Osokin, A.R. and Podlazov, A.V. (2002) Self-Organized Criticality (SOC) model of solar flares. Il nuovo cimento C, 25 (5\6). pp. 761-767. ISSN 1826-9885
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Abstract
To describe the distributionof the total number of flares per time unit p(E), we bring forward a new self-organized critical model subject to uniform small-scale magnetic element and driving and dissipation. Due to diversity and complex interrelation of processes in the solar atmosphere, one needs to find the “main” process that “drives” the other ones. Magnetic-field reconnection in the sunatmosphere was usually treated as the mainpro cess by the SOC models. We, however, give the crucial role to the annihilation of oppositely charged magnetic elements on the sun surface, the elements being intersections of magnetic tubes with the sunsurface.
| Item Type: | Article |
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| Additional Information: | Paper presented at the International Meeting on THEMIS and the New Frontiers of Solar Atmosphere Dynamics, Rome, Italy, March 19-21, 2001. |
| Uncontrolled Keywords: | Flares, bursts, and related phenomena |
| Subjects: | 500 Scienze naturali e Matematica > 550 Scienze della Terra > 551 Geologia, Idrologia, Meteorologia > 551.5 Meteorologia (Classificare qui l'atmosfera) (Classificare la previsione e le previsioni di specifici fenomeni meteorologici in 551.64; classificare la Micrometeorologia in 551.66) > 551.52 Termodinamica, interazioni atmosferiche con la superficie terrestre, temperature, radiazioni > 551.527 Radiazioni (per fenomeni ottici, vedi 551.565) > 551.5271 Radiazione solare |
| Depositing User: | Marina Spanti |
| Date Deposited: | 12 Mar 2020 17:17 |
| Last Modified: | 12 Mar 2020 17:17 |
| URI: | http://eprints.bice.rm.cnr.it/id/eprint/15078 |
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