Articles | Volume 21, issue 6
https://doi.org/10.5194/npg-21-1075-2014
© Author(s) 2014. This work is distributed under
the Creative Commons Attribution 3.0 License.
the Creative Commons Attribution 3.0 License.
https://doi.org/10.5194/npg-21-1075-2014
© Author(s) 2014. This work is distributed under
the Creative Commons Attribution 3.0 License.
the Creative Commons Attribution 3.0 License.
Research article
| 
11 Nov 2014
Research article |
| 11 Nov 2014
Wavevector anisotropy of plasma turbulence at ion kinetic scales: solar wind observations and hybrid simulations
Institut für Theoretische Physik, Technische Universität Braunschweig, Mendelssohnstr. 3, 38106 Braunschweig, Germany
Institute for Space Sciences, Atomiştilor 409, P.O. Box MG-23, Bucharest-Măgurele 77125, Romania
Y. Narita
Space Research Institute, Austrian Academy of Sciences, Schmiedlstr. 6, 8042 Graz, Austria
Institut für Geophysik und extraterrestrische Physik, Technische Universität Braunschweig, Mendelssohnstr. 3, 38106 Braunschweig, Germany
U. Motschmann
Institut für Theoretische Physik, Technische Universität Braunschweig, Mendelssohnstr. 3, 38106 Braunschweig, Germany
Deutsches Zentrum für Luft- und Raumfahrt, Institut für Planetenforschung, Rutherfordstr. 2, 12489 Berlin, Germany
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Gurbax S. Lakhina, Bruce T. Tsurutani, George J. Morales, Annick Pouquet, Masahiro Hoshino, Juan Alejandro Valdivia, Yasuhito Narita, and Roger Grimshaw
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Yasuhito Narita and Zoltán Vörös
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A method is proposed to determine the temporal decay rate of turbulent fluctuations, and is applied to four-point magnetic field data in interplanetary space. The measured decay, interpreted as the energy transfer rate in turbulence, is larger than the theoretical estimate from the fluid turbulence theory. The faster decay represents one of the differences in turbulent processes between fluid and plasma media.
Yasuhito Narita
Nonlin. Processes Geophys., 24, 203–214, https://doi.org/10.5194/npg-24-203-2017, https://doi.org/10.5194/npg-24-203-2017, 2017
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Various methods in the single-spacecraft data analysis are reviewed to determine physical properties of waves, turbulent fluctuations, and wave-wave and wave-particle interactions in the space plasma environment using the magnetic field, the electric field, and the plasma data.
Yasuhito Narita, Yoshihiro Nishimura, and Tohru Hada
Ann. Geophys., 35, 639–644, https://doi.org/10.5194/angeo-35-639-2017, https://doi.org/10.5194/angeo-35-639-2017, 2017
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An algorithm is proposed to estimate the spectral index of the turbulence energy spectrum directly in the wavenumber domain using multiple-sensor-array data. In contrast to the conventional method using time series data and Fourier transform of the fluctuation energy onto the frequency domain, the proposed algorithm does not require the assumption of Taylor's frozen inflow hypothesis, enabling direct comparison of the spectra in the wavenumber domain with various theoretical predictions.
Yasuhito Narita
Ann. Geophys., 35, 325–331, https://doi.org/10.5194/angeo-35-325-2017, https://doi.org/10.5194/angeo-35-325-2017, 2017
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In situ spacecraft data in space plasma are obtained often as time series data. Using Taylor's frozen-in flow hypothesis, one can interpret the time series data as spatial variations swept by the slow and passing by the spacecraft. A quantitative method for estimating the error for Taylor's hypothesis is developed here.
Martin Volwerk, Daniel Schmid, Bruce T. Tsurutani, Magda Delva, Ferdinand Plaschke, Yasuhito Narita, Tielong Zhang, and Karl-Heinz Glassmeier
Ann. Geophys., 34, 1099–1108, https://doi.org/10.5194/angeo-34-1099-2016, https://doi.org/10.5194/angeo-34-1099-2016, 2016
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The behaviour of mirror mode waves in Venus's magnetosheath is investigated for solar minimum and maximum conditions. It is shown that the total observational rate of these waves does not change much; however, the distribution over the magnetosheath is significantly different, as well as the growth and decay of the waves during these different solar activity conditions.
