Shock Location and CME 3-D Reconstruction of a Solar Type II Radio Burst with LOFAR

机译：带有LOFAR的太阳能II型无线电爆发的震荡位置和CME 3-D重建

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Type II radio bursts are evidence of shocks in the solar atmosphere and inner heliosphere emitting radio waves ranging from sub-meter to kilometre lengths. These shocks may be associated with coronal mass ejections (CMEs) reaching speeds higher than the local magneto-sonic speed. Radio imaging of decametre wavelengths (20-90 MHz) is now possible with the Low Frequency Array (LOFAR), opening a new radio window to study coronal shocks which leave the inner solar corona and enter the interplanetary medium and to understand their association with CMEs.

机译：II型无线电爆炸是太阳大气层和内部日球层受到冲击的证据，发出的电波范围从亚米到千米。这些冲击可能与冠状物质抛射（CME）达到的速度高于局部磁声速有关。现在可以使用低频阵列（LOFAR）对十米波长（20-90 MHz）进行无线电成像，从而打开一个新的无线电窗口来研究日冕电击，这些电击将离开内部太阳日冕并进入行星际介质，并了解它们与CME的关系。

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《2018 2nd URSI Atlantic Radio Science Meeting》|2018年|1-1|共1页
会议地点 Meloneras(ES)
作者
Pietro Zucca; Diana E. Morosan; Alexis Rouillard; Richard Fallows; Peter T. Gallagher; Jasmina Magdalenić; K-Ludwig Klein; Christian Vocks; Gottfried Mann;
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Netherlands Institute for Radio Astronomy, ASTRON, Dwingeloo, Postbus 2, 7990 AA, The Netherlands;

School of Physics, Trinity College Dublin, Astrophysics Research Group, Dublin, 2, Ireland;

Institut de Recherche en Astrophysique et Planetologie, Toulouse Cedex 4, 9 Ave. du Colonel Roche, 31028, France;

Netherlands Institute for Radio Astronomy, ASTRON, Dwingeloo, Postbus 2, 7990 AA, The Netherlands;

School of Physics, Trinity College Dublin, Astrophysics Research Group, Dublin, 2, Ireland;

Royal Observatory of Belgium, Solar-Terrestrial Center of Excellence, Brussels, Avenue Circulaire 3, 1180, Belgium;

UMR CNRS 8109, Observatoire de Paris, LESIA, Meudon, 92195, France;

Leibniz-Institut für Astrophysik Potsdam (AIP), Potsdam, An der Sternwarte 16, 14482, Germany;

Leibniz-Institut für Astrophysik Potsdam (AIP), Potsdam, An der Sternwarte 16, 14482, Germany;

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专利

1. Type II solar radio bursts predicted by 3-D MHD CME and kinetic radio emission simulations [J] . J. M. Schmidt, Iver H. Cairns Journal of Geophysical Research, A. Space Physics: JGR . 2014,第1期

机译：通过3-D MHD CME和动态无线电发射模拟预测的II型太阳无线电脉冲
2. CME-driven Shock and Type II Solar Radio Burst Band Splitting [J] . Nicolina Chrysaphi, Eduard P. Kontar, Gordon D. Holman, The Astrophysical journal . 2018,第2期

机译：CME驱动的电击和II型太阳能无线电突发频带分裂
3. Solar type III radio burst time characteristics at LOFAR frequencies and the implications for electron beam transport [J] . Hamish A. S. Reid, Eduard P. Kontar Astronomy and astrophysics . 2018,第8期

机译：LOFAR频率的太阳III类无线电突发时间特性及其对电子束传输的影响
4. Shock Location and CME 3-D Reconstruction of a Solar Type II Radio Burst with LOFAR [C] . Pietro Zucca, Diana E. Morosan, Alexis Rouillard, URSI Atlantic Radio Science Meeting . 2018

机译：带龙马的太阳能II无线电爆裂的冲击位置和CME 3-D重建
5. Influence of CME interaction on the intensities of type II radio bursts [D] . Nunes, Steven Michael 2007

机译：CME交互作用对II型无线电脉冲串强度的影响
6. Low Altitude Solar Magnetic Reconnection Type III Solar Radio Bursts and X-ray Emissions [O] . I. H. Cairns, V. V. Lobzin, A. Donea, -1

机译：低空太阳磁重连III型太阳射电爆发和X射线发射
7. Shock location and CME 3D reconstruction of a solar type II radio burst with LOFAR [O] . P. Zucca, D. E. Morosan, A. P. Rouillard, 2018

机译：洛伐华太阳能II无线电爆裂的冲击位置和CME 3D重建
8. Shock-Associated Kilometric Radio Emission and Solar Metric Type II Bursts. [R] . Kahler, S. W., Cliver, E. W., Cane, H. V. 1989

机译：冲击相关的公斤无线电发射和太阳公制II型爆发。

Shock Location and CME 3-D Reconstruction of a Solar Type II Radio Burst with LOFAR

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