Statistical methods for the analysis of rotation measure grids in large scale structures in the SKA era

VACCA, VALENTINAVALENTINAVACCAOppermann, NielsNielsOppermannEnsslin, Torsten A.Torsten A.EnsslinSelig, MarcoMarcoSeligJunklewitz, HenrikHenrikJunklewitzGreiner, MaksimMaksimGreinerJasche, JensJensJascheHales, Chris A.Chris A.HalesReneicke, MartinMartinReneickeCARRETTI, ETTOREETTORECARRETTIFERETTI, LUIGINALUIGINAFERETTIFerrari, ChiaraChiaraFerrariGiovannini, GabrieleGabrieleGiovanniniGOVONI, FEDERICAFEDERICAGOVONIHorellou, CathyCathyHorellouIdeguchi, ShinsukeShinsukeIdeguchiJohnston-Hollitt, MelanieMelanieJohnston-HollittMURGIA, MATTEOMATTEOMURGIAPaladino, RositaRositaPaladinoPizzo, RobertoRobertoPizzoScaife, AnnaAnnaScaife2020-04-202020-04-2020151824-8039http://hdl.handle.net/20.500.12386/24112To better understand the origin and properties of cosmological magnetic fields, a detailed knowledge of magnetic fields in the large-scale structure of the Universe (galaxy clusters, filaments) is crucial. We propose a new statistical approach to study magnetic fields on large scales with the rotation measure grid data that will be obtained with the new generation of radio interferometers.ELETTRONICOenStatistical methods for the analysis of rotation measure grids in large scale structures in the SKA eraConference paper10.22323/1.215.0114https://pos.sissa.it/215/114/2015aska.confE.114VFIS/05 - ASTRONOMIA E ASTROFISICA