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Cambridge University Press (CUP), Proceedings of the International Astronomical Union, S259(4), p. 89-90, 2008

DOI: 10.1017/s1743921309030117

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GMIMS: the Global Magneto-Ionic Medium Survey

Journal article published in 2008 by Maik Wolleben, T. L. Landecker, E. Carretti, J. M. Dickey ORCID, A. Fletcher, B. M. Gaensler ORCID, J. L. Han, M. Haverkorn, J. P. Leahy, N. M. McClure-Griffiths, D. McConnell, W. Reich, A. R. Taylor
This paper was not found in any repository, but could be made available legally by the author.
This paper was not found in any repository, but could be made available legally by the author.

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Abstract

AbstractThe Global Magneto-Ionic Medium Survey (GMIMS) is a project to map the diffuse polarized emission over the entire sky, Northern and Southern hemispheres, from 300 MHz to 1.8 GHz. With an angular resolution of 30–60 arcmin and a frequency resolution of 1 MHz or better, GMIMS will provide the first spectro-polarimetric data set of the large-scale polarized emission over the entire sky, observed with single-dish telescopes. GMIMS will provide an invaluable resource for studies of the magneto-ionic medium of the Galaxy in the local disk, halo, and its transition.

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