An Ionospheric Conductance Gradient Driver for Subauroral Picket Fence Visible Signatures Near STEVE Events
Author:
Affiliation:
1. Dartmouth College Hanover NH USA
2. Naval Research Laboratory Washington DC USA
3. Embry Riddle Aeronautical University Daytona Beach FL USA
Funder
U.S. Naval Research Laboratory
Dartmouth College
Publisher
American Geophysical Union (AGU)
Subject
Space and Planetary Science,Geophysics
Link
https://onlinelibrary.wiley.com/doi/pdf/10.1029/2022JA030863
Reference27 articles.
1. Steve: The Optical Signature of Intense Subauroral Ion Drifts
2. Auroral ionospheric conductances during disturbed conditions;Brekke A.;Annales Geophysicae,1989
3. Burleigh M.(2022).GEMINI simulation data for picket fence study repository “Dartmouth College Prof Kristina A Lynch”. Retrieved fromhttps://rcweb.dartmouth.edu/LynchK/
4. Cross-scale coupling in the auroral acceleration region
5. Examining the Auroral Ionosphere in Three Dimensions Using Reconstructed 2D Maps of Auroral Data to Drive the 3D GEMINI Model
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1. Generation of Top‐Boundary Conditions for 3D Ionospheric Models Constrained by Auroral Imagery and Plasma Flow Data;Journal of Geophysical Research: Space Physics;2024-08
2. 3D Simulation of an Extreme SAID Flow Channel;Journal of Geophysical Research: Space Physics;2024-06
3. It's Not Easy Being Green: Kinetic Modeling of the Emission Spectrum Observed in STEVE's Picket Fence;Geophysical Research Letters;2023-11-03
4. The Inner Structure of STEVE‐Linked SAID;Geophysical Research Letters;2023-04-25
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