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Local structure of the magnetotail current sheet : 2001 Cluster observations. / Runov, A; Sergeev, VA; Nakamura, R; Baumjohann, W; Apatenkov, S; Asano, Y; Takada, T; Volwerk, M; Voros, Z; Zhang, TL; Sauvaud, JA; Reme, H; Balogh, A.

In: Annales Geophysicae, Vol. 24, No. 1, 2006, p. 247-262.

Research output: Contribution to journalArticlepeer-review

Harvard

Runov, A, Sergeev, VA, Nakamura, R, Baumjohann, W, Apatenkov, S, Asano, Y, Takada, T, Volwerk, M, Voros, Z, Zhang, TL, Sauvaud, JA, Reme, H & Balogh, A 2006, 'Local structure of the magnetotail current sheet: 2001 Cluster observations', Annales Geophysicae, vol. 24, no. 1, pp. 247-262. https://doi.org/10.5194/angeo-24-247-2006

APA

Runov, A., Sergeev, VA., Nakamura, R., Baumjohann, W., Apatenkov, S., Asano, Y., Takada, T., Volwerk, M., Voros, Z., Zhang, TL., Sauvaud, JA., Reme, H., & Balogh, A. (2006). Local structure of the magnetotail current sheet: 2001 Cluster observations. Annales Geophysicae, 24(1), 247-262. https://doi.org/10.5194/angeo-24-247-2006

Vancouver

Author

Runov, A ; Sergeev, VA ; Nakamura, R ; Baumjohann, W ; Apatenkov, S ; Asano, Y ; Takada, T ; Volwerk, M ; Voros, Z ; Zhang, TL ; Sauvaud, JA ; Reme, H ; Balogh, A. / Local structure of the magnetotail current sheet : 2001 Cluster observations. In: Annales Geophysicae. 2006 ; Vol. 24, No. 1. pp. 247-262.

BibTeX

@article{2103f411f9274dc98a17ab0920d12805,
title = "Local structure of the magnetotail current sheet: 2001 Cluster observations",
abstract = "Thirty rapid crossings of the magnetotail current sheet by the Cluster spacecraft during July-October 2001 at a geocentric distance of 19 RE are examined in detail to address the structure of the current sheet. We use four-point magnetic field measurements to estimate electric current density; the current sheet spatial scale is estimated by integration of the translation velocity calculated from the magnetic field temporal and spatial derivatives. The local normal-related coordinate system for each case is defined by the combining Minimum Variance Analysis (MVA) and the curlometer technique. Numerical parameters characterizing the plasma sheet conditions for these crossings are provided to facilitate future comparisons with theoretical models. Three types of current sheet distributions are distinguished: center-peaked (type I), bifurcated (type II) and asymmetric (type III) sheets. Comparison to plasma parameter distributions show that practically all cases display non-Harris-type behavior, i.e. interior current peaks are embedded into a thicker plasma sheet. The asymmetric sheets with an off-equatorial current density peak most likely have a transient nature. The ion contribution to the electric current rarely agrees with the current computed using the curlometer technique, indicating that either the electron contribution to the current is strong and variable, or the current density is spatially or temporally structured.",
keywords = "magnetospheric physics, magnetotail, plasma sheet, BIFURCATED CURRENT SHEET, MAGNETIC-FIELD, PLASMA SHEET, EARTHS MAGNETOSPHERE, ELECTRIC-CURRENT, ART., SUBSTORM, DYNAMICS, PARTICLE, GEOTAIL",
author = "A Runov and VA Sergeev and R Nakamura and W Baumjohann and S Apatenkov and Y Asano and T Takada and M Volwerk and Z Voros and TL Zhang and JA Sauvaud and H Reme and A Balogh",
year = "2006",
doi = "10.5194/angeo-24-247-2006",
language = "Английский",
volume = "24",
pages = "247--262",
journal = "Annales Geophysicae",
issn = "0992-7689",
publisher = "Copernicus GmbH ",
number = "1",

}

RIS

TY - JOUR

T1 - Local structure of the magnetotail current sheet

T2 - 2001 Cluster observations

AU - Runov, A

AU - Sergeev, VA

AU - Nakamura, R

AU - Baumjohann, W

AU - Apatenkov, S

AU - Asano, Y

AU - Takada, T

AU - Volwerk, M

AU - Voros, Z

AU - Zhang, TL

AU - Sauvaud, JA

AU - Reme, H

AU - Balogh, A

PY - 2006

Y1 - 2006

N2 - Thirty rapid crossings of the magnetotail current sheet by the Cluster spacecraft during July-October 2001 at a geocentric distance of 19 RE are examined in detail to address the structure of the current sheet. We use four-point magnetic field measurements to estimate electric current density; the current sheet spatial scale is estimated by integration of the translation velocity calculated from the magnetic field temporal and spatial derivatives. The local normal-related coordinate system for each case is defined by the combining Minimum Variance Analysis (MVA) and the curlometer technique. Numerical parameters characterizing the plasma sheet conditions for these crossings are provided to facilitate future comparisons with theoretical models. Three types of current sheet distributions are distinguished: center-peaked (type I), bifurcated (type II) and asymmetric (type III) sheets. Comparison to plasma parameter distributions show that practically all cases display non-Harris-type behavior, i.e. interior current peaks are embedded into a thicker plasma sheet. The asymmetric sheets with an off-equatorial current density peak most likely have a transient nature. The ion contribution to the electric current rarely agrees with the current computed using the curlometer technique, indicating that either the electron contribution to the current is strong and variable, or the current density is spatially or temporally structured.

AB - Thirty rapid crossings of the magnetotail current sheet by the Cluster spacecraft during July-October 2001 at a geocentric distance of 19 RE are examined in detail to address the structure of the current sheet. We use four-point magnetic field measurements to estimate electric current density; the current sheet spatial scale is estimated by integration of the translation velocity calculated from the magnetic field temporal and spatial derivatives. The local normal-related coordinate system for each case is defined by the combining Minimum Variance Analysis (MVA) and the curlometer technique. Numerical parameters characterizing the plasma sheet conditions for these crossings are provided to facilitate future comparisons with theoretical models. Three types of current sheet distributions are distinguished: center-peaked (type I), bifurcated (type II) and asymmetric (type III) sheets. Comparison to plasma parameter distributions show that practically all cases display non-Harris-type behavior, i.e. interior current peaks are embedded into a thicker plasma sheet. The asymmetric sheets with an off-equatorial current density peak most likely have a transient nature. The ion contribution to the electric current rarely agrees with the current computed using the curlometer technique, indicating that either the electron contribution to the current is strong and variable, or the current density is spatially or temporally structured.

KW - magnetospheric physics

KW - magnetotail, plasma sheet

KW - BIFURCATED CURRENT SHEET

KW - MAGNETIC-FIELD

KW - PLASMA SHEET

KW - EARTHS MAGNETOSPHERE

KW - ELECTRIC-CURRENT

KW - ART.

KW - SUBSTORM

KW - DYNAMICS

KW - PARTICLE

KW - GEOTAIL

U2 - 10.5194/angeo-24-247-2006

DO - 10.5194/angeo-24-247-2006

M3 - статья

VL - 24

SP - 247

EP - 262

JO - Annales Geophysicae

JF - Annales Geophysicae

SN - 0992-7689

IS - 1

ER -

ID: 36758781