Results 51 to 60 of about 1,276 (215)
Abstract Soft proton contamination presents a persistent threat to the performance of space‐based X‐ray observatories such as ESA's upcoming Solar‐wind Magnetosphere Ionosphere Link Explorer (SMILE). This study develops a machine‐learning framework for modeling soft proton fluxes in the 92.2–159.7 keV range, tailored to SMILE's elliptical, highly ...
Simon Mischel +2 more
wiley +1 more source
3D propagation of relativistic solar protons through interplanetary space [PDF]
Context. Solar Energetic Particles (SEPs) with energy in the GeV range can propagate to Earth from their acceleration region near the Sun and produce Ground Level Enhancements (GLEs).
Marsh, M.S +23 more
core +1 more source
Turbulent Magnetic Reconnection as an Acceleration Mechanism in Earth’s Magnetotail
Using electric and magnetic fields measured by the Magnetospheric Multiscale (MMS) mission, we construct a test-particle simulation of a turbulent magnetic reconnection region to investigate observed ion acceleration. We identify three types of energized
Daniel D. Sega, Robert E. Ergun
doaj +1 more source
Abstract We estimate the cosmic dust flux to Earth through the study of rare micrometeorites that preserve part of their precursor features during atmospheric entry heating, namely unmelted and scoriaceous subtypes. Combining high‐precision mass balance measurements, X‐ray computed microtomography and scanning electron microscopy, we studied mass, size
S. Ottaviani +7 more
wiley +1 more source
Interhemispheric comparison of spectral width boundary as observed by the SuperDARN radars [PDF]
International audiencePrevious studies have shown that dayside equatorward edge of coherent HF radar backscatter having broad Doppler spectral width is coincident with the equatorward edge of the cusp particle precipitation.
Milan, S. E. +23 more
core +1 more source
The radial evolution of particles accelerated at corotating interaction regions (CIRs) is not fully understood, particularly the distance range over which this particle acceleration occurs and how the energy spectra are modulated by transport through the
M. J. Starkey +5 more
doaj +1 more source
Observing the Earth's Plasmasphere and Ionosphere From the Lunar Surface
Abstract We present the analysis of the first lunar‐based observational characterization of the Earth's plasmasphere and ionosphere using Global Navigation Satellite Systems signals tracked from the lunar surface by the Lunar GNSS Receiver Experiment (LuGRE). The Earth‐Moon geometry enables limb sounding of the plasmasphere at altitudes exceeding 3,000
C. Cesaroni +8 more
wiley +1 more source
Radial evolution of interplanetary coronal mass ejection-associated particle acceleration observed by Solar Orbiter and ACE [PDF]
On 2022 March 10 a coronal mass ejection erupted from the Sun, resulting in Solar Orbiter observations at 0.45 au of both dispersive solar energetic particles arriving prior to the interplanetary coronal mass ejection (ICME) and locally accelerated ...
Mason, G. M. +7 more
core +2 more sources
Turbulence-driven Anisotropic Acceleration of Energetic Electrons in Solar Wind Current Sheets
Coherent structures in the solar wind, such as current sheets, are widely recognized as potential sites for energy dissipation and particle acceleration.
L. D. Wang +8 more
doaj +1 more source
Modulation of cosmic-ray ground-level enhancements by solar-wind stream interfaces: a case study [PDF]
Ground-level enhancements (GLEs) provide crucial insights into the acceleration and transport of solar energetic particles (SEPs). We present a comprehensive analysis of GLE 72, which occurred on 10 September 2017, coinciding with a solar-wind stream ...
O. Ogunjobi, O. Ogunjobi, W. T. Sivla
doaj +1 more source

