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Richard L, Sorriso-Valvo L, Yordanova E, Graham DB, Khotyaintsev YV. Turbulence in Magnetic Reconnection Jets from Injection to Sub-Ion Scales. Phys Rev Lett 2024; 132:105201. [PMID: 38518330 DOI: 10.1103/physrevlett.132.105201] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 03/16/2023] [Revised: 10/02/2023] [Accepted: 02/05/2024] [Indexed: 03/24/2024]
Abstract
We investigate turbulence in magnetic reconnection jets in the Earth's magnetotail using data from the Magnetospheric Multiscale spacecraft. We show that signatures of a limited inertial range are observed in many reconnection jets. The observed turbulence develops on the timescale of a few ion gyroperiods, resulting in intermittent multifractal energy cascade from the characteristic scale of the jet down to the ion scales. We show that at sub-ion scales, the fluctuations are close to monofractal and predominantly kinetic Alfvén waves. The observed energy transfer rate across the inertial range is ∼10^{8} J kg^{-1} s^{-1}, which is the largest reported for space plasmas so far.
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Affiliation(s)
- Louis Richard
- Swedish Institute of Space Physics, Uppsala 751 21, Sweden and Department of Physics and Astronomy, Space and Plasma Physics, Uppsala University, Uppsala 751 20, Sweden
| | - Luca Sorriso-Valvo
- CNR/ISTP-Istituto per la Scienza e la Tecnologia dei Plasmi, 70126 Bari, Italy; Space and Plasma Physics, School of Electrical Engineering and Computer Science, KTH Royal Institute of Technology, Stockholm 114 28, Sweden; and Swedish Institute of Space Physics, Uppsala 751 21, Sweden
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2
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Carbone F, Alberti T, Faranda D, Telloni D, Consolini G, Sorriso-Valvo L. Local dimensionality and inverse persistence analysis of atmospheric turbulence in the stable boundary layer. Phys Rev E 2022; 106:064211. [PMID: 36671155 DOI: 10.1103/physreve.106.064211] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 05/05/2022] [Accepted: 11/30/2022] [Indexed: 06/17/2023]
Abstract
The dynamics across different scales in the stable atmospheric boundary layer has been investigated by means of two metrics, based on instantaneous fractal dimensions and grounded in dynamical systems theory. The wind velocity fluctuations obtained from data collected during the Cooperative Atmosphere-Surface Exchange Study-1999 experiment were analyzed to provide a local (in terms of scales) and an instantaneous (in terms of time) description of the fractal properties and predictability of the system. By analyzing the phase-space projections of the continuous turbulent, intermittent, and radiative regimes, a progressive transformation, characterized by the emergence of multiple low-dimensional clusters embedded in a high-dimensional shell and a two-lobe mirror symmetrical structure of the inverse persistence, have been found. The phase space becomes increasingly complex and anisotropic as the turbulent fluctuations become uncorrelated. The phase space is characterized by a three-dimensional structure for the continuous turbulent samples in a range of scales compatible with the inertial subrange, where the phase-space-filling turbulent fluctuations dominate the dynamics, and is low dimensional in the other regimes. Moreover, lower-dimensional structures present a stronger persistence than the higher-dimensional structures. Eventually, all samples recover a three-dimensional structure and higher persistence level at large scales, far from the inertial subrange. The two metrics obtained in the analysis can be considered as proxies for the decorrelation time and the local anisotropy in the turbulent flow.
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Affiliation(s)
- Francesco Carbone
- National Research Council, Institute of Atmospheric Pollution Research, C/o University of Calabria, 87036 Rende, Italy
| | - Tommaso Alberti
- National Institute for Astrophysics, Institute for Space Astrophysics and Planetology, 00133 Roma, Italy
| | - Davide Faranda
- Laboratoire des Sciences du Climat et de lEnvironnement, CEA Saclay lOrme des Merisiers, UMR 8212 CEA-CNRS-UVSQ, Université Paris-Saclay & IPSL, 91191, Gif-sur-Yvette, France
- London Mathematical Laboratory, London W6 8RH, United Kindgom
- LMD/IPSL, Ecole Normale Superieure, PSL Research University, 75005 Paris, France
| | - Daniele Telloni
- National Institute for Astrophysics, Astrophysical Observatory of Torino, 10025 Pino Torinese, Italy
| | - Giuseppe Consolini
- National Institute for Astrophysics, Institute for Space Astrophysics and Planetology, 00133 Roma, Italy
| | - Luca Sorriso-Valvo
- Swedish Institute of Space Physics, Ångström Laboratory, SE-751 21 Uppsala, Sweden
- National Research Council, Institute for Plasma Science and Technology, 70126 Bari, Italy
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Carbone F, Telloni D, Zank G, Sorriso-Valvo L. Transition to turbulence in a five-mode Galerkin truncation of two-dimensional magnetohydrodynamics. Phys Rev E 2021; 104:025201. [PMID: 34525508 DOI: 10.1103/physreve.104.025201] [Citation(s) in RCA: 1] [Impact Index Per Article: 0.3] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 04/19/2021] [Accepted: 07/09/2021] [Indexed: 11/07/2022]
Abstract
The chaotic dynamics of a low-order Galerkin truncation of the two-dimensional magnetohydrodynamic system, which reproduces the dynamics of fluctuations described by nearly incompressible magnetohydrodynamic in the plane perpendicular to a background magnetic field, is investigated by increasing the external forcing terms. Although this is the case closest to two-dimensional hydrodynamics, which shares some aspects with the classical Feigenbaum scenario of transition to chaos, the presence of magnetic fluctuations yields a very complex interesting route to chaos, characterized by the splitting into multiharmonic structures of the field amplitudes, and a mixing of phase-locking and free phase precession acting intermittently. When the background magnetic field lies in the plane, the system supports the presence of Alfvén waves thus lowering the nonlinear interactions. Interestingly enough, the dynamics critically depends on the angle between the direction of the magnetic field and the reference system of the wave vectors. Above a certain critical angle, independently from the external forcing, a breakdown of the phase locking appears, accompanied with a suppression of the chaotic dynamics, replaced by a simple periodic motion.
