Results 211 to 220 of about 61,376 (298)

Multiscale modelling of the impact of solar arrays on a spacecraft electrostatic charging.

, 2017
Antoine Brunet
openalex   +1 more source

Universal Portable Functional Control System for Small Spacecraft Onboard Equipment

, 2019
Stanislav Podshivalov, Alexander Zlobin, Т.В. Кондранин, Sergey Negodyaev   +3 more
openalex   +1 more source

Multiple Reconnection X‐Lines at the Earth's Magnetopause in the Presence of Magnetosheath Flow

Journal of Geophysical Research: Space Physics, Volume 131, Issue 3, March 2026.
Abstract Magnetic reconnection occurs continuously along long X‐lines at the Earth's magnetopause. The maximum magnetic shear model predicts the locations of these long X‐lines for a wide range of upstream solar wind conditions. One of the more perplexing observational results is that these X‐lines appear to be stationary, even in the presence of ...
S. A. Fuselier, K. J. Trattner, S. M. Petrinec, S. K. Vines, K. LLera, N. Aunai, B. Michotte de Welle, A. Ghisalberti, J. L. Burch, D. J. Gershman   +9 more
wiley   +1 more source

Martian ionospheric response during the may 2024 solar superstorm. [PDF]

Nat Commun
Parrott J, Sánchez-Cano B, Svedhem H, Witasse O, Meggi D, Wilson C, Cardesín-Moinelo A, Müller-Wodarg I.   +7 more
europepmc   +1 more source

Propagation Velocities and Growth Rates of Short Large‐Amplitude Magnetic Structures (SLAMS) in the Foreshock of Earth

Journal of Geophysical Research: Space Physics, Volume 131, Issue 3, March 2026.
Abstract Short Large‐Amplitude Magnetic Structures (SLAMS) are believed to play important roles in the physics governing the formation of quasi‐parallel shocks. These isolated non‐linear structures, frequently observed in the foreshock, have been suggested to be building blocks for the shock and have been shown to drive shock reformation. In this work,
S. Bergman, T. Karlsson, T. K. Wong Chan
wiley   +1 more source

The Tandem Reconnection and Cusp Electrodynamics Reconnaissance Satellites (TRACERS) Science Operations Center. [PDF]

Space Sci Rev
Christopher IW, Kletzing CA, Crawford D, Piker C, Wilkinson D, Steele K, Petrinec SM, Bounds S, Vaclavik S, Omar S, Shults E, Winter M, Miles DM.   +12 more
europepmc   +1 more source

Compression of Mercury's Dayside Magnetopause to the Surface: A Three‐Dimensional Model of Magnetospheric Structure and Dynamics

Journal of Geophysical Research: Space Physics, Volume 131, Issue 3, March 2026.
Abstract We apply a hybrid model (kinetic ions, fluid electrons) to provide context for MErcury Surface Space ENvironment, GEochemistry, and Ranging (MESSENGER) observations of Disappearing Dayside Magnetosphere (DDM) events at Mercury. Such events have been observed on four occasions and are caused by Coronal Mass Ejections completely removing the ...
Georg Glebe, C. Michael Haynes, Sven Simon   +2 more
wiley   +1 more source

Electromagnetic viscosity supported anomalous electric field in the electron diffusion region of collisionless magnetic reconnection. [PDF]

Nat Commun
Zhong ZH, Zhou M, Graham DB, Pang Y, Khotyaintsev YV, Song LJ, Li HM, Tang RX, Deng XH.   +8 more
europepmc   +1 more source

A Concluded Nanotechnology based Spacecraft

, 2014
T. Sivakumar
openalex   +1 more source

Early Solar Wind and Dynamo Magnetic Field Topology Predictions for (16) Psyche and Other Asteroids

Journal of Geophysical Research: Planets, Volume 131, Issue 3, March 2026.
Abstract Asteroid (16) Psyche is a metal‐rich body that might record an ancient coherent magnetization if some relict crust or mantle is preserved. Herein, we use magnetohydrodynamic simulations to predict (16) Psyche's field topology for several distinct pathways: (i) an early solar wind‐induced magnetization imparted after a larger body was impacted,
Atma Anand, Jonathan Carroll‐Nellenback, Eric G. Blackman, John A. Tarduno   +3 more
wiley   +1 more source