Veltri, P. and Malara, F. (1997) Theoretical models for MHD turbulence in the solar wind. Il nuovo cimento C, 20 C (6). pp. 859-870. ISSN 1826-9885
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Abstract
The in situ measurements of velocity, magnetic field, density and temperature fluctuations performed in the solar wind have greatly improved our knowledge of MHD turbulence not only from the point of view of space physics but also from the more general point of view of plasma physics. These fluctuations which extend over a wide range of frequencies (about 5 decades), a fact which seems to be the signature of turbulent nonlinear energy cascade, display, mainly in the trailing edge of high-speed streams, a number of features characteristic of a self-organized situation: i) a high degree of correlation between magnetic and velocity field fluctuations, ii) a very low level of fluctuations in mass density and magnetic-field intensity, iii) a considerable anisotropy revealed by minimum variance analysis of the magnetic-field correlation tensor. Many fundamental processes in plasma physics, which were largely unknown or not understood before their observations in the solar wind, have been explained, by building up analytical models or performing numerical simulations. We discuss the most recent analytical theories and numerical simulations and outline the limits implicit in any analysis which consider the low-frequency solar-wind fluctuations as a superposition of linear modes. The characterization of low-frequency fluctuations during Alfv´enic periods, which results from the models discussed, is finally presented.
| Item Type: | Article |
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| Additional Information: | Paper presented at the VII Cosmic Physics National Conference, Rimini, October 26-28, 1994. |
| Uncontrolled Keywords: | Solar physics; magnetohydrodynamic waves; conference proceedings |
| Subjects: | 500 Scienze naturali e Matematica > 530 Fisica 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) > 551.5276 Radiazioni cosmiche (Include il rumore cosmico) (Classificare qui i raggi cosmici) |
| Depositing User: | Marina Spanti |
| Date Deposited: | 09 Feb 2018 09:11 |
| Last Modified: | 09 Feb 2018 09:11 |
| URI: | http://eprints.bice.rm.cnr.it/id/eprint/12393 |
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