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Affiliation(s)
- Francesco Carbone
- National Research Council - Institute of Atmospheric Pollution Research, C/o University of Calabria, 87036 Rende, Italy
| | - Daniele Telloni
- National Institute for Astrophysics - Astrophysical Observatory of Torino, Via Osservatorio 20, 10025 Pino Torinese, Italy
| | - Gary Zank
- Center for Space Plasma and Aeronomic Research (CSPAR), University of Alabama in Huntsville, Huntsville, Alabama 35899, USA and Department of Space Science, University of Alabama in Huntsville, Huntsville, Alabama 35899, USA
| | - Luca Sorriso-Valvo
- Swedish Institute of Space Physics, Ångström Laboratory, Lägerhyddsvägen 1, SE-751 21 Uppsala, Sweden and CNR, Istituto per la Scienza e Tecnologia dei Plasmi, Via Amendola 122/D, 70126 Bari, Italy
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Bandyopadhyay R, Sorriso-Valvo L, Chasapis A, Hellinger P, Matthaeus WH, Verdini A, Landi S, Franci L, Matteini L, Giles BL, Gershman DJ, Moore TE, Pollock CJ, Russell CT, Strangeway RJ, Torbert RB, Burch JL. In Situ Observation of Hall Magnetohydrodynamic Cascade in Space Plasma. Phys Rev Lett 2020; 124:225101. [PMID: 32567898 DOI: 10.1103/physrevlett.124.225101] [Citation(s) in RCA: 8] [Impact Index Per Article: 2.0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 07/12/2019] [Revised: 04/07/2020] [Accepted: 05/01/2020] [Indexed: 05/20/2023]
Abstract
We present estimates of the turbulent energy-cascade rate derived from a Hall-magnetohydrodynamic (MHD) third-order law. We compute the contribution from the Hall term and the MHD term to the energy flux. Magnetospheric Multiscale (MMS) data accumulated in the magnetosheath and the solar wind are compared with previously established simulation results. Consistent with the simulations, we find that at large (MHD) scales, the MMS observations exhibit a clear inertial range dominated by the MHD flux. In the subion range, the cascade continues at a diminished level via the Hall term, and the change becomes more pronounced as the plasma beta increases. Additionally, the MHD contribution to interscale energy transfer remains important at smaller scales than previously thought. Possible reasons are offered for this unanticipated result.
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Affiliation(s)
- Riddhi Bandyopadhyay
- Department of Physics and Astronomy, University of Delaware, Newark, Delaware 19716, USA
| | - Luca Sorriso-Valvo
- Departamento de Física, Escuela Politécnica Nacional, 170517 Quito, Ecuador and Istituto per la Scienza e Tecnologia dei Plasmi, Consiglio Nazionale delle Ricerche, 87036 Bari, Italy
| | - Alexandros Chasapis
- Laboratory for Atmospheric and Space Physics, University of Colorado Boulder, Boulder, Colorado 80303, USA
| | - Petr Hellinger
- Astronomical Institute, CAS, Bocni II/1401, CZ-14100 Prague, Czech Republic and Institute of Atmospheric Physics, CAS, Bocni II/1401, CZ-14100 Prague, Czech Republic
| | - William H Matthaeus
- Department of Physics and Astronomy, University of Delaware, Newark, Delaware 19716, USA and Bartol Research Institute, University of Delaware, Newark, Delaware 19716, USA
| | - Andrea Verdini
- Dipartimento di Fisica e Astronomia, Universitá degli Studi di Firenze, 50125 Firenze, Italy and INAF, Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, I-50125 Firenze, Italy
| | - Simone Landi
- Dipartimento di Fisica e Astronomia, Universitá degli Studi di Firenze, 50125 Firenze, Italy and INAF, Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, I-50125 Firenze, Italy
| | - Luca Franci
- School of Physics and Astronomy, Queen Mary University of London, London E1 4NS, United Kingdom and INAF, Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, I-50125 Firenze, Italy
| | - Lorenzo Matteini
- LESIA, Observatoire de Paris, Meudon, France and INAF, Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, I-50125 Firenze, Italy
| | - Barbara L Giles
- NASA Goddard Space Flight Center, Greenbelt, Maryland 20771, USA
| | | | - Thomas E Moore
- NASA Goddard Space Flight Center, Greenbelt, Maryland 20771, USA
| | | | | | | | - Roy B Torbert
- University of New Hampshire, Durham, New Hampshire 03824, USA
| | - James L Burch
- Southwest Research Institute, San Antonio, Texas 78238-5166, USA
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Sorriso-Valvo L, Catapano F, Retinò A, Le Contel O, Perrone D, Roberts OW, Coburn JT, Panebianco V, Valentini F, Perri S, Greco A, Malara F, Carbone V, Veltri P, Pezzi O, Fraternale F, Di Mare F, Marino R, Giles B, Moore TE, Russell CT, Torbert RB, Burch JL, Khotyaintsev YV. Turbulence-Driven Ion Beams in the Magnetospheric Kelvin-Helmholtz Instability. Phys Rev Lett 2019; 122:035102. [PMID: 30735422 DOI: 10.1103/physrevlett.122.035102] [Citation(s) in RCA: 5] [Impact Index Per Article: 1.0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 09/20/2018] [Revised: 12/10/2018] [Indexed: 05/20/2023]
Abstract
The description of the local turbulent energy transfer and the high-resolution ion distributions measured by the Magnetospheric Multiscale mission together provide a formidable tool to explore the cross-scale connection between the fluid-scale energy cascade and plasma processes at subion scales. When the small-scale energy transfer is dominated by Alfvénic, correlated velocity, and magnetic field fluctuations, beams of accelerated particles are more likely observed. Here, for the first time, we report observations suggesting the nonlinear wave-particle interaction as one possible mechanism for the energy dissipation in space plasmas.
