Standard

Flux transfer events interpreted in terms of a generalized model for petschek-type reconnection. / Semenov, V. S.; Kubyshkin, I. V.; Biemat, H. K.; Heyn, M. F.; Rijnbeek, R. P.; Besser, B. P.; Farrugia, C. J.

в: Advances in Space Research, Том 11, № 9, 1991, стр. 25-28.

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

Harvard

Semenov, VS, Kubyshkin, IV, Biemat, HK, Heyn, MF, Rijnbeek, RP, Besser, BP & Farrugia, CJ 1991, 'Flux transfer events interpreted in terms of a generalized model for petschek-type reconnection', Advances in Space Research, Том. 11, № 9, стр. 25-28. https://doi.org/10.1016/0273-1177(91)90004-4

APA

Semenov, V. S., Kubyshkin, I. V., Biemat, H. K., Heyn, M. F., Rijnbeek, R. P., Besser, B. P., & Farrugia, C. J. (1991). Flux transfer events interpreted in terms of a generalized model for petschek-type reconnection. Advances in Space Research, 11(9), 25-28. https://doi.org/10.1016/0273-1177(91)90004-4

Vancouver

Semenov VS, Kubyshkin IV, Biemat HK, Heyn MF, Rijnbeek RP, Besser BP и пр. Flux transfer events interpreted in terms of a generalized model for petschek-type reconnection. Advances in Space Research. 1991;11(9):25-28. https://doi.org/10.1016/0273-1177(91)90004-4

Author

Semenov, V. S. ; Kubyshkin, I. V. ; Biemat, H. K. ; Heyn, M. F. ; Rijnbeek, R. P. ; Besser, B. P. ; Farrugia, C. J. / Flux transfer events interpreted in terms of a generalized model for petschek-type reconnection. в: Advances in Space Research. 1991 ; Том 11, № 9. стр. 25-28.

BibTeX

@article{92e05cca8fa747d79c60c796b820e101,
title = "Flux transfer events interpreted in terms of a generalized model for petschek-type reconnection",
abstract = "In Petschek's reconnection model MHD waves play the dominant role in energy conversion, and these waves are responsible for propagating the disturbances resulting from reconnection into the system at large. Petschek's model, originally developed to describe a steady-state configuration, may be generalised to describe unsteady phenomena by incorporating a time-varying reconnection rate. With this generalised model it is possible to unify the observations of high-speed flow signatures and flux transfer event (FTE) signatures observed at the dayside magnetopause within a single description; previously, such signatures were commonly attributed to 'steady' and 'unsteady' phenomena, respectively. We show some preliminary results which indicate that FTE signatures result from transient variations in the reconnection rate, and discuss a physical model for these signatures obtained from an extension of Petschek's original analysis to include skewed magnetic field configurations and a finite length of the reconnection line.",
author = "Semenov, {V. S.} and Kubyshkin, {I. V.} and Biemat, {H. K.} and Heyn, {M. F.} and Rijnbeek, {R. P.} and Besser, {B. P.} and Farrugia, {C. J.}",
year = "1991",
doi = "10.1016/0273-1177(91)90004-4",
language = "English",
volume = "11",
pages = "25--28",
journal = "Advances in Space Research",
issn = "0273-1177",
publisher = "Elsevier",
number = "9",

}

RIS

TY - JOUR

T1 - Flux transfer events interpreted in terms of a generalized model for petschek-type reconnection

AU - Semenov, V. S.

AU - Kubyshkin, I. V.

AU - Biemat, H. K.

AU - Heyn, M. F.

AU - Rijnbeek, R. P.

AU - Besser, B. P.

AU - Farrugia, C. J.

PY - 1991

Y1 - 1991

N2 - In Petschek's reconnection model MHD waves play the dominant role in energy conversion, and these waves are responsible for propagating the disturbances resulting from reconnection into the system at large. Petschek's model, originally developed to describe a steady-state configuration, may be generalised to describe unsteady phenomena by incorporating a time-varying reconnection rate. With this generalised model it is possible to unify the observations of high-speed flow signatures and flux transfer event (FTE) signatures observed at the dayside magnetopause within a single description; previously, such signatures were commonly attributed to 'steady' and 'unsteady' phenomena, respectively. We show some preliminary results which indicate that FTE signatures result from transient variations in the reconnection rate, and discuss a physical model for these signatures obtained from an extension of Petschek's original analysis to include skewed magnetic field configurations and a finite length of the reconnection line.

AB - In Petschek's reconnection model MHD waves play the dominant role in energy conversion, and these waves are responsible for propagating the disturbances resulting from reconnection into the system at large. Petschek's model, originally developed to describe a steady-state configuration, may be generalised to describe unsteady phenomena by incorporating a time-varying reconnection rate. With this generalised model it is possible to unify the observations of high-speed flow signatures and flux transfer event (FTE) signatures observed at the dayside magnetopause within a single description; previously, such signatures were commonly attributed to 'steady' and 'unsteady' phenomena, respectively. We show some preliminary results which indicate that FTE signatures result from transient variations in the reconnection rate, and discuss a physical model for these signatures obtained from an extension of Petschek's original analysis to include skewed magnetic field configurations and a finite length of the reconnection line.

UR - http://www.scopus.com/inward/record.url?scp=0008580289&partnerID=8YFLogxK

U2 - 10.1016/0273-1177(91)90004-4

DO - 10.1016/0273-1177(91)90004-4

M3 - Article

AN - SCOPUS:0008580289

VL - 11

SP - 25

EP - 28

JO - Advances in Space Research

JF - Advances in Space Research

SN - 0273-1177

IS - 9

ER -

ID: 53095606