Results 61 to 70 of about 5,188 (295)
Planetary magnetospheres [PDF]
A concise overview is presented of our understanding of planetary magnetospheres (and in particular, of that of the Earth), as of the end of 1981. Emphasis is placed on processes of astrophysical interest, e.g., on particle acceleration, collision-free ...
Ness, N. F., Stern, D. P.
core +1 more source
The Keplerian regime of charged particles in planetary magnetospheres
The dynamics of a charged particle orbiting around a rotating magnetic planet is studied. The system is modelled by the two-body Hamiltonian perturbed by an axially-symmetric function which goes to infinity as soon as the particle approaches the planet. The perturbation consists in a magnetic dipole field and a corotational electric field.
Jesús Palacián +6 more
openaire +3 more sources
Observation of a Knotted Electron Diffusion Region in Earth's Magnetotail Reconnection
Abstract Magnetic reconnection is a fundamental plasma process that alters the magnetic field topology and releases magnetic energy. Most numerical simulations and spacecraft observations assume a two‐dimensional diffusion region, with the electron diffusion region (EDR) embedded in the same plane as the ion diffusion region (IDR) and a uniform guide ...
Xinmin Li +8 more
wiley +1 more source
Using Mars Atmosphere and Volatile EvolutioN Magnetometer observations, we report the first statistical study of ultralow frequency (ULF) waves at the Martian foreshock.
Nahuel Andrés +5 more
doaj +1 more source
Detection of Equatorial Plasma Velocity Modulations Associated With Planetary Period Oscillations in Saturn's Magnetosphere [PDF]
T. J. Bradley +3 more
openalex +1 more source
Extreme Magnetopause Deformation Induced by High‐Speed Jet From Foreshock Transient
Abstract This study presents comprehensive observations of intense high‐speed jets (HSJs) and their global impacts on the inner magnetosphere and ionosphere, using multi‐satellite and ground‐based observations. Cluster‐4, located near the bow shock, observed signatures associated with foreshock transients generated by a solar wind directional ...
Hyangpyo Kim +8 more
wiley +1 more source
Mercury’s plasma environment after BepiColombo’s third flyby
Understanding Mercury’s magnetosphere is crucial for advancing our comprehension of how the solar wind interacts with the planetary magnetospheres. Despite previous missions, several gaps remain in our knowledge of Mercury’s plasma environment.
Lina Z. Hadid +24 more
doaj +1 more source
Continuum radiation in planetary magnetospheres [PDF]
With the completion of the Voyager tour of the outer planets, radio and plasma wave instruments have executed the first survey of the wave spectra of Earth, Jupiter, Saturn, Uranus, and Neptune.
Kurth, W. S.
core +1 more source
ENA imaging simulation of the distant planetary magnetosphere and ENA emission discussion of the solar wind [PDF]
Li Lü +4 more
openalex +1 more source
Abstract Geomagnetically Induced Currents (GICs) are a hazard to power systems. In this letter, we present a case study to understand why a Sudden‐Commencement‐associated 20A GIC spike, measured at mid‐latitude in Virginia, US, increased to 30A within 2 min of interplanetary shock arrival.
Bhagyashree Waghule +3 more
wiley +1 more source

