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A reconnection layer associated with a magnetic cloud. / Farrugia, C. J.; Vasquez, B.; Richardson, I. G.; Torbert, R. B.; Burlaga, L. F.; Biernat, H. K.; Mühlbachler, S.; Ogilvie, K. W.; Lepping, R. P.; Scudder, J. D.; Berdichevsky, D. E.; Semenov, V. S.; Kubyshkin, I. V.; Phan, T. D.; Lin, R. P.

в: Advances in Space Research, Том 28, № 5, 2001, стр. 759-764.

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

Harvard

Farrugia, CJ, Vasquez, B, Richardson, IG, Torbert, RB, Burlaga, LF, Biernat, HK, Mühlbachler, S, Ogilvie, KW, Lepping, RP, Scudder, JD, Berdichevsky, DE, Semenov, VS, Kubyshkin, IV, Phan, TD & Lin, RP 2001, 'A reconnection layer associated with a magnetic cloud', Advances in Space Research, Том. 28, № 5, стр. 759-764. https://doi.org/10.1016/S0273-1177(01)00529-4

APA

Farrugia, C. J., Vasquez, B., Richardson, I. G., Torbert, R. B., Burlaga, L. F., Biernat, H. K., Mühlbachler, S., Ogilvie, K. W., Lepping, R. P., Scudder, J. D., Berdichevsky, D. E., Semenov, V. S., Kubyshkin, I. V., Phan, T. D., & Lin, R. P. (2001). A reconnection layer associated with a magnetic cloud. Advances in Space Research, 28(5), 759-764. https://doi.org/10.1016/S0273-1177(01)00529-4

Vancouver

Farrugia CJ, Vasquez B, Richardson IG, Torbert RB, Burlaga LF, Biernat HK и пр. A reconnection layer associated with a magnetic cloud. Advances in Space Research. 2001;28(5):759-764. https://doi.org/10.1016/S0273-1177(01)00529-4

Author

Farrugia, C. J. ; Vasquez, B. ; Richardson, I. G. ; Torbert, R. B. ; Burlaga, L. F. ; Biernat, H. K. ; Mühlbachler, S. ; Ogilvie, K. W. ; Lepping, R. P. ; Scudder, J. D. ; Berdichevsky, D. E. ; Semenov, V. S. ; Kubyshkin, I. V. ; Phan, T. D. ; Lin, R. P. / A reconnection layer associated with a magnetic cloud. в: Advances in Space Research. 2001 ; Том 28, № 5. стр. 759-764.

BibTeX

@article{65e022be2f384a26bc848897c399b637,
title = "A reconnection layer associated with a magnetic cloud",
abstract = "We examine a 3-hour long interval on December 24, 1996, containing a magnetic hole associated with an interplanetary magnetic cloud. Two sets of perturbations are observed by the Wind spacecraft at 1 AU. In the first, the field and flow rotate at constant field strength, and the plasma is accelerated to the local Alfven speed. We show this to be a rotational discontinuity. In the second, observed 25 min later, the plasma is heated and the field decreases. We show this to be a slow shock. The whole structure is in pressure balance. We interpret the observations as MHD discontinuities arriving with varying delays from a reconnection site closer to the Sun. Energetic particle observations suggest further that ejecta material is present for many hours prior to the magnetic cloud observation and separated from it by the layer. This suggests that reconnection took place between field lines of a CME of which the magnetic cloud formed a part.",
author = "Farrugia, {C. J.} and B. Vasquez and Richardson, {I. G.} and Torbert, {R. B.} and Burlaga, {L. F.} and Biernat, {H. K.} and S. M{\"u}hlbachler and Ogilvie, {K. W.} and Lepping, {R. P.} and Scudder, {J. D.} and Berdichevsky, {D. E.} and Semenov, {V. S.} and Kubyshkin, {I. V.} and Phan, {T. D.} and Lin, {R. P.}",
year = "2001",
doi = "10.1016/S0273-1177(01)00529-4",
language = "English",
volume = "28",
pages = "759--764",
journal = "Advances in Space Research",
issn = "0273-1177",
publisher = "Elsevier",
number = "5",

}

RIS

TY - JOUR

T1 - A reconnection layer associated with a magnetic cloud

AU - Farrugia, C. J.

AU - Vasquez, B.

AU - Richardson, I. G.

AU - Torbert, R. B.

AU - Burlaga, L. F.

AU - Biernat, H. K.

AU - Mühlbachler, S.

AU - Ogilvie, K. W.

AU - Lepping, R. P.

AU - Scudder, J. D.

AU - Berdichevsky, D. E.

AU - Semenov, V. S.

AU - Kubyshkin, I. V.

AU - Phan, T. D.

AU - Lin, R. P.

PY - 2001

Y1 - 2001

N2 - We examine a 3-hour long interval on December 24, 1996, containing a magnetic hole associated with an interplanetary magnetic cloud. Two sets of perturbations are observed by the Wind spacecraft at 1 AU. In the first, the field and flow rotate at constant field strength, and the plasma is accelerated to the local Alfven speed. We show this to be a rotational discontinuity. In the second, observed 25 min later, the plasma is heated and the field decreases. We show this to be a slow shock. The whole structure is in pressure balance. We interpret the observations as MHD discontinuities arriving with varying delays from a reconnection site closer to the Sun. Energetic particle observations suggest further that ejecta material is present for many hours prior to the magnetic cloud observation and separated from it by the layer. This suggests that reconnection took place between field lines of a CME of which the magnetic cloud formed a part.

AB - We examine a 3-hour long interval on December 24, 1996, containing a magnetic hole associated with an interplanetary magnetic cloud. Two sets of perturbations are observed by the Wind spacecraft at 1 AU. In the first, the field and flow rotate at constant field strength, and the plasma is accelerated to the local Alfven speed. We show this to be a rotational discontinuity. In the second, observed 25 min later, the plasma is heated and the field decreases. We show this to be a slow shock. The whole structure is in pressure balance. We interpret the observations as MHD discontinuities arriving with varying delays from a reconnection site closer to the Sun. Energetic particle observations suggest further that ejecta material is present for many hours prior to the magnetic cloud observation and separated from it by the layer. This suggests that reconnection took place between field lines of a CME of which the magnetic cloud formed a part.

UR - http://www.scopus.com/inward/record.url?scp=6444245282&partnerID=8YFLogxK

U2 - 10.1016/S0273-1177(01)00529-4

DO - 10.1016/S0273-1177(01)00529-4

M3 - Article

AN - SCOPUS:6444245282

VL - 28

SP - 759

EP - 764

JO - Advances in Space Research

JF - Advances in Space Research

SN - 0273-1177

IS - 5

ER -

ID: 53086344