Horia Comişel, Yasuhiro Nariyuki, Yasuhito Narita, and Uwe Motschmann
Ann. Geophys., 34, 975–984, https://doi.org/10.5194/angeo-34-975-2016, https://doi.org/10.5194/angeo-34-975-2016, 2016
Ferdinand Plaschke and Yasuhito Narita
Ann. Geophys., 34, 759–766, https://doi.org/10.5194/angeo-34-759-2016, https://doi.org/10.5194/angeo-34-759-2016, 2016
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Spacecraft-mounted magnetic field instruments (magnetometers) need to be routinely calibrated. This involves determining the magnetometer outputs in vanishing ambient magnetic fields, the so-called offsets. We introduce and test a new method to determine these offsets with high accuracy, the mirror mode method, which is complementary to existing methods. The mirror mode method should be highly beneficial to current and future magnetic field observations near Earth, other planets, and comets.
Patrick Meier, Karl-Heinz Glassmeier, and Uwe Motschmann
Ann. Geophys., 34, 691–707, https://doi.org/10.5194/angeo-34-691-2016, https://doi.org/10.5194/angeo-34-691-2016, 2016
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A new type of wave has been detected by the magnetometer of the Rosetta spacecraft close to comet P67/Churyumov-Gerasimenko. We provide the analytical model of this wave excitation from linear perturbation theory. A modified ion-Weibel instability is identified as source of this wave excited by a cometary current. The waves predominantly grow perpendicular to this current. A fan-like phase structure results from superposing the strongest growing waves in a cometary rest frame.
Rudolf A. Treumann, Wolfgang Baumjohann, and Yasuhito Narita
Ann. Geophys., 34, 673–689, https://doi.org/10.5194/angeo-34-673-2016, https://doi.org/10.5194/angeo-34-673-2016, 2016
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Y. Narita, H. Comişel, and U. Motschmann
Ann. Geophys., 34, 591–593, https://doi.org/10.5194/angeo-34-591-2016, https://doi.org/10.5194/angeo-34-591-2016, 2016
Y. Narita, E. Marsch, C. Perschke, K.-H. Glassmeier, U. Motschmann, and H. Comişel
Ann. Geophys., 34, 393–398, https://doi.org/10.5194/angeo-34-393-2016, https://doi.org/10.5194/angeo-34-393-2016, 2016
Y. Narita, R. Nakamura, W. Baumjohann, K.-H. Glassmeier, U. Motschmann, and H. Comişel
Ann. Geophys., 34, 85–89, https://doi.org/10.5194/angeo-34-85-2016, https://doi.org/10.5194/angeo-34-85-2016, 2016
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Four-spacecraft Cluster observations of turbulent fluctuations in the magnetic reconnection region in the geomagnetic tail show for the first time an indication of ion Bernstein waves, electromagnetic waves that propagate nearly perpendicular to the mean magnetic field and are in resonance with ions. Bernstein waves may influence current sheet dynamics in the reconnection outflow such as a bifurcation of the current sheet.
Y. Narita
Ann. Geophys., 33, 1413–1419, https://doi.org/10.5194/angeo-33-1413-2015, https://doi.org/10.5194/angeo-33-1413-2015, 2015
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A lot of efforts have been put into understanding the turbulence structure in space and astrophysical plasmas, in particular how the filamentary structure develops as the length scale of the turbulent fluctuations changes from large to smaller ones. Motivated by the recent spacecraft observations in the solar wind, an analytic model is proposed to explain the nature of filament-formation processes in space plasma turbulence with a successful test against the spacecraft observations.
