Polarization in Low Frequency Radio Astronomy

Baptiste Cecconi

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arXiv · 1901.03599

Polarization in Low Frequency Radio Astronomy

Baptiste Cecconi

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Abstract

This chapter introduces the concepts of polarimetry in the case of low frequency radio astronomy. In this regime radio waves are usually not the signature of atomic or molecular transitions lines, but rather that of unstable particle distribution functions releasing their free energy through electromagnetic radiation. As the radio source region is usually magnetized, the propagation medium (at least close to the source) is anisotropic, and the polarization depends on the local magnetic field direction, the propagation mode and the direction of propagation.

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Baptiste Cecconi. 2019-01-11. Polarization in Low Frequency Radio Astronomy. https://arxiv.org/abs/1901.03599

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