Results 211 to 220 of about 1,721,894 (339)
Global MHD Simulations: Magnetosphere–Ionosphere Coupling Dependence on Conductance Model
Abstract Eighty‐five geomagnetic storms were simulated with the space weather modeling framework Geospace model using two different ionospheric conductance models. One set used the legacy conductances within the Ridley ionosphere model, while the other set used the newly developed conductance model for extreme events conductance model.
T. I. Pulkkinen +9 more
wiley +1 more source
High Energy Neutrino Astrophysics
V. J. Stenger +3 more
openaire +3 more sources
Extreme properties of a compact and massive accreting black hole host in the first 500 Myr. [PDF]
Tripodi R +31 more
europepmc +1 more source
Astrophysics Uniquely Enabled by Observations of High-Energy Cosmic Neutrinos [PDF]
M. Ackermann
openalex +1 more source
Abstract The Geospace Dynamics Constellation (GDC) mission aims to investigate the dynamic coupling between the magnetosphere, ionosphere, and thermosphere by resolving key spatiotemporal processes at scales ranging from local to global. A key aspect is GDC's ability to reconstruct hemispheric‐scale high‐latitude electrodynamics with comprehensive ...
J. S. Shim +6 more
wiley +1 more source
A young progenitor for the most common planetary systems in the Galaxy. [PDF]
Livingston JH +41 more
europepmc +1 more source
Editorial: High-energy astrophysics research enabled by the probe-class mission concept HEX-P [PDF]
Daniel Stern +2 more
openalex +1 more source
Abstract We investigate the empirical relationship between the spacecraft potential (Vs) measured by the Electric Field Double Probes, and the electron density (Ne) measured by the Fast Plasma Instrument on the MMS spacecraft. We derive their relationship during fast‐mode intervals when the Active Spacecraft Potential Control Devices are off.
H. Laakso +4 more
wiley +1 more source
Superluminous supernovae: diverse rise times explain diverse spectra. [PDF]
Nicholl M.
europepmc +1 more source
Abstract Loss of relativistic electrons with energies above 0.5 MeV through the magnetopause, commonly referred to as magnetopause shadowing, has been extensively investigated using both simulations and observations. However, direct and systematic observational evidence remains limited. In this study, we extend a previously developed magnetopause model
Kyung‐Chan Kim, Dae‐Young Lee
wiley +1 more source

