|
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
|
|
|
References
|
