Affiliation:
1. Planetary Environmental and Astrobiological Research Laboratory School of Atmospheric Sciences Sun Yat‐sen University Zhuhai China
2. Key Laboratory of Tropical Atmosphere‐Ocean System Sun Yat‐sen University Ministry of Education Zhuhai China
3. Institute of Geology and Geophysics Chinese Academy of Sciences Beijing China
Abstract
AbstractThe polar wind, consisting of low‐energy ions and electrons, is an outflow along the open magnetic field lines from the polar cap ionosphere to the magnetosphere. Previous studies found that both solar radiation and solar wind electromagnetic energy are the two main energy sources for the polar wind. The polar rain, being field‐aligned precipitating electrons from the solar wind to the polar cap, may provide additional energies for the polar wind. This scenario is complicated as simulation studies show that polar rain changes the electric potential structures over the polar cap ionosphere. It is unclear how the polar rain affects the polar wind ion outflow. In this study, we show a positive correlation between the polar wind and the polar rain. Meanwhile, the polar wind is generally diminished in regions with strong Earth's magnetic field, suggesting the |B| modulates the penetration depth of the polar rain through the magnetic mirror force and thus the energy dissipation of the polar rain. Therefore, the polar rain can be an additional energy source for the polar wind although the polar rain has generally smaller energies and intensities than the particle precipitations in the auroral regions.
Funder
National Natural Science Foundation of China
Publisher
American Geophysical Union (AGU)
Subject
Space and Planetary Science,Geophysics
Cited by
1 articles.
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