A turbulent Faraday screen produces survey-dependent scatter in rotation measures, with magnitude set by the power spectrum of Faraday depth structure and by the wavelength coverage of the survey.
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RM jitter: Wavelength-dependent Scatter in Rotation Measure Related to Faraday Complexity
A turbulent Faraday screen produces survey-dependent scatter in rotation measures, with magnitude set by the power spectrum of Faraday depth structure and by the wavelength coverage of the survey.