Automated Technique for the Detection of Step‐Like Solar Wind Dynamic Pressure Changes: Application to the Response of the Transpolar Potential to Solar Wind Dynamic Pressure Fronts
Author:
Affiliation:
1. Space Sciences Institute Boulder CO USA
2. Cooperative Institute for Research in Environmental Sciences University of Colorado Boulder CO USA
3. NASA Goddard Space Flight Center Greenbelt MD USA
Funder
National Aeronautics and Space Administration
Publisher
American Geophysical Union (AGU)
Subject
Space and Planetary Science,Geophysics
Link
https://onlinelibrary.wiley.com/doi/pdf/10.1029/2021JA029198
Reference27 articles.
1. Relationship between solar wind dynamic pressure and amplitude of geomagnetic sudden commencement (SC)
2. Statistical study of the effect of solar wind dynamic pressure fronts on the dayside and nightside ionospheric convection
3. Evaluation of the Hill-Siscoe transpolar potential saturation model during a solar wind dynamic pressure pulse
4. Effect of solar wind pressure pulses on the size and strength of the auroral oval
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1. Why Are Some Solar Wind Pressure Pulses Followed by Geomagnetic Storms?;Journal of Geophysical Research: Space Physics;2023-08
2. Local Time Response of Auroral Electrojet During Magnetically Disturbed Periods: DMSP and CHAMP Coordinated Observations;Journal of Geophysical Research: Space Physics;2022-08
3. Geomagnetic Response to Rapid Increases in Solar Wind Dynamic Pressure: Event Detection and Large Scale Response;Frontiers in Astronomy and Space Sciences;2022-05-05
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