Show simple item record

Correlation and Taylor scale variability in the interplanetary magnetic field fluctuations as a function of solar wind speed

dc.contributor.authorWeygand, James M.en_US
dc.contributor.authorMatthaeus, W. H.en_US
dc.contributor.authorDasso, S.en_US
dc.contributor.authorKivelson, M. G.en_US
dc.date.accessioned2013-01-03T19:40:11Z
dc.date.available2013-01-03T19:40:11Z
dc.date.issued2011-08en_US
dc.identifier.citationWeygand, James M.; Matthaeus, W. H.; Dasso, S.; Kivelson, M. G. (2011). "Correlation and Taylor scale variability in the interplanetary magnetic field fluctuations as a function of solar wind speed." Journal of Geophysical Research: Space Physics 116(A8): n/a-n/a. <http://hdl.handle.net/2027.42/95101>en_US
dc.identifier.issn0148-0227en_US
dc.identifier.issn2156-2202en_US
dc.identifier.urihttps://hdl.handle.net/2027.42/95101
dc.publisherCambridge Univ. Pressen_US
dc.publisherWiley Periodicals, Inc.en_US
dc.subject.otherCorrelation Scaleen_US
dc.subject.otherTaylor Scaleen_US
dc.subject.otherMagnetic Field Turbulenceen_US
dc.subject.otherSolar Wind Turbulenceen_US
dc.titleCorrelation and Taylor scale variability in the interplanetary magnetic field fluctuations as a function of solar wind speeden_US
dc.typeArticleen_US
dc.rights.robotsIndexNoFollowen_US
dc.subject.hlbsecondlevelAstronomy and Astrophysicsen_US
dc.subject.hlbtoplevelScienceen_US
dc.description.peerreviewedPeer Revieweden_US
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/95101/1/jgra21350.pdf
dc.identifier.doi10.1029/2011JA016621en_US
dc.identifier.sourceJournal of Geophysical Research: Space Physicsen_US
dc.identifier.citedreferencePerri, S., E. Yordanova, V. Carbone, P. Veltri, L. Sorriso‐Valvo, R. Bruno, and M. André ( 2009 ), Magnetic turbulence in space plasmas: Scale‐dependent effects of anisotropy, J. Geophys. Res., 114, A02102, doi: 10.1029/2008JA013491.en_US
dc.identifier.citedreferenceMcFadden, J. P., C. W. Carlson, D. Larson, M. Ludham, R. Abiad, B. Elliott, P. Turin, M. Marckwordt, and V. Angelopoulos ( 2008 ), The THEMIS, ESA plasma instrument and in‐flight calibration, Space Sci. Rev., 141, 277 – 302, doi: 10.1007/s11214‐008‐9440‐2.en_US
dc.identifier.citedreferenceMilano, L. J., W. H. Matthaeus, P. Dmitruk, and D. C. Montgomery ( 2001 ), Local anisotropy in incompressible magnetohydrodynamic turbulence, Phys. Plasmas, 8, 2673, doi: 10.1063/1.1369658.en_US
dc.identifier.citedreferenceMukai, T., S. Machida, Y. Saito, M. Hirahara, T. Terasawa, N. Kaya, T. Obara, M. Ejiri, and A. Nishida ( 1994 ), The low energy particle (LEP) experiment onboard the Geotail satellite, J. Geomag. Geoelectr., 46, 669 – 692, doi: 10.5636/jgg.46.669.en_US
dc.identifier.citedreferenceNozdrachev, M. N., V. A. Styazhkin, A. A. Zarutsky, S. I. Klimov, S. P. Savin, A. A. Skalsky, A. A. Petrukovich, Y. V. Lissakov, I. S. Arshinkov, N. Abadgiev, and A. Bochev ( 1995 ), Magnetic field measurements onboard the Interball tail spacecraft: The FM‐3I instrument, in Interball Mission and Payload, pp. 228 – 229, CNES, Toulouse, France.en_US
dc.identifier.citedreferenceOsman, K. R., and T. S. Horbury ( 2007 ), Multispacecraft measurement of anisotropic correlation functions in the solar wind turbulence, Astrophys. J., 654, L103 – L106, doi: 10.1086/510906.en_US
dc.identifier.citedreferenceOughton, S., and W. H. Matthaeus ( 2005 ), Parallel and perpendicular cascades in solar wind turbulence, Nonlinear Process. Geophys., 12, 299 – 310, doi: 10.5194/npg‐12‐299‐2005.en_US
