Pizzo, RBonafede, AHeald, GKuniyoshi, MReich, WSobey, CAsgekar, ABentum, M JBernardi, GBest, PhillipBreitling, FBroderick, JCiardi, Benedettade Gasperin, FDuscha, SFalcke, HFallows, R AFerrari, CFrieswijk, WGunst, A WHassall, T. EHoeft, MKarastergiou, Avan Leeuwen, JMcKean, J PPolatidis, A.G.Röttgering, H. J. ARottgering, HubbSluman, JStappers, B. W.Vermeulen, R.C.Yatawatta, SOrru, EGarrett, M AHessels, J. W. T.Butcher, HarveyKondratiev, V. I.Wise, M JHaverkorn, MarijkeAlexov, A.Steinmetz, M.Iacobelli, M.Anderson, J MBeck, RainerBell, Michael RMulcahy, D.D.Avruch, Ian M.van Bemmel, Illsede Geus, EugeneEngels, DieterHamaker, Johan P.Kuper, G.Mann, GottfriedMunk, HTang, YToribio, C.Vocks, Christian2015-12-130004-6361http://hdl.handle.net/1885/75139Aims. The characteristic outer scale of turbulence (i.e. the scale at which the dominant source of turbulence injects energy to the interstellar medium) and the ratio of the random to ordered components of the magnetic field are key parameters to characteAuthor/s retain copyrightKeywords: ISM: general; ISM: magnetic fields; ISM: structure; Radio continuum: general; Radio continuum: ISM; Techniques: interferometric; Estimation; Magnetic fields; Power spectrum; Synchrotron radiation; Turbulence ISM: general; ISM: magnetic fields; ISM: structure; Radio continuum: general; Radio continuum: ISM; Techniques: interferometric201310.1051/0004-6361/2013220132016-02-24