The Library

Global scale-invariant dissipation in collisionless plasma turbulence

Tools

Kiyani, K., Chapman, Sandra C., Khotyaintsev, Yu. V., Dunlop, M. W. and Sahraoui, F.. (2009) Global scale-invariant dissipation in collisionless plasma turbulence. Physical Review Letters, Vol.103 (No.7). Article no. 075006 . ISSN 0031-9007

Full text not available from this repository.

Abstract

A higher-order multiscale analysis of the dissipation range of collisionless plasma turbulence is presented using in situ high-frequency magnetic field measurements from the Cluster spacecraft in a stationary interval of fast ambient solar wind. The observations, spanning five decades in temporal scales, show a crossover from multifractal intermittent turbulence in the inertial range to non-Gaussian mono-scaling in the dissipation range. This presents a strong observational constraint on theories of dissipation mechanisms in turbulent collisionless plasmas.

Item Type: Journal Article
Subjects: Q Science > QB Astronomy
Q Science > QC Physics
Divisions: Faculty of Science > Physics
Library of Congress Subject Headings (LCSH): Collisionless plasmas, Plasma turbulence, Magnetohydrodynamics, Magnetic fields, Solar wind, Anisotropy
Journal or Publication Title: Physical Review Letters
Publisher: American Physical Society
ISSN: 0031-9007
Official Date: 14 August 2009
Volume: Vol.103
Number: No.7
Number of Pages: 4
Page Range: Article no. 075006
Identification Number: 10.1103/PhysRevLett.103.075006
Status: Peer Reviewed
Publication Status: Published
Access rights to Published version: Restricted or Subscription Access
Funder: Science and Technology Facilities Council (Great Britain) (STFC)
References:

[1] R. Bruno and V. Carbone, Living Rev. Solar Phys. 2, 4
(2005).
[2] W. H. Matthaeus et al., Phys. Rev. Lett. 95, 231101 (2005).
[3] L. Sorriso-Valvo et al., Phys. Rev. Lett. 99, 115001
(2007).
[4] B. Hnat, S. C. Chapman, and G. Rowlands, Phys. Rev.
Lett. 94, 204502 (2005).
[5] S. C. Chapman and B. Hnat, Geophys. Res. Lett. 34,
L17103 (2007).
[6] T. S. Horbury, M. Forman, and S. Oughton, Phys. Rev.
Lett. 101, 175005 (2008).
[7] R. J. Leamon et al., Astrophys. J. 537, 1054 (2000).
[8] J. C. Kasper, A. J. Lazarus, and S. P. Gary, Phys. Rev. Lett.
101, 261103 (2008).
[9] J. A. Araneda, Y. Maneva, and E. Marsch, Phys. Rev. Lett.
102, 175001 (2009).
[10] P. J. Coleman, Jr., Astrophys. J. 153, 371 (1968).
[11] K.W. Behannon, Rev. Geophys. 16, 125 (1978).
[12] R. J. Leamon et al., J. Geophys. Res. 103, 4775 (1998).
[13] C.W. Smith, K. Hamilton, B. J. Vasquez, and R. J.
Leamon, Astrophys. J. 645, L85 (2006).
[14] F. Sahraoui, M. L. Goldstein, P. Robert, and Yu.V.
Khotyaintsev, Phys. Rev. Lett. 102, 231102 (2009).
[15] D. Sundkvist, A. Retino`, A. Vaivads, and S. D. Bale, Phys.
Rev. Lett. 99, 025004 (2007).
[16] J. P. Eastwood, T. D. Phan, S. D. Bale, and A. Tjulin, Phys.
Rev. Lett. 102, 035001 (2009).
[17] J. Cho and A. Lazarian, Astrophys. J. Lett. 615, L41
(2004).
[18] S. Galtier and E. Buchlin, Astrophys. J. 656, 560 (2007).
[19] O. Alexandrova, V. Carbone, P. Veltri, and L. Sorriso-
Valvo, Astrophys. J. 674, 1153 (2008).
[20] R. J. Leamon, W. H. Matthaeus, C.W. Smith, and H. K.
Wong, Astrophys. J. Lett. 507, L181 (1998).
[21] S. D. Bale, P. J. Kellogg, F. S. Mozer, T. S. Horbury, and
H. Reme, Phys. Rev. Lett. 94, 215002 (2005).
[22] Y. Narita, K.-H. Glassmeier, and R. A. Treumann, Phys.
Rev. Lett. 97, 191101 (2006).
[23] F. Sahraoui et al., Phys. Rev. Lett. 96, 075002 (2006).
[24] O. Alexandrova, C. Lacombe, and A. Mangeney, Ann.
Geophys. 26, 3585 (2008).
[25] D. Shaikh and P. K. Shukla, Phys. Rev. Lett. 102, 045004
(2009).
[26] D. Biskamp, E. Schwarz, and J. Drake, Phys. Rev. Lett. 76,
1264 (1996).
[27] G. G. Howes et al., Phys. Rev. Lett. 100, 065004 (2008).
[28] S. Saito, S. P. Gary, H. Li, and Y. Narita, Phys. Plasmas 15,
102305 (2008).
[29] F. Valentini, P. Veltri, F. Califano, and A. Mangeney, Phys.
Rev. Lett. 101, 025006 (2008).
[30] N. Cornilleau-Wehrlin et al., Space Sci. Rev. 79, 107
(1997).
[31] A. Balogh et al., Space Sci. Rev. 79, 65 (1997).
[32] P. M. E. De´cre´au et al., Space Sci. Rev. 79, 157 (1997).
[33] H. Reme et al., Space Sci. Rev. 79, 303 (1997).
[34] K. H. Kiyani, S. C. Chapman, and N.W. Watkins, Phys.
Rev. E 79, 036109 (2009).
[35] K. Kiyani, S. C. Chapman, and B. Hnat, Phys. Rev. E 74,
051122 (2006).
[36] G. Boffetta, A. Celani, A. Crisanti, and R. Prandi, Phys.
Rev. E 59, 3724 (1999).
[37] N. Cornilleau-Wehrlin et al., Ann. Geophys. 21, 437
(2003).
URI: http://wrap.warwick.ac.uk/id/eprint/17422

Data sourced from Thomson Reuters' Web of Knowledge

Request changes or add full text files to a record

Actions (login required)

View Item View Item