Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Solar and Stellar Astrophysics
Scientist
High Altitude Observatory, NCAR, Boulder, CO, USA; Altitude Observatory, National Center for Atmospheric Research, Boulder, CO, USA; Altitude Observatory, Boulder, CO, USA; of Geophysics, School of Earth and Space Sciences, Peking University, Beijing, China
Max-Planck-Institut für Sonnensystemforschung, Max-Planck Str.2, Katlenburg-Lindau, 37191, Germany; Department of Geophysics, Peking University, Department of Geophysics, Peking University, Beijing, 100871, China für Sonnensystemforschung, Katlenburg-Lindau, Germany; Department of Geophysics, Peking University, Beijing, PR China of Earth and Space Sciences, Peking University, Beijing, PR China
Max-Planck-Institut für Sonnensystemforschung, Katlenburg-Lindau 37191, Germany; Department of Geophysics, Peking University, Beijing 100871, China
Max-Planck-Institut für Sonnensystemforschung, Katlenburg-Lindau, Germany of Earth and Space Sciences, Peking University, Beijing, China of Earth and Space Sciences, Peking University, Beijing 100871, PR China
Max-Planck-Institut für Sonnensystemforschung, Katlenburg-Lindau, Germany ; Department of Geophysics, Peking University, Beijing, PR China
High Altitude Observatory, National Center for Atmospheric Research, Boulder, CO 80307, USA
Department of Geophysics, Peking University, Beijing, PR China; Max-Planck-Institut für Sonnensystemforschung, Katlenburg-Lindau, Germany
Department of Geophysics, Peking University, Beijing 100871, China; Max-Planck-Institut für Sonnensystemforschung, 37191 Katlenburg-Lindau, Germany
School of Forestry and Wildlife Sciences, Auburn University, Auburn, Alabama, USA
A magnetic null geometry reconstructed from Cluster spacecraft observations
Buffered Electropolishing -- a New Way for Achieving Extremely Smooth Surface Finish on Nb SRF Cavities To be Used in Particle Accelerators
China's changing landscape during the 1990s: Large-scale land transformations estimated with satellite data
Cool and Hot Components of a Coronal Bright Point
Does the Kinetic Alfven Wave or Oblique Whistler Wave dominate the Dissipation Range of Solar Wind Turbulence?
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