Results 101 to 110 of about 5,027 (230)
COVEN: Providing a Variety of Threshold‐Based Forecasts for the Outer Radiation Belt
Abstract We present a suite of VAMPIRE (Van Allen belt Multi‐day Predictions by Implementing a Random Forest for Electrons) models capable of predicting if the outer radiation belt crosses set percentile thresholds. We use Random Forest classification models to predict if the daily ∼2 MeV electron flux level across the outer radiation belt exceeds ...
D. J. Weston +3 more
wiley +1 more source
Magnetospheres of the outer planets [PDF]
The five qualitatively different types of magnetism that a planet body can exhibit are outlined. Potential sources of energetic particles in a planetary magnetosphere are discussed. The magnetosphere of Uranus and Neptune are then described using Pioneer
Vanallen, James A.
core +1 more source
Triggering the Magnetopause Reconnection by Solar Wind Discontinuities
Magnetic reconnection is one of the most universal processes in space plasma that is responsible for charged particle acceleration and the mixing and heating of plasma populations.
Alexander Lukin +6 more
doaj +1 more source
Investigating Potential Benefits of Future Sub‐L1 Missions With STEREO‐A
Abstract We present the first statistical study of geomagnetic storm forecasting using in situ data from the STEREO‐A spacecraft as a sub‐L1 monitor. Between November 2022 and June 2024, STEREO‐A crossed the Sun–Earth line, covering longitudinal and radial separations of ±15° $\pm 15{}^{\circ}$ from the Sun–Earth line and 0.01–0.06 au from Earth.
E. Weiler +6 more
wiley +1 more source
Current status of models of Jupiter's magnetosphere in the light of Pioneer data [PDF]
The salient features of the various models of Jupiter's magnetosphere are compared with each other and with the major findings of Pioneer 10 and 11. No single model explains all the major phenomena detected by the Pioneers.
Auer, P., Prakash, A.
core +1 more source
Radial Evolution of Turbulence Spectra on the Jovian Magnetosheath Flanks: Juno Observations
The Jovian magnetosheath provides a unique environment for examining the radial evolution of magnetosheath turbulence due to its large spatial extent.
Hui Li +3 more
doaj +1 more source
Abstract The Kelvin‐Helmholtz instability (KHI) mediates the viscous‐like solar‐terrestrial interaction by generating magnetopause surface waves that quickly become non‐linear. Basic theory predicts the locally most‐unstable linear wave dominates.
H. M. Kelly +5 more
wiley +1 more source
STRUCTURE AND DYNAMICS OF PLANETARY MAGNETOSPHERES
The interactions between the ambient plasmas and the objects of the Solar System result in variable exchanges both in time and space of mass, momentum and energy within different types of magnetospheres. The characterization of the sources, the general circulation and the losses of the magnetospheric plasmas as well as the identification of the ...
openaire +1 more source
Energetic particles of the outer regions of planetary magnetospheres [PDF]
High energy particles, with energies above those attainable by adiabatic or steady-state electric field acceleration, have been observed in and around the outer regions of planetary magnetospheres.
Bratenahl, A. +2 more
core +1 more source
Regional and Seasonal Effects of Geomagnetic Storms on Terrestrial Weather
Abstract It has long been a mystery why small Total Solar Irradiation changes have significant effects on Earth's climate. Solar cycle correlation studies abound but cannot conclusively point to a viable physical mechanism. Here, I show that geomagnetic storms have a profound terrestrial weather impact.
J. Raeder
wiley +1 more source