dc.identifier.citedreferenceRème, H., et al. ( 1997 ), The Cluster ion spectrometry (CIS) experiment, Space Sci. Rev., 79, 303 – 350, doi: 10.1023/A:1004929816409.en_US
dc.identifier.citedreferenceRichardson, J. D., and C. W. Smith ( 2003 ), The radial temperature profile of the solar wind, Geophys. Res. Lett., 30 ( 5 ), 1206, doi: 10.1029/2002GL016551.en_US
dc.identifier.citedreferenceRichardson, J. D., K. L. Paularena, A. J. Lazarus, and J. W. Belcher ( 1995 ), Radial evolution of the solar wind from IMP 8 to Voyager 2, Geophys. Res. Lett., 22, 325, doi: 10.1029/94GL03273.en_US
dc.identifier.citedreferenceRoberts, D. A., M. L. Goldstein, L. W. Klein, and W. H. Matthaeus ( 1987 ), Origin and evolution of fluctuations in the solar wind: Helios observations and Helios‐Voyager comparisons, J. Geophys. Res., 92, 12,023 – 12,035, doi: 10.1029/JA092iA11p12023.en_US
dc.identifier.citedreferenceRuffolo, D., W. H. Matthaeus, and P. Cuychai ( 2004 ), Separation of magnetic field lines in two‐component turbulence, Astrophys. J., 614, 420 – 434, doi: 10.1086/423412.en_US
dc.identifier.citedreferenceSmith, C. W., J. L. Heureux, N. F. Ness, M. H. Acuna, L. F. Burlaga, and J. Scheiffele ( 1998 ), The ACE magnetic fields experiment, Space Sci. Rev., 86, 613 – 632, doi: 10.1023/A:1005092216668.en_US
dc.identifier.citedreferenceSmith, C. W., W. H. Matthaeus, G. P. Zank, N. F. Ness, S. Oughton, and J. D. Richardson ( 2001 ), Heating of the low‐latitude solar wind by dissipation of turbulent magnetic fluctuations, J. Geophys. Res., 106, 8253 – 8272, doi: 10.1029/2000JA000366.en_US
dc.identifier.citedreferenceTaylor, G. I. ( 1938 ), The spectrum of turbulence, Proc. R. Soc. A, 164, 476 – 490.en_US
dc.identifier.citedreferenceTu, C. Y., and E. Marsch ( 1995 ), MHD structures, waves and turbulence in the solar wind, Space Sci. Rev., 73, 1 – 210, doi: 10.1007/BF00748891.en_US
dc.identifier.citedreferenceVelli, M. ( 2003 ), MHD turbulence and the heating of astrophysical plasma, Plasma Phys. Controlled Fusion, 45, A205, doi: 10.1088/0741‐3335/45/12A/014.en_US
dc.identifier.citedreferenceWeygand, J. M., W. H. Matthaeus, S. Dasso, M. G. Kivelson, and R. J. Walker ( 2007 ), Taylor scale and effective magnetic Reynolds number determination from the plasma sheet and the solar wind magnetic field fluctuations, J. Geophys. Res., 112, A10201, doi: 10.1029/2007JA012486.en_US
dc.identifier.citedreferenceWeygand, J. M., W. H. Matthaeus, S. Dasso, and M. G. Kivelson ( 2009 ), Anisotropy of the Taylor scale and the correlation scale in plasma sheet and solar wind magnetic field fluctuations, J. Geophys. Res., 114, A07213, doi: 10.1029/2008JA013766.en_US
dc.identifier.citedreferenceWeygand, J. M., W. H. Matthaeus, M. El Alaoui, S. Dasso, and M. G. Kivelson ( 2010 ), Anisotropy of the Taylor scale and the correlation scale in plasma sheet magnetic field fluctuations as a function of auroral electrojet activity, J. Geophys. Res., 115, A12250, doi: 10.1029/2010JA015499.en_US
dc.identifier.citedreferenceWilliams, L. L., G. P. Zank, and W. H. Matthaeus ( 1995 ), Dissipation of pickup‐induced waves: A solar wind temperature increase in the outer heliosphere? J. Geophys. Res., 100, 17,059 – 17,067, doi: 10.1029/95JA01261.en_US
dc.identifier.citedreferenceAuster, H. U., et al. ( 2008 ), The THEMIS fluxgate magnetometer, Space Sci. Rev., 141, 235 – 264, doi: 10.1007/s11214‐008‐9365‐9.en_US
dc.identifier.citedreferenceBalogh, A., et al. ( 1997 ), The Cluster magnetic field investigation, Space Sci. Rev., 79, 65 – 91, doi: 10.1023/A:1004970907748.en_US
