Results 81 to 90 of about 3,269,942 (182)
Positive Association Between Coastal Sea Surface Temperatures and Humid Heat Stress on Nearby Land
Abstract Large populations along Earth's coastlines are exposed to climate hazards including extreme humid heat. Considering observed coastal ocean warming and increased coastal marine heatwave (MHW) activity, we seek to uncover if, how, and where coastal ocean temperatures are linked with heat and humidity on land nearby.
Noel V. A. Siegert, Radley M. Horton
wiley +1 more source
Coronal mass ejections (CMEs) on stars can change the stars’ magnetic field configurations and mass-loss rates during the eruption and propagation and therefore, may affect the stars’ rotation properties on long timescales.
Yu Xu +5 more
doaj +1 more source
Stellar Coronal Mass Ejections with HWO: A Science Case Concept
The primary mission of the Habitable World Observatory (HWO) will be to constrain the prevalence of life on Earth-like planets. These planets will be subject to impacts by energetic particles generated from coronal mass ejection (CME) shocks that can dramatically deplete ozone, a key biosignature gas.
Loyd, R. O. Parke +5 more
openaire +2 more sources
Interplanetary Type IV Solar Radio Bursts: A Comprehensive Catalog and Statistical Results
Decameter hectometric (DH; 1–14 MHz) type IV radio bursts are produced by flare-accelerated electrons trapped in postflare loops or the moving magnetic structures associated with the coronal mass ejections (CMEs).
Atul Mohan +4 more
doaj +1 more source
Doppler-shifted Signatures in the Chromospheric Line Profiles of II Pegasi
Stellar flares are frequently accompanied by prominence eruptions, coronal mass ejections (CMEs), and other forms of plasma motion. Based on the long-term high-resolution spectroscopic monitoring data set of the RS CVn-type star II Pegasi (II Peg), we ...
Dongtao Cao, Shenghong Gu
doaj +1 more source
(Exo)planetary environments are forced by stellar activity, which manifest through variable radiation, particle and magnetic fluxes, stellar winds, flares, and magnetic storms known as coronal mass ejections (CMEs). Recent studies have shown that planets
Sakshi Gupta, Souvik Roy, Dibyendu Nandy
doaj +1 more source
Coronal mass ejections (CMEs) are among the most energetic phenomena in our solar system, with significant implications for space weather. Understanding their early dynamics remains challenging due to observational limitations in the low corona.
Shantanu Jain +4 more
doaj +1 more source
Young solar-type stars frequently produce superflares, serving as a unique window into the young Sun-Earth environments. Large solar flares are closely linked to coronal mass ejections (CMEs) associated with filament/prominence eruptions, but ...
Kosuke Namekata +16 more
doaj +1 more source
Where are the stellar coronal mass ejections?
Flares and coronal mass ejections (CMEs) can have serious effects on their surroundings: they can erode or completely destroy atmospheres of orbiting planets over time and also have high importance in stellar evolution.
Krisztián Vida +8 more
core +1 more source
We carry out this study on the solar energetic particle (SEP) event that occurred on 2023 August 5 over the ascending phase of the current solar cycle 25.
Kazi A. Firoz, Y. P. Li, W. Q. Gan
doaj +1 more source

