Interstellar magnetic fields - Open Access .click

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Magnetic fields in interstellar water masers

2008
We report the first detection of Zeeman splitting in the (616−523) rotational transition of interstellar H2O masers. The measurements of Stokes parameter V and I spectra (circular polarization) have been performed at the MPIfR 100-m telescope. Depending on the hyperfine transition that is actually masing, we derive typical magnetic field strengths of B‖
D. Fiebig, R. Güsten
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Magnetic fields in dense interstellar clouds

Philosophical Transactions of the Royal Society of London. Series A, Mathematical and Physical Sciences, 1981
Abstract Evidence is presented that shows that magnetic fields pervade the entire interstellar medium including interstellar gas clouds of both low and high density. The magnetic field in the ‘seed’ gas from which the denser clouds form is 0.2-0.3 nT (1T — 104G). Zeeman effect measurements of neutral hydrogen show that stronger fields
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The Interstellar Magnetic Field

2022
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Interstellar Polarization, Galactic Magnetic Fields, and Ferromagnetism

Science, 1949
L, Spitzer, J W, Tukey
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Magnetic field morphology in interstellar clouds with the velocity gradient technique

Nature Astronomy, 2019
Alex S. Hill, Yue HU, Felix Lockman
exaly

Interstellar Magnetic Fields

2004
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Three‐dimensional structure of the outer heliosphere in the presence of the interstellar and interplanetary magnetic fields

AIP Conference Proceedings, 2004
Nikolai V. Pogorelov
exaly

Multi‐component 3D modeling of the heliospheric interface: effects of interstellar magnetic field

AIP Conference Proceedings, 2006
V V Izmodenov
exaly