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Affiliation(s)
- Luca Sorriso-Valvo
- Nanotec/CNR, U.O.S. di Cosenza, Ponte P. Bucci, cubo 31C, 87036 Rende, Italy and Departamento de Física, Escuela Politécnica Nacional, 170517 Quito, Ecuador
| | - Filomena Catapano
- Dipartimento di Fisica, Università della Calabria, Ponte P. Bucci, cubo 31C, 87036 Rende, Italy and LPP-CNRS/Ecole Polytechnique/Sorbonne Université, 91128 Palaiseau Cedex, France
| | - Alessandro Retinò
- LPP-CNRS/Ecole Polytechnique/Sorbonne Université, 91128 Palaiseau Cedex, France
| | - Olivier Le Contel
- LPP-CNRS/Ecole Polytechnique/Sorbonne Université, 91128 Palaiseau Cedex, France
| | - Denise Perrone
- Department of Physics, Imperial College of London, London SW7 2AZ, United Kingdom
| | - Owen W Roberts
- Space Research Institute, Austrian Academy of Sciences, Schmiedlstrasse 6, 8042 Graz, Austria
| | - Jesse T Coburn
- Dipartimento di Fisica, Università della Calabria, Ponte P. Bucci, cubo 31C, 87036 Rende, Italy
| | - Vincenzo Panebianco
- Dipartimento di Fisica, Università della Calabria, Ponte P. Bucci, cubo 31C, 87036 Rende, Italy
| | - Francesco Valentini
- Dipartimento di Fisica, Università della Calabria, Ponte P. Bucci, cubo 31C, 87036 Rende, Italy
| | - Silvia Perri
- Dipartimento di Fisica, Università della Calabria, Ponte P. Bucci, cubo 31C, 87036 Rende, Italy
| | - Antonella Greco
- Dipartimento di Fisica, Università della Calabria, Ponte P. Bucci, cubo 31C, 87036 Rende, Italy
| | - Francesco Malara
- Dipartimento di Fisica, Università della Calabria, Ponte P. Bucci, cubo 31C, 87036 Rende, Italy
| | - Vincenzo Carbone
- Dipartimento di Fisica, Università della Calabria, Ponte P. Bucci, cubo 31C, 87036 Rende, Italy
| | - Pierluigi Veltri
- Dipartimento di Fisica, Università della Calabria, Ponte P. Bucci, cubo 31C, 87036 Rende, Italy
| | - Oreste Pezzi
- Gran Sasso Science Institute, Viale F. Crispi 7, 67100 L'Aquila, Italy and Dipartimento di Fisica, Università della Calabria, Ponte P. Bucci, cubo 31C, 87036 Rende, Italy
| | - Federico Fraternale
- Dipartimento di Scienza Applicata e Tecnologia, Politecnico di Torino, 10129 Torino, Italy
| | - Francesca Di Mare
- Department of Physics, University of Oslo, Sem Sælands Vei 26, Fysikkbygningen 0371 Oslo, Norway
| | - Raffaele Marino
- Laboratoire de Mécanique des Fluides et d'Acoustique, CNRS, École Centrale de Lyon, Université Claude Bernard Lyon 1, INSA de Lyon, F-69134 Écully, France
| | - Barbara Giles
- NASA, Goddard Space Flight Center, Greenbelt, Maryland 20771, USA
| | - Thomas E Moore
- NASA, Goddard Space Flight Center, Greenbelt, Maryland 20771, USA
| | - Christopher T Russell
- Institute of Geophysics and Planetary Physics, and Department of Earth, Planetary, and Space Sciences, University of California, Los Angeles, California 90095-1567, USA
| | - Roy B Torbert
- Space Science Center, University of New Hampshire, Durham, New Hampshire 03824, USA
| | - Jim L Burch
- Southwest Research Institute, San Antonio, Texas 78238-5166, USA
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Camporeale E, Sorriso-Valvo L, Califano F, Retinò A. Coherent Structures and Spectral Energy Transfer in Turbulent Plasma: A Space-Filter Approach. Phys Rev Lett 2018; 120:125101. [PMID: 29694094 DOI: 10.1103/physrevlett.120.125101] [Citation(s) in RCA: 8] [Impact Index Per Article: 1.3] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 11/02/2017] [Revised: 02/15/2018] [Indexed: 06/08/2023]
Abstract
Plasma turbulence at scales of the order of the ion inertial length is mediated by several mechanisms, including linear wave damping, magnetic reconnection, the formation and dissipation of thin current sheets, and stochastic heating. It is now understood that the presence of localized coherent structures enhances the dissipation channels and the kinetic features of the plasma. However, no formal way of quantifying the relationship between scale-to-scale energy transfer and the presence of spatial structures has been presented so far. In the Letter we quantify such a relationship analyzing the results of a two-dimensional high-resolution Hall magnetohydrodynamic simulation. In particular, we employ the technique of space filtering to derive a spectral energy flux term which defines, in any point of the computational domain, the signed flux of spectral energy across a given wave number. The characterization of coherent structures is performed by means of a traditional two-dimensional wavelet transformation. By studying the correlation between the spectral energy flux and the wavelet amplitude, we demonstrate the strong relationship between scale-to-scale transfer and coherent structures. Furthermore, by conditioning one quantity with respect to the other, we are able for the first time to quantify the inhomogeneity of the turbulence cascade induced by topological structures in the magnetic field. Taking into account the low space-filling factor of coherent structures (i.e., they cover a small portion of space), it emerges that 80% of the spectral energy transfer (both in the direct and inverse cascade directions) is localized in about 50% of space, and 50% of the energy transfer is localized in only 25% of space.
