Results 31 to 40 of about 4,955 (149)
Mercury's magnetospheric substorm and storm
Magnetospheric substorms and magnetic storms are explosive energy storage and release processes occurring during the interactions between the solar wind and planetary magnetospheres. They are accompanied by complex plasma dynamics processes and they have
Jiutong Zhao, Weijie Sun, Qiugang Zong
doaj +1 more source
Solar wind driving and magnetospheric preconditioning during omega band substorm events
Omega bands are mesoscale structures in the auroral oval that appear during periods of enhanced geomagnetic activity. Omega band formation has previously been associated with highly localized drivers in the magnetotail and global compression regions in ...
Vivian Cribb +8 more
doaj +1 more source
Quantifying Non‐Maxwellian Properties of Ion Populations During Reconnection at Earth's Magnetopause
Abstract We investigate ion velocity‐space features within the exhaust of magnetopause reconnection using a global hybrid‐Vlasov simulation. The Hermite transform and Gaussian Mixture Model (GMM) are applied to quantify the complexity of velocity‐space structures that arise during the mixing of magnetospheric and magnetosheath ion populations.
I. Zaitsev +7 more
wiley +1 more source
Recently we proposed a spatio-temporal model of auroral absorption for isolated substorms based on linear prediction filter technique, which describes the precipitation effects as a sum of properly weighted and time-delayed contributions of short ...
M. A. Shukhtina +2 more
doaj +1 more source
Altitude Dependence of Quasi‐Static Potential Drop: The Effect of Ionospheric Protons
Abstract Using an improved kinetic model that incorporates cold ionospheric protons and oxygen ions, we investigate the factors controlling the altitude range of the auroral acceleration region (AAR). In this model, parallel electric fields are generated via Dispersive Alfven Wave‐ Modified electron Acoustic Wave (DAW‐MEAW) coupling and sustained by ...
Run Shi +4 more
wiley +1 more source
Dynamic mesoscale flow structures move across the open field line regions of the polar caps and then enter the nightside plasma sheet where they can cause important space weather disturbances, such as streamers, substorms, and omega bands.
Larry R. Lyons +10 more
doaj +1 more source
Abstract This study presents a high‐resolution three‐dimensional global magnetohydrodynamic (MHD) simulation of the historic geomagnetic storm of 10–11 May 2024, using observational data for the ACE solar wind input. This extreme event was characterized by intense solar wind dynamic pressure (∼50 nPa) and exceptionally strong interplanetary magnetic ...
Kyung Sun Park
wiley +1 more source
Abstract At subauroral latitudes, discrete auroras, such as strong thermal emission velocity enhancement and stable auroral red arcs, have been extensively studied. On the other hand, diffuse emissions at subauroral latitudes have not been studied well.
M. Gomi +25 more
wiley +1 more source
CUTLASS/IMAGE observations of high latitude convection features during substorms [PDF]
International audienceThe CUTLASS Finland HF radar has been operational since February 1995. The radar frequently observes backscatter during the midnight sector from a latitude range 70?75° geographic, latitudes often associated with the polar cap ...
Lühr, H., Yeoman, T.K.
core +5 more sources
Convection Velocity Covariance Estimated From SuperDARN Observations
Abstract An examination of the spatial covariance of the high‐latitude plasma convection velocity is presented. The covariance was calculated from patterns of plasma convection estimated from Super Dual Auroral Radar Network observations. The convection patterns were calculated on a magnetic latitude—magnetic local time grid from 55° ${}^{\circ}$ to 88.
W. A. Bristow, M. F. Wilcox
wiley +1 more source

