Depression of nonlinearity in decaying isotropic MHD turbulence

Spectral method simulations show that undriven magnetohydrodynamic turbulence spontaneously generates coherent spatial correlations of several types, associated with local Beltrami fields, directional alignment of velocity and magnetic fields, and antialignment of magnetic and fluid acceleration com...

Descripción completa

Guardado en:
Detalles Bibliográficos
Autor principal: Servidio, S.
Otros Autores: Matthaeus, W.H, Dmitruk, P.
Formato: Capítulo de libro
Lenguaje:Inglés
Publicado: 2008
Acceso en línea:Registro en Scopus
DOI
Handle
Registro en la Biblioteca Digital
Aporte de:Registro referencial: Solicitar el recurso aquí
LEADER 05292caa a22006857a 4500
001 PAPER-6042
003 AR-BaUEN
005 20230518203543.0
008 190411s2008 xx ||||fo|||| 00| 0 eng|d
024 7 |2 scopus  |a 2-s2.0-40849098674 
040 |a Scopus  |b spa  |c AR-BaUEN  |d AR-BaUEN 
030 |a PRLTA 
100 1 |a Servidio, S. 
245 1 0 |a Depression of nonlinearity in decaying isotropic MHD turbulence 
260 |c 2008 
270 1 0 |m Servidio, S.; Bartol Research Institute, Department of Physics and Astronomy, University of Delaware, Newark, DE 19716, United States 
506 |2 openaire  |e Política editorial 
504 |a Frisch, U., (1995) Turbulence: The Legacy of A.N. Kolmogorov, , Cambridge U. Press, Cambridge, England 
504 |a Taylor, J.B., (1974) Phys. Rev. Lett., 33, p. 1139. , PRLTAO 0031-9007 10.1103/PhysRevLett.33.1139 
504 |a Mininni, P.D., Gómez, D.O., Mahajan, S.M., (2002) Astrophys. J., 567, p. 81. , ASJOAB 0004-637X 10.1086/339850 
504 |a Stribling, T., Matthaeus, W.H., (1991) Phys. Fluids B, 3, p. 1848. , PFBPEI 0899-8221 10.1063/1.859654 
504 |a Ohsaki, S., Yoshida, Z., (2005) Phys. Plasmas, 12, p. 064505. , PHPAEN 1070-664X 10.1063/1.1936585 
504 |a Ting, A.C., Montgomery, D., Matthaeus, W.H., (1986) Phys. Fluids, 29, p. 3261. , PFLDAS 0031-9171 10.1063/1.865843 
504 |a Montgomery, D., Turner, L., Vahala, G., (1978) Phys. Fluids, 21, p. 757. , PFLDAS 0031-9171 10.1063/1.862295 
504 |a Matthaeus, W.H., Montgomery, D., (1980) Ann. N.Y. Acad. Sci., 357, p. 203. , ANYAA9 0077-8923 10.1111/j.1749-6632.1980.tb29687.x 
504 |a Mininni, P.D., Montgomery, D., Pouquet, A., (2005) Phys. Fluids, 17, p. 035112. , PFLDAS 0031-9171 10.1063/1.1863260 
504 |a Kraichnan, R.H., Panda, R., (1988) Phys. Fluids, 31, p. 2395. , PFLDAS 0031-9171 10.1063/1.866591 
504 |a Pelz, R.B., Yakhot, V., Orszag, S.A., Shtilman, L., Levich, E., (1985) Phys. Rev. Lett., 54, p. 2505. , PRLTAO 0031-9007 10.1103/PhysRevLett.54.2505 
504 |a Kerr, R.M., (1987) Phys. Rev. Lett., 59, p. 783. , PRLTAO 0031-9007 10.1103/PhysRevLett.59.783 
504 |a Ashurst, Wm.T., Kerstein, A.R., Kerr, R.M., Gibson, C.H., (1987) Phys. Fluids, 30, p. 2343. , PFLDAS 0031-9171 10.1063/1.866513 