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Affiliation(s)
- E Camporeale
- Center for Mathematics and Computer Science (CWI), Amsterdam 1098 XG, The Netherlands
| | - L Sorriso-Valvo
- CNR-Nanotec-Unità di Cosenza, Ponte P. Bucci, cubo 31C, 87036 Rende, Italy
| | - F Califano
- Dipartimento di Fisica "E. Fermi," Università di Pisa, Largo B. Pontecorvo 3, I-56127 Pisa, Italy
| | - A Retinò
- Centre National de la Recherche Scientifique, LPP UMR 7648, Ecole Polytechnique, Universit Pierre et Marie Curie Paris VI, Observatoire de Paris, Route de Saclay Palaiseau 91128, France
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Rossi A, Campo D, Fortuna MC, Garelli V, Pranteda G, De Vita G, Sorriso-Valvo L, Di Nunno D, Carlesimo M. A preliminary study on topical cetirizine in the therapeutic management of androgenetic alopecia. J DERMATOL TREAT 2017; 29:149-151. [PMID: 28604133 DOI: 10.1080/09546634.2017.1341610] [Citation(s) in RCA: 10] [Impact Index Per Article: 1.4] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 10/19/2022]
Abstract
BACKGROUND Androgenetic alopecia (AGA) is a common form of scalp hair loss that affects up to 50% of males between 18 and 40 years old. Several molecules are commonly used for the treatment of AGA, acting on different steps of its pathogenesis (Minoxidil, Finasteride, Serenoa repens) and show some side effects. In literature, on the basis of hypertrichosis observed in patients treated with analogues of prostaglandin PGF2a, it was supposed that prostaglandins would have an important role in the hair growth: PGE and PGF2a play a positive role, while PGD2 a negative one. OBJECTIVE We carried out a pilot study to evaluate the efficacy of topical cetirizine versus placebo in patients with AGA. PATIENTS AND METHODS A sample of 85 patients was recruited, of which 67 were used to assess the effectiveness of the treatment with topical cetirizine, while 18 were control patients. RESULTS We found that the main effect of cetirizine was an increase in total hair density, terminal hair density and diameter variation from T0 to T1, while the vellus hair density shows an evident decrease. The use of a molecule as cetirizine, with no notable side effects, makes possible a good compliance by patients. CONCLUSION Our results have shown that topical cetirizine 1% is responsible for a significant improvement of the initial framework of AGA.
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Affiliation(s)
- A Rossi
- a Department of Internal Medicine and Medical Specialties , "Sapienza", University of Rome , Rome , Italy
| | - D Campo
- b Istituto Ortodermico Italiano , Rome , Italy
| | - M C Fortuna
- a Department of Internal Medicine and Medical Specialties , "Sapienza", University of Rome , Rome , Italy
| | - V Garelli
- a Department of Internal Medicine and Medical Specialties , "Sapienza", University of Rome , Rome , Italy
| | - G Pranteda
- a Department of Internal Medicine and Medical Specialties , "Sapienza", University of Rome , Rome , Italy
| | - G De Vita
- c CNR-Nanotec, U.O.S. di Rende, Ponte P. Bucci, cubo 31C, 87036 Rende (CS) , Italy
| | - L Sorriso-Valvo
- c CNR-Nanotec, U.O.S. di Rende, Ponte P. Bucci, cubo 31C, 87036 Rende (CS) , Italy
| | - D Di Nunno
- a Department of Internal Medicine and Medical Specialties , "Sapienza", University of Rome , Rome , Italy
| | - M Carlesimo
- a Department of Internal Medicine and Medical Specialties , "Sapienza", University of Rome , Rome , Italy
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8
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Carlesimo M, Garelli V, Fortuna MC, De Vita G, Sorriso-Valvo L, Buccolini F, Melini A, Di Nunno D, Pranteda G, Rossi A. Vascular Psoriasis Area Severity Index: A dermoscopic standard technique for assessing severity psoriasis and therapeutic management. J Dermatol Sci 2017; 86:249-251. [PMID: 28365082 DOI: 10.1016/j.jdermsci.2017.03.010] [Citation(s) in RCA: 3] [Impact Index Per Article: 0.4] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 08/08/2016] [Revised: 01/04/2017] [Accepted: 03/20/2017] [Indexed: 11/16/2022]
Affiliation(s)
- M Carlesimo
- Dipartimento di Medicina Interna e Specialità Mediche, "Sapienza" Università di Roma, Italy
| | - V Garelli
- Dipartimento di Medicina Interna e Specialità Mediche, "Sapienza" Università di Roma, Italy.
