Sub-Auroral Polarization Streams: A complex interaction between the magnetosphere, ionosphere, and thermosphere
Author:
Publisher
IOP Publishing
Subject
General Physics and Astronomy
Link
http://stacks.iop.org/1742-6596/767/i=1/a=012021/pdf
Reference43 articles.
1. Reconnection at the Magnetospheric Boundary: Results from Global Magnetohydrodynamic Simulations
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4. On the relationship of SAPS to storm-enhanced density
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1. SubAuroral Red Arcs Generated by Inner Magnetospheric Heat Flux and by SubAuroral Polarization Streams;Geophysical Research Letters;2024-09
2. The Relation Among the Ring Current, Subauroral Polarization Stream, and the Geospace Plume: MAGE Simulation of the 31 March 2001 Super Storm;Journal of Geophysical Research: Space Physics;2023-12
3. The Contribution of Plasma Sheet Bubbles to Stormtime Ring Current Buildup and Evolution of Its Energy Composition;Journal of Geophysical Research: Space Physics;2023-11
4. Multiple Longitude Sector Storm‐Enhanced Density (SED) and Long‐Lasting Subauroral Polarization Stream (SAPS) During the 26–28 February 2023 Geomagnetic Storm;Journal of Geophysical Research: Space Physics;2023-08-31
5. Explaining Ionospheric Ion Upflow in the Subauroral Polarization Streams;Remote Sensing;2022-12-13
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