Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Solar and Stellar Astrophysics
Scientist
Max-Planck-Institut für Sonnensystemforschung, Katlenburg-Lindau, Germany
Department of Geophysics, Peking University, Beijing 100871, China
Max-Planck-Institut für Sonnensystemforschung, Katlenburg-Lindau, Germany; Department of Geophysics, Peking University, Beijing, China
Do Oblique Alfvén/Ion-cyclotron or Fast-mode/Whistler Waves Dominate the Dissipation of Solar Wind Turbulence near the Proton Inertial Length?
Identification of prominence ejecta by the proton distribution function and magnetic fine structure in interplanetary coronal mass ejections in the inner heliosphere
Multi-scale Anti-correlation Between Electron Density and Magnetic Field Strength in the Solar Wind
Possible Evidence of Alfvén-cyclotron Waves in the Angle Distribution of Magnetic Helicity of Solar Wind Turbulence
Prominence material identified in magnetic cloud
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