1 Byrne, J. P., Maloney, S. A., McAteer, R. T. J., Refojo, J. M. & Gallagher, P. T. Propagation of an Earth-directed coronal mass ejection in three dimensions. Nature Commun. 1, 74 (2010).

2 Roussev, I. I. et al. Explaining fast ejections of plasma and exotic X-ray emission from the solar corona. Nature Phys. 8, 845–849 (2012).

3 Vourlidas, A. et al. Comprehensive analysis of coronal mass ejection mass and energy properties over a full solar cycle. Astrophys. J. 722, 1522–1538 (2010).

4 Klassen, A. et al. Solar energetic electron events and coronal shocks. Astron. Astrophys. 385, 1078–1088 (2002).

5 Grechnev, V. V. et al. Coronal shock waves, EUV waves, and their relation to CMEs. I. Reconciliation of EIT Waves, Type II radio bursts, and leading edges of CMEs. Sol. Phys. 273, 433–460 (2011).

6 Vršnak, B. & Cliver, E. W. Origin of coronal shock waves. invited review. Sol. Phys. 253, 215–235 (2008).

7 Drury, L. O. Origin of cosmic rays. Astropart. Phys. 39, 52–60 (2012).

8 Wild, J. P. Observations of the spectrum of high-intensity solar radiation at metre wavelengths. III. Isolated bursts. Aust. J. Sci. Res. A 3, 541–557 (1950).

9 Mann, G. et al. Catalogue of solar type II radio bursts observed from September 1990 to December 1993 and their statistical analysis. Astron. Astrophys. Suppl. 119, 489–498 (1996).

10 Mann, G. & Klassen, A. Electron beams generated by shock waves in the solar corona. Astron. Astrophys. 441, 319–326 (2005).

11 Zlobec, P., Messerotti, M., Karlicky, M. & Urbarz, H. Fine structures in time profiles of type II bursts at frequencies above 200 MHz. Sol. Phys. 144, 373–384 (1993).

12 Guo, F. & Giacalone, J. The effect of large-scale magnetic turbulence on the acceleration of electrons by perpendicular collisionless shocks. Astrophys. J. 715, 406–411 (2010).

13 Gallagher, P. T. & Long, D. M. Large-scale bright fronts in the solar corona: A review of EIT waves. Space Sci. Rev. 158, 365–396 (2011).

14 Gopalswamy, N. et al. EUV wave reflection from a coronal hole. Astrophys. J. 691, L123–L127 (2009).

15 Wang, Y-M. EIT waves and fast-mode propagation in the solar corona. Astrophys. J. 543, L89–L93 (2000).

16 Long, D. M., Gallagher, P. T., McAteer, R. T. J. & Bloomfield, D. S. Deceleration and dispersion of large-scale coronal bright fronts. Astron. Astrophys. 531, A42–A42 (2011).

17 Maia, D. J. F. & Pick, M. Revisiting the origin of impulsive electron events: Coronal magnetic restructuring. Astrophys. J. 609, 1082–1097 (2004).

18 Kozarev, K. A., Korreck, K. E., Lobzin, V. V., Weber, M. A. & Schwadron, N. A. Off-limb solar coronal wavefronts from SDO/AIA extreme-ultraviolet observations—Implications for particle production. Astrophys. J. 733, L25 (2011).

19 Vršnak, B. et al. Broadband metric-range radio emission associated with a moreton/EIT wave. Astrophys. J. 625, L67–L70 (2005).

20 Warmuth, A., Vršnak, B., Magdalenić, J., Hanslmeier, A. & Otruba, W. A multiwavelength study of solar flare waves. II. Perturbation characteristics and physical interpretation. Astron. Astrophys. 418, 1117–1129 (2004).

21 Zhukov, A. N., Rodriguez, L. & de Patoul, J. STEREO/SECCHI observations on 8 December 2007: Evidence against the wave hypothesis of the EIT wave origin. Sol. Phys. 259, 73–85 (2009).

22 Delannée, C., Török, T., Aulanier, G. & Hochedez, J-F. A new model for propagating parts of EIT waves: A current shell in a CME. Sol. Phys. 247, 123–150 (2008).

23 Kahler, S. W. Solar sources of heliospheric energetic electron events—Shocks or flares? Space Sci. Rev. 129, 359–390 (2007).

24 Pesnell, W. D., Thompson, B. J. & Chamberlin, P. C. The solar dynamics observatory (SDO). Sol. Phys. 275, 3–15 (2012).

