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Article Contents
1 Introduction
2 Models of Faraday rotation towards background sources in galaxies
3 Number density of polarized background sources
4 Recognition of regular galactic field structures from a limited sample of background sources
5 Magnetic field reconstruction from RM grids of inclined galaxies
6 Discussion
7 Application to LOFAR and SKA
8 Conclusions

List of tables
List of figures

Copyright ESO 2008
Published by EDP Sciences