Results 101 to 110 of about 372 (130)

Interstellar magnetic field effects on the heliosphere

AIP Conference Proceedings, 2003
This paper summarizes the numerical results obtained by three‐dimensional MHD simulations of the interaction between the solar wind and interstellar medium in Ratkiewicz and Ben‐Jaffel [2002], Ratkiewicz and McKenzie [2002], and Ratkiewicz and Webb [2002].
Ratkiewicz, R., Ben-Jaffel, L., McKenzie, J., Webb, G.   +3 more
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Interstellar: The Galactic Magnetic Field

Publications of the Astronomical Society of Australia, 1969
Over a period of one year from March 1967, the 24-inch rotatable telescope at Siding Spring Observatory was used to make polarization measurements for about 1400 stars, most of which were within 400 pc of the Sun. It was found that the E vectors of the polarization formed quite definite patterns on the sky which could only be produced if the magnetic ...
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Interstellar Polarization and Magnetic Fields

1987
Since the work of Davis and Greenstein, polarization of starlight is quite gene­rally considered as one of the most spectacular manifestation of the presence of magnetic fields in the interstellar space. If polarization measurements are quali­tatively able to indicate the general pattern of the magnetic fields, a quantita­tive analysis seems more ...
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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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The effect of magnetic fields on interstellar clouds

Symposium - International Astronomical Union, 1967
I should like to say something about the equilibrium of the gas in spiral arms and about the interaction of interstellar clouds. The polarization of the light of distant stars shows that there is a quasi-regular magnetic field inside the clouds, and the Faraday rotation indicates the same for the gas between the clouds.
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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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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  

Interstellar Magnetic Fields

2004
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Magnetic fields in halos of spiral galaxies and the interstellar disk-halo connection

AIP Conference Proceedings, 2005
R -J Dettmar, Dettmar Ralf-Jürgen
exaly