Shock location and CME 3D reconstruction of a solar type II radio burst with LOFAR

A. Asgekar; A. Deller; A. G. Polatidis; A. Karastergiou; A. Krankowski; A. Nelles; A. P. Rouillard; A. Rowlinson; A. Shulevski; A. W. Gunst

Shock location and CME 3D reconstruction of a solar type II radio burst with LOFAR

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arxiv 1804.01025 v1 pith:NJM2ZHC7 submitted 2018-04-03 astro-ph.SR

Shock location and CME 3D reconstruction of a solar type II radio burst with LOFAR

P. Zucca , D. E. Morosan , A. P. Rouillard , R. Fallows , P. T. Gallagher , J. Magdalenic , K-L. Klein , G. Mann

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C. Vocks E. P. Carley M. M. Bisi E. P. Kontar H. Rothkaehl B. Dabrowski A. Krankowski J. Anderson A. Asgekar M. E. Bell M. J. Bentum P. Best R. Blaauw F. Breitling J. W. Broderick W. N. Brouw M. Bruggen H. R. Butcher B. Ciardi E. de Geus A. Deller S. Duscha J. Eisloffel M. A. Garrett J. M. Grie{\ss}meier A. W. Gunst G. Heald M. Hoeft J. Horandel M. Iacobelli E. Juette A. Karastergiou J. van Leeuwen D. McKay-Bukowski H. Mulder H. Munk A. Nelles E. Orru H. Paas V. N. Pandey R. Pekal R. Pizzo A. G. Polatidis W. Reich A. Rowlinson D. J. Schwarz A. Shulevski J. Sluman O. Smirnov C. Sobey M. Soida S. Thoudam M. C. Toribio R. Vermeulen R. J. van Weeren O. Wucknitz P. Zarka

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Type II radio bursts are evidence of shocks in the solar atmosphere and inner heliosphere that emit radio waves ranging from sub-meter to kilometer lengths. These shocks may be associated with CMEs and reach speeds higher than the local magnetosonic speed. Radio imaging of decameter wavelengths (20-90 MHz) is now possible with LOFAR, opening a new radio window in which to study coronal shocks that leave the inner solar corona and enter the interplanetary medium and to understand their association with CMEs. To this end, we study a coronal shock associated with a CME and type II radio burst to determine the locations at which the radio emission is generated, and we investigate the origin of the band-splitting phenomenon.

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