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Inverse reconstruction technique based on time-dependent Petschek-type reconnection model : First application to THEMIS magnetotail observations. / Ivanova, V.; Liu, J.; Kiehas, S.; Semenov, V.; Biernat, H.

In: Annales Geophysicae, Vol. 27, No. 12, 28.12.2009, p. 4369-4377.

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

Harvard

Ivanova, V, Liu, J, Kiehas, S, Semenov, V & Biernat, H 2009, 'Inverse reconstruction technique based on time-dependent Petschek-type reconnection model: First application to THEMIS magnetotail observations', Annales Geophysicae, vol. 27, no. 12, pp. 4369-4377. https://doi.org/10.5194/angeo-27-4369-2009

APA

Ivanova, V., Liu, J., Kiehas, S., Semenov, V., & Biernat, H. (2009). Inverse reconstruction technique based on time-dependent Petschek-type reconnection model: First application to THEMIS magnetotail observations. Annales Geophysicae, 27(12), 4369-4377. https://doi.org/10.5194/angeo-27-4369-2009

Vancouver

Ivanova V, Liu J, Kiehas S, Semenov V, Biernat H. Inverse reconstruction technique based on time-dependent Petschek-type reconnection model: First application to THEMIS magnetotail observations. Annales Geophysicae. 2009 Dec 28;27(12):4369-4377. https://doi.org/10.5194/angeo-27-4369-2009

Author

Ivanova, V. ; Liu, J. ; Kiehas, S. ; Semenov, V. ; Biernat, H. / Inverse reconstruction technique based on time-dependent Petschek-type reconnection model : First application to THEMIS magnetotail observations. In: Annales Geophysicae. 2009 ; Vol. 27, No. 12. pp. 4369-4377.

BibTeX

@article{a3aa2ee0cf3440039967c0e833e2dee7,
title = "Inverse reconstruction technique based on time-dependent Petschek-type reconnection model: First application to THEMIS magnetotail observations",
abstract = "We apply the inverse reconstruction technique based on the two-dimensional time-dependent Petschek-type reconnection model to a dual bipolar magnetic structure observed by THEMIS B probe in the Earth's magnetotail during a substorm on 22 February 2008 around 04:35 UT. The technique exploits the recorded bipolar magnetic field variation as an input and provides the reconnection electric field and the location of the X-line as an output. As a result of the technique application, we get (1) the electric field, reaching ∼1.1 mV/m at the maximum and consisting of two successive pulses with total duration of ∼6 min, and (2) the approximate X-line position located in the magnetotail between 18 and 20 RE.",
keywords = "Space plasma physics (Magnetic reconnection)",
author = "V. Ivanova and J. Liu and S. Kiehas and V. Semenov and H. Biernat",
year = "2009",
month = dec,
day = "28",
doi = "10.5194/angeo-27-4369-2009",
language = "English",
volume = "27",
pages = "4369--4377",
journal = "Annales Geophysicae",
issn = "0992-7689",
publisher = "Copernicus GmbH ",
number = "12",

}

RIS

TY - JOUR

T1 - Inverse reconstruction technique based on time-dependent Petschek-type reconnection model

T2 - First application to THEMIS magnetotail observations

AU - Ivanova, V.

AU - Liu, J.

AU - Kiehas, S.

AU - Semenov, V.

AU - Biernat, H.

PY - 2009/12/28

Y1 - 2009/12/28

N2 - We apply the inverse reconstruction technique based on the two-dimensional time-dependent Petschek-type reconnection model to a dual bipolar magnetic structure observed by THEMIS B probe in the Earth's magnetotail during a substorm on 22 February 2008 around 04:35 UT. The technique exploits the recorded bipolar magnetic field variation as an input and provides the reconnection electric field and the location of the X-line as an output. As a result of the technique application, we get (1) the electric field, reaching ∼1.1 mV/m at the maximum and consisting of two successive pulses with total duration of ∼6 min, and (2) the approximate X-line position located in the magnetotail between 18 and 20 RE.

AB - We apply the inverse reconstruction technique based on the two-dimensional time-dependent Petschek-type reconnection model to a dual bipolar magnetic structure observed by THEMIS B probe in the Earth's magnetotail during a substorm on 22 February 2008 around 04:35 UT. The technique exploits the recorded bipolar magnetic field variation as an input and provides the reconnection electric field and the location of the X-line as an output. As a result of the technique application, we get (1) the electric field, reaching ∼1.1 mV/m at the maximum and consisting of two successive pulses with total duration of ∼6 min, and (2) the approximate X-line position located in the magnetotail between 18 and 20 RE.

KW - Space plasma physics (Magnetic reconnection)

UR - http://www.scopus.com/inward/record.url?scp=72449204141&partnerID=8YFLogxK

U2 - 10.5194/angeo-27-4369-2009

DO - 10.5194/angeo-27-4369-2009

M3 - Article

AN - SCOPUS:72449204141

VL - 27

SP - 4369

EP - 4377

JO - Annales Geophysicae

JF - Annales Geophysicae

SN - 0992-7689

IS - 12

ER -

ID: 52653345