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A 2-SATELLITE STUDY OF NIGHTSIDE FLUX-TRANSFER EVENTS IN THE PLASMA SHEET. / Sergeev, V.A.; ELPHIC, RC; MOZER, FS; SAINTMARC, A; SAUVAUD, JA.

In: Planetary and Space Science, Vol. 40, No. 11, 11.1992, p. 1551-1572.

Research output: Contribution to journalArticlepeer-review

Harvard

Sergeev, VA, ELPHIC, RC, MOZER, FS, SAINTMARC, A & SAUVAUD, JA 1992, 'A 2-SATELLITE STUDY OF NIGHTSIDE FLUX-TRANSFER EVENTS IN THE PLASMA SHEET', Planetary and Space Science, vol. 40, no. 11, pp. 1551-1572. https://doi.org/10.1016/0032-0633(92)90052-P

APA

Sergeev, V. A., ELPHIC, RC., MOZER, FS., SAINTMARC, A., & SAUVAUD, JA. (1992). A 2-SATELLITE STUDY OF NIGHTSIDE FLUX-TRANSFER EVENTS IN THE PLASMA SHEET. Planetary and Space Science, 40(11), 1551-1572. https://doi.org/10.1016/0032-0633(92)90052-P

Vancouver

Sergeev VA, ELPHIC RC, MOZER FS, SAINTMARC A, SAUVAUD JA. A 2-SATELLITE STUDY OF NIGHTSIDE FLUX-TRANSFER EVENTS IN THE PLASMA SHEET. Planetary and Space Science. 1992 Nov;40(11):1551-1572. https://doi.org/10.1016/0032-0633(92)90052-P

Author

Sergeev, V.A. ; ELPHIC, RC ; MOZER, FS ; SAINTMARC, A ; SAUVAUD, JA. / A 2-SATELLITE STUDY OF NIGHTSIDE FLUX-TRANSFER EVENTS IN THE PLASMA SHEET. In: Planetary and Space Science. 1992 ; Vol. 40, No. 11. pp. 1551-1572.

BibTeX

@article{5ce9b92db7664a84ab6b1c0a4459807e,
title = "A 2-SATELLITE STUDY OF NIGHTSIDE FLUX-TRANSFER EVENTS IN THE PLASMA SHEET",
abstract = "High time resolution measurements of magnetic and electric fields and of the kiloelectronvolt electron flux at X approximately -21 R(e) in the central magnetotail were used in the study of short-duration (time scale 1 min) magnetic field events during two consecutive substorms on 23 March 1979. These events were observed at ISEE-1 and 2 (having 0.3 R(e) separation along the Z-coordinate), both inside and outside of the thinned plasma sheet, close (in time) to the polarity reversal of the plasma flow from tailward to earthward direction in association with the transient plasma sheet expansions. The enhanced magnetic flux closure (southward B(z) during tailward streaming events, northward during earthward streaming events), plus enhanced plasma flow during these events, suggest that they are nightside magnetic flux transfer events (NFTEs). The typical behaviour of the magnetic field during a NFTE (compression, rotation then field decrease), the signatures of overpressure in such structures and their close correlation with ground-based observed auroral activations and high energy particle bursts signify that NFTE structures may result from the impulsive reconnection in the plasmasheet. Systematic differences in the magnetic variations found at ISEE-1 and 2 indicate current concentration at the outer plasmasheet boundary during the passage of a NFTE. Two NFTEs appeared to have structures similar to magnetic flux ropes. The NFTE structure and associated current system, as well as the interpretation of NFTE signatures in terms of the impulsive reconnection, are discussed. During the {"}poleward leap{"} stage of one substorm, the spacecraft within the central part of the plasma sheet observed the intense earthward magnetic flux transport associated with superimposed NFTE structures. The estimated amount of this flux transfer explained well the observed amplitude of the poleward expansion of the westward electrojet in the conjugate auroral zone.",
keywords = "ELECTRIC-FIELD, SUBSTORM EXPANSION, GEOMAGNETIC TAIL, ISEE SATELLITES, BOUNDARY-LAYER, MAGNETIC-FIELD, NEUTRAL SHEET, RECONNECTION, MAGNETOTAIL, MAGNETOSPHERE",
author = "V.A. Sergeev and RC ELPHIC and FS MOZER and A SAINTMARC and JA SAUVAUD",
year = "1992",
month = nov,
doi = "10.1016/0032-0633(92)90052-P",
language = "Английский",
volume = "40",
pages = "1551--1572",
journal = "Planetary and Space Science",
issn = "0032-0633",
publisher = "Elsevier",
number = "11",

}

RIS

TY - JOUR

T1 - A 2-SATELLITE STUDY OF NIGHTSIDE FLUX-TRANSFER EVENTS IN THE PLASMA SHEET

AU - Sergeev, V.A.

