Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
U. Alabama, Huntsville, AL, USA
Alabama University
Alabama Univ., Huntsville, AL
Center for Space Plasma and Aeronomic Research, Department of Mechanical and Aerospace Engineering, University of Alabama in Huntsville, Huntsville, AL 35899
Center for Space Plasma and Aeronomic Research, University of Alabama in Huntsville
Alabama, Univ., Huntsville, AL
Center for Space Plasma and Aeronomic Research, University of Alabama, Huntsville, AL 35899 for Space Plasma and Aeronomic Research Department of Mechancial and Aerospace Engineering, The University of Alabama in Huntsville, Huntsville, AL 35899, USA of Earth and Space Science, University of Science and Technology of China, HefeiChina
Alabama, University, Huntsville, AL
Alabama Univ., Huntsville.
CSPAR, University of Alabama in Huntsville, Huntsville, AL 35899, USA
Center for Space Plasma and Aeronomic Research and Department of Mechanical and Aerospace Engineering, University of Alabama, Huntsville, AL 35899.
Center for Space Plasma and Aeronomic Research and Department of Mechanical and Aerospace Engineering, University of Alabama in Huntsville, Huntsville, AL 35899, USA
Center for Space Plasma and Aeronomic Research, The University of Alabama in Huntsville
University of Alabama in Huntsville, USA
Center for Space Plasma and Aeronomic Research and Department of Mechanical and Aerospace Engineering, The University of Alabama in Huntsville, Huntsville, AL 35899, USA
University of Science and Technology of China, Hefei, People's Republic of China
University of Science & Technology of China China
A Global Coronal Hole and Streamer Model
A Global Solar Wind Model Based on Surface Measurements of Magnetic Field and Transverse Velocity from GONG
A Numerical Analysis of Propagation of a Non-Linear Alfven Wave in a Non-Uniform Solar Atmosphere
A numerical simulation for the propagation of disturbance in the solar corona. II - The effects of thermal conduction and radiation
A two-dimensional MHD global coronal model - Steady-state streamers
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