford, CA 94305; Max-Planck-Institut für Aeronomie, Postfach 20, Katlenburg-Lindau D-37191, Germany
W. W. Hansen Experimental Physics Laboratory, Stanford University, Stanford, CA 94305, USA
Max-Planck-Institut für Sonnensystemforschung, Max-Planck-Straße 2, 37191 Katlenburg-Lindau, Germany
Max-Planck-Institut für Sonnensystemforschung, 37191 Katle
3D Numerical Simulations of f-Mode Propagation Through Magnetic Flux Tubes
A New Component of Solar Dynamics: North-South Diverging Flows Migrating toward the Equator with an 11 Year Period
A procedure for the inversion of f-mode travel times for solar flows
Accurate p-mode measurements of the G0V metal-rich CoRoT target HD 52265
Acoustic scattering by flux tubes: is the Born approximation valid?
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