Results 161 to 170 of about 39,453 (210)
3D volumetric tomography of clouds using machine learning for climate analysis. [PDF]
Ronen R+5 more
europepmc +1 more source
Ionospheric Scintillation and Geomagnetic Disturbance Caused by Space Hurricanes
Abstract A space hurricane is a large‐scale, cyclone‐shaped aurora characterized by a rotating magnetic structure and shears in plasma convection, driven by high‐latitude magnetic reconnection. It typically forms near the magnetic poles in summertime, providing an efficient energy transport channel from the solar wind to the Earth's magnetosphere under
Sheng Lu+13 more
wiley +1 more source
Tracing the inner edge of the habitable zone with sulfur chemistry. [PDF]
Jordan S, Shorttle O, Rimmer PB.
europepmc +1 more source
Beacon2Science: Enhancing STEREO/HI Beacon Data With Machine Learning for Efficient CME Tracking
Abstract Observing and forecasting coronal mass ejections (CMEs) in real‐time is crucial due to the strong geomagnetic storms they can generate that can have a potentially damaging effect, for example, on satellites and electrical devices. With its near‐real‐time availability, Solar TErrestrial RElations Observatory‐heliospheric imagers (STEREO/HI ...
J. Le Louëdec+3 more
wiley +1 more source
Impact-driven oxidation of organics explains chondrite shock metamorphism dichotomy. [PDF]
Kurosawa K+5 more
europepmc +1 more source
NOAA's National Centers for Environmental Information Space Weather Data Inventory Status
Abstract We present here an updated overview of the Space Weather data curated and/or generated, improved, archived, and disseminated by the Solar Terrestrial Physics (STP) Section of the National Centers for Environmental Information (NCEI) in the National Oceanic and Atmospheric Administration (NOAA).
Alessandra Abe Pacini+2 more
wiley +1 more source
Revealing an unexpectedly low electron injection threshold via reinforced shock acceleration. [PDF]
Raptis S+5 more
europepmc +1 more source
Evaluating the Parker Model With the Trans‐Heliospheric Survey
Abstract The solar wind's expansion through the heliosphere is often studied by “radial trends”—the average trends in fluid parameters as functions of radial distance from the Sun. This study utilizes the latest version of the Trans‐Heliospheric Survey, a compilation of in‐situ magnetic field and proton measurements from 13 different spacecraft ...
Carson P. Brown+6 more
wiley +1 more source
Io's tidal response precludes a shallow magma ocean. [PDF]
Park RS+20 more
europepmc +1 more source
Abstract We present a novel method to quantify the event‐specific spatial evolution of plasmaspheric hiss wave power using a Drift‐Diffusion model. Constrained by Polar Operational Environmental Satellites/Meteorological Operational Satellites data, the model simulates low‐altitude electron distributions, accounting for azimuthal drift, pitch‐angle ...
Zhi‐Gu Li+4 more
wiley +1 more source