Simulations of observed auroral brightening caused by solar wind dynamic pressure enhancements under different interplanetary magnetic field conditions

Author:

Peng Z.12,Wang C.1,Hu Y. Q.3,Kan J. R.14,Yang Y. F.5

Affiliation:

1. State Key Laboratory of Space Weather, Center for Space and Applied Research; Chinese Academy of Sciences; Beijing China

2. Shandong Provincial Key Laboratory of Optical Astronomy and Solar-Terrestrial Environment; Weihai China

3. Chinese Academy of Sciences Key Laboratory of Basic Plasma Physics, School of Earth and Space Sciences; University of Science and Technology of China; Hefei China

4. Geophysical Institute; University of Alaska Fairbanks; Fairbanks Alaska USA

5. National Center for Space Weather; China Meteorology Administration; Beijing China

Publisher

American Geophysical Union (AGU)

Subject

Paleontology,Space and Planetary Science,Earth and Planetary Sciences (miscellaneous),Atmospheric Science,Earth-Surface Processes,Geochemistry and Petrology,Soil Science,Water Science and Technology,Ecology,Aquatic Science,Forestry,Oceanography,Geophysics

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