I. Richter, C. Koenders, H.-U. Auster, D. Frühauff, C. Götz, P. Heinisch, C. Perschke, U. Motschmann, B. Stoll, K. Altwegg, J. Burch, C. Carr, E. Cupido, A. Eriksson, P. Henri, R. Goldstein, J.-P. Lebreton, P. Mokashi, Z. Nemeth, H. Nilsson, M. Rubin, K. Szegö, B. T. Tsurutani, C. Vallat, M. Volwerk, and K.-H. Glassmeier
Ann. Geophys., 33, 1031–1036, https://doi.org/10.5194/angeo-33-1031-2015, https://doi.org/10.5194/angeo-33-1031-2015, 2015
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We present a first report on magnetic field measurements made in the coma of comet 67P/C-G in its low-activity state. The plasma environment is dominated by quasi-coherent, large-amplitude, compressional magnetic field oscillations around 40mHz, differing from the observations at strongly active comets where waves at the cometary ion gyro-frequencies are the main feature. We propose a cross-field current instability associated with the newborn cometary ions as a possible source mechanism.
H. Comişel, Y. Narita, and U. Motschmann
Ann. Geophys., 33, 345–350, https://doi.org/10.5194/angeo-33-345-2015, https://doi.org/10.5194/angeo-33-345-2015, 2015
D. Schmid, M. Volwerk, F. Plaschke, Z. Vörös, T. L. Zhang, W. Baumjohann, and Y. Narita
Ann. Geophys., 32, 651–657, https://doi.org/10.5194/angeo-32-651-2014, https://doi.org/10.5194/angeo-32-651-2014, 2014
M. Wilczek, H. Xu, and Y. Narita
Nonlin. Processes Geophys., 21, 645–649, https://doi.org/10.5194/npg-21-645-2014, https://doi.org/10.5194/npg-21-645-2014, 2014
Y. Narita
Nonlin. Processes Geophys., 21, 41–47, https://doi.org/10.5194/npg-21-41-2014, https://doi.org/10.5194/npg-21-41-2014, 2014
C. Perschke, Y. Narita, S. P. Gary, U. Motschmann, and K.-H. Glassmeier
Ann. Geophys., 31, 1949–1955, https://doi.org/10.5194/angeo-31-1949-2013, https://doi.org/10.5194/angeo-31-1949-2013, 2013
Y. Narita, R. Nakamura, and W. Baumjohann
Ann. Geophys., 31, 1605–1610, https://doi.org/10.5194/angeo-31-1605-2013, https://doi.org/10.5194/angeo-31-1605-2013, 2013
Related subject area
Subject: Nonlinear Waves, Pattern Formation, Turbulence | Topic: Ionosphere, magnetosphere, planetary science, solar science
Lifetime estimate for plasma turbulence
Review article: Wave analysis methods for space plasma experiment
Reversals in the large-scale αΩ-dynamo with memory
Brief Communication: The double layer in the separatrix region during magnetic reconnection
Yasuhito Narita and Zoltán Vörös
Nonlin. Processes Geophys., 24, 673–679, https://doi.org/10.5194/npg-24-673-2017, https://doi.org/10.5194/npg-24-673-2017, 2017
Short summary
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A method is proposed to determine the temporal decay rate of turbulent fluctuations, and is applied to four-point magnetic field data in interplanetary space. The measured decay, interpreted as the energy transfer rate in turbulence, is larger than the theoretical estimate from the fluid turbulence theory. The faster decay represents one of the differences in turbulent processes between fluid and plasma media.
Yasuhito Narita
Nonlin. Processes Geophys., 24, 203–214, https://doi.org/10.5194/npg-24-203-2017, https://doi.org/10.5194/npg-24-203-2017, 2017
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L. K. Feschenko and G. M. Vodinchar
Nonlin. Processes Geophys., 22, 361–369, https://doi.org/10.5194/npg-22-361-2015, https://doi.org/10.5194/npg-22-361-2015, 2015
J. Guo and B. Yu
Nonlin. Processes Geophys., 22, 167–171, https://doi.org/10.5194/npg-22-167-2015, https://doi.org/10.5194/npg-22-167-2015, 2015
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The key finding is that an electron beam can be generated in the separatrix region as magnetic reconnection proceeds. This electron beam could trigger the ion-acoustic instability, and a double layer accompanied with electron holes can be found during the nonlinear evolution stage of this instability.
Cited articles
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Chen, C. H. K., Mallet, A., Schekochihin, A. A., Horbury, T. S., Wicks, R. T., and Bale S. D.: Three-dimensional structure of solar wind turbulence, Astrophys. J., 758, 120, 5 pp., https://doi.org/10.1088/0004-637X/758/2/120, 2012.
