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MAGNETOTAIL VIEWS AT 33RE : IMP 8 MAGNETOMETER OBSERVATIONS. / KAYMAZ, Z; SISCOE, GL; TSYGANENKO, NA; LEPPING, RP.

In: JOURNAL OF GEOPHYSICAL RESEARCH-EARTH SURFACE, Vol. 99, No. A5, 01.05.1994, p. 8705-8730.

Research output: Contribution to journalArticlepeer-review

Harvard

KAYMAZ, Z, SISCOE, GL, TSYGANENKO, NA & LEPPING, RP 1994, 'MAGNETOTAIL VIEWS AT 33RE: IMP 8 MAGNETOMETER OBSERVATIONS', JOURNAL OF GEOPHYSICAL RESEARCH-EARTH SURFACE, vol. 99, no. A5, pp. 8705-8730. https://doi.org/10.1029/93JA03564

APA

KAYMAZ, Z., SISCOE, GL., TSYGANENKO, NA., & LEPPING, RP. (1994). MAGNETOTAIL VIEWS AT 33RE: IMP 8 MAGNETOMETER OBSERVATIONS. JOURNAL OF GEOPHYSICAL RESEARCH-EARTH SURFACE, 99(A5), 8705-8730. https://doi.org/10.1029/93JA03564

Vancouver

KAYMAZ Z, SISCOE GL, TSYGANENKO NA, LEPPING RP. MAGNETOTAIL VIEWS AT 33RE: IMP 8 MAGNETOMETER OBSERVATIONS. JOURNAL OF GEOPHYSICAL RESEARCH-EARTH SURFACE. 1994 May 1;99(A5):8705-8730. https://doi.org/10.1029/93JA03564

Author

KAYMAZ, Z ; SISCOE, GL ; TSYGANENKO, NA ; LEPPING, RP. / MAGNETOTAIL VIEWS AT 33RE : IMP 8 MAGNETOMETER OBSERVATIONS. In: JOURNAL OF GEOPHYSICAL RESEARCH-EARTH SURFACE. 1994 ; Vol. 99, No. A5. pp. 8705-8730.

BibTeX

@article{dd48799cfc564776a790ab7a9dc0dda9,
title = "MAGNETOTAIL VIEWS AT 33RE: IMP 8 MAGNETOMETER OBSERVATIONS",
abstract = "This paper presents magnetic field vector (B) maps, electric current vector (curl B) maps, magnetic force (JxB) contour maps, and total field contour maps covering the full tail cross section in the yz plane. The maps are based on 16 years of 5-min averages of IMP 8 magnetic field data. During this time, IMP 8 traversed the tail between -25R(E) and -40R(E) in the x direction. Its average x distance was -33R(E). For this average distance we show separate maps for low and high dipole tilts, corresponding to equinox and northern hemisphere summer seasons. The low-tilt (equinox) maps show symmetrical field and current patterns; the high-tilt (solstice) maps show the cross-tail current sheet arcing above the equatorial diagonal in the center and dipping below it on the flanks. The shape of warped current sheet fits Fairfield's (1980) displaced ellipse model fairly well. The distance at which the current sheet is hinged to the magnetic equator is found to be 9.88R(E) and is independent of Kp. The z profile of current density shows a central peak, 3R(E) full width at half maximum, and smaller, flanking shoulders. A Harris sheet profile with a 7R(E) thickness fits the B(x) profile. Though these are magnetic field data, the JxB maps clearly outline the plasma sheet. This approach also gives a 7R(E) thickness. Many of the average field and current features inferred and demonstrated in earlier studies are confirmed here; some of them are seen for the first time in full cross-section view. Among new features revealed are a large current vortex in the winter hemisphere lobe, a dawn-dusk asymmetry in the JxB force in the plasma sheet (it is stronger on the duskside), and a separation of the cross-tail current sheet into core and wing parts.",
keywords = "MAGNETOSPHERIC MAGNETIC-FIELD, GEOMAGNETIC NEUTRAL SHEET, TAIL CURRENT SHEET, PLASMA SHEET, POSITION, SHAPE, CONFIGURATION",
author = "Z KAYMAZ and GL SISCOE and NA TSYGANENKO and RP LEPPING",
year = "1994",
month = may,
day = "1",
doi = "10.1029/93JA03564",
language = "English",
volume = "99",
pages = "8705--8730",
journal = "Journal of Geophysical Research: Biogeosciences",
issn = "0148-0227",
publisher = "American Geophysical Union",
number = "A5",