25 Lemen, J. R. et al. The Atmospheric Imaging Assembly (AIA) on the Solar Dynamics Observatory (SDO). Sol. Phys. 275, 17–40 (2012).

26 Kerdraon, A. & Delouis, J-M. in Coronal Physics from Radio and Space Observations Vol. 483 (ed. Trottet, G.) 192–201 (Lecture Notes in Physics, Springer, 1997).

27 Dulk, G. A. Radio emission from the sun and stars. Annu. Rev. Astron. Astrophys. 23, 169–224 (1985).

28 Boischot, A. et al. A new high-gain, broadband, steerable array to study Jovian decametric emission. Icarus 43, 399–407 (1980).

29 Bougeret, J. L. et al. S/WAVES: The radio and plasma wave investigation on the STEREO mission. Space Sci. Rev. 136, 487–528 (2008).

30 Benz, A. O. et al. A world-wide net of solar radio spectrometers: e-CALLISTO. Earth Moon and Planets 104, 277–285 (2009).

31 Zucca, P. et al. Observations of low frequency solar radio bursts from the Rosse solar-terrestrial observatory. Sol. Phys. 280, 591–602 (2012).

32 Burgess, D. Simulations of electron acceleration at collisionless shocks: The effects of surface fluctuations. Astrophys. J. 653, 316–324 (2006).

33 Stewart, R. T. & Magun, A. Radio evidence for electron acceleration by transverse shock waves in herringbone Type II solar bursts. Proc. Astron. Soc. Aust. 4, 53–55 (1980).

34 Schmidt, J. M. & Cairns, I. H. Type II radio bursts: 2. Application of the new analytic formalism. J. Geophys. Res. 117, 11104 (2012).

35 Brueckner, G. E. et al. The large angle spectroscopic coronagraph (LASCO). Sol. Phys. 162, 357–402 (1995).

36 Vourlidas, A., Lynch, B. J., Howard, R. A. & Li, Y. How many CMEs have flux ropes? Deciphering the signatures of shocks, flux ropes, and prominences in coronagraph observations of CMEs. Sol. Phys. 192 (2012).

37 Maloney, S. A. & Gallagher, P. T. STEREO direct imaging of a coronal mass ejection-driven shock to 0.5 AU. Astrophys. J. 736, L5 (2011).

38 Feng, S. W. et al. Radio signatures of coronal-mass-ejection-streamer interaction and source diagnostics of type II radio burst. Astrophys. J. 753, 21 (2012).

39 Feng, S. W. et al. Diagnostics on the source properties of a type II radio burst with spectral bumps. Astrophys. J. 767, 29 (2013).

40 Bain, H. M., Krucker, S., Glesener, L. & Lin, R. P. Radio imaging of shock-accelerated electrons associated with an erupting plasmoid on 2010 November 3. Astrophys. J. 750, 44 (2012).

41 Ball, L. & Melrose, D. B. Shock drift acceleration of electrons. Publ. Astron. Soc. Aust. 18, 361–373 (2001).

42 Wu, C. S. A fast Fermi process—Energetic electrons accelerated by a nearly perpendicular bow shock. J. Geophys. Res. 89, 8857–8862 (1984).

43 Holman, G. D. & Pesses, M. E. Solar type II radio emission and the shock drift acceleration of electrons. Astrophys. J. 267, 837–843 (1983).

44 Guo, F. & Giacalone, J. Particle acceleration at a flare termination shock: Effect of large-scale magnetic turbulence. Astrophys. J. 753, 28–28 (2012).

45 Vandas, M. & Karlický, M. Electron acceleration in a wavy shock front. Astron. Astrophys. 531, A55 (2011).

46 Lowe, R. E. & Burgess, D. The properties and causes of rippling in quasi-perpendicular collisionless shock fronts. Ann. Geophys. 21, 671–679 (2003).

47 Aurass, H. & Mann, G. Radio observation of electron acceleration at solar flare reconnection outflow termination shocks. Astrophys. J. 615, 526–530 (2004).

48 Van Haarlem, M. P. et al. LOFAR: The low-frequency array. Astron. Astrophys. 556, A2 (2013).

49 Stewart, R. T. & McLean, D. J. Correcting low-frequency solar radio source positions for ionospheric refraction. Proc. Astron. Soc. Australia 4, 386–389 (1982).