| | - M C Fortuna
- Dipartimento di Medicina Interna e Specialità Mediche, "Sapienza" Università di Roma, Italy
| | - G De Vita
- Dipartimento di Fisica, Università della Calabria, ponte P. Bucci, cubo 31C, 87036 Rende, Italy; CNR-Nanotec, UOS di Cosenza, ponte P. Bucci, cubo 31C, 87036 Rende, Italy
| | - L Sorriso-Valvo
- CNR-Nanotec, UOS di Cosenza, ponte P. Bucci, cubo 31C, 87036 Rende, Italy
| | | | | | - D Di Nunno
- Dipartimento di Medicina Interna e Specialità Mediche, "Sapienza" Università di Roma, Italy
| | - G Pranteda
- Dipartimento di Medicina Interna e Specialità Mediche, "Sapienza" Università di Roma, Italy
| | - A Rossi
- Dipartimento di Medicina Interna e Specialità Mediche, "Sapienza" Università di Roma, Italy
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Malara F, Di Mare F, Nigro G, Sorriso-Valvo L. Fast algorithm for a three-dimensional synthetic model of intermittent turbulence. Phys Rev E 2016; 94:053109. [PMID: 27967054 DOI: 10.1103/physreve.94.053109] [Citation(s) in RCA: 9] [Impact Index Per Article: 1.1] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 08/30/2016] [Indexed: 11/07/2022]
Abstract
Synthetic turbulence models are useful tools that provide realistic representations of turbulence, necessary to test theoretical results, to serve as background fields in some numerical simulations, and to test analysis tools. Models of one-dimensional (1D) and 3D synthetic turbulence previously developed still required large computational resources. A "wavelet-based" model of synthetic turbulence, able to produce a field with tunable spectral law, intermittency, and anisotropy, is presented here. The rapid algorithm introduced, based on the classic p-model of intermittent turbulence, allows us to reach a broad spectral range using a modest computational effort. The model has been tested against the standard diagnostics for intermittent turbulence, i.e., the spectral analysis, the scale-dependent statistics of the field increments, and the multifractal analysis, all showing an excellent response.
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Affiliation(s)
- Francesco Malara
- Dipartimento di Fisica, Università della Calabria, Ponte P. Bucci, cubo 31 C, 87036 Rende (CS), Italy
| | - Francesca Di Mare
- Dipartimento di Fisica, Università della Calabria, Ponte P. Bucci, cubo 31 C, 87036 Rende (CS), Italy
| | - Giuseppina Nigro
- Dipartimento di Fisica, Università della Calabria, Ponte P. Bucci, cubo 31 C, 87036 Rende (CS), Italy
| | - Luca Sorriso-Valvo
- Nanotec/CNR, U.O.S. di Rende, Ponte P. Bucci, cubo 31 C, 87036 Rende (CS), Italy
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Sorriso-Valvo L, Marino R, Lijoi L, Perri S, Carbone V. SELF-CONSISTENT CASTAING DISTRIBUTION OF SOLAR WIND TURBULENT FLUCTUATIONS. ACTA ACUST UNITED AC 2015. [DOI: 10.1088/0004-637x/807/1/86] [Citation(s) in RCA: 16] [Impact Index Per Article: 1.8] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/12/2022]
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Chasapis A, Retinò A, Sahraoui F, Vaivads A, Khotyaintsev YV, Sundkvist D, Greco A, Sorriso-Valvo L, Canu P. THIN CURRENT SHEETS AND ASSOCIATED ELECTRON HEATING IN TURBULENT SPACE PLASMA. ACTA ACUST UNITED AC 2015. [DOI: 10.1088/2041-8205/804/1/l1] [Citation(s) in RCA: 77] [Impact Index Per Article: 8.6] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/12/2022]
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Sorriso-Valvo L, De Vita G, Kazachenko MD, Krucker S, Primavera L, Servidio S, Vecchio A, Welsch BT, Fisher GH, Lepreti F, Carbone V. SIGN SINGULARITY AND FLARES IN SOLAR ACTIVE REGION NOAA 11158. ACTA ACUST UNITED AC 2015. [DOI: 10.1088/0004-637x/801/1/36] [Citation(s) in RCA: 13] [Impact Index Per Article: 1.4] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/12/2022]
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Carbone F, Sorriso-Valvo L. Experimental analysis of intermittency in electrohydrodynamic instability. Eur Phys J E Soft Matter 2014; 37:17. [PMID: 25039006 DOI: 10.1140/epje/i2014-14061-x] [Citation(s) in RCA: 1] [Impact Index Per Article: 0.1] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 03/04/2014] [Revised: 05/23/2014] [Accepted: 06/23/2014] [Indexed: 06/03/2023]
Abstract
The properties of turbulent electroconvective fluctuations generated in a nematic liquid crystal under the action of an external oscillating electric field are investigated. In particular, the spectral properties and the scaling behaviour of probability density functions (PDFs) of light intensity fluctuations are considered at different voltages. At intermediate voltage, in the weak turbulent regime, PDFs are Gaussian at large scales and show increasingly enhanced wings at smaller scales, recalling the typical signature of intermittency in isotropic fluid flows. When the voltage is increased, dynamical scattering regimes appear, characterized by increasing complexity. In order to get a quantitative estimate of intermittency, PDFs are modeled through the Castaing distribution, and structure functions are estimated in the framework of Extended Self-Similarity. Results support the generation of small-scale fluctuations through a fragmentation process of large-scale structures. The persistent anisotropic properties of the fluctuations are highlighted by the results.