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Comişel, H., Verscharen, D., Narita, Y., and Motschmann, U.: Spectral evolution of two-dimensional kinetic plasma turbulence in the wavenumber-frequency domain, Phys. Plasmas, 20, 090701, https://doi.org/10.1063/1.4820936, 2013.
Cumming, A., Arras, P., and Zweibel, E.: Magnetic field evolution in neutron star crusts due to the Hall effect and Ohmic decay, Astrophys. J., 609, 999–1017, https://doi.org/10.1086/421324, 2004.
Dasso, S., Milano, L. J., Matthaeus, W. H., and Smith, C. W.: Anisotropy in fast and slow solar wind fluctuations, Astrophys. J., 635, L181–L184, https://doi.org/10.1086/499559, 2005.
Dastgeer, S. and Zank, G. P.: Anisotropic turbulence in two-dimensional electron magnetohydrodynamics, Astrophys. J., 599, 715–722, https://doi.org/10.1086/379225, 2003.
Dieckmann, M. E., Ynnerman, A., Chapman, S. C, Rowlands, G., and Andersson, N.: Simulating thermal noise, Physica Scripta, 69, 456–460, https://doi.org/10.1238/Physica.Regular.069a00456, 2004.
Drake, D. J., Schroeder, J. W. R., Howes, G. G., Kletzing, C. A., Skiff, F., Carter, T. A., and Auerbach, D. W.: Alfvén wave collisions, the fundamental building block of plasma turbulence. IV. Laboratory experiment, Phys. Plasmas, 20, 072901, https://doi.org/10.1063/1.4813242, 2013.
Gary, S. P., Saito, S., and Narita, Y.: Whistler turbulence wavevector anisotropies: particle-in-cell simulations, Astrophys. J., 716, 1332–1335, https://doi.org/10.1088/0004-637X/716/2/1332, 2010.
Howes, G. G., Tenbarge, J. M., Dorland, W., Quataert, E., Schekochihin, A. A., Numata, R., and Tatsuno T.: Gyrokinetic simulations of solar wind turbulence from ion to electron scales, Phys. Rev. Lett., 107, 035004, https://doi.org/10.1103/PhysRevLett.109.255001, 2011.
Howes, G. G., Drake, D. J., Nielson, K. D., Carter, T. A., Kletzing, C. A., and Skiff, F.: Toward astrophysical turbulence in the laboratory, Phys. Rev. Lett., 109, 255001, https://doi.org/10.1103/PhysRevLett.109.255001, 2012.
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Matthaeus, W. H., Goldstein, M. L., and Roberts, D. A.: Evidence for the presence of quasi-two-dimensional nearly incompressible fluctuations in the solar wind, J. Geophys. Res., 95, 20673–20683, https://doi.org/10.1029/JA095iA12p20673,1990.
Matthaeus, W. H., Gosh, S., Ougton, S., and Roberts, D. A.: Anisotropic three-dimensional MHD turbulence, J. Geophys. Res., 101, 7619–7630, https://doi.org/10.1029/95JA03830, 1996.
Matthaeus, W. H. and Gosh, S.: Spectral decomposition of solar wind turbulence: Three-component model, AIP Conf. Proc. The solar wind nine conference, 5–9 October 1998, Nantucket, Massachusetts, 471, 519–522, https://doi.org/10.1063/1.58688, 1999.
Müller, J., Simon, S., Motschmann, U., Schüle, J., Glassmeier, K.-H., and Pringle, G. J.: Adaptive hybrid model for space plasma simulations, Comp. Phys. Comm., 182, 946–966, https://doi.org/10.1016/j.cpc.2010.12.033, 2011.
Narita, Y. and Glassmeier, K.-H.: Anisotropy evolution of magnetic field fluctuation through the bow shock, Earth Planet. Space, 62, e1–e4, https://doi.org/10.5047/eps.2010.02.001, 2010.
Narita, Y., Glassmeier, K.-H., and Motschmann, U.: High-resolution wave number spectrum using multi-point measurements in space – the Multi-point Signal Resonator (MSR) technique, Ann. Geophys., 29, 351–360, https://doi.org/10.5194/angeo-29-351-2011, 2011.
