Results 231 to 240 of about 128,880 (312)
Abstract We present a case study of large amplitude, compressional Pc5 waves observed by GOES 13 and 15 at geosynchronous orbit near noon. These waves were excited near the arrival time of two consecutive solar wind dynamic pressure spikes at the magnetopause, the second of which was associated with a large and rapid southward turning of the ...
C. Lazzeri +8 more
wiley +1 more source
Towards a Global Scale Quantum Information Network: A Study Applied to Satellite-Enabled Distributed Quantum Computing. [PDF]
de Forges de Parny L +10 more
europepmc +1 more source
Perspectives of Earth and Space Scientists, Volume 7, Issue 1, December 2026.
Li Li
wiley +1 more source
Abstract Visible spectra of the Enceladus particle plume and E ring contain evidence for a change in spectral slope around 0.5 μm. This feature can be seen in data obtained by both the Visual and Infrared Mapping Spectrometer and Imaging Science Subsystem onboard the Cassini Spacecraft, and is consistent with the slope change seen in the surface ...
M. M. Hedman, S. M. MacKenzie
wiley +1 more source
Polarimetric calibration of the Tunable Magnetograph for the Sunrise III mission
Campos-Jara A +9 more
europepmc +1 more source
Analysis of HERV-K (HML2) Expression in Colorectal Cancer Samples. [PDF]
Obrezanenko VS +21 more
europepmc +1 more source
Abstract Cosmic rays (CRs) are energetic particles originating from galactic and extragalactic sources. When arriving into the solar system and the Sun's heliosphere, they are diverted and modulated by the magnetic activity of the Sun. This modulation can be quantified by the modulation parameter ϕ $\phi $ determined with the Force‐field approximation (
Pauli Väisänen +5 more
wiley +1 more source
Exploring the extremes: The cosmic laboratory. [PDF]
Huang Y, He S, Ge L, Li Z, Mao Y, Liu J.
europepmc +1 more source
Jovian Auroral Proton Precipitation
Abstract The total power of the Jovian aurora is about 1013–1014 W with ultraviolet emission observed in the Lyman and Werner bands of molecular hydrogen. X‐ray, radio, and infrared emissions have also been observed. The Jovian Auroral Distributions Experiment and the Jovian Energetic Particle Detector Instrument onboard the Juno spacecraft, orbiting ...
S. J. Houston +4 more
wiley +1 more source