504 |a Moffat, H.K., (1984) Turbulence and Chaotic Phenomena in Fluids, , North-Holland, Amsterdam 
504 |a Belcher, J.W., Davis Jr., L., (1971) J. Geophys. Res., 76, p. 3534. , JGREA2 0148-0227 10.1029/JA076i016p03534 
504 |a Dobrowolny, M., Mangeney, A., Veltri, P., (1980) Phys. Rev. Lett., 45, p. 144. , PRLTAO 0031-9007 10.1103/PhysRevLett.45.144 
504 |a Mason, J., (2006) Phys. Rev. Lett., 97, p. 255002. , PRLTAO 0031-9007 10.1103/PhysRevLett.97.255002 
504 |a Boldyrev, S., (2006) Phys. Rev. Lett., 96, p. 115002. , PRLTAO 0031-9007 10.1103/PhysRevLett.96.115002 
504 |a Matthaeus, W.H., Pouquet, A., Mininni, P.D., Dmitruk, P., Breech, B., Phys. Rev. Lett., , PRLTAO 0031-9007 
504 |a Ghosh, S., Hossain, M., Matthaeus, W.H., (1993) Comput. Phys. Commun., 74, p. 18. , CPHCBZ 0010-4655 10.1016/0010-4655(93)90103-J 
504 |a Brown, M.R., (1997) J. Plasma Phys., 57, p. 203. , JPLPBZ 0022-3778 10.1017/S0022377896005211 
520 3 |a Spectral method simulations show that undriven magnetohydrodynamic turbulence spontaneously generates coherent spatial correlations of several types, associated with local Beltrami fields, directional alignment of velocity and magnetic fields, and antialignment of magnetic and fluid acceleration components. These correlations suppress nonlinearity to levels lower than what is obtained from Gaussian fields, and occur in spatial patches. We suggest that this rapid relaxation leads to non-Gaussian statistics and spatial intermittency. © 2008 The American Physical Society.  |l eng 
593 |a Bartol Research Institute, Department of Physics and Astronomy, University of Delaware, Newark, DE 19716, United States 
593 |a Departmento de Física, Facultad de Ciencias Exactas y Naturales, Ciudad Universitaria, 1428, Buenos Aires, Argentina 
690 1 0 |a COMPUTER SIMULATION 
690 1 0 |a CONTROL NONLINEARITIES 
690 1 0 |a CORRELATION METHODS 
690 1 0 |a MAGNETIC FIELDS 
690 1 0 |a MAGNETOHYDRODYNAMICS 
690 1 0 |a BELTRAMI FIELDS 
690 1 0 |a MAGNETOHYDRODYNAMIC TURBULENCE 
690 1 0 |a TURBULENCE 
700 1 |a Matthaeus, W.H. 
700 1 |a Dmitruk, P. 
773 0 |d 2008  |g v. 100  |k n. 9  |p Phys Rev Lett  |x 00319007  |w (AR-BaUEN)CENRE-386  |t Physical Review Letters 
856 4 1 |u https://www.scopus.com/inward/record.uri?eid=2-s2.0-40849098674&doi=10.1103%2fPhysRevLett.100.095005&partnerID=40&md5=8140c5304484d0fd0938f59570bbda27  |y Registro en Scopus 
856 4 0 |u https://doi.org/10.1103/PhysRevLett.100.095005  |y DOI 
856 4 0 |u https://hdl.handle.net/20.500.12110/paper_00319007_v100_n9_p_Servidio  |y Handle 
856 4 0 |u https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00319007_v100_n9_p_Servidio  |y Registro en la Biblioteca Digital 
961 |a paper_00319007_v100_n9_p_Servidio  |b paper  |c PE 
962 |a info:eu-repo/semantics/article  |a info:ar-repo/semantics/artículo  |b info:eu-repo/semantics/publishedVersion 
963 |a VARI 
999 |c 66995