Results 61 to 70 of about 1,308 (218)
MMS Observations of Multi‐Species Wave‐Particle Interactions and Rapid Foreshock Evolution
Abstract The ion foreshock is the region upstream of Earth's bow shock where magnetic field lines connect to the quasi‐parallel shock surface. Within this region, there exist a variety of backstreaming ion populations from the shock ramp that can generate ultra‐low frequency (ULF) waves through wave‐particle interactions. In this work, we use data from
Guan Le +11 more
wiley +1 more source
The prediction of coronal and interplanetary magnetic fields [PDF]
Solar coronal structure and interplanetary magnetic fields prediction based on magnetic models, testing accuracy at solar ...
openaire +1 more source
A Complete Theory for Nondiffusive Field Line Random Walk in Magnetic Turbulence
Previous analytical and numerical investigations of the stochastic properties of field lines in magnetic turbulence have been based on determining the running field-line diffusion coefficient.
A. Shalchi
doaj +1 more source
Abstract We present a case study of large amplitude, compressional Pc5 waves observed by GOES 13 and 15 at geosynchronous orbit near noon. These waves were excited near the arrival time of two consecutive solar wind dynamic pressure spikes at the magnetopause, the second of which was associated with a large and rapid southward turning of the ...
C. Lazzeri +8 more
wiley +1 more source
Axial Flux Evolution of Small-scale Magnetic Flux Ropes from 0.06 to 10 au
Small-scale magnetic flux ropes (SMFRs) fill much of the solar wind, but their origin and evolution are debated. We apply our recently developed, improved Grad–Shafranov algorithm for the detection and reconstruction of SMFRs to data from Parker Solar ...
Hameedullah Farooki +4 more
doaj +1 more source
Neutral Wind Dynamics in High‐Latitude Regions During the 17 March 2013 Storm
Abstract Neutral winds play a critical role in transporting mass, momentum, and energy throughout the upper atmosphere. During geomagnetic storms, momentum is transferred to the thermosphere primarily through ion–neutral collisions, along with other forces. This study investigates high‐latitude neutral wind dynamics during the 17 March 2013 storm using
A. Alhothali +2 more
wiley +1 more source
Abstract Auroral precipitation plays a key role in coupling the Magnetosphere–Ionosphere–Thermosphere system by modifying ionospheric conductance, currents, atmospheric heating, and upper‐atmospheric dynamics. Leveraging 17 years of electron spectrum data from the Defense Meteorological Satellite Program (DMSP), we developed a Machine Learning‐based ...
V. Sai Gowtam, Hyunju Connor
wiley +1 more source
Hybrid Simulations of the Cusp and Dayside Magnetosheath Dynamics Under Quasi-Radial Interplanetary Magnetic Fields. [PDF]
Ng J +4 more
europepmc +1 more source
Assessment of Spacecraft Internal Charging in the Earth's Outer Radiation Belt
Abstract The internal charging effects triggered by energetic (>100 keV) electrons in the Earth's radiation belts can cause anomalies and failures of electronic components aboard spacecraft. Given the critical importance of safeguarding space assets, it is essential to estimate internal charging risks, which depend highly on the distribution of ...
Yuan Lei +4 more
wiley +1 more source
Forecast and Nowcast Solar Energetic Particles (SEP) Radiation Doses in Near Earth/Moon Space
Abstract Solar energetic particle (SEP) events pose a critical radiation hazard to human space exploration, and extreme SEPs must be mitigated operationally to avoid serious health impacts. Accurate prediction of SEP‐induced radiation exposure is essential to ensure mission safety.
Jiajun Liu +2 more
wiley +1 more source

