Results 121 to 130 of about 4,214,854 (199)
Russian version of nos. 62-78 bound together (barcode no. 0072068)197 p.Reviews and evaluates over 550 studies in an effort to determine the effects on humans and other biological systems of exposure to static magnetic fields and to time-varying fields ...
World Health Organization +2 more
core
CHANG-ES XL: Magnetic Field Structures in the Disk and Halo of NGC 891
We present new Karl G. Jansky Very Large Array S -band (2–4 GHz) observations of the edge-on spiral galaxy NGC 891, complemented by C -band data, to investigate the structure of its radio continuum halo.
N. Pourjafari +13 more
doaj +1 more source
Cosmic-void observations reconciled with primordial magnetogenesis. [PDF]
Hosking DN, Schekochihin AA.
europepmc +1 more source
86th Annual Meeting of the Meteoritical Society (2024)
Meteoritics &Planetary Science, Volume 59, Issue S1, Page A1-A468, August 2024.
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
Polarized thermal emission from dust in a galaxy at redshift 2.6. [PDF]
Geach JE +7 more
europepmc +1 more source
Magnetic Field of the Quasar 1604+159 from Parsec to Kiloparsec Scale
We present a multifrequency polarimetric study for the quasar 1604+159. The source was observed at the L band with the American Very Long Baseline Array and the L , X , and U bands with the Very Large Array.
Xu-Zhi Hu +5 more
doaj +1 more source
Electromagnetic Conversion into Kinetic and Thermal Energies. [PDF]
Brandenburg A, Protiti NN.
europepmc +1 more source
Intergalactic Medium Rotation Measure of Primordial Magnetic Fields
The Faraday rotation effect, quantified by the rotation measure (RM), is a powerful probe of the large-scale magnetization of the Universe—tracing magnetic fields not only on galaxy and galaxy cluster scales but also in the intergalactic medium (IGM ...
Salome Mtchedlidze +7 more
doaj +1 more source
A Simple Model of the Radio–Infrared Correlation Depending on Gas Surface Density and Redshift
We introduce a simple parametric model of the radio–infrared correlation (i.e., the ratio between the IR luminosity and the 1.4 GHz radio luminosity, q _IR ) by considering the energy loss rate of high-energy cosmic-ray (CR) electrons governed by ...
Ilsang Yoon
doaj +1 more source

