Results 191 to 200 of about 78,655 (291)
Abstract This study investigated a large‐scale ionospheric irregularities event over low‐ to mid‐latitude China during the 1 December 2023 geomagnetic storm using ROTI data, loss‐of‐lock (LoL) in L2 from 250 GNSS receivers, and S4 data from 16 ISMs.
Yi Zeng +4 more
wiley +1 more source
Observation of sub-relativistic collisionless shock generation and breakout dynamics. [PDF]
Bai Y +6 more
europepmc +1 more source
The Prediction of Short‐Term Atmospheric Density in Lower Thermosphere
Abstract Accurate short‐term prediction of atmospheric density in the lower thermosphere (85–125 km) is essential for precise orbit determination and satellite drag mitigation, particularly during geomagnetic storms. Although physics‐based models such as NRLMSIS 2.1 provide empirical estimates, their effectiveness is limited under extreme space weather.
Zheng Li +4 more
wiley +1 more source
Magnetic reconnection in the plasma disk at 23 Jupiter radii. [PDF]
Wang JZ +9 more
europepmc +1 more source
Abstract Magnetotail current sheet (CS) flapping is a universal plasma phenomenon observed at multiple planets, yet its triggering mechanisms remain poorly understood outside of Earth. At Mars, single‐spacecraft observations have also reported tail flapping, but the processes responsible for its onset have never been identified.
Yuanzheng Wen +18 more
wiley +1 more source
Acceleration noise due to space magnetic field for heliocentric gravitational wave detector. [PDF]
Peng JH +6 more
europepmc +1 more source
Abstract Comprehension of the ophiolitic mélange plays a key role in the tectonic reconstruction of an ancient orogenic belt in terms of plate tectonics. The tectonic nature of the NNW‐trending southern Jinshajiang ophiolitic mélange is still controversial.
Di Xin +4 more
wiley +1 more source
Exploring the extremes: The cosmic laboratory. [PDF]
Huang Y, He S, Ge L, Li Z, Mao Y, Liu J.
europepmc +1 more source
Magnetosphere of Mars at Almost Radial Interplanetary Magnetic Field
Abstract We have studied the structure of the Martian magnetosphere under conditions of an almost radial interplanetary magnetic field (IMF). Under such conditions, the currents driven by the motional electric field −1cVsw×BIMF ${-}\frac{1}{c}{\mathbf{V}}_{sw}\times {\mathbf{B}}_{\mathit{IMF}}$ are expected to be strongly reduced, and the induced ...
E. Dubinin +9 more
wiley +1 more source
Analyzing AZ-non-Maxwellian distributions in Earth's magnetosphere: MMS observations. [PDF]
Abid AA +7 more
europepmc +1 more source

