Studying Galactic interstellar turbulence through fluctuations in synchrotron emission: First LOFAR Galactic foreground detection

The characteristic outer scale of turbulence and the ratio of the random to ordered components of the magnetic field are key parameters to characterise magnetic turbulence in the interstellar gas, which affects the propagation of cosmic rays within the Galaxy. We provide new constraints to those two...

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Bibliographic Details
Main Authors: Iacobelli, M, Haverkorn, M, Orrú, E, Pizzo, R, Anderson, J, Beck, R, Bell, MR, Bonafede, A, Chyzy, K, Dettmar, R, Enßlin, T, Heald, G, Horellou, C, Horneffer, A, Jurusik, W, Junklewitz, H, Kuniyoshi, M, Mulcahy, D, Paladino, R, Reich, W, Scaife, A, Sobey, C, Sotomayor-Beltran, C, Alexov, A, Asgekar, A
Format: Journal article
Language:English
Published: 2013