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Affiliation(s)
- Francesco Carbone
- CNR-IPCF - U.O.S. Cosenza, Ponte P. Bucci, cubo 31C, 87036, Rende (CS), Italy
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14
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Maruca BA, Bale SD, Sorriso-Valvo L, Kasper JC, Stevens ML. Collisional thermalization of hydrogen and helium in solar-wind plasma. Phys Rev Lett 2013; 111:241101. [PMID: 24483639 DOI: 10.1103/physrevlett.111.241101] [Citation(s) in RCA: 2] [Impact Index Per Article: 0.2] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 08/23/2013] [Indexed: 06/03/2023]
Abstract
In situ observations of the solar wind frequently show the temperature of α particles (fully ionized helium) Tα to significantly differ from that of protons (ionized hydrogen) Tp. Many heating processes in the plasma act preferentially on α particles, even as collisions among ions act to gradually establish thermal equilibrium. Measurements from the Wind spacecraft's Faraday cups reveal that, at r=1.0 AU from the Sun, the observed values of the α-proton temperature ratio, θαp≡Tα/Tp, has a complex, bimodal distribution. This study applied a simple model for the radial evolution of θαp to these data to compute expected values of θαp at r=0.1 AU. These inferred θαp values have no trace of the bimodality seen in the θαp values measured at r=1.0 AU but are instead consistent with the actions of the known mechanisms for α-particle preferential heating. This result underscores the importance of collisional processes in the dynamics of the solar wind and suggests that similar mechanisms may lead to preferential α-particle heating in both slow and fast wind.
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Affiliation(s)
- B A Maruca
- Space Sciences Laboratory, University of California, 7 Gauss Way, Berkeley, California 94720, USA
| | - S D Bale
- Space Sciences Laboratory, University of California, 7 Gauss Way, Berkeley, California 94720, USA and Department of Physics, University of California, LeConte Hall, Berkeley, California 94720, USA
| | - L Sorriso-Valvo
- Space Sciences Laboratory, University of California, 7 Gauss Way, Berkeley, California 94720, USA and IPCF-CNR, U.O. Cosenza, Ponte P. Bucci, Cubo 31C, 87036 Rende, Italy
| | - J C Kasper
- Department of Atmospheric, Oceanic and Space Sciences, University of Michigan, Ann Arbor, Michigan 48109, USA and Harvard-Smithsonian Center for Astrophysics, Cambridge, Massachusetts 02138, USA
| | - M L Stevens
- Harvard-Smithsonian Center for Astrophysics, Cambridge, Massachusetts 02138, USA
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15
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Martin LN, De Vita G, Sorriso-Valvo L, Dmitruk P, Nigro G, Primavera L, Carbone V. Cancellation properties in Hall magnetohydrodynamics with a strong guide magnetic field. Phys Rev E Stat Nonlin Soft Matter Phys 2013; 88:063107. [PMID: 24483577 DOI: 10.1103/physreve.88.063107] [Citation(s) in RCA: 1] [Impact Index Per Article: 0.1] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 06/28/2013] [Revised: 11/15/2013] [Indexed: 06/03/2023]
Abstract
We present a signed measure analysis of compressible Hall magnetohydrodynamic turbulence with an external guide field. Signed measure analysis allows us to characterize the scaling behavior of the sign-oscillating flow structures and their geometrical properties (fractal dimensions of structures). A reduced numerical model, valid when a strong guide magnetic field is present, is used here. In order to discuss the effect of the Hall term, different values for the ion skin depth are considered in the simulations. Results show that as the Hall term is increased, the fractal dimension of the current and vorticity sheets decreases. This observation, together with previous analysis of the same fields, provides a comprehensive description of the effect of the Hall force on the formation of structures. Two main processes are identified, namely, the widening and unraveling of the sheets.
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Affiliation(s)
- L N Martin
- Departamento de Física, Facultad de Ciencias Exactas y Naturales, Universidad de Buenos Aires and IFIBA, CONICET, Buenos Aires 1428, Argentina
| | - G De Vita
- Dipartimento di Fisica, Università degli Studi della Calabria, 87036 Rende, Cosenza, Italy
| | - L Sorriso-Valvo
- CNR, IPCF, UOS di Cosenza, 87036 Rende, Cosenza, Italy and Space Sciences Laboratory, University of California, Berkeley, Berkeley, California 94720, USA
| | - P Dmitruk
- Departamento de Física, Facultad de Ciencias Exactas y Naturales, Universidad de Buenos Aires and IFIBA, CONICET, Buenos Aires 1428, Argentina
| | - G Nigro
- Dipartimento di Fisica, Università degli Studi della Calabria, 87036 Rende, Cosenza, Italy
| | - L Primavera
- Dipartimento di Fisica, Università degli Studi della Calabria, 87036 Rende, Cosenza, Italy
| | - V Carbone
- Dipartimento di Fisica, Università degli Studi della Calabria, 87036 Rende, Cosenza, Italy
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16
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Perri S, Carbone V, Vecchio A, Bruno R, Korth H, Zurbuchen TH, Sorriso-Valvo L. Phase-synchronization, energy cascade, and intermittency in solar-wind turbulence. Phys Rev Lett 2012; 109:245004. [PMID: 23368334 DOI: 10.1103/physrevlett.109.245004] [Citation(s) in RCA: 2] [Impact Index Per Article: 0.2] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Received: 05/31/2012] [Indexed: 06/01/2023]
Abstract
The energy cascade in solar wind magnetic turbulence is investigated using MESSENGER data in the inner heliosphere. The decomposition of magnetic field time series in intrinsic functions, each characterized by a typical time scale, reveals phase reorganization. This allows for the identification of structures of all sizes generated by the nonlinear turbulent cascade, covering both the inertial and the dispersive ranges of the turbulent magnetic power spectrum. We find that the correlation (or anticorrelation) of phases occurs between pairs of neighboring time scales, whenever localized peaks of magnetic energy are present at both scales, consistent with the local character of the energy transfer process.
