Energy spectrum of turbulent fluctuations in boundary driven reduced magnetohydrodynamics

The turbulent dynamics of a bundle of magnetic flux ropes driven at their endpoints with steady convective motions was studied. Two dimensionless parameters controlling the response of the system were identified. It was found that the external driving generates a broadband perpendicular energy spect...

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Autor principal: Dmitruk, P.
Otros Autores: Gómez, D.O, Matthaeus, W.H
Formato: Capítulo de libro
Lenguaje:Inglés
Publicado: 2003
Acceso en línea:Registro en Scopus
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100 1 |a Dmitruk, P. 
245 1 0 |a Energy spectrum of turbulent fluctuations in boundary driven reduced magnetohydrodynamics 
260 |c 2003 
270 1 0 |m Dmitruk, P.; Bartol Research Institute, University of Delaware, Newark, DE 19716, United States 
506 |2 openaire  |e Política editorial 
504 |a Kolmogorov, A.N., (1941) Dokl. Akad. Nauk SSSR, 30, p. 301 
504 |a Iroshnikov, P.S., (1963) Astron. Zh., 40, p. 742 
504 |a Kraichnan, R., (1965) Phys. Fluids, 8, p. 1385 
504 |a Fyfe, D., Montgomery, D., Joyce, G., (1977) J. Plasma Phys., 17, p. 369 
504 |a Matthaeus, W.H., Zhou, Y., (1989) Phys. Fluids B, 1, p. 1929 
504 |a Muller, W.-C., Biskamp, D., (2000) Phys. Rev. Lett., 84, p. 475 
504 |a Shebalin, J.V., Matthaeus, W.H., Montgomery, D., (1983) J. Plasma Phys., 29, p. 525 
504 |a Oughton, S., Priest, E.R., Matthaeus, W.H., (1994) J. Fluid Mech., 280, p. 95 
504 |a Goldreich, P., Sridhar, S., (1997) Astrophys. J., 485, p. 680 
504 |a Kinney, R., McWilliams, J.C., (1998) Phys. Rev. E, 57, p. 7111 
504 |a Matthaeus, W.H., Ghosh, S., Oughton, S., Roberts, D.A., (1996) J. Geophys. Res., [Atmos.], 101, p. 7619 
504 |a Zank, G.P., Matthaeus, W.H., (1992) J. Plasma Phys., 48, p. 85 
504 |a Strauss, H., (1976) Phys. Fluids, 19, p. 134 
504 |a Montgomery, D.C., (1982) Phys. Scr., T, T2-1, p. 83 
504 |a Ng, C.S., Bhattacharjee, A., (1997) Phys. Plasmas, 4, p. 605 
504 |a Galtier, S., Nazarenko, S.V., Newell, A.C., Pouquet, A., (2000) J. Plasma Phys., 63, p. 447 
504 |a Parker, E.N., (1972) Astrophys. J., 174, p. 499 
504 |a Van Ballegooijen, A.A., (1986) Astrophys. J., 311, p. 1001 
504 |a Longcope, D.W., Sudan, R.N., (1994) Astrophys. J., 437, p. 491 
504 |a Mikić, Z., Schnack, D.D., Van Hoven, G., (1989) Astrophys. J., 338, p. 1148 
504 |a Hendrix, D.L., Van Hoven, G., (1996) Astrophys. J., 467, p. 887 
504 |a Milano, L., Dmitruk, P., Mandrini, C., Gómez, D.O., Demoulin, P., (1999) Astrophys. J., 521, p. 889 
504 |a Gómez, D.O., Ferro Fontán, C., (1992) Astrophys. J., 394, p. 662 
504 |a Galsgaard, K., Nordlund, A., (1996) J. Geophys. Res. [Atmos.], 101, p. 13445 
504 |a Dmitruk, P., Gómez, D.O., (1999) Astrophys. J. Lett., 527, pp. L63 
504 |a Mandrini, C.H., Demoulin, P., Klimchuk, J.A., (2000) Astrophys. J., 530, p. 999 
504 |a Canute, C., Hussaini, M.Y., Quarteroni, A., Zang, T.A., (1988) Spectral Methods in Fluid Dynamics, p. 1. , Springer, New York 
504 |a Hendrix, D.L., Van Hoven, G., Mikic, Z., Schnack, D.D., (1996) Astrophys. J., 470, p. 1192 
504 |a Sreenivasan, K.R., (1984) Phys. Fluids, 27, p. 1048 
504 |a Batchelor, G.K., (1953) The Theory of Homogeneous Turbulence, p. 106. , Cambridge University Press, Cambridge, UK 
504 |a Frisch, U., (1996) Turbulence, p. 69. , Cambridge University Press, Cambridge, UK 
504 |a Bhattacharjee, A., Ng, C.S., (2001) Astrophys. J., 548, p. 318 
504 |a Zhou, Y., (1995) Phys. Fluids, 7, p. 2092 
504 |a Grappin, R., Pouquet, A., Léorat, J., (1983) Astron. Astrophys., 126, p. 51 
520 3 |a The turbulent dynamics of a bundle of magnetic flux ropes driven at their endpoints with steady convective motions was studied. Two dimensionless parameters controlling the response of the system were identified. It was found that the external driving generates a broadband perpendicular energy spectrum with a slope which is determined by the time scale ratio.  |l eng 
593 |a Bartol Research Institute, University of Delaware, Newark, DE 19716, United States 
593 |a Departmento de Física, Fac. de Ciencias Exactas y Naturales, Ciudad Universitaria, 1428 Buenos Aires, Argentina 
690 1 0 |a CURRENT DENSITY 
690 1 0 |a HEAT CONVECTION 
690 1 0 |a MAGNETOHYDRODYNAMICS 
690 1 0 |a TURBULENCE 
690 1 0 |a CONVECTIVE MOTIONS 
690 1 0 |a MAGNETIC FLUX 
700 1 |a Gómez, D.O. 
700 1 |a Matthaeus, W.H. 
773 0 |d 2003  |g v. 10  |h pp. 3584-3591  |k n. 9  |p Phys Plasmas  |x 1070664X  |w (AR-BaUEN)CENRE-6479  |t Physics of Plasmas 
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