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Determination of reconnected flux via remote sensing. / Kiehas, S. A.; Semenov, V. S.; Kubyshkin, I. V.; Kubyshkina, M. V.; Penz, T.; Biernat, H. K.; Nakamura, R.

In: Advances in Space Research, Vol. 41, No. 8, 2008, p. 1292-1297.

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

Harvard

Kiehas, SA, Semenov, VS, Kubyshkin, IV, Kubyshkina, MV, Penz, T, Biernat, HK & Nakamura, R 2008, 'Determination of reconnected flux via remote sensing', Advances in Space Research, vol. 41, no. 8, pp. 1292-1297. https://doi.org/10.1016/j.asr.2007.05.069

APA

Kiehas, S. A., Semenov, V. S., Kubyshkin, I. V., Kubyshkina, M. V., Penz, T., Biernat, H. K., & Nakamura, R. (2008). Determination of reconnected flux via remote sensing. Advances in Space Research, 41(8), 1292-1297. https://doi.org/10.1016/j.asr.2007.05.069

Vancouver

Kiehas SA, Semenov VS, Kubyshkin IV, Kubyshkina MV, Penz T, Biernat HK et al. Determination of reconnected flux via remote sensing. Advances in Space Research. 2008;41(8):1292-1297. https://doi.org/10.1016/j.asr.2007.05.069

Author

Kiehas, S. A. ; Semenov, V. S. ; Kubyshkin, I. V. ; Kubyshkina, M. V. ; Penz, T. ; Biernat, H. K. ; Nakamura, R. / Determination of reconnected flux via remote sensing. In: Advances in Space Research. 2008 ; Vol. 41, No. 8. pp. 1292-1297.

BibTeX

@article{32647e90cc1843f88066de2511e8d9b7,
title = "Determination of reconnected flux via remote sensing",
abstract = "Magnetic reconnection is one of the most fundamental processes in the magnetosphere. We present here a simple method to determine the essential parameters of reconnection such as reconnected flux and location of the reconnection site out of single spacecraft data via remote sensing. On the basis of a time-dependent reconnection model, the dependence of the reconnected flux on the magnetic field z-component Bz is shown. The integral of Bz over time is proportional to the reconnected flux and depends on the distance between the reconnection site and the actual position where Bz is measured. This distance can be estimated from analysis of magnetic field Bz data. We apply our method to Cluster measurements in the Earth's magnetotail.",
keywords = "Cluster, Magnetic reconnection, Magnetotail, Reconnected flux",
author = "Kiehas, {S. A.} and Semenov, {V. S.} and Kubyshkin, {I. V.} and Kubyshkina, {M. V.} and T. Penz and Biernat, {H. K.} and R. Nakamura",
year = "2008",
doi = "10.1016/j.asr.2007.05.069",
language = "English",
volume = "41",
pages = "1292--1297",
journal = "Advances in Space Research",
issn = "0273-1177",
publisher = "Elsevier",
number = "8",

}

RIS

TY - JOUR

T1 - Determination of reconnected flux via remote sensing

AU - Kiehas, S. A.

AU - Semenov, V. S.

AU - Kubyshkin, I. V.

AU - Kubyshkina, M. V.

AU - Penz, T.

AU - Biernat, H. K.

AU - Nakamura, R.

PY - 2008

Y1 - 2008

N2 - Magnetic reconnection is one of the most fundamental processes in the magnetosphere. We present here a simple method to determine the essential parameters of reconnection such as reconnected flux and location of the reconnection site out of single spacecraft data via remote sensing. On the basis of a time-dependent reconnection model, the dependence of the reconnected flux on the magnetic field z-component Bz is shown. The integral of Bz over time is proportional to the reconnected flux and depends on the distance between the reconnection site and the actual position where Bz is measured. This distance can be estimated from analysis of magnetic field Bz data. We apply our method to Cluster measurements in the Earth's magnetotail.

AB - Magnetic reconnection is one of the most fundamental processes in the magnetosphere. We present here a simple method to determine the essential parameters of reconnection such as reconnected flux and location of the reconnection site out of single spacecraft data via remote sensing. On the basis of a time-dependent reconnection model, the dependence of the reconnected flux on the magnetic field z-component Bz is shown. The integral of Bz over time is proportional to the reconnected flux and depends on the distance between the reconnection site and the actual position where Bz is measured. This distance can be estimated from analysis of magnetic field Bz data. We apply our method to Cluster measurements in the Earth's magnetotail.

KW - Cluster

KW - Magnetic reconnection

KW - Magnetotail

KW - Reconnected flux

UR - http://www.scopus.com/inward/record.url?scp=40649111636&partnerID=8YFLogxK

U2 - 10.1016/j.asr.2007.05.069

DO - 10.1016/j.asr.2007.05.069

M3 - Article

AN - SCOPUS:40649111636

VL - 41

SP - 1292

EP - 1297

JO - Advances in Space Research

JF - Advances in Space Research

SN - 0273-1177

IS - 8

ER -

ID: 18137343