AU - ELPHIC, RC

AU - MOZER, FS

AU - SAINTMARC, A

AU - SAUVAUD, JA

PY - 1992/11

Y1 - 1992/11

N2 - High time resolution measurements of magnetic and electric fields and of the kiloelectronvolt electron flux at X approximately -21 R(e) in the central magnetotail were used in the study of short-duration (time scale 1 min) magnetic field events during two consecutive substorms on 23 March 1979. These events were observed at ISEE-1 and 2 (having 0.3 R(e) separation along the Z-coordinate), both inside and outside of the thinned plasma sheet, close (in time) to the polarity reversal of the plasma flow from tailward to earthward direction in association with the transient plasma sheet expansions. The enhanced magnetic flux closure (southward B(z) during tailward streaming events, northward during earthward streaming events), plus enhanced plasma flow during these events, suggest that they are nightside magnetic flux transfer events (NFTEs). The typical behaviour of the magnetic field during a NFTE (compression, rotation then field decrease), the signatures of overpressure in such structures and their close correlation with ground-based observed auroral activations and high energy particle bursts signify that NFTE structures may result from the impulsive reconnection in the plasmasheet. Systematic differences in the magnetic variations found at ISEE-1 and 2 indicate current concentration at the outer plasmasheet boundary during the passage of a NFTE. Two NFTEs appeared to have structures similar to magnetic flux ropes. The NFTE structure and associated current system, as well as the interpretation of NFTE signatures in terms of the impulsive reconnection, are discussed. During the "poleward leap" stage of one substorm, the spacecraft within the central part of the plasma sheet observed the intense earthward magnetic flux transport associated with superimposed NFTE structures. The estimated amount of this flux transfer explained well the observed amplitude of the poleward expansion of the westward electrojet in the conjugate auroral zone.

AB - High time resolution measurements of magnetic and electric fields and of the kiloelectronvolt electron flux at X approximately -21 R(e) in the central magnetotail were used in the study of short-duration (time scale 1 min) magnetic field events during two consecutive substorms on 23 March 1979. These events were observed at ISEE-1 and 2 (having 0.3 R(e) separation along the Z-coordinate), both inside and outside of the thinned plasma sheet, close (in time) to the polarity reversal of the plasma flow from tailward to earthward direction in association with the transient plasma sheet expansions. The enhanced magnetic flux closure (southward B(z) during tailward streaming events, northward during earthward streaming events), plus enhanced plasma flow during these events, suggest that they are nightside magnetic flux transfer events (NFTEs). The typical behaviour of the magnetic field during a NFTE (compression, rotation then field decrease), the signatures of overpressure in such structures and their close correlation with ground-based observed auroral activations and high energy particle bursts signify that NFTE structures may result from the impulsive reconnection in the plasmasheet. Systematic differences in the magnetic variations found at ISEE-1 and 2 indicate current concentration at the outer plasmasheet boundary during the passage of a NFTE. Two NFTEs appeared to have structures similar to magnetic flux ropes. The NFTE structure and associated current system, as well as the interpretation of NFTE signatures in terms of the impulsive reconnection, are discussed. During the "poleward leap" stage of one substorm, the spacecraft within the central part of the plasma sheet observed the intense earthward magnetic flux transport associated with superimposed NFTE structures. The estimated amount of this flux transfer explained well the observed amplitude of the poleward expansion of the westward electrojet in the conjugate auroral zone.

KW - ELECTRIC-FIELD

KW - SUBSTORM EXPANSION

KW - GEOMAGNETIC TAIL

KW - ISEE SATELLITES

KW - BOUNDARY-LAYER

KW - MAGNETIC-FIELD

KW - NEUTRAL SHEET

KW - RECONNECTION

KW - MAGNETOTAIL

KW - MAGNETOSPHERE

U2 - 10.1016/0032-0633(92)90052-P

DO - 10.1016/0032-0633(92)90052-P

M3 - статья

VL - 40

SP - 1551

EP - 1572

JO - Planetary and Space Science

JF - Planetary and Space Science

SN - 0032-0633

IS - 11

ER -

ID: 36636260