Results 61 to 70 of about 1,150,056 (199)
Magnetorotational Instability in a Solar Near-surface Mean-field Dynamo
We address the question whether the magnetorotational instability (MRI) can operate in the near-surface shear layer (NSSL) of the Sun and how it affects the interaction with the dynamo process.
Axel Brandenburg +3 more
doaj +1 more source
A Statistical Study on Force-Freeness of Solar Magnetic Fields in the Photosphere
It is an indisputable fact that solar magnetic fields are force-free in the corona, where force free fields means that current and magnetic fields are parallel and there is no Lorentz force in the fields.
Ai +34 more
core +1 more source
The magnetometer (MAG) payload on board India’s first solar mission, Aditya-L1, is a dual-sensor fluxgate magnetometer designed to measure the interplanetary magnetic field (IMF) while operating in a halo orbit around the first Sun–Earth Lagrangian point
Vipin K. Yadav +2 more
doaj +1 more source
Stability of Magnetic Fluids in Magnetic Fields [PDF]
Stability of magnetic fluids in magnetic fields is one of the major factors determining the possibility of their practical use and resource of their exploitation.
I.M. Arefyev, T.A. Arefyeva
doaj
Magnetically Assisted Vorticity Production in Decaying Acoustic Turbulence
We study vorticity production in isothermal, subsonic, acoustic (nonvortical), and decaying turbulence due to the presence of magnetic fields. Using three-dimensional numerical simulations, we find that the resulting kinetic energy cascade follows the ...
Axel Brandenburg, Evan Scannapieco
doaj +1 more source
Primordial magnetic fields at preheating
Using lattice techniques we investigate the generation of long range cosmological magnetic fields during a cold electroweak transition. We will show how magnetic fields arise, during bubble collisions, in the form of magnetic strings.
A Duif +35 more
core +2 more sources
Proposed Resolution to the Solar Open Magnetic Flux Problem
The solar magnetic fields emerging from the photosphere into the chromosphere and corona are comprised of a combination of closed (field lines with both ends rooted at the Sun) and open (field lines with only one end at the Sun) fields.
C. Nick Arge +4 more
doaj +1 more source
Magnetic Fields of Neutron Stars
This article briefly reviews our current understanding of the evolution of magnetic fields in neutron stars, which basically defines the evolutionary pathways between different observational classes of neutron stars. The emphasis here is on the evolution
Konar, Sushan
core +1 more source
We report the detection of the ordered alignment between the magnetic field and kpc-scale bubbles in the nearby spiral galaxy, NGC 628. Applying the Velocity Gradient Technique on CO spectroscopic data from the ALMA-PHANGS, the magnetic field of NGC 628 ...
Mengke Zhao +11 more
doaj +1 more source
Physics in Very Strong Magnetic Fields: Introduction and Overview
This paper provides an introduction to a number of astrophysics problems related to strong magnetic fields. The first part deals with issues related to atoms, condensed matter and high-energy processes in very strong magnetic fields, and how these issues
Lai, Dong
core +1 more source

