Standard

Reconnection active layers. / Biernat, H. K.; Heyn, M. F.; Semenov, V. S.

в: Advances in Space Research, Том 6, № 1, 1986, стр. 119-121.

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

Harvard

Biernat, HK, Heyn, MF & Semenov, VS 1986, 'Reconnection active layers', Advances in Space Research, Том. 6, № 1, стр. 119-121. https://doi.org/10.1016/0273-1177(86)90022-0

APA

Biernat, H. K., Heyn, M. F., & Semenov, V. S. (1986). Reconnection active layers. Advances in Space Research, 6(1), 119-121. https://doi.org/10.1016/0273-1177(86)90022-0

Vancouver

Biernat HK, Heyn MF, Semenov VS. Reconnection active layers. Advances in Space Research. 1986;6(1):119-121. https://doi.org/10.1016/0273-1177(86)90022-0

Author

Biernat, H. K. ; Heyn, M. F. ; Semenov, V. S. / Reconnection active layers. в: Advances in Space Research. 1986 ; Том 6, № 1. стр. 119-121.

BibTeX

@article{51b22c882f0647a1a8764f080ac6847b,
title = "Reconnection active layers",
abstract = "The analysis presented shows that the classical model of non-linear magnetic field line reconnection changes considerably in the presence of sheared magnetic fields and/or high tangential plasma flow components. This shear excites large amplitude Alfv{\'e}n waves on both sides of the reconnection layer where the magnetic field is rotated to a common direction within the layer. In addition two slow shock (or rarefaction) waves within the reconnection layer are necessary to account for the remaining shear in plasma flow. The detailed structures of such reconnection layers with implications for magnetopause reconnection events are discussed.",
author = "Biernat, {H. K.} and Heyn, {M. F.} and Semenov, {V. S.}",
year = "1986",
doi = "10.1016/0273-1177(86)90022-0",
language = "English",
volume = "6",
pages = "119--121",
journal = "Advances in Space Research",
issn = "0273-1177",
publisher = "Elsevier",
number = "1",

}

RIS

TY - JOUR

T1 - Reconnection active layers

AU - Biernat, H. K.

AU - Heyn, M. F.

AU - Semenov, V. S.

PY - 1986

Y1 - 1986

N2 - The analysis presented shows that the classical model of non-linear magnetic field line reconnection changes considerably in the presence of sheared magnetic fields and/or high tangential plasma flow components. This shear excites large amplitude Alfvén waves on both sides of the reconnection layer where the magnetic field is rotated to a common direction within the layer. In addition two slow shock (or rarefaction) waves within the reconnection layer are necessary to account for the remaining shear in plasma flow. The detailed structures of such reconnection layers with implications for magnetopause reconnection events are discussed.

AB - The analysis presented shows that the classical model of non-linear magnetic field line reconnection changes considerably in the presence of sheared magnetic fields and/or high tangential plasma flow components. This shear excites large amplitude Alfvén waves on both sides of the reconnection layer where the magnetic field is rotated to a common direction within the layer. In addition two slow shock (or rarefaction) waves within the reconnection layer are necessary to account for the remaining shear in plasma flow. The detailed structures of such reconnection layers with implications for magnetopause reconnection events are discussed.

UR - http://www.scopus.com/inward/record.url?scp=46149140309&partnerID=8YFLogxK

U2 - 10.1016/0273-1177(86)90022-0

DO - 10.1016/0273-1177(86)90022-0

M3 - Article

AN - SCOPUS:46149140309

VL - 6

SP - 119

EP - 121

JO - Advances in Space Research

JF - Advances in Space Research

SN - 0273-1177

IS - 1

ER -

ID: 53096565