Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
SISSA Trieste
University of Durham
Rice, Department of Physics, Houston, TX 77005
Montana State University
Rice Univ., USA
Lockheed Martin Solar and Astrophysics Lab, 3251 Hanover Street, L9 / 41, Building 252, Palo Alto, CA 94304 Space Institute, 6100 Main St. MS 108, Houston, TX 77005, USA
LMSAL
Rice University
University of Durham, United Kingdom
Max-Planck-Institut für extraterrestrische Physik, Garching bei München, Germany, Stanford-Lockheed Institute for Space Research, Palo Alto, CA, USA Martin Advanced Technology Center, Department L9-41, Building 252
Durham University, United Kingdom
Rice University.
Rice Univ
Department of Physics and Astronomy, Rice University
University of Montana
Lockheed Martin Solar and Astrophysics Laboratory
Lockheed Martin Solar and Astrophysics Lab.
Lockheed Martin Solar & Astrophysics Lab
Glasgow, University, Scotland
University of Colorado at Boulder
Institute of Astronomy, United Kingdom
Lockheed Martin Solar and Astrophysics Lab., Org. L9-41, B / 252 3251 Hanover St, Palo Alto, CA 94304, USA University, Department of Physics and Astronomy 6100 Main St., Houston, TX 77005
Rice University, Department of Physics and Astronomy MS-108 6100 Main St., Houston, TX 77005, USA
Rice University, 6100 Main Street, Houston, TX 77005
Lockheed Martin Solar and Astrophysics Lab., Org. L9-41, B / 252 3251 Hanover St, Palo Alto, CA 94544, USA Martin Solar and Astrophysics Laboratory, O / L9-41, B252 3251 Hanover Street, Palo Alto, CA 95304, USA
Lockheed Martin Solar and Astrophysics Lab., Org. L9-41, B / 252 3251 Hanover Street, Palo Alto, CA 94304, USA of Cambridge
Lockheed Martin Solar & Astrophysics Lab.
Lockheed-Martin ATC, Solar and A
3D Magnetic Modeling of Active Regions Using STEREO/EUVI
A Hubble Space Telescope NICMOS and ACS Morphological Study of z~2 Submillimetre Galaxies
A LABOCA survey of the Extended Chandra Deep Field South - submillimeter properties of near-IR selected galaxies
A Method for Characterizing Rotation Rates in the Soft X-Ray Corona
A Plasma Analog of Planetary Ring Dynamics
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