Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Solar and Stellar Astrophysics
Scientist
Stanford University
W.W.Hansen Experimental Physics Laboratory
Stanford University.
Stanford University, Stanford, CA, USA
Stanford University National Lab., Denmark
Hansen Experimental Physics Laboratory, Annex A201, Stanford University, Stanford, CA 94305-4085.
Stanford University, Stanford, CA, USA;
W. W. Hansen Experimental Physics Laboratory, Stanford University, 445 Via Palou, Stanford, CA 94305-4085
HEPL Annex A201, Stanford University
Center for Space Science and Astrophysics, Stanford University, Stanford, CA 94305, USA
W. W. Hansen Experimental Physics Laboratory, Stanford University, Stanford, CA 94305-4085 W. Hansen Experimental Laboratory, Stanford University, 455 Via Palou, Stanford, CA 94305
HEPL Annex A201, Stanford University, Stanford, CA 94305-4085.
High Altitude Observatory, Boulder, CO; Aarhus University, Denmark
Hansen Experimental Physics Laboratory
HEPL, Stanford University
Stanford
CSSA, Stanford University
W.W. Hansen Experimental Physics Laboratory, Stanford University
Stanford University, W.W. Hansen Experimental Physics Laboratory 4085, Stanford, CA 94305-4085, USA University, Hansen Experimental Physics Laboratory, HEPL Annex, Stanford, CA 94305-4085, USA Experimental Physics Laboratory, HEPL Annex Stanford University, Stanford, CA 94305-4085, USA
Hansen Experimental Physics Laboratory, HEPL Annex, Stanford University, Stanford, CA 94305-4085, USA
Stanford University, HEPL Annex A, Stanford, CA 94305-4085, USA Stanford University., CSSA
Stanford. University
Stanford University - HEPL Solar Physics, 491 South Service Road, Stanford, CA 94305, USA University, HEPL Annex, A201, Stanford, CA 94305, USA University, HEPL 491 South Service Road, Stanford, CA 94305, USA
Hansen Expe
A comparison of methods for inverting helioseismic data
A Comparison Of Solar High-degree p-mode Parameters From HMI And MDI
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 Measurement of the Rotation Rate in the Deep Solar Interior
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