Results 81 to 90 of about 474,973 (216)
Toroidal Magnetic Flux Budget in Mean-field Dynamo Model of Solar Cycles 23 and 24
We study the toroidal magnetic flux budget of the axisymmetric part of a data-driven 3D mean-field dynamo model of Solar Cycles 23 and 24. The model simulates the global solar dynamo that includes the effects of the formation and evolution of bipolar ...
Valery V. Pipin, Alexander G. Kosovichev
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Bessel beams are plane waves with amplitude profiles described by Bessel functions. They are important because they propagate ‘diffraction-free’ and because they can carry orbital angular momentum.
C Ryu, K C Henderson, M G Boshier
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Dynamical Stability of Hypermassive Neutron Stars against Quasi-radial Perturbations
The dynamical stability of differentially rotating neutron stars, including hypermassive neutron stars, is of paramount importance in understanding the fate of the postmerger remnant of binary neutron stars mergers and the formation of a black hole ...
Paweł Szewczyk +2 more
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Monte Carlo Studies of Transverse Faraday Rotation Profiles
Faraday Rotation measurements are a very important tool for investigating the magnetic (B) fields associated with the relativistic jets of Active Galactic Nuclei (AGN); for example, a toroidal or helical B field component should give rise to a systematic
Murphy Eoin, Gabuzda Denise
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Characteristics of axisymmetric viscous incompressible flow passing a torus rotating about its centerline [PDF]
The present numerically investigates the axisymmetric flow past a rotating torus in a viscous incompressible fluid. The surface of the torus rotates with constant velocity around its centerline.
Pairin Suwannasri
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It is observed that the magnitude of the toroidal rotation speed is reduced by the central electron cyclotron resonance heating (ECRH) regardless of the direction of the toroidal rotation.
Lee, SG +16 more
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Chiral Magnetic Phases in Moire Bilayers of Magnetic Dipoles
In magnetic insulators, the sense of rotation of the magnetization is associated with novel phases of matter and exotic transport phenomena. Aimed to find new sources of chiral magnetism rooted in intrinsic fields and geometry, twisted square bilayers of
Ignacio Tapia +2 more
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A spectral MHD code for the non-linear study of magnetic neutron stars
EThOS - Electronic Theses Online ServiceGBUnited ...
Robertshaw, Oliver
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We build a multilayer magnetohydrodynamic shallow-water model to study the thickness and shape of the solar tachocline. This allows us to include characteristics of both the overshoot and the radiative parts of the tachocline.
Mausumi Dikpati, Peter A. Gilman
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Quasi-Toroidal Oscillations in Rotating Relativistic Stars
Quasi-toroidal oscillations in slowly rotating stars are examined in the framework of general relativity. The oscillation frequency to first order of the rotation rate is not a single value even for uniform rotation unlike the Newtonian case.
Quasi-toroidal Oscillations +1 more
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