}

RIS

TY - JOUR

T1 - MAGNETOTAIL VIEWS AT 33RE

T2 - IMP 8 MAGNETOMETER OBSERVATIONS

AU - KAYMAZ, Z

AU - SISCOE, GL

AU - TSYGANENKO, NA

AU - LEPPING, RP

PY - 1994/5/1

Y1 - 1994/5/1

N2 - This paper presents magnetic field vector (B) maps, electric current vector (curl B) maps, magnetic force (JxB) contour maps, and total field contour maps covering the full tail cross section in the yz plane. The maps are based on 16 years of 5-min averages of IMP 8 magnetic field data. During this time, IMP 8 traversed the tail between -25R(E) and -40R(E) in the x direction. Its average x distance was -33R(E). For this average distance we show separate maps for low and high dipole tilts, corresponding to equinox and northern hemisphere summer seasons. The low-tilt (equinox) maps show symmetrical field and current patterns; the high-tilt (solstice) maps show the cross-tail current sheet arcing above the equatorial diagonal in the center and dipping below it on the flanks. The shape of warped current sheet fits Fairfield's (1980) displaced ellipse model fairly well. The distance at which the current sheet is hinged to the magnetic equator is found to be 9.88R(E) and is independent of Kp. The z profile of current density shows a central peak, 3R(E) full width at half maximum, and smaller, flanking shoulders. A Harris sheet profile with a 7R(E) thickness fits the B(x) profile. Though these are magnetic field data, the JxB maps clearly outline the plasma sheet. This approach also gives a 7R(E) thickness. Many of the average field and current features inferred and demonstrated in earlier studies are confirmed here; some of them are seen for the first time in full cross-section view. Among new features revealed are a large current vortex in the winter hemisphere lobe, a dawn-dusk asymmetry in the JxB force in the plasma sheet (it is stronger on the duskside), and a separation of the cross-tail current sheet into core and wing parts.

AB - This paper presents magnetic field vector (B) maps, electric current vector (curl B) maps, magnetic force (JxB) contour maps, and total field contour maps covering the full tail cross section in the yz plane. The maps are based on 16 years of 5-min averages of IMP 8 magnetic field data. During this time, IMP 8 traversed the tail between -25R(E) and -40R(E) in the x direction. Its average x distance was -33R(E). For this average distance we show separate maps for low and high dipole tilts, corresponding to equinox and northern hemisphere summer seasons. The low-tilt (equinox) maps show symmetrical field and current patterns; the high-tilt (solstice) maps show the cross-tail current sheet arcing above the equatorial diagonal in the center and dipping below it on the flanks. The shape of warped current sheet fits Fairfield's (1980) displaced ellipse model fairly well. The distance at which the current sheet is hinged to the magnetic equator is found to be 9.88R(E) and is independent of Kp. The z profile of current density shows a central peak, 3R(E) full width at half maximum, and smaller, flanking shoulders. A Harris sheet profile with a 7R(E) thickness fits the B(x) profile. Though these are magnetic field data, the JxB maps clearly outline the plasma sheet. This approach also gives a 7R(E) thickness. Many of the average field and current features inferred and demonstrated in earlier studies are confirmed here; some of them are seen for the first time in full cross-section view. Among new features revealed are a large current vortex in the winter hemisphere lobe, a dawn-dusk asymmetry in the JxB force in the plasma sheet (it is stronger on the duskside), and a separation of the cross-tail current sheet into core and wing parts.

KW - MAGNETOSPHERIC MAGNETIC-FIELD

KW - GEOMAGNETIC NEUTRAL SHEET

KW - TAIL CURRENT SHEET

KW - PLASMA SHEET

KW - POSITION

KW - SHAPE

KW - CONFIGURATION

U2 - 10.1029/93JA03564

DO - 10.1029/93JA03564

M3 - Article

VL - 99

SP - 8705

EP - 8730

JO - Journal of Geophysical Research: Biogeosciences

JF - Journal of Geophysical Research: Biogeosciences

SN - 0148-0227

IS - A5

ER -

ID: 28014513