22.12.2013 Views

Investigations of Faraday Rotation Maps of Extended Radio Sources ...

Investigations of Faraday Rotation Maps of Extended Radio Sources ...

Investigations of Faraday Rotation Maps of Extended Radio Sources ...

SHOW MORE
SHOW LESS

You also want an ePaper? Increase the reach of your titles

YUMPU automatically turns print PDFs into web optimized ePapers that Google loves.

List <strong>of</strong> Figures<br />

1.1 nπ-ambiguity . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 12<br />

1.2 RM distribution <strong>of</strong> Hydra A . . . . . . . . . . . . . . . . . . . . . . 14<br />

1.3 <strong>Radio</strong> map <strong>of</strong> the Coma cluster . . . . . . . . . . . . . . . . . . . . . 17<br />

1.4 RM cluster point source sample . . . . . . . . . . . . . . . . . . . . 20<br />

2.1 RM distribution <strong>of</strong> PKS 1246-410 . . . . . . . . . . . . . . . . . . . 30<br />

2.2 RM - ϕ 0 scatter plots . . . . . . . . . . . . . . . . . . . . . . . . . . 32<br />

3.1 RM autocorrelation function <strong>of</strong> A400, A2634 and Hydra A . . . . . . 57<br />

3.2 Magnetic autocorrelation function w(r) in real space . . . . . . . . . . 58<br />

3.3 Magnetic energy spectrum for A2634, A400 and Hydra A . . . . . . . 59<br />

3.4 Dependence <strong>of</strong> the magnetic field strength on the integration interval . 60<br />

3.5 Testing the window function by calculating χ 2 (x ⊥ ) . . . . . . . . . . 61<br />

3.6 Fourier transformed RM map <strong>of</strong> A400 and Hydra A . . . . . . . . . 62<br />

3.7 Response function for A2634 . . . . . . . . . . . . . . . . . . . . . . 63<br />

3.8 Expected and measured magnetic field in comparison . . . . . . . . . 64<br />

3.9 Determination <strong>of</strong> the spectral indeces . . . . . . . . . . . . . . . . . . 65<br />

4.1 Flow chart <strong>of</strong> the algorithm Pacman . . . . . . . . . . . . . . . . . . 75<br />

4.2 Testing the Pacman algorithm . . . . . . . . . . . . . . . . . . . . . 81<br />

4.3 Comparision between Pacman and standard fit RM aps . . . . . . . . 85<br />

4.4 A pixel-by-pixel comparison between Pacman and standard fit RM Map 86<br />

4.5 Various Power Spectra for the Cluster Source A2255E . . . . . . . . 87<br />

4.6 A pixel-by-pixel comparison between Pacman and standard fit RM<br />

Map for Hydra A North . . . . . . . . . . . . . . . . . . . . . . . . . 89<br />

4.7 Various power spectra for Hydra North . . . . . . . . . . . . . . . . . 91<br />

4.8 Various power spectra for Hydra North using different thresholds . . . 92<br />

4.9 A reduced χ 2 νij and Ṽ map <strong>of</strong> Hydra North . . . . . . . . . . . . . . 93<br />

4.10 Individual RM fits across an RM jump . . . . . . . . . . . . . . . . 95<br />

4.11 Various power spectra for Hydra South . . . . . . . . . . . . . . . . . 96<br />

5.1 Generated RM maps with known power spectrum . . . . . . . . . . . 106<br />

5.2 Calculated power spectra for the test case . . . . . . . . . . . . . . . 107<br />

5.3 RM maps <strong>of</strong> Hydra North . . . . . . . . . . . . . . . . . . . . . . . 109<br />

5.4 Window function in comparison to the RM dispersion . . . . . . . . 110<br />

5.5 Various power spectra for different scaling exponents α B . . . . . . . 112<br />

5.6 The log-likelihood for various scaling parameters α B . . . . . . . . . 113<br />

viii

Hooray! Your file is uploaded and ready to be published.

Saved successfully!

Ooh no, something went wrong!