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A reconstruction method for the reconnection rate applied to Cluster magnetotail measurements. / Penz, T.; Semenov, V. S.; Ivanova, V. V.; Biernat, H. K.; Sergeev, V. A.; Nakamura, R.; Kubyshkin, I. V.; Ivanov, I. B.; Heyn, M. F.

в: Advances in Space Research, Том 37, № 7, 26.05.2006, стр. 1388-1393.

Результаты исследований: Научные публикации в периодических изданиях › статья › Рецензирование

Harvard

Penz, T, Semenov, VS, Ivanova, VV, Biernat, HK, Sergeev, VA, Nakamura, R, Kubyshkin, IV, Ivanov, IB & Heyn, MF 2006, 'A reconstruction method for the reconnection rate applied to Cluster magnetotail measurements', Advances in Space Research, Том. 37, № 7, стр. 1388-1393. https://doi.org/10.1016/j.asr.2005.05.020

APA

Penz, T., Semenov, V. S., Ivanova, V. V., Biernat, H. K., Sergeev, V. A., Nakamura, R., Kubyshkin, I. V., Ivanov, I. B., & Heyn, M. F. (2006). A reconstruction method for the reconnection rate applied to Cluster magnetotail measurements. Advances in Space Research, 37(7), 1388-1393. https://doi.org/10.1016/j.asr.2005.05.020

Vancouver

Penz T, Semenov VS, Ivanova VV, Biernat HK, Sergeev VA, Nakamura R и пр. A reconstruction method for the reconnection rate applied to Cluster magnetotail measurements. Advances in Space Research. 2006 Май 26;37(7):1388-1393. https://doi.org/10.1016/j.asr.2005.05.020

Author

Penz, T. ; Semenov, V. S. ; Ivanova, V. V. ; Biernat, H. K. ; Sergeev, V. A. ; Nakamura, R. ; Kubyshkin, I. V. ; Ivanov, I. B. ; Heyn, M. F. / A reconstruction method for the reconnection rate applied to Cluster magnetotail measurements. в: Advances in Space Research. 2006 ; Том 37, № 7. стр. 1388-1393.

BibTeX

@article{9d5ada63607243d99aaaf8bc28b31dc4,
title = "A reconstruction method for the reconnection rate applied to Cluster magnetotail measurements",
abstract = "We apply a theoretical model to describe the behavior of nightside flux transfer events (NFTEs) measured by Cluster satellites in the Earth magnetotail. Based on the Cagniard-deHoop method we calculate the magnetic field and plasma flow time series observed by a satellite. Our aim is to solve an inverse problem to obtain the reconnection rate from the measured plasma data. The ill-posed inverse problem is treated with the method of regularization, since the solution of the Cagniard-deHoop method is given in the form of a convolution integral, which is well known in the theory of inverse problems. This method is applied to Cluster measurements from September 8th, 2002, where a series of Earthward propagating 1-min scale magnetic field and plasma flow variations were observed outside of the plasma sheet, which are consistent with the theoretical picture of NFTEs. Estimations of the satellite position with respect to the reconnection site and of the Alfv{\'e}n velocity are made because they are necessary parameters for the model. The reconnection rate is found to be in the range of 1-2 mV/m and the reconnection site at about 29 Re tailwards.",
keywords = "Cluster spacecraft, Flux transfer events, Inverse problem, Reconnection",
author = "T. Penz and Semenov, {V. S.} and Ivanova, {V. V.} and Biernat, {H. K.} and Sergeev, {V. A.} and R. Nakamura and Kubyshkin, {I. V.} and Ivanov, {I. B.} and Heyn, {M. F.}",
year = "2006",
month = may,
day = "26",
doi = "10.1016/j.asr.2005.05.020",
language = "English",
volume = "37",
pages = "1388--1393",
journal = "Advances in Space Research",
issn = "0273-1177",
publisher = "Elsevier",
number = "7",

}

RIS

TY - JOUR

T1 - A reconstruction method for the reconnection rate applied to Cluster magnetotail measurements

AU - Penz, T.

AU - Semenov, V. S.

AU - Ivanova, V. V.

AU - Biernat, H. K.

AU - Sergeev, V. A.

AU - Nakamura, R.

AU - Kubyshkin, I. V.

AU - Ivanov, I. B.

AU - Heyn, M. F.

PY - 2006/5/26

Y1 - 2006/5/26

N2 - We apply a theoretical model to describe the behavior of nightside flux transfer events (NFTEs) measured by Cluster satellites in the Earth magnetotail. Based on the Cagniard-deHoop method we calculate the magnetic field and plasma flow time series observed by a satellite. Our aim is to solve an inverse problem to obtain the reconnection rate from the measured plasma data. The ill-posed inverse problem is treated with the method of regularization, since the solution of the Cagniard-deHoop method is given in the form of a convolution integral, which is well known in the theory of inverse problems. This method is applied to Cluster measurements from September 8th, 2002, where a series of Earthward propagating 1-min scale magnetic field and plasma flow variations were observed outside of the plasma sheet, which are consistent with the theoretical picture of NFTEs. Estimations of the satellite position with respect to the reconnection site and of the Alfvén velocity are made because they are necessary parameters for the model. The reconnection rate is found to be in the range of 1-2 mV/m and the reconnection site at about 29 Re tailwards.

AB - We apply a theoretical model to describe the behavior of nightside flux transfer events (NFTEs) measured by Cluster satellites in the Earth magnetotail. Based on the Cagniard-deHoop method we calculate the magnetic field and plasma flow time series observed by a satellite. Our aim is to solve an inverse problem to obtain the reconnection rate from the measured plasma data. The ill-posed inverse problem is treated with the method of regularization, since the solution of the Cagniard-deHoop method is given in the form of a convolution integral, which is well known in the theory of inverse problems. This method is applied to Cluster measurements from September 8th, 2002, where a series of Earthward propagating 1-min scale magnetic field and plasma flow variations were observed outside of the plasma sheet, which are consistent with the theoretical picture of NFTEs. Estimations of the satellite position with respect to the reconnection site and of the Alfvén velocity are made because they are necessary parameters for the model. The reconnection rate is found to be in the range of 1-2 mV/m and the reconnection site at about 29 Re tailwards.

KW - Cluster spacecraft

KW - Flux transfer events

KW - Inverse problem

KW - Reconnection

UR - http://www.scopus.com/inward/record.url?scp=33646722463&partnerID=8YFLogxK

U2 - 10.1016/j.asr.2005.05.020

DO - 10.1016/j.asr.2005.05.020

M3 - Article

AN - SCOPUS:33646722463

VL - 37

SP - 1388

EP - 1393

JO - Advances in Space Research

JF - Advances in Space Research

SN - 0273-1177

IS - 7

ER -

ID: 36928745