000003052 001__ 3052
000003052 005__ 20170116144134.0
000003052 037__ $$aSCART-2017-0019
000003052 100__ $$aKrupar, V
000003052 245__ $$aAn Analysis of Interplanetary Solar Radio Emissions Associated with a Coronal Mass Ejection
000003052 260__ $$c2016
000003052 520__ $$aCoronal mass ejections (CMEs) are large-scale eruptions of magnetized plasma that may cause severe geomagnetic storms if Earth directed. Here, we report a rare instance with comprehensive in situ and remote sensing observations of a CME combining white-light, radio, and plasma measurements from four different vantage points. For the first time, we have successfully applied a radio direction-finding technique to an interplanetary type II burst detected by two identical widely separated radio receivers. The derived locations of the type II and type III bursts are in general agreement with the white-light CME reconstruction. We find that the radio emission arises from the flanks of the CME and are most likely associated with the CME-driven shock. Our work demonstrates the complementarity between radio triangulation and 3D reconstruction techniques for space weather applications.
000003052 594__ $$aSTCE
000003052 6531_ $$asolar–terrestrial relations, Sun: coronal mass ejections: CMEs, Sun: radio radiation
000003052 700__ $$aEastwood, J
000003052 700__ $$aKruparova, O
000003052 700__ $$aSantolik, O 
000003052 700__ $$aSoucek, J 
000003052 700__ $$aMagdalenic, J
000003052 700__ $$aVourlidas, A
000003052 700__ $$aMaksimovic, M 
000003052 700__ $$aBonnin, X 
000003052 700__ $$aBothmer, V
000003052 700__ $$aand, 6 coauthors
000003052 773__ $$n1$$pThe Astrophysical Journal Letters$$v823$$y2016
000003052 8560_ $$fjasmina.magdalenic@observatoire.be
000003052 905__ $$apublished in
000003052 980__ $$aREFERD