Results 101 to 110 of about 1,655 (241)
Abstract Solar eclipses provide unique opportunities to investigate geospace dynamics driven by rapid, localized reductions in solar radiation. On December 4th $4\text{t}\text{h}$, 2021, a total solar eclipse occurred over West Antarctica during substorms.
Yu Hong +11 more
wiley +1 more source
Foreshock Ion Properties at Earth's Bow Shock: Dependence on Upstream Conditions and Shock Geometry
Abstract Solar wind ion reflection at collisionless shocks regulates foreshock plasma dynamics, yet the quantitative dependence of foreshock ion properties on upstream and shock‐related parameters remains unclear, causing difficulties in predicting foreshock disturbances.
Runyi Liu +4 more
wiley +1 more source
Ray Tracing Method in a General Non‐Dipole Magnetic Field
Abstract We present a new general mathematical formulation of the Eikonal equations for ray tracing, which can use any internal magnetic field model. The analytical and tractable expressions are conveniently based on a vector formalism, which is independent of any coordinate system.
P.‐L. Blelly +4 more
wiley +1 more source
The Energy Cascade Rate in Supersonic Magnetohydrodynamic Turbulence
Three-dimensional direct numerical simulations are implemented to investigate the energy cascade rate in compressible isothermal magnetohydrodynamic turbulence. Utilizing an exact law derived from the Kármán–Howarth equation, we examine the contributions
Gonzalo Javier Alvarez +4 more
doaj +1 more source
Dayside Polar Cap Aurora and Their Connection to NBZ Currents
Abstract During northward interplanetary magnetic field (IMF) conditions, magnetic reconnection between the Earth's magnetosphere and the IMF takes place on high latitudes, causing the auroral oval to contract. During those times several auroral structures may appear inside the polar cap, such as cusp aurora, high latitude dayside aurora (HiLDA) and ...
Maria Chloi Katrougkalou +4 more
wiley +1 more source
Spatiotemporal Properties of Compressible Magnetohydrodynamic Turbulence from Space Plasma
It is well established that Alfvénic turbulence undergoes a weak-to-strong transition as energy cascades to smaller scales, but whether this occurs in compressible magnetohydrodynamic (MHD) turbulence remains unclear.
Siqi Zhao +4 more
doaj +1 more source
Abstract A key process in solar‐terrestrial interactions is magnetic reconnection at the magnetopause. In addition to in situ observations of plasma entry at the magnetopause, some of the important global aspects of magnetic reconnection are addressed using plasma observations in the Earth's magnetospheric cusp region. Ions injected at the magnetopause
K. J. Trattner +22 more
wiley +1 more source
Abstract The Cassini spacecraft spent 13 years orbiting Saturn, quasi‐continuously measuring Saturn's radio emissions. One of the key elements of the radio spectrum at Saturn is the Saturn Kilometric Radiation (SKR), and several studies have been written on events called Low Frequency Extensions (LFEs) which represent strong, continuous extensions of ...
C. M. Jackman +11 more
wiley +1 more source
Plasma turbulence is a ubiquitous dynamical process that transfers energy across many spatial and temporal scales and affects energetic particle transport.
Siqi Zhao +4 more
doaj +1 more source
The Species‐ and Energy‐Dependent Effects of EMIC Waves on Ring Current Ions
Abstract Wave‐particle interactions are a major mechanism responsible for dissipating energy and redistributing particles within geospace. This study investigates the effects of electromagnetic ion cyclotron waves on ring current ions. We present a case study of the effects of EMIC waves on the ring current during the 15 August 2015 geomagnetic storm ...
Cristian P. Ferradas +5 more
wiley +1 more source

