Results 161 to 170 of about 5,169 (254)
Forming Prominences Accounting for Partial Ionization Effects
One of the most striking structures in the solar atmosphere are prominences, predominantly coronal structures, with thermodynamic conditions that vary from chromospheric internally to the corona that surrounds them.
V. Jerčić +2 more
doaj +1 more source
Relativistic magnetohydrodynamical simulations of the resonant corrugation of a fast shock front [PDF]
Camilia Demidem +2 more
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Interplanetary coronal mass ejections (ICMEs) are the primary sources of geomagnetic storms at Earth. The negative out-of-ecliptic component ( B _z ) of magnetic field in the ICME or its associated sheath region is necessary for it to be geoeffective ...
Talwinder Singh +3 more
doaj +1 more source
High‐resolution global magnetohydrodynamic simulation of bursty bulk flows [PDF]
M. Wiltberger +3 more
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Radiative Cooling Changes the Dynamics of Magnetically Arrested Disks
We study magnetically arrested disks (MADs) around rotating black holes (BHs) under the influence of radiative cooling. We introduce a critical value of the mass accretion rate ${\dot{M}}_{{\rm{crit}}}$ for which the cooling by the synchrotron process ...
Akshay Singh +2 more
doaj +1 more source
Exploring the Nature of EUV Waves in a Radiative Magnetohydrodynamic Simulation [PDF]
Can Wang, Feng Chen, M. D. Ding
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Smoothed particle magnetohydrodynamic simulations of protostellar outflows with misaligned magnetic field and rotation axes [PDF]
Benjamin T. Lewis +2 more
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The life cycle of the Central Molecular Zone - II. Distribution of atomic and molecular gas tracers. [PDF]
Armillotta L +2 more
europepmc +1 more source
Effective resistivity for magnetohydrodynamic simulation of collisionless magnetic reconnection [PDF]
Haowei Zhang, Zhiwei Ma, Tong Chen
openalex +1 more source

