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Cited article:

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Peak flux of flares associated with coronal mass ejections

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Towards understanding the frequency distribution of solar flares—part 1: a Stochastic-Diffusive model of solar flares

Z. L. Du
Astrophysics and Space Science 359 (1) (2015)
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The Chandrayaan-1 X-ray Spectrometer: First results

S.Z. Weider, B.J. Kellett, B.M. Swinyard, I.A. Crawford, K.H. Joy, M. Grande, C.J. Howe, J. Huovelin, S. Narendranath, L. Alha, M. Anand, P.S. Athiray, N. Bhandari, J.A. Carter, A.C. Cook, L.C. d'Uston, V.A. Fernandes, O. Gasnault, J.N. Goswami, J.P.D. Gow, A.D. Holland, D. Koschny, D.J. Lawrence, B.J. Maddison, S. Maurice, et al.
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Statistical Study of the Reconnection Rate in Solar Flares Observed withYohkohSXT

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Different Power-Law Indices in the Frequency Distributions of Flares with and without Coronal Mass Ejections

S. Yashiro, S. Akiyama, N. Gopalswamy and R. A. Howard
The Astrophysical Journal 650 (2) L143 (2006)
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Non-thermal broadening of coronal emission lines in the onset phase of solar flares and CMEs

H. R. M. Kay, S. A. Matthews, L. K. Harra and J. L. Culhane
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Solar flares with and without SOHO/LASCO coronal mass ejections and type II shocks

A. Hillaris, V. Petousis, E. Mitsakou, C. Vassiliou, X. Moussas, J. Polygiannakis, P. Preka-Papadema, C. Caroubalos, C. Alissandrakis, P. Tsitsipis, A. Kontogeorgos, J.-L. Bougeret and G. Dumas
Advances in Space Research 38 (5) 1007 (2006)
https://doi.org/10.1016/j.asr.2005.11.003