The Day‐Side Magnetic Reconnection Rate and Cusp Ion Dispersion During the May 2024 Geomagnetic Storm
Open Access
- 29 March 2026
- journal article
- research article
- Published by American Geophysical Union (AGU) in Journal of Geophysical Research: Space Physics
- Vol. 131 (4)
Abstract
No abstract availableKeywords
This publication has 39 references indexed in Scilit:
- High‐resolution global magnetohydrodynamic simulation of bursty bulk flowsJournal of Geophysical Research: Space Physics, 2015
- Comparative analysis of dayside magnetic reconnection models in global magnetosphere simulationsJournal of Geophysical Research: Space Physics, 2014
- Kelvin‐Helmholtz instability of the magnetospheric boundary in a three‐dimensional global MHD simulation during northward IMF conditionsJournal of Geophysical Research: Space Physics, 2013
- Synthesis of various ionospheric convection patterns for IMF BY‐dominated periods: Split crescent cells, exchange cells, and theta aurora formationJournal of Geophysical Research, 2008
- Remote sensing of the spatial and temporal structure of magnetopause and magnetotail reconnection from the ionosphereReviews of Geophysics, 2008
- Fractal reconnection structures on the magnetopauseGeophysical Research Letters, 2005
- A statistical comparison of SuperDARN spectral width boundaries and DMSP particle precipitation boundaries in the nightside ionosphereGeophysical Research Letters, 2004
- Inner magnetospheric modeling with the Rice Convection ModelSpace Science Reviews, 2003
- The response of the HF radar spectral width boundary to a switch in the IMF By direction: Ionospheric consequences of transient dayside reconnection?Journal of Geophysical Research, 2001
- Configuration of the magnetosphere‐ionosphere convection system under northward IMF conditions with nonzero IMF ByJournal of Geophysical Research, 1999