000004097 001__ 4097
000004097 005__ 20190204144510.0
000004097 037__ $$aCTALK-2019-0095
000004097 100__ $$aZucca, P.
000004097 245__ $$aKinematics and shock locations of a spatial resolved solar type II radio burst with LOFAR
000004097 260__ $$c2017
000004097 269__ $$c2017-07-24
000004097 520__ $$aType II radio bursts are evidence of shocks in the solar atmosphere emitting radio waves ranging from metric to kilometric lengths. These shocks may be associated with coronal mass ejections (CMEs) reaching super-Alfvénic speeds. Radio imaging of the decameter wavelengths is now possible with the Low Frequency Array (LOFAR), opening a new radio window to study coronal radio shocks leaving the inner solar corona and entering the interplanetary medium and understand their association with CMEs. Here, we study a coronal shock associated with a CME and type II radio burst to determine the location where the shock is triggered in relation to the propagating CME, the ambient medium Alfvén speed and the orientation of the coronal magnetic field. The type II shock imaging and spectra were obtained using 91 simultaneous tied-array beams of LOFAR while the CME was observed by the Large Angle and Spectrometric Coronagraph (LASCO) on board the Solar and Heliospheric Observatory (SOHO). Using the tied array beam observing mode of LOFAR we were able to locate the type II radio shock position between 45 and 75 MHz and relate it to the expanding flank of a CME leaving the inner corona. The radio emission associated with the type II shock was found to be located at the flank of the CME in a region where the mach number is between 1.5 to 2.0 and the shock geometry is quasi-perpendicular.
000004097 594__ $$aSTCE
000004097 700__ $$aMorosan, D.
000004097 700__ $$aGallagher, Peter T.
000004097 700__ $$aFallows, R.
000004097 700__ $$aRouillard, A.
000004097 700__ $$aMagdalenic, J.
000004097 700__ $$aVocks, C.
000004097 700__ $$aMarqué, C.
000004097 700__ $$aKlein, K-L.
000004097 700__ $$aMann, G.
000004097 773__ $$tSolar Heliospheric and INterplanetary Environment (SHINE 2017)
000004097 8560_ $$fjasmina.magdalenic@observatoire.be
000004097 906__ $$aContributed
000004097 980__ $$aCTALKCONT