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Affiliation(s)
- S Perri
- Dipartimento di Fisica, Università della Calabria, 87036 Rende, Cosenza, Italy
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17
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Carbone F, Vecchio A, Sorriso-Valvo L. Spatio-temporal dynamics, patterns formation and turbulence in complex fluids due to electrohydrodynamics instabilities. Eur Phys J E Soft Matter 2011; 34:75. [PMID: 21805393 DOI: 10.1140/epje/i2011-11075-x] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 04/04/2011] [Accepted: 07/07/2011] [Indexed: 05/31/2023]
Abstract
The complex spatio-temporal dynamics generated by electrohydrodynamics instabilities in a nematic liquid crystal under the action of a driving oscillating electric field is investigated. Quasi-stationary convective structures which are visible at large scales are broken into chaotic patterns at higher driving voltages, thus generating small-scale structures. Scaling analysis reveals that these small-scale structures self-organize in a network of subleading structures which are reminescent of convective rolls. This network persists well inside the chaotic regimes, disappearing only at very high voltages, where stochastic dynamical scattering mode takes place.
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Affiliation(s)
- F Carbone
- INLN, Université de Nice Sophia-Antipolis, CNRS, 1361 route des Lucioles, 06560, Valbonne, France
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18
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Carbone F, Sorriso-Valvo L, Versace C, Strangi G, Bartolino R. Anisotropy of spatiotemporal decorrelation in electrohydrodynamic turbulence. Phys Rev Lett 2011; 106:114502. [PMID: 21469865 DOI: 10.1103/physrevlett.106.114502] [Citation(s) in RCA: 2] [Impact Index Per Article: 0.2] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 07/23/2010] [Revised: 02/23/2011] [Indexed: 05/30/2023]
Abstract
Nonlinear straining and random sweeping spatiotemporal decorrelation properties, originally introduced as the main processes for turbulent fluctuations decorrelation in usual fluid flows, have been observed experimentally in anisotropic electroconvective turbulence generated in a nematic liquid crystal under the action of an external oscillating electric field. A transition between both processes occurs when the instability is driven toward states of increasing complexity, thus showing that decorrelation mechanisms in turbulent media are more universal than naively expected. A model for both decorrelation mechanisms is introduced, its comparison with experimental results providing an estimate of the characteristic sweeping velocity.
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Affiliation(s)
- F Carbone
- Dipartimento di Fisica, Università della Calabria, Ponte Pietro Bucci 31C, I-87036 Rende (CS), Italy
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19
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Carbone V, Marino R, Sorriso-Valvo L, Noullez A, Bruno R. Scaling laws of turbulence and heating of fast solar wind: the role of density fluctuations. Phys Rev Lett 2009; 103:061102. [PMID: 19792547 DOI: 10.1103/physrevlett.103.061102] [Citation(s) in RCA: 20] [Impact Index Per Article: 1.3] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 10/16/2008] [Indexed: 05/28/2023]
Abstract
Incompressible and isotropic magnetohydrodynamic turbulence in plasmas can be described by an exact relation for the energy flux through the scales. This Yaglom-like scaling law has been recently observed in the solar wind above the solar poles observed by the Ulysses spacecraft, where the turbulence is in an Alfvénic state. An analogous phenomenological scaling law, suitably modified to take into account compressible fluctuations, is observed more frequently in the same data set. Large-scale density fluctuations, despite their low amplitude, thus play a crucial role in the basic scaling properties of turbulence. The turbulent cascade rate in the compressive case can, moreover, supply the energy dissipation needed to account for the local heating of the nonadiabatic solar wind.
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Affiliation(s)
- V Carbone
- Dipartimento di Fisica, Università della Calabria, I-87036 Rende (CS), Italy
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20
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Ciuchi F, Sorriso-Valvo L, Mazzulla A, Redondo JM. Fractal aggregates evolution of methyl red in liquid crystal. Eur Phys J E Soft Matter 2009; 29:139-147. [PMID: 19513769 DOI: 10.1140/epje/i2009-10460-4] [Citation(s) in RCA: 1] [Impact Index Per Article: 0.1] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Received: 01/26/2009] [Revised: 03/30/2009] [Accepted: 04/07/2009] [Indexed: 05/27/2023]
Abstract
The spontaneous formation of dendritic aggregates is observed in a two-dimensional confined layered system consisting of a film composed of liquid crystal, dye and solvent cast above a polymer substrate. The observed aggregates are promoted by phase separation processes induced by dye diffusion and solvent evaporation. The growth properties of the aggregates are studied through the temporal evolution of their topological properties (surface, perimeter, fractal dimension). The fractal dimension of the completely formed structures, when they are coexistent with different types of structures, is consistent with theoretical and experimental values obtained for Diffusion-Limited Aggregates. Under different experimental conditions (temperature and local dye concentration) the structure forms without interactions with other kinds of structures, and its equilibrium fractal dimension is smaller. The fractal dimension is thus not a universal property of the observed structures, but rather depends on the experimental conditions.
