Janvier, G., Aulanier, V., Bommier, B., and Schmieder, P.,Démoulin, and Pariat, E., Electronic currents in flare ribbons: Observations and three-dimensional standard model, Astrophys. Hood, A.W., Archontis, V., and MacTaggart, D., 3D MHD flux emergence experiments: Idealised models and coronal interactions, Sol. and Bercik, B.T., Welsch, I et al., Global forces in eruptive solar flares: The Lorentz force acting on the solar atmosphere and the solar interior, Sol. and Lindsey, C., Seismic emission from the solar flares of 2003 October 28 and 29, Astrophys. L27–元0.ĭonea, A., Seismic transients from flares in solar cycle 23, Space Sci. 3151–3162.Ĭanou, A., Amari, T., Bommier, V., et al., Evidence for a pre-eruptive twisted flux rope using the Themis Vector Magnetograph, Astrophys. Lindsey, et al., A statistical correlation of sunquakes based on their seismic and white-light emission, Sol. Apparently, this was hindered by the nonstationarity of the phenomena at this activity center with a magnetic field of composite topology and multiple flare-generating centers.īuitrago-Casas, J.C., Martínez Oliveros, C. In this case, there was no development of a high-energy sigmoid flare with the formation and ejection of large-scale magnetized ropes. This rearrangement occurred in the proximity of a small region (sigmoid) presumably identified by the location of the primary pulse energy release. Rearrangement of the magnetic configuration in the analyzed event is confirmed: field lines and strong currents at low altitudes above the polarity boundary line are transformed into the currents along the system of loops oriented at wide angles to the neutral line. The reasons of such sunquakes are discussed. The disturbance, which propagated downwards and generated a source of acoustic waves (sunquake), was simultaneous with an outburst of hard X-radiation. The M flare that arises after magnetic field emersion in a small spot is analyzed.
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