Interstellar Turbulence I: Observations and Processes
, 2004 This two-part review summarizes interstellar turbulence and its implications. The first part begins with diagnostics and energy sources. Turbulence theory is considered in detail, including the basic fluid equations, solenoidal and compressible modes ...
Elmegreen, Bruce G., Scalo, John
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New insights into the interstellar medium of the dwarf galaxy IC 10: connection between magnetic fields, the radio–infrared correlation and star formation [PDF]
, 2017 Aritra Basu +6 more
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The Huge Magnetic Toroids in the Milky Way Halo
The Astrophysical JournalThe 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
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, 2002 Using linear kinetic plasma theory the relation between electron density and magnetic field fluctuations for low-frequency plasma waves for Maxwellian background distribution functions of arbitrary temperatures in an uniform magnetic field is derived.
Schlickeiser, R., Lerche, I.
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LOCAL INTERSTELLAR MAGNETIC FIELD DETERMINED FROM THE INTERSTELLAR BOUNDARY EXPLORER RIBBON
The Astrophysical Journal Letters, 2016 ABSTRACT The solar wind emanating from the Sun interacts with the local interstellar medium (LISM), forming the heliosphere. Hydrogen energetic neutral atoms (ENAs) produced by the solar-interstellar interaction carry important information about plasma properties from the boundaries of the heliosphere, and are currently being measured by
E. J. Zirnstein +5 more
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Magnetic Field Amplification Associated with the Richtmyer-Meshkov Instability
, 2012 The amplification of a magnetic field due to the Richtmyer-Meshkov instability (RMI) is investigated by two-dimensional MHD simulations. Single-mode analysis is adopted to reveal definite relation between the nonlinear evolution of RMI and the field ...
Abdo +26 more
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Do Androids Dream of Magnetic Fields? Using Neural Networks to Interpret the Turbulent Interstellar Medium [PDF]
, 2019 J. E. G. Peek, Blakesley Burkhart
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Why take the square root? An assessment of interstellar magnetic field strength estimation methods [PDF]
, 2021 Raphael Skalidis +4 more
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INTERSTELLAR MAGNETIC FIELD SURROUNDING THE HELIOPAUSE
The Astrophysical Journal, 2010 This paper presents a three-dimensional analytical solution, in the limit of very low plasma β-ratio, for the distortion of the interstellar magnetic field surrounding the heliopause. The solution is obtained using a line dipole method that is the integration of point dipole along a semi-infinite line; it represents the magnetic field caused by the ...
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Concerning the origin of the magnetic fields on stars and in interstellar space [PDF]
Origin of magnetic fields on stars and in interstellar ...
Biermann, L.
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