Results 161 to 170 of about 52,369 (271)

A Comparison of MAVEN SIR Observations With the Stationary WSA‐ENLIL Solar Wind Model

Journal of Geophysical Research: Space Physics, Volume 130, Issue 12, December 2025.
Abstract Predicting times of arrival and properties of space weather events, such as coronal mass ejections and stream interaction regions (SIRs), has become an important focus of the space physics community within recent years. Extensive efforts have been undertaken to model these space weather events throughout the heliosphere in order to better ...
Sarah Henderson, Rachael Filwett, Sophia Owen, Jasper Halekas, Jacob Gruesbeck   +4 more
wiley   +1 more source

A MAGNETOHYDRODYNAMIC MODEL OF THE M87 JET. II. SELF-CONSISTENT QUAD-SHOCK JET MODEL FOR OPTICAL RELATIVISTIC MOTIONS AND PARTICLE ACCELERATION [PDF]

, 2014
Masanori Nakamura, David L. Meier, Masanori Nakamura, David L. Meier   +3 more
openalex   +1 more source

Entropy-bounded solutions to the Cauchy problem of compressible planar non-resistive magnetohydrodynamics equations with far field vacuum [PDF]

, 2023
Jinkai Li, Mingjie Li, Yang Liu, Xin Zhong   +3 more
openalex   +1 more source

Fluid Flow at the Top of Jupiter's Dynamo Region

Journal of Geophysical Research: Planets, Volume 130, Issue 12, December 2025.
Abstract The magnetic main field (MF) and secular variation (SV) models for Jupiter can be used to gain insights about the internal dynamo and the flow that drives the field. We use two such models computed from Juno observations up to spherical harmonic degrees 16 and 8 for the MF and SV, respectively.
S. Sharan, M. A. Pais, H. Amit, B. Langlais   +3 more
wiley   +1 more source

Non-resonant magnetohydrodynamics streaming instability near magnetized relativistic shocks [PDF]

, 2013
Fabien Casse, Alexandre Marcowith, Rony Keppens   +2 more
openalex   +1 more source

CNN‐Based Model for 3D CME Parameter Prediction – A Proof of Concept

Journal of Geophysical Research: Machine Learning and Computation, Volume 2, Issue 4, December 2025.
Abstract Accurate 3D reconstruction of coronal mass ejections (CMEs) is essential for understanding their propagation and improving space weather forecasts. In this study, we present a proof‐of‐concept deep learning framework that predicts seven parameters from synthetic multi‐view coronagraph images.
Harshita Gandhi, Huw Morgan, Cory Thomas
wiley   +1 more source

Time fractional modeling of MHD natural convection flow between parallel plates via caputo-fabrizio integral. [PDF]

Sci Rep
Masood K.
europepmc   +1 more source

MHD Forecasting of Solar Wind With Coronal Mass Ejections

Space Weather, Volume 23, Issue 12, December 2025.
Abstract We present a model, implemented as an online service, for predicting the speed and density of solar wind in the inner heliosphere and near Earth. The model is based on a numerical magnetohydrodynamics code PLUTO. The inner boundary maps are continuously obtained from the National Centers for Environmental Prediction, where they are updated 1 ...
S. Arutyunyan, A. Kodukov, M. Subbotin, D. Pavlov   +3 more
wiley   +1 more source

A time-fractional model of hydromagnetic slip flow of viscous fluid in rotational frame with heat and mass transfer. [PDF]

Sci Rep
Ahmad S, Ali F, Khan I, Khan N, Alqasem OA, Elwahab MEA, Omer ASA.   +6 more
europepmc   +1 more source

Numerical analysis of magnetohydrodynamics Casson nanofluid flow with activation energy, Hall current and thermal radiation. [PDF]

Sci Rep, 2023
Suresh Kumar Y, Hussain S, Raghunath K, Ali F, Guedri K, Eldin SM, Khan MI.   +6 more
europepmc   +1 more source