Narita, Y., Comişel, H., and Motschmann, U.; Spatial structure of ion-scale plasma turbulence, Front. Phys., 2, 13, https://doi.org/10.3389/fphy.2014.00013, 2014.
Rème, H., Aoustin, C., Bosqued, J. M., Dandouras, I., Lavraud, B., Sauvaud, J. A., Barthe, A., Bouyssou, J., Camus, Th., Coeur-Joly, O., Cros, A., Cuvilo, J., Ducay, F., Garbarowitz, Y., Medale, J. L., Penou, E., Perrier, H., Romefort, D., Rouzaud, J., Vallat, C., Alcaydé, D., Jacquey, C., Mazelle, C., d'Uston, C., Möbius, E., Kistler, L. M., Crocker, K., Granoff, M., Mouikis, C., Popecki, M., Vosbury, M., Klecker, B., Hovestadt, D., Kucharek, H., Kuenneth, E., Paschmann, G., Scholer, M., Sckopke, N., Seidenschwang, E., Carlson, C. W., Curtis, D. W., Ingraham, C., Lin, R. P., McFadden, J. P., Parks, G. K., Phan, T., Formisano, V., Amata, E., Bavassano-Cattaneo, M. B., Baldetti, P., Bruno, R., Chionchio, G., Di Lellis, A., Marcucci, M. F., Pallocchia, G., Korth, A., Daly, P. W., Graeve, B., Rosenbauer, H., Vasyliunas, V., McCarthy, M., Wilber, M., Eliasson, L., Lundin, R., Olsen, S., Shelley, E. G., Fuselier, S., Ghielmetti, A. G., Lennartsson, W., Escoubet, C. P., Balsiger, H., Friedel, R., Cao, J.-B., Kovrazhkin, R. A., Papamastorakis, I., Pellat, R., Scudder, J., and Sonnerup, B.: First multispacecraft ion measurements in and near the Earth's magnetosphere with the identical Cluster ion spectrometry (CIS) experiment, Ann. Geophys., 19, 1303–1354, https://doi.org/10.5194/angeo-19-1303-2001, 2001.
Saito, S., Gary, S. P., Li, H., and Narita, Y.: Whistler turbulence: Particle-in-cell simulations, Phys. Plasmas, 15, 102305, https://doi.org/10.1063/1.2997339, 2008.
Saito, S., Gary, S. P., and Narita, Y.: Wavenumber spectrum of whistler turbulence: Particle-in-cell simulation, Phys. Plasmas, 17, 122316, https://doi.org/10.1063/1.3526602, 2010.
Saito, S. and Gary, S. P.: Beta dependence of electron heating in decaying whistler turbulence: Particle-in-cell simulations, Phys. Plasmas, 19, 012312, https://doi.org/10.1063/1.3676155, 2012.
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Shebalin, J. V., Matthaeus, W. H., and Montgomery, D.: Anisotropy in MHD turbulence due to a mean magnetic field, J. Plasma Phys., 29, 525–547, https://doi.org/10.1017/S0022377800000933, 1983.
Smith, C. W., Vasquez, B. J., and Hamilton, K.: Interplanetary magnetic fluctuation anisotropy in the inertial range, J. Geophys. Res., 111, A09111, https://doi.org/10.1029/2006JA011651, 2006.
Valentini, F., Califano, F., and Veltri, P.: Two-dimensional kinetic turbulence in the solar wind, Phys. Rev. Lett., 104, 205002, https://doi.org/10.1103/PhysRevLett.104.205002, 2010.
Verscharen, D., Marsch, E., Motschmann, U., and Müller, J.: Kinetic cascade beyond magnetohydrodynamics of solar wind turbulence in two-dimensional hybrid simulations, Phys. Plasmas, 19, 022305, https://doi.org/10.1063/1.3682960, 2012.
Yoon, P. H., Schlickeiser, R., and Kolberg, U.: Thermal fluctuation levels of magnetic and electric fields in unmagnetized plasma: The rigorous relativistic kinetic theory, Phys. Plasmas, 21, 032109, https://doi.org/10.1063/1.4868232, 2014.
