Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
the QUEST Collaboration
Yale
Yale University
Yale Univ.
Yale Univeristy
Yale University, New Haven, CT
Yale University.
Applied Research Corp., Landover, MD
NASA, Goddard Space Flight Center, Laboratory for Astronomy and Solar Physics, Greenbelt, Md.
Yale University Observatory, New Haven, Conn.
Yale University, New Haven, CT, USA; Goddard Space Flight Center, Greenbelt, MD
NASA, Goddard Space Flight Center, Laboratory for Planetary Atmospheres, Greenbelt, MD
Department of Astronomy, Yale University
Astronomy Department, Yale University, Box 208101, New Haven, CT 06520-8101, USA
Department of Astronomy, Yale University, New Haven, CT 06520
NASA, Goddard Space Flight Center, Laboratory for Planetary Atmospheres, Greenbelt, Md.
National Aeronautics and Space Administration. Goddard Space Flight Center, Greenbelt, MD.
NASA, Washington, D.C.
Center for Solar and Space Research, P.O. Box 208101, New Haven, Connecticut 06520-8101
JHU-APL, USNO, Yale
Yale / CSSR
NASA, Goddard Space Flight Center, Greenbelt, Md.
Yale University, Department of Astronomy, P.O. Box 208101, New Haven, CT 06250-8101, USA
Department of Astronomy, Yale University, P.O. Box 208101, New Haven, CT 06520, USA
Department of Astronomy, Yale University, P.O. Box 208101, New Haven, CT 06250-8101.
Citta Universitaria, Catania, Italy
South Florida, University, Tampa, Fla.
Department of Astronomy, Yale University, P.O. Box 208101, New Haven, CT 06520-8101.
Rochester, University, Rochester, N.Y.
Department of Astronomy, University of South Florida, Tampa, Florida.
C. E. Kenneth Mees Observatory, Bristol Springs, N.Y.
Yale University., New Haven, CT, US
Yale Univ
2-D Stellar Evolution Code Including Arbitrary Magnetic Fields. I. Mathematical Techniques and Test Cases
2D solar modeling
3D convection simulations of the outer layers of the Sun using realistic physics
3D Structures in Turbulent Convection and How to Read Them
a 2-D Stellar Evolution Code Including Arbitrary Magnetic Fields
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