Results 101 to 110 of about 13,189 (224)
Abstract The 1–100 keV electron precipitation during storm time has been studied by applying the updated ELSPEC inversion method to field‐aligned electron density profiles measured by the EISCAT Tromsø radar at L = 6.5. The statistical properties of peak energy, total energy flux, and total number flux as a function of MLT have been studied for the two
N. M. Ellahouny +6 more
wiley +1 more source
Coronal shocks associated with CMEs and flares and their space weather consequences
We study the geoeffectiveness of a sample of complex events; each includes a coronal type II burst, accompanied by a GOES SXR flare and LASCO CME. The radio bursts were recorded by the ARTEMIS-IV radio spectrograph, in the 100-650 MHz range; the GOES SXR
A. Hillaris +7 more
core +1 more source
Abstract The May 2024 superstorm, as the most intense geomagnetic storm since 2003, caused a variety of disturbances in the magnetosphere‐ionosphere‐thermosphere system. This study investigates the long‐lasting electron density depletion in the polar region and the underlying ionosphere‐thermosphere coupling, based on a comprehensive set of ...
Lei Cai +8 more
wiley +1 more source
SPACE WEATHER AND A STATE OF CARDIOVASCULAR SYSTEM OF HUMAN BEING WITH A WEAKENED ADAPTATION SYSTEM
As has been shown in [Samsonov et al., 2013] even at the considerable disturbances of space weather parameters a healthy human being did not undergo painful symptoms although measurements of objective physiological indices showed their changes.
S. N. Samsonov
doaj +1 more source
The SGR 1806-20 magnetar signature on the Earth's magnetic field
SGRs denote ``soft $\gamma$-ray repeaters'', a small class of slowly spinning neutron stars with strong magnetic fields. On 27 December 2004, a giant flare was detected from magnetar SGR 1806-20.
Alexandrescu +23 more
core +1 more source
Abstract Sudden changes in the ground magnetic field, driven by geomagnetic activity, can ultimately generate geomagnetically induced currents (GICs), which can have a significant impact on artificial technology systems. High rates of change in the horizontal geomagnetic field (dH/dt) can be used as a substitute for the strength of GICs.
C. M. Zhang +10 more
wiley +1 more source
Comparison between indices during geomagnetic disturbances
En este trabajo se comparan los índices aurorales AE, AU, AL y el índice PC de Troshichev, medido en Thule, durante perturbaciones geomagnéticas de distintas intensidades. Para la identificación de las mismas se han usado los índices Dst y AE. Se han analizado catorce tormentas, con valores mínimos de Dst entre -50 nT y -600 nT (86% de las cuales eran ...
Patricia Fernández de Campra +1 more
openaire +4 more sources
Forecasting Local Ionospheric Parameters Using Transformers
Abstract We present a novel method for forecasting key ionospheric parameters using transformer‐based neural networks. The model provides accurate forecasts and uncertainty quantification of the F2‐layer peak plasma frequency (foF2), the F2‐layer peak density height (hmF2), and total electron content for a given geographic location.
D. J. Alford‐Lago +4 more
wiley +1 more source
Segmentation and Tracking of Eruptive Solar Phenomena With Convolutional Neural Networks
Abstract Solar eruptive events are complex phenomena, which most often include coronal mass ejections (CME), CME‐driven compressive and shock waves, flares, and filament eruptions. CMEs are large eruptions of magnetized plasma from the Sun's outer atmosphere or corona, that propagate outward into the interplanetary space.
Oleg Stepanyuk, Kamen Kozarev
wiley +1 more source
Plasma pressure distribution in the inner magnetosphere is one of the key parameters for understanding the main magnetospheric processes including geomagnetic storms and substorms.
Antonova +41 more
core +1 more source

