Results 71 to 80 of about 584 (191)
Polytropic Index and Thermodynamic Behavior of the Central Plasma Sheet Near Lunar Distances
Abstract In addition to making near‐Earth observations, the THEMIS/ARTEMIS mission is uniquely positioned at lunar distance, in the deep magnetotail, reaching distances of 60 RE ${R}_{E}$ and further. This vantage point allows ARTEMIS to access the plasma sheet and measure entropy evolution across convective channels, plasma flow gradients ...
Ephrem Tesfaye Desta +2 more
wiley +1 more source
Theta Aurora: Transpolar Arcs Linked to a Folded Magnetotail Neutral Sheet
Abstract Nightside‐originating transpolar arcs (TPAs) represent a distinct mechanism of magnetosphere‐ionosphere energy transfer during northward IMF conditions. Nightside‐originating TPAs originate from the nightside auroral oval and grow across the polar cap to connect to the dayside, appearing to cross multiple topological boundaries as they develop.
S. C. Hill +9 more
wiley +1 more source
Collisionless electron–ion shocks are fundamental to astrophysical plasmas, yet their behavior in strong magnetic fields remains poorly understood.
Mohamad Shalaby +2 more
doaj +1 more source
Beyond the Electrostatic Approach: Numerical Simulations of Martian Ionospheric Irregularities
Abstract Numerical simulations play an essential role in the study of ionospheric irregularities. In the past few decades, electrostatic simulations have successfully simulated the nonlinear evolution of terrestrial ionospheric irregularities. However, the Mars Atmosphere and Volatile EvolutioN (MAVEN) observations reveal that the Martian ionospheric ...
Konghan Jiang, Jiuhou Lei, Maodong Yan
wiley +1 more source
Abstract The auroral‐like sporadic E‐layer is typically observed at altitudes between 100 and 150 km within the South American Magnetic Anomaly region. However, the occurrence of an unusual layer event detected above this altitude range on 18 July 2017 has raised intriguing questions regarding the physical processes responsible for the substantial ...
Lígia A. Da Silva +21 more
wiley +1 more source
How Plasma Properties of the Fanaroff–Riley Jet Can Shape Its Morphology
Extragalactic jets are broadly classified into two categories based on radio observations: core-brightened jets, known as Fanaroff–Riley Type I (FR I), and edge-brightened jets, classified as Type II (FR II).
Priyesh Kumar Tripathi +5 more
doaj +1 more source
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
Abstract We investigated the spatial distributions and pitch‐angle distributions of 30–300 eV H+ and O+ ion fluxes using data obtained by the low‐energy particle experiments‐ion mass analyzer (LEPi) onboard the Arase satellite. A statistical analysis over 3.7 years reveals that the H+ ion flux is enhanced at L > 4 from the premidnight sector through ...
Masahito Nosé +12 more
wiley +1 more source
Fundamental Poloidal Wave Event Extending From Midnight to Dawn
Abstract Fundamental poloidal (P1) waves are a class of magnetospheric standing Alfvén waves characterized by field line oscillations in the meridional plane. P1 waves are infrequently excited in the ring current region and are believed to be the source of giant pulsations (Pgs) observed on the ground. Pgs are mostly detected on the morning side with a
Kazue Takahashi +2 more
wiley +1 more source
This Version 2.1 release extends the theoretical IIMHD-Drive framework by adding supplementary simulation material. In addition to the main Version 2.0 PDF, this update includes: • a simple 1D Python toy-model (iimhd_simulation.py) illustrating velocity growth inside the MHD duct based on the analytical relations of the paper, • a README explaining ...
openaire +3 more sources

