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Energy balance during bursty reconnection. / Semenov, V. S.; Volkonskaya, N. N.; Biernat, H. K.

In: Advances in Space Research, Vol. 26, No. 3, 09.03.2000, p. 561-564.

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

Harvard

Semenov, VS, Volkonskaya, NN & Biernat, HK 2000, 'Energy balance during bursty reconnection', Advances in Space Research, vol. 26, no. 3, pp. 561-564. https://doi.org/10.1016/S0273-1177(99)01092-3

APA

Semenov, V. S., Volkonskaya, N. N., & Biernat, H. K. (2000). Energy balance during bursty reconnection. Advances in Space Research, 26(3), 561-564. https://doi.org/10.1016/S0273-1177(99)01092-3

Vancouver

Semenov VS, Volkonskaya NN, Biernat HK. Energy balance during bursty reconnection. Advances in Space Research. 2000 Mar 9;26(3):561-564. https://doi.org/10.1016/S0273-1177(99)01092-3

Author

Semenov, V. S. ; Volkonskaya, N. N. ; Biernat, H. K. / Energy balance during bursty reconnection. In: Advances in Space Research. 2000 ; Vol. 26, No. 3. pp. 561-564.

BibTeX

@article{e01dac7b65324700a8a69dc3fdc50086,
title = "Energy balance during bursty reconnection",
abstract = "In this paper we study the energy budget during magnetic reconnection. To this end, we concentrate on time-varying reconnection. Our considerations are based on the generalization of the Petschek model for a time varying reconnection rate. For the sake of simplicity, we consider a 2D asymmetric current sheet configuration with an incompressible plasma. Under these circumstances, the reconnection problem can be formulated in an analytical way, and a particularly clear insight can be gained. It turns out that as a result of the fast motion of the outflow region, magnetic energy is accumulated external to its leading front, whereas it is rarefied in the wake region.",
author = "Semenov, {V. S.} and Volkonskaya, {N. N.} and Biernat, {H. K.}",
year = "2000",
month = mar,
day = "9",
doi = "10.1016/S0273-1177(99)01092-3",
language = "English",
volume = "26",
pages = "561--564",
journal = "Advances in Space Research",
issn = "0273-1177",
publisher = "Elsevier",
number = "3",

}

RIS

TY - JOUR

T1 - Energy balance during bursty reconnection

AU - Semenov, V. S.

AU - Volkonskaya, N. N.

AU - Biernat, H. K.

PY - 2000/3/9

Y1 - 2000/3/9

N2 - In this paper we study the energy budget during magnetic reconnection. To this end, we concentrate on time-varying reconnection. Our considerations are based on the generalization of the Petschek model for a time varying reconnection rate. For the sake of simplicity, we consider a 2D asymmetric current sheet configuration with an incompressible plasma. Under these circumstances, the reconnection problem can be formulated in an analytical way, and a particularly clear insight can be gained. It turns out that as a result of the fast motion of the outflow region, magnetic energy is accumulated external to its leading front, whereas it is rarefied in the wake region.

AB - In this paper we study the energy budget during magnetic reconnection. To this end, we concentrate on time-varying reconnection. Our considerations are based on the generalization of the Petschek model for a time varying reconnection rate. For the sake of simplicity, we consider a 2D asymmetric current sheet configuration with an incompressible plasma. Under these circumstances, the reconnection problem can be formulated in an analytical way, and a particularly clear insight can be gained. It turns out that as a result of the fast motion of the outflow region, magnetic energy is accumulated external to its leading front, whereas it is rarefied in the wake region.

UR - http://www.scopus.com/inward/record.url?scp=0040954555&partnerID=8YFLogxK

U2 - 10.1016/S0273-1177(99)01092-3

DO - 10.1016/S0273-1177(99)01092-3

M3 - Article

AN - SCOPUS:0040954555

VL - 26

SP - 561

EP - 564

JO - Advances in Space Research

JF - Advances in Space Research

SN - 0273-1177

IS - 3

ER -

ID: 53087225