Polaris Flare CO enhancement by MHD waves

B2FIND2026-03-19 收录

星际介质分子形成

磁流体动力学

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https://b2find.eudat.eu/dataset/c8b4e278-41cd-5384-adbb-90ef9bc04376 数据链接链接失效反馈

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The formation of molecular gas in interstellar clouds is a slow process, but can be enhanced by gas compression. Magnetohydrodynamic (MHD) waves can create compressed...

Magnetohydrodynamic Data of Gyration of Macroparticles

磁流体动力学

粒子运动分析

The data is the obtained using the autotracker application of the 'Tracker' software. The data is time versus x-y corditanates of a marked particle subject to movment in present of E X B drift. This d

DataCite Commons2024-12-20 更新100

Small-scale behavior of Hall magnetohydrodynamic turbulence

等离子体湍流模拟

磁流体动力学

Decaying Hall magnetohydrodynamic (HMHD) turbulence is studied using three-dimensional (3D) direct numerical simulations with grids up to 768(3) points and two different types...

University Corporation for Atmospheric Research80

Parallel computing of magnetohydrodynamic simulations based on conservative perturbed model

磁流体动力学

并行计算

The data records the change of energy with time and the time consumption of single step calculation. The folder also contains the paper chart.

科学数据银行2022-10-26 更新30

sj-zip-1-pic-10.1177_09544062211023094 - Supplemental material for MHD nanofluid flow around a permeable stretching sheet with thermal radiation and viscous dissipation

纳米流体

磁流体动力学

Supplemental material, sj-zip-1-pic-10.1177_09544062211023094 for MHD nanofluid flow around a permeable stretching sheet with thermal radiation and viscous dissipation by Rana MA Muntazir, Muhammad Mu

DataCite Commons2024-08-28 更新90

Dynamo action at low magnetic Prandtl numbers: Mean flow versus fully...

磁流体动力学

发电机效应

We compute numerically the threshold for dynamo action in Taylor-Green (TG) swirling flows. Kinematic dynamo calculations, for which the flow field is fixed to its time average,...

DASH Search60

Polaris Flare CO enhancement by MHD waves

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