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Estimate of plasma conductivity in the diffusion region in the magnetotail current sheet during reconnection pulses. / Semenov, Vladimir S.; Bogdanova, Julia V.; Kornilova, Tatjana A.

In: European Space Agency, (Special Publication) ESA SP, No. 389, 01.12.1996, p. 147-151.

Research output: Contribution to journal › Article › peer-review

Harvard

Semenov, VS, Bogdanova, JV & Kornilova, TA 1996, 'Estimate of plasma conductivity in the diffusion region in the magnetotail current sheet during reconnection pulses', European Space Agency, (Special Publication) ESA SP, no. 389, pp. 147-151.

APA

Semenov, V. S., Bogdanova, J. V., & Kornilova, T. A. (1996). Estimate of plasma conductivity in the diffusion region in the magnetotail current sheet during reconnection pulses. European Space Agency, (Special Publication) ESA SP, (389), 147-151.

Vancouver

Semenov VS, Bogdanova JV, Kornilova TA. Estimate of plasma conductivity in the diffusion region in the magnetotail current sheet during reconnection pulses. European Space Agency, (Special Publication) ESA SP. 1996 Dec 1;(389):147-151.

Author

Semenov, Vladimir S. ; Bogdanova, Julia V. ; Kornilova, Tatjana A. / Estimate of plasma conductivity in the diffusion region in the magnetotail current sheet during reconnection pulses. In: European Space Agency, (Special Publication) ESA SP. 1996 ; No. 389. pp. 147-151.

BibTeX

@article{7d78fe8607bb4e91ba01486a33a84bcc,
title = "Estimate of plasma conductivity in the diffusion region in the magnetotail current sheet during reconnection pulses",
abstract = "Models of time-varying Petschek-like magnetic reconnection assume that plasma conductivity drops abruptly in a local region (diffusion region) of the current sheet. This is accompanied by appearance of a strong pulse of electric field accelerating the electrons which precipitate into the ionosphere and produce the auroral breakup. The speed of poleward arc motion in that case should be proportional to the Ey -field in the diffusion region. Based on model equation describing the relationship between the reconnection rate and plasma conductivity as a function of time , we can evaluate the time variation of the size of the diffusion region and plasma conductivity using as input the observed motion of auroral arcs. By studying 9 events for which auroral TV measurements during auroral breakup have been available, we found that for the typical parameters of the current sheet in the magnetotail, the conductivity has to drop down to the value ∼105 CGS which is 10 orders less than its classical value.",
author = "Semenov, {Vladimir S.} and Bogdanova, {Julia V.} and Kornilova, {Tatjana A.}",
year = "1996",
month = dec,
day = "1",
language = "English",
pages = "147--151",
journal = "European Space Agency, (Special Publication) ESA SP",
issn = "0379-6566",
publisher = "ESA Publication Division",
number = "389",

}

RIS

TY - JOUR

T1 - Estimate of plasma conductivity in the diffusion region in the magnetotail current sheet during reconnection pulses

AU - Semenov, Vladimir S.

AU - Bogdanova, Julia V.

AU - Kornilova, Tatjana A.

PY - 1996/12/1

Y1 - 1996/12/1

N2 - Models of time-varying Petschek-like magnetic reconnection assume that plasma conductivity drops abruptly in a local region (diffusion region) of the current sheet. This is accompanied by appearance of a strong pulse of electric field accelerating the electrons which precipitate into the ionosphere and produce the auroral breakup. The speed of poleward arc motion in that case should be proportional to the Ey -field in the diffusion region. Based on model equation describing the relationship between the reconnection rate and plasma conductivity as a function of time , we can evaluate the time variation of the size of the diffusion region and plasma conductivity using as input the observed motion of auroral arcs. By studying 9 events for which auroral TV measurements during auroral breakup have been available, we found that for the typical parameters of the current sheet in the magnetotail, the conductivity has to drop down to the value ∼105 CGS which is 10 orders less than its classical value.

AB - Models of time-varying Petschek-like magnetic reconnection assume that plasma conductivity drops abruptly in a local region (diffusion region) of the current sheet. This is accompanied by appearance of a strong pulse of electric field accelerating the electrons which precipitate into the ionosphere and produce the auroral breakup. The speed of poleward arc motion in that case should be proportional to the Ey -field in the diffusion region. Based on model equation describing the relationship between the reconnection rate and plasma conductivity as a function of time , we can evaluate the time variation of the size of the diffusion region and plasma conductivity using as input the observed motion of auroral arcs. By studying 9 events for which auroral TV measurements during auroral breakup have been available, we found that for the typical parameters of the current sheet in the magnetotail, the conductivity has to drop down to the value ∼105 CGS which is 10 orders less than its classical value.

UR - http://www.scopus.com/inward/record.url?scp=5244223248&partnerID=8YFLogxK

M3 - Article

AN - SCOPUS:5244223248

SP - 147

EP - 151

JO - European Space Agency, (Special Publication) ESA SP

JF - European Space Agency, (Special Publication) ESA SP

SN - 0379-6566

IS - 389

ER -

ID: 53089145