Results 91 to 100 of about 9,065 (177)
Europa is Embedded in Non‐Maxwellian, Anisotropic Electron Distributions
Abstract In September 2022, the Juno spacecraft flew by Europa, providing new insight into the electron pitch angle and energy distributions via the Jovian Auroral Distributions Experiment electron analyzers (JADE‐E). We fit these observations with two anisotropic kappa distributions (cold and hot), accounting for spacecraft potential, which we find to
S. P. Ellis +10 more
wiley +1 more source
FOXTAIL is a new hybrid magnetohydrodynamic-kinetic code used to describe interactions between energetic particles and Alfv\'en eigenmodes in tokamaks with realistic geometries.
Hellsten, Torbjörn +2 more
core +1 more source
Short‐Term Variability of Jupiter's Satellite Footprints as Spotted by JWST
Abstract We present the main Alfvén wing (MAW) spots of Io and Europa as observed by the Near‐Infrared Spectrograph onboard the James Webb Space Telescope. These auroral footprint features have been measured previously, but only in emission. Here, the derived ionospheric H3+ ${\mathrm{H}}_{3}^{+}$ emission, temperature and column density are reported ...
Katie L. Knowles +10 more
wiley +1 more source
Nonlinear wave interaction and spin models in the MHD regime
Here we consider the influence on the electron spin in the MHD regime. Recently developed models which include spin-velocity correlations are taken as a starting point. A theoretical argument is presented, suggesting that in the MHD regime a single fluid
Brodin G +12 more
core +1 more source
Electron heating in kinetic-Alfvén-wave turbulence. [PDF]
Zhou M, Liu Z, Loureiro NF.
europepmc +1 more source
The coronal heating problem has been a major challenge in solar physics, and a tremendous amount of effort has been made over the past several decades to solve it.
Tong Shi +8 more
doaj +1 more source
Wave-particle energy exchange directly observed in a kinetic Alfvén-branch wave
Alfvén waves are fundamental plasma modes that provide a mechanism for the transfer of energy between particles and fields. Here the authors confirm experimentally the conservative energy exchange between Alfvén wave fields and plasma particles via high ...
Daniel J. Gershman +19 more
doaj +1 more source
Modeling the Effects of a Light Bridge on Properties of Magnetohydrodynamic Waves in Solar Pores
Solar pores are ideal magnetic structures for wave propagation and transport of energy radially outwards across the upper layers of the solar atmosphere.
Luiz A. C. A. Schiavo +9 more
doaj +1 more source
Direct Evidence for Two-Fluid Effects in Molecular Clouds
We present a combination of theoretical and simulation-based examinations of the role of two-fluid ambipolar drift on molecular line widths. The dissipation provided by ion-neutral interactions can produce a significant difference between the widths of ...
Ballesteros-Paredes +28 more
core +1 more source
Prevalence of Small-scale Jets from the Networks of the Solar Transition Region and Chromosphere
As the interface between the Sun's photosphere and corona, the chromosphere and transition region play a key role in the formation and acceleration of the solar wind.
Boerner, P. +26 more
core +1 more source

