Results 141 to 150 of about 188,313 (285)
One of the basic fluid mechanics problems of fluid flows over a revolving disk has both theoretical and real-world applications. The flow over a rotating disk has been the subject of numerous theoretical studies because it has many real-world ...
Yasmin Humaira +4 more
doaj +1 more source
MHD simulations on the interaction of the solar wind with the magnetosphere [PDF]
Chi Wang
openalex +1 more source
Abstract Locally generated fast magnetosonic (local MS) waves in the Martian ionosphere have been reported recently, which are different from the solar wind‐driven MS waves. However, their effects on particle scattering have not been reported yet. This study pioneers the investigation of electron, proton, and oxygen atomic ion scattering induced by ...
Fei Yao +3 more
wiley +1 more source
Enhanced heat transfer and fluid motion in 3D nanofluid with anisotropic slip and magnetic field
A mathematical model is envisaged that discusses the motion of 3D nanofluids (NFs) with anisotropic slip influence magnetic field past a stretching sheet.
Li Shuguang +7 more
doaj +1 more source
MHD Gleichgewicht und MHD-Stabilität in Rennbahngeometrie
The transverse field of a racetrack Tokamak in equilibrium is calculated for surface currents and Zarge aspect ratio via the law of Biot-Savart, and its structure is discussed. The discontinuities of the curvature lead to jumps in the vertical component and to the appearance of a horizontal component.
openaire +1 more source
Abstract Hot and tenuous plasmas have velocity distribution functions (VDFs) significantly different from Maxwellian distributions. Characterizing how these differences impact wave damping and emission necessitates sophisticated methods for determining the associated dielectric plasma response.
K. G. Klein +8 more
wiley +1 more source
Global existence for the MHD system in critical spaces [PDF]
Hammadi Abidi, Marius Paicu
openalex +1 more source
Reconstructing the Geometry of a Hot Flow Anomaly With Bounding Jets in Magnetosheath
Abstract When interplanetary magnetic field discontinuities interact with planetary bow shocks, hot flow anomalies (HFAs) form in the solar wind and can extend into the magnetosheath. Here we reconstruct the three‐dimensional geometry of an HFA bounded by two jet regions in the terrestrial magnetosheath.
Yufei Zhou +13 more
wiley +1 more source
Algebraic Approaches to the geopotential Forecast and Nonlinear MHD Equations [PDF]
Xiaoping Xu
openalex +1 more source

