Results 71 to 80 of about 2,730 (182)
Abstract Precise characterization of the electron density profile is crucial for optimizing high frequency communications. Reconstruction models often assume an instantaneous ionospheric response to solar forcing or using time delays, neglecting the time‐integrated cumulative “memory effect” of plasma dynamics.
Hongwei Gong +9 more
wiley +1 more source
Abstract On 10 May 2024, Earth was hit by a CME that drove the largest geomagnetic storm in 20 years. Multi‐spacecraft observations previously showed that the ∼100 nT north‐south IMF bz ${b}_{z}$ variation was driven by Kelvin‐Helmholtz waves with wavelength ∼250 RE ${R}_{E}$ and reconnection jets in the ±z $\pm z$‐direction (Nykyri, 2024a, https://doi.
Katariina Nykyri +17 more
wiley +1 more source
Operational prediction of solar flares using a transformer-based framework. [PDF]
Abduallah Y, Wang JTL, Wang H, Xu Y.
europepmc +1 more source
Driving Influences of the Doppler Flash Observed by SuperDARN HF Radars in Response to Solar Flares. [PDF]
Chakraborty S +5 more
europepmc +1 more source
Prolonged Photosensitivity Following Exposure to Glyphosate Herbicide
Photodermatology, Photoimmunology &Photomedicine, Volume 42, Issue 5, September 2026.
Jean Ayer +2 more
wiley +1 more source
Four New Horsemen of an Apocalypse? Solar Flares, Super-volcanoes, Pandemics, and Artificial Intelligence. [PDF]
Noy I, Uher T.
europepmc +1 more source
Survey of electron density changes in the daytime ionosphere over the Arecibo observatory due to lightning and solar flares. [PDF]
da Silva CL +3 more
europepmc +1 more source
Turbulent acceleration in solar flares [PDF]
AbstractTurbulent acceleration in the impulsive phase of solar flares is reviewed, with the emphasis on bulk energization of nonrelativistic electrons and prompt acceleration of the gamma-ray emitting nonrelativistic ions and relativistic electrons. The primary energy release in a flare cannot be due to collisional dissipation.
openaire +1 more source
We present a comprehensive study of type III radio bursts and their association with solar flares of magnitude M1.0 and larger, as observed by four widely separated spacecraft (Parker Solar Probe, Solar Orbiter, STEREO-A, and Wind). Our main focus is the
Vratislav Krupar +10 more
doaj +1 more source