dc.identifier.citedreferenceBatchelor, G. K. ( 1970 ), Theory of Homogeneous Turbulence, Cambridge Univ. Press, Cambridge, U. K.,en_US
dc.identifier.citedreferenceBieber, J. W., W. H. Matthaeus, C. W. Smith, W. Wanner, M.‐B. Kallenrode, and G. Wibberenz ( 1994 ), Proton and electron mean free paths: The Palmer consensus revisited, Astrophys. J., 420, 294 – 306, doi: 10.1086/173559.en_US
dc.identifier.citedreferenceBieber, J. W., W. Wanner, and W. H. Matthaeus ( 1996 ), Dominant two‐dimensional solar wind turbulence with implications for cosmic ray transport, J. Geophys. Res., 101, 2511 – 2522, doi: 10.1029/95JA02588.en_US
dc.identifier.citedreferenceBorovsky, J. E. ( 2008 ), Flux tube texture of the solar wind: strands of the magnetic carpet at 1 AU? J. Geophys. Res., 113, A08110, doi: 10.1029/2007JA012684.en_US
dc.identifier.citedreferenceBorovsky, J. E., R. C. Elphic, H. O. Funsten, and M. F. Thomsen ( 1997 ), The Earth's plasma sheet as a laboratory for turbulence in high‐beta MHD, J. Plasma Phys., 57, 1 – 34, doi: 10.1017/S0022377896005259.en_US
dc.identifier.citedreferenceBurlaga, L. F. ( 1991 a), Multifractal structure of the interplanetary magnetic field: Voyager 2 observations near 25 AU, 1987‐1988, Geophys. Res. Lett., 18, 69 – 72, doi: 10.1029/90GL02596.en_US
dc.identifier.citedreferenceBurlaga, L. F. ( 1991 b), Multifractal structure of speed fluctuations in recurrent streams at 1 AU and near 6 AU, Geophys. Res. Lett., 18, 1651 – 1654, doi: 10.1029/91GL01221.en_US
dc.identifier.citedreferenceBurlaga, L. F. ( 1991 c), Intermittent turbulence in the solar wind, J. Geophys. Res., 96, 5847 – 5851, doi: 10.1029/91JA00087.en_US
dc.identifier.citedreferenceBurlaga, L. F., and L. W. Klein ( 1986 ), Fractal structure of the interplanetary magnetic field, J. Geophys. Res., 91, 347 – 350, doi: 10.1029/JA091iA01p00347.en_US
dc.identifier.citedreferenceDasso, S., L. J. Milano, W. H. Matthaeus, and C. W. Smith ( 2005 ), Anisotropy in fast and slow solar wind fluctuations, Astrophys. J., 635, L181 – L184, doi: 10.1086/499559.en_US
dc.identifier.citedreferenceDuffy, P., and K. M. Blundell ( 2005 ), Cosmic ray transport and acceleration, Plasma Phys. Controlled Fusion, 47, B667, doi: 10.1088/0741‐3335/47/12B/S49.en_US
dc.identifier.citedreferenceEscoubet, C. P., R. Schmidt, and M. L. Goldstein ( 1997 ), Cluster‐science and mission overview, Space Sci. Rev., 79, 11 – 32, doi: 10.1023/A:1004923124586.en_US
dc.identifier.citedreferenceFrank, L. A., K. L. Ackerson, W. R. Paterson, J. A. Lee, M. R. English, and G. L. Pickett ( 1994 ), The Comprehensive Plasma Instrumentation (CPI) for the Geotail spacecraft, J. Geomag. Geoelectr., 46, 23 – 37, doi: 10.5636/jgg.46.23.en_US
dc.identifier.citedreferenceGazis, P. R., A. Barnes, J. D. Mihalov, and A. J. Lazarus ( 1994 ), Solar wind velocity and temperature in the outer heliosphere, J. Geophys. Res., 99, 6561 – 6573, doi: 10.1029/93JA03144.en_US
dc.identifier.citedreferenceGoldstein, M. L., D. A. Roberts, and C. A. Fitch ( 1994 ), Properties of the fluctuating magnetic helicity in the inertial and dissipation ranges of solar wind turbulence, J. Geophys. Res., 99, 11,519 – 11,538, doi: 10.1029/94JA00789.en_US
dc.identifier.citedreferenceGoldstein, M. L., D. A. Roberts, and W. H. Matthaeus ( 1995 ), Magnetohydrodynamic turbulence in the solar wind, Annu. Rev. Astron. Astrophys., 33, 283 – 325, doi: 10.1146/annurev.aa.33.090195.001435.en_US
dc.identifier.citedreferenceGreco, A., P. Chuychai, W. H. Matthaeus, S. Servidio, and P. Dmitruk ( 2008 ), Intermittent MHD structures and classical discontinuities, Geophys. Res. Lett., 35, L19111, doi: 10.1029/2008GL035454.en_US
