Results 301 to 310 of about 536,719 (375)
Quantum Entanglement Asymmetry and the Cosmic Matter-Antimatter Imbalance: A Theoretical and Observational Analysis. [PDF]
Neukart F.
europepmc +1 more source
On the Possibility of Driving the Electron Flux Probabilistic Models by the AE Index
Abstract We present the new probabilistic model of the electron fluxes designed to assess the risks of the spacecraft surface charging for missions with near‐equatorial orbits in the inner magnetosphere. It is a second model developed within a frame of the European Space Agency's activity “Plasma Environment Modeling in the Earth's Magnetosphere ...
S. Dubyagin +8 more
wiley +1 more source
Signal Processing for the Cluster Wideband Data Burst Mode
Abstract The Wideband Data instrument is part of the Cluster spacecraft Wave Experiment Consortium. Its primary data path is a direct connection to the spacecraft data handling system providing real time downlink to the ground stations of the Deep Space Network and Panska Ves Observatory.
K. H. Yearby +2 more
wiley +1 more source
Magnetic Confinement of a Bubble of Supercooled <sup>3</sup>He-A. [PDF]
Whitehead L +11 more
europepmc +1 more source
Gamma-ray cosmology in the upcoming CTAO era [PDF]
Lucas Gréaux, J. Biteau, E. Pueschel
openalex +1 more source
Abstract Whistler‐mode chorus waves play a key role in driving radiation belt dynamics by enabling both acceleration of electrons to relativistic energies as well as their loss into the atmosphere via pitch‐angle scattering. The ratio between the electron plasma frequency (fpe ${f}_{pe}$) and the electron gyrofrequency (fce ${f}_{ce}$) significantly ...
K. A. Bunting +5 more
wiley +1 more source
Challenges to the [Formula: see text]CDM cosmology. [PDF]
Efstathiou G.
europepmc +1 more source
Differentiating Plumes and Local Torus Segments of Enceladus
Abstract Enceladus's south polar plumes and their surrounding torus segments (local plasma regions formed by plume material diffusion) are key to understanding its magnetospheric interaction; however, clear observational criteria to distinguish them remain lacking.
Shangchun Teng +6 more
wiley +1 more source
Could dark energy be changing over time? [PDF]
Mann A.
europepmc +1 more source

