Depolarization of radio synchrotron emission in spiral galaxies.

Astronomy and Astrophysics – Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

3

Polarization, Techniques: Polarimetric, Radio Continuum: Galaxies, Galaxies: Spiral, Galaxies: Magnetic Fields, Galaxies: Ism

Scientific paper

The internal depolarization of linearly polarized radio synchrotron emission of spiral galaxies by differential Faraday rotation in regular magnetic fields and by Faraday dispersion in random magnetic fields is formulated in one dimension as a function of radio wavelength λ. The random fields are modeled as a number of cells along the line of sight which obey a Kolmogorov spectrum in size and in field strength and have an isotropic distribution of orientation. A graphic representation of the calculation procedure is introduced for the Faraday dispersion function. Given a set of typical parameters for spiral galaxies, our model predicts that the fractional polarization is an oscillating function of λ^2^ with minima near zero and decreasing amplitude. Compared with single-size cells, the depolarizing effect of the Kolmogorov-type random fields is much smaller; they only smear the effect of the regular field. However, the random fields have a strong effect on the Faraday polarization angle at long wavelengths and distort its linear relation with λ^2^. As a result, Faraday rotation measures at decimeter wavelengths oscillate in λ^2^ so that their sign may reverse without reversals in the regular magnetic field. Our model is able to explain observational phenomena like polarized emission around λ90 cm, anomalous variation of depolarization with wavelength, excess rotation measures at λ20 cm, and the lack of a correlation between Faraday rotation measure and depolarization at λ>=20cm.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Depolarization of radio synchrotron emission in spiral galaxies. does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Depolarization of radio synchrotron emission in spiral galaxies., we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Depolarization of radio synchrotron emission in spiral galaxies. will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-828662

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.