dc.identifier.citedreferenceGreco, A., W. H. Matthaeus, S. Servidio, and P. Dmitruk ( 2009 ), Waiting‐time distributions of magnetic discontinuities: Clustering or Poisson process? Phys. Rev. E, 80, 046401, doi: 10.1103/PhysRevE.80.046401.en_US
dc.identifier.citedreferenceKokubun, S., T. Yamamoto, M. H. Acuna, K. Hayashi, K. Shiokawa, and H. Kawano ( 1994 ), The Geotail magnetic field experiment, J. Geomag. Geoelectr., 46, 7 – 21, doi: 10.5636/jgg.46.7.en_US
dc.identifier.citedreferenceKolmogorov, A. N. ( 1941 ), The local structure of turbulence in incompressible viscous fluid for very large Reynolds' numbers, Dokl. Akad. Nauk SSSR, 30, 301 – 305.en_US
dc.identifier.citedreferenceKraichnan, R. H. ( 1965 ), Inertial‐range spectrum of hydromagnetic turbulence, Phys. Fluids, 8, 1385, doi: 10.1063/1.1761412.en_US
dc.identifier.citedreferenceLazarus, A. J., and K. I. Paularena ( 1998 ), A comparison of solar wind parameters from experiments on the IMP 8 and Wind spacecraft, in Measurement Techniques in Space Plasmas, Geophys. Monogr. Ser., vol. 102, edited by J. E. Borovsky, R. F. Pfaff, and D. T. Young, pp. 85 – 90, AGU, Washington, D. C.,en_US
dc.identifier.citedreferenceLeamon, R. J., W. H. Matthaeus, C. W. Smith, G. P. Zank, and D. J. Mullan ( 2000 ), MHD driven kinetic dissipation in the solar wind and corona, Astrophys. J., 537, 1054, doi: 10.1086/309059.en_US
dc.identifier.citedreferenceLepping, R. P., et al. ( 1995 ), The WIND magnetic field investigation, Space Sci. Rev., 71, 207 – 229, doi: 10.1007/BF00751330.en_US
dc.identifier.citedreferenceLin, R. P., et al. ( 1995 ), A three‐dimensional plasma and energetic particle investigation for the Wind spacecraft, Space Sci. Rev., 71, 125 – 153, doi: 10.1007/BF00751328.en_US
dc.identifier.citedreferenceMatthaeus, W. H., M. L. Goldstein, and D. A. Roberts ( 1990 ), Evidence for the presence of quasi‐two‐dimensional nearly incompressible fluctuations in the solar wind, J. Geophys. Res., 95, 20,673 – 20,683, doi: 10.1029/JA095iA12p20673.en_US
dc.identifier.citedreferenceMatthaeus, W. H., S. Dasso, J. M. Weygand, L. J. Milano, C. W. Smith, and M. G. Kivelson ( 2005 ), Spatial correlation of the solar wind turbulence from two point measurements, Phys. Rev. Lett., 95, 231101, doi: 10.1103/PhysRevLett.95.231101.en_US
dc.identifier.citedreferenceMatthaeus, W. H., J. M. Weygand, P. Chuychai, S. Dasso, C. W. Smith, and M. G. Kivelson ( 2008 ), Interplanetary magnetic Taylor scale and implications for plasma dissipation, Astrophys. J., 678, L141, doi: 10.1086/588525.en_US
dc.identifier.citedreferenceMcComas, D. J., S. J. Bame, P. Barker, W. C. Feldman, J. L. Phillips, P. Riley, and J. W. Griffee ( 1998 ), Solar Wind Electron Proton Alpha Monitor (SWEPAM) for the Advanced Composition Explorer, Space Sci. Rev., 86, 563 – 612, doi: 10.1023/A:1005040232597.en_US
dc.owningcollnameInterdisciplinary and Peer-Reviewed


Files in this item

Show simple item record

Remediation of Harmful Language

The University of Michigan Library aims to describe library materials in a way that respects the people and communities who create, use, and are represented in our collections. Report harmful or offensive language in catalog records, finding aids, or elsewhere in our collections anonymously through our metadata feedback form. More information at Remediation of Harmful Language.

Accessibility

If you are unable to use this file in its current format, please select the Contact Us link and we can modify it to make it more accessible to you.