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Magnetic fields
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Sun: flares
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1por van Driel-Gesztelyi, L., Goff, C.P., Démoulin, P., Culhane, J.L., Matthews, S.A., Harra, L.K., Mandrini, C.H., Klein, K.-L., Kurokawa, H.“... main conclusions. First, we link the first two impulsive flares to tether-cutting reconnections...”
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2por Green, L.M., López Fuentes, M.C., Mandrini, C.H., Démoulin, P., Van Driel-Gesztelyi, L., Culhane, J.L.“.... This paper studies the magnetic helicity evolution in an active region (NOAA 8100) in which the main...”
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3por Harra, L.K., Démoulin, P., Mandrini, C.H., Matthews, S.A., Van Driel-Gesztelyi, L., Culhane, J.L., Fletcher, L.“... the main phase, the ongoing magnetic reconnection is demonstrated by upflows located at the edges...”
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4por Mandrini, C.H., Nuevo, F.A., Vásquez, A.M., Démoulin, P., van Driel-Gesztelyi, L., Baker, D., Culhane, J.L., Cristiani, G.D., Pick, M.“... and be released into the SW via magnetic reconnection, which occurs in at least two main steps. We analyse data...”
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