Results 61 to 70 of about 3,496,469 (217)
This diagram illustrates the wavy flow configuration of the model in a Cartesian coordinate system. It represents the heat and mass transfer characteristics of ternary hybrid nanofluids over a vertically wavy surface in the presence of an induced magnetic field and double‐diffusive mixed convection.
Latif Ahmad +4 more
wiley +1 more source
Magnetic fields in barred galaxies - III. The southern peculiar galaxy NGC 2442 [PDF]
Observations of the southern peculiar galaxy NGC 2442 with the Australia Telescope Compact Array in total and linearly polarized radio continuum at $\lambda$6 cm are presented and compared with previously obtained H $\alpha$ data.
Beck, R +15 more
core +1 more source
The Huge Magnetic Toroids in the Milky Way Halo
The magnetic fields in our Milky Way can be revealed by the distribution of Faraday rotation measures (RMs) of radio sources behind the Galaxy and of radio pulsars inside the Galaxy. Based on the antisymmetry of the Faraday sky in the inner Galaxy to the
J. Xu, J. L. Han
doaj +1 more source
Magnetic Fields in Nearby Galaxies
14 pages, 4 figures, 2 tables. Review paper published in: "The dynamic interstellar medium: a celebration of the Canadian Galactic Plane Survey", 2010, Eds. R. Kothes, T.L. Landecker & A.G.
openaire +2 more sources
Colorectal cancer is a heterogeneous, adaptive disease shaped by population‐level risk, genomic and epigenetic alterations, tumor ecosystem evolution, and treatment pressure. This review integrates epidemiology, risk factors, signaling networks, clinical presentation, screening, molecular diagnosis, and stage‐ and biomarker‐guided management while ...
Kairui Wan +6 more
wiley +1 more source
On the vertigo due to static magnetic fields. [PDF]
Vertigo is sometimes experienced in and around MRI scanners. Mechanisms involving stimulation of the vestibular system by movement in magnetic fields or magnetic field spatial gradients have been proposed.
Antunes, Andre +19 more
core +2 more sources
Magnetic Field Strengths in the Vicinity of Sgr A* via 18 cm Zeeman Observations
Very Large Array (VLA) observations of 18 cm OH absorption lines were used to determine the strength of the line-of-sight magnetic field in the Galactic center region. This study is an extension of the VLA OH Zeeman observations of Killeen et al.
K. L. Thompson +2 more
doaj +1 more source
Abstract Bayesian inference methods such as Markov Chain Monte Carlo (MCMC) typically require repeated computations of the likelihood function, but in some scenarios, this is infeasible and alternative methods are needed. Simulation‐based inference methods address this problem by using machine learning to amortize computations.
L. M. Wolniewicz, P. Sadowski, C. Corti
wiley +1 more source
Understanding the role that magnetic fields play on the stage of galaxy formation requires accurate methods for inferring the properties of extragalactic magnetic fields.
Tara Dacunha +3 more
doaj +1 more source

