Search Results - "Luoni, M. L."

Tracing magnetic helicity from the solar corona to the interplanetary space by Luoni, M.L., Mandrini, C.H., Dasso, Sergio, van Driel-Gesztelyi, L., Démoulin, P.

“…On October 14, 1995, a C1.6 long duration event (LDE) started in active region (AR) NOAA 7912 at approximately 5:00 UT and lasted for about 15 h. On October…”
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Large scale MHD properties of interplanetary magnetic clouds by Dasso, S., Mandrini, C.H., Démoulin, P., Luoni, M.L., Gulisano, A.M.

“…Magnetic Clouds (MCs) are the interplanetary manifestation of Coronal Mass Ejections. These huge astrophysical objects travel from the Sun toward the external…”
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Twisted Flux Tube Emergence Evidenced in Longitudinal Magnetograms: Magnetic Tongues by Luoni, M. L., Démoulin, P., Mandrini, C. H., van Driel-Gesztelyi, L.

“…Bipolar active regions (ARs) are thought to be formed by twisted flux tubes, as the presence of such twist is theoretically required for a cohesive rise…”
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Origin of the Submillimeter Radio Emission During the Time-Extended Phase of a Solar Flare by Trottet, G., Raulin, J.-P., Giménez de Castro, G., Lüthi, T., Caspi, A., Mandrini, C. H., Luoni, M. L., Kaufmann, P.

“…Solar flares observed in the 200 – 400 GHz radio domain may exhibit a slowly varying and time-extended component which follows a short (few minutes) impulsive…”
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The magnetic field topology associated with two M flares by Luoni, M.L., Mandrini, C.H., Cristiani, G.D., Démoulin, P.

“…On 27 October, 2003, two GOES M-class flares occurred in an interval of 3 h in active region NOAA 10486. The two flares were confined and their associated…”
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Observed flux density enhancement at submillimeter wavelengths during an X-class flare by Cristiani, G., Giménez de Castro, C.G., Luoni, M.L., Mandrini, C.H., Rovira, M.G., Kaufmann, P., Machado, M.

“…We analyse the 30 October, 2004, X1.2/SF solar event that occurred in AR 10691 (N13 W18) at around 11:44 UT. Observations at 212 and 405 GHz of the Solar…”
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Comparison of 30 THz impulsive burst time development to microwaves, H-alpha, EUV, and GOES soft X-rays by Miteva, R, Kaufmann, P, Cabezas, D. P, Cassiano, M. M, Fernandes, L. O. T, Freeland, S. L, Karlicky, M, Kerdraon, A, Kudaka, A. S, Luoni, M. L, Marcon, R, Raulin, J. -P, Trottet, G, White, S. M

“…A&A 586, A91 (2016) The recent discovery of impulsive solar burst emission in the 30 THz band is raising new interpretation challenges. One event associated…”
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12 Years of Stellar Activity Observations in Argentina by Mauas, Pablo J. D, Buccino, A, Diaz, R, Vieytes, M, Petrucci, R, Jofre, E, Abrevaya, X, Luoni, M. L, Valenzuela, P

“…We present an observational program we started in 1999, to systematically obtain mid-resolution spectra of late-type stars, to study in particular…”
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Origin of the submillimeter radio emission during the time-extended phase of a solar flare by Trottet, G, Raulin, J. -P, de Castro, G. Giménez, Lüthi, T, Caspi, A, Mandrini, C. H, Luoni, M. L, Kaufmann, P

“…Solar Physics, Vol. 273, Issue 2, pp. 339-361; 2011 November 8 Solar flares observed in the 200-400 GHz radio domain may exhibit a slowly varying and…”
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The magnetic field topology associated to two M flares by Luoni, M. L, Mandrini, C. H, Cristiani, G, Démoulin, P

“…Adv.SpaceRes.39:1382-1388,2007 On 27 October, 2003, two GOES M-class flares occurred in the lapse of three hours in active region NOAA 10486. The two flares…”
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Observed flux density enhancement at submillimeter wavelengths during an X-class flare by Cristiani, G, de Castro, C. G. Giménez, Luoni, M. L, Mandrini, C. H, Rovira, M. G, Kaufmann, P

“…Adv.SpaceRes.39:1447-1452,2007 We analyse the 30 October, 2004, X1.2/SF solar event that occurred in AR 10691 (N13 W18) at around 11:44 UT. Observations at 212…”
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