Standard

Plasma sheet location of the nightside equatorward arcs. / Dubyagin, SV; Sergeev, VA; Kubyshkina, MV; Yahnin, AG.

PROCEEDINGS OF THE FIFTH INTERNATIONAL CONFERENCE ON SUBSTORMS. ред. / A Wilson. ESA Publication Division, 2000. стр. 287-290 (ESA SPECIAL PUBLICATIONS; Том 443).

Результаты исследований: Публикации в книгах, отчётах, сборниках, трудах конференцийстатья в сборнике материалов конференциинаучнаяРецензирование

Harvard

Dubyagin, SV, Sergeev, VA, Kubyshkina, MV & Yahnin, AG 2000, Plasma sheet location of the nightside equatorward arcs. в A Wilson (ред.), PROCEEDINGS OF THE FIFTH INTERNATIONAL CONFERENCE ON SUBSTORMS. ESA SPECIAL PUBLICATIONS, Том. 443, ESA Publication Division, стр. 287-290, 5th International Conference on Substorms, ST PETERSBURG, 16/05/00.

APA

Dubyagin, SV., Sergeev, VA., Kubyshkina, MV., & Yahnin, AG. (2000). Plasma sheet location of the nightside equatorward arcs. в A. Wilson (Ред.), PROCEEDINGS OF THE FIFTH INTERNATIONAL CONFERENCE ON SUBSTORMS (стр. 287-290). (ESA SPECIAL PUBLICATIONS; Том 443). ESA Publication Division.

Vancouver

Dubyagin SV, Sergeev VA, Kubyshkina MV, Yahnin AG. Plasma sheet location of the nightside equatorward arcs. в Wilson A, Редактор, PROCEEDINGS OF THE FIFTH INTERNATIONAL CONFERENCE ON SUBSTORMS. ESA Publication Division. 2000. стр. 287-290. (ESA SPECIAL PUBLICATIONS).

Author

Dubyagin, SV ; Sergeev, VA ; Kubyshkina, MV ; Yahnin, AG. / Plasma sheet location of the nightside equatorward arcs. PROCEEDINGS OF THE FIFTH INTERNATIONAL CONFERENCE ON SUBSTORMS. Редактор / A Wilson. ESA Publication Division, 2000. стр. 287-290 (ESA SPECIAL PUBLICATIONS).

BibTeX

@inproceedings{9c78ba47a7bd444786ac248d7a1e263f,
title = "Plasma sheet location of the nightside equatorward arcs",
abstract = "We performed two tests to check the constancy of proton pressure along the field lines crossing the tail equator at r similar to 8...20 RE We use the isotropic boundaries as the reference field lines when comparing the pressure measured at low altitude with the plasma sheet pressure computed from either the magnetic field models or empiric formulas. The tests show that both pressure values are close to each other indicating a high degree of isotropy of the proton distributions.Based on these results we analysed the pressure values at low altitudes near the equatorward auroral arcs on the nightside. These pressure values in five cases ranged between 0.1 and 0.4 nPa indicating that the equatorward arcs originate in the current sheet portion of the plasma sheet (at distances >10-12 Re). This is also consistent with are location near (or poleward of) the electron isotropic boundary, whose interpretation as the boundary of nonadiabatic scattering in the weak (",
keywords = "CONFIGURATION",
author = "SV Dubyagin and VA Sergeev and MV Kubyshkina and AG Yahnin",
year = "2000",
language = "Английский",
isbn = "92-9092-772-0",
series = "ESA SPECIAL PUBLICATIONS",
publisher = "ESA Publication Division",
pages = "287--290",
editor = "A Wilson",
booktitle = "PROCEEDINGS OF THE FIFTH INTERNATIONAL CONFERENCE ON SUBSTORMS",
address = "Франция",
note = "null ; Conference date: 16-05-2000 Through 20-05-2000",

}

RIS

TY - GEN

T1 - Plasma sheet location of the nightside equatorward arcs

AU - Dubyagin, SV

AU - Sergeev, VA

AU - Kubyshkina, MV

AU - Yahnin, AG

PY - 2000

Y1 - 2000

N2 - We performed two tests to check the constancy of proton pressure along the field lines crossing the tail equator at r similar to 8...20 RE We use the isotropic boundaries as the reference field lines when comparing the pressure measured at low altitude with the plasma sheet pressure computed from either the magnetic field models or empiric formulas. The tests show that both pressure values are close to each other indicating a high degree of isotropy of the proton distributions.Based on these results we analysed the pressure values at low altitudes near the equatorward auroral arcs on the nightside. These pressure values in five cases ranged between 0.1 and 0.4 nPa indicating that the equatorward arcs originate in the current sheet portion of the plasma sheet (at distances >10-12 Re). This is also consistent with are location near (or poleward of) the electron isotropic boundary, whose interpretation as the boundary of nonadiabatic scattering in the weak (

AB - We performed two tests to check the constancy of proton pressure along the field lines crossing the tail equator at r similar to 8...20 RE We use the isotropic boundaries as the reference field lines when comparing the pressure measured at low altitude with the plasma sheet pressure computed from either the magnetic field models or empiric formulas. The tests show that both pressure values are close to each other indicating a high degree of isotropy of the proton distributions.Based on these results we analysed the pressure values at low altitudes near the equatorward auroral arcs on the nightside. These pressure values in five cases ranged between 0.1 and 0.4 nPa indicating that the equatorward arcs originate in the current sheet portion of the plasma sheet (at distances >10-12 Re). This is also consistent with are location near (or poleward of) the electron isotropic boundary, whose interpretation as the boundary of nonadiabatic scattering in the weak (

KW - CONFIGURATION

M3 - статья в сборнике материалов конференции

SN - 92-9092-772-0

T3 - ESA SPECIAL PUBLICATIONS

SP - 287

EP - 290

BT - PROCEEDINGS OF THE FIFTH INTERNATIONAL CONFERENCE ON SUBSTORMS

A2 - Wilson, A

PB - ESA Publication Division

Y2 - 16 May 2000 through 20 May 2000

ER -

ID: 36631781