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Affiliation(s)
- F Ciuchi
- Regional Laboratory LICRYL-INFM/CNR, Ponte Pietro Bucci, Cubo 33B, I-87036, Rende (CS), Italy
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21
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Ferjani S, Sorriso-Valvo L, De Luca A, Barna V, De Marco R, Strangi G. Statistical analysis of random lasing emission properties in nematic liquid crystals. Phys Rev E Stat Nonlin Soft Matter Phys 2008; 78:011707. [PMID: 18763973 DOI: 10.1103/physreve.78.011707] [Citation(s) in RCA: 1] [Impact Index Per Article: 0.1] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 09/05/2007] [Revised: 03/26/2008] [Indexed: 05/26/2023]
Abstract
A statistical analysis of random lasing events observed in dye-doped nematic-liquid-crystal films is reported. The occurrence of random laser action in such complex fluids is due to residual resonances in the multiple scattering of spontaneously emitted photons. The Shannon entropy and a local-Poisson test are used here in order to quantitatively characterize the chaotic behavior of laser spikes and gain further understanding of the mechanisms underlying the lasing effect in strongly scattering organized fluids arising by an unexpected interplay of localization and amplification.
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Affiliation(s)
- Sameh Ferjani
- Dipartimento di Fisica, Università della Calabria, and CNISM-Unità di Cosenza, Ponte P. Bucci, Cubo 31C, Rende CS, Italy
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22
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Sorriso-Valvo L, Marino R, Carbone V, Noullez A, Lepreti F, Veltri P, Bruno R, Bavassano B, Pietropaolo E. Observation of inertial energy cascade in interplanetary space plasma. Phys Rev Lett 2007; 99:115001. [PMID: 17930445 DOI: 10.1103/physrevlett.99.115001] [Citation(s) in RCA: 49] [Impact Index Per Article: 2.9] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 02/27/2007] [Indexed: 05/20/2023]
Abstract
Direct evidence for the presence of an inertial energy cascade, the most characteristic signature of hydromagnetic turbulence (MHD), is observed in the solar wind by the Ulysses spacecraft. After a brief rederivation of the equivalent of Yaglom's law for MHD turbulence, a linear relation is indeed observed for the scaling of mixed third-order structure functions involving Elsässer variables. This experimental result firmly establishes the turbulent character of low-frequency velocity and magnetic field fluctuations in the solar wind plasma.
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Affiliation(s)
- L Sorriso-Valvo
- Licryl Regional Laboratory - INFM/CNR, Ponte P. Bucci, Cubo 33C, 87036 Rende (CS), Italy
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23
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Carbone V, Sorriso-Valvo L, Vecchio A, Lepreti F, Veltri P, Harabaglia P, Guerra I. Clustering of polarity reversals of the geomagnetic field. Phys Rev Lett 2006; 96:128501. [PMID: 16605965 DOI: 10.1103/physrevlett.96.128501] [Citation(s) in RCA: 2] [Impact Index Per Article: 0.1] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 10/03/2005] [Indexed: 05/08/2023]
Abstract
Often in nature the temporal distribution of inhomogeneous stochastic point processes can be modeled as a realization of renewal Poisson processes with a variable rate. Here we investigate one of the classical examples, namely, the temporal distribution of polarity reversals of the geomagnetic field. In spite of the commonly used underlying hypothesis, we show that this process strongly departs from a Poisson statistics, the origin of this failure stemming from the presence of temporal clustering. We find that a Lévy statistics is able to reproduce paleomagnetic data, thus suggesting the presence of long-range correlations in the underlying dynamo process.
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Affiliation(s)
- V Carbone
- Dipartimento di Fisica, Università della Calabria, Ponte P. Bucci, Cubo 31C, 87036 Rende (CS), Italy
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24
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Vecchio A, Carbone V, Lepreti F, Primavera L, Sorriso-Valvo L, Veltri P, Alfonsi G, Straus T. Proper orthogonal decomposition of solar photospheric motions. Phys Rev Lett 2005; 95:061102. [PMID: 16090935 DOI: 10.1103/physrevlett.95.061102] [Citation(s) in RCA: 3] [Impact Index Per Article: 0.2] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 03/24/2005] [Indexed: 05/03/2023]
Abstract
The spatiotemporal dynamics of the solar photosphere is studied by performing a proper orthogonal decomposition (POD) of line of sight velocity fields computed from high resolution data coming from the MDI/SOHO instrument. Using this technique, we are able to identify and characterize the different dynamical regimes acting in the system. Low-frequency oscillations, with frequencies in the range 20-130 microHz, dominate the most energetic POD modes (excluding solar rotation), and are characterized by spatial patterns with typical scales of about 3 Mm. Patterns with larger typical scales of approximately 10 Mm, are associated to p-modes oscillations at frequencies of about 3000 microHz.
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Affiliation(s)
- A Vecchio
- Dipartimento di Fisica, Università della Calabria, and Istituto Nazionale di Fisica della Materia, Unità di Cosenza, 87030 Rende (CS), Italy
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25
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Carbone V, Sorriso-Valvo L, Martines E, Antoni V, Veltri P. Intermittency and turbulence in a magnetically confined fusion plasma. Phys Rev E Stat Phys Plasmas Fluids Relat Interdiscip Topics 2000; 62:R49-R52. [PMID: 11088522 DOI: 10.1103/physreve.62.r49] [Citation(s) in RCA: 2] [Impact Index Per Article: 0.1] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 03/02/2000] [Indexed: 05/23/2023]
Abstract
We investigate the intermittency of magnetic turbulence as measured in reversed field pinch plasmas. We show that the probability distribution functions of magnetic field differences are not scale invariant; that is, the wings of these functions are more important at the smallest scales, a classical signature of intermittency. We show that scaling laws appear also in a region very close to the external wall of the confinement device, and we present evidences that the observed intermittency increases moving towards the wall.
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Affiliation(s)
- V Carbone
- Dipartimento di Fisica, Universita degli studi della Calabria, 87036 Rende (CS), ItalyIstituto Nazionale di Fisica della Materia, Unita di Cosenza, 87036 Italy
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