Standard

Energy flow inside a reconnection layer containing slow shocks. / Heyn, M. F.; Rijnbeek, R. P.; Biernat, H. K.; Semenov, V. S.; Farrugia, C. J.; Southwood, D. J.; Paschmann, G.; Sckopke, N.; Russell, C. T.

в: Advances in Space Research, Том 8, № 9-10, 1988, стр. 239-244.

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

Harvard

Heyn, MF, Rijnbeek, RP, Biernat, HK, Semenov, VS, Farrugia, CJ, Southwood, DJ, Paschmann, G, Sckopke, N & Russell, CT 1988, 'Energy flow inside a reconnection layer containing slow shocks', Advances in Space Research, Том. 8, № 9-10, стр. 239-244. https://doi.org/10.1016/0273-1177(88)90136-6

APA

Heyn, M. F., Rijnbeek, R. P., Biernat, H. K., Semenov, V. S., Farrugia, C. J., Southwood, D. J., Paschmann, G., Sckopke, N., & Russell, C. T. (1988). Energy flow inside a reconnection layer containing slow shocks. Advances in Space Research, 8(9-10), 239-244. https://doi.org/10.1016/0273-1177(88)90136-6

Vancouver

Heyn MF, Rijnbeek RP, Biernat HK, Semenov VS, Farrugia CJ, Southwood DJ и пр. Energy flow inside a reconnection layer containing slow shocks. Advances in Space Research. 1988;8(9-10):239-244. https://doi.org/10.1016/0273-1177(88)90136-6

Author

Heyn, M. F. ; Rijnbeek, R. P. ; Biernat, H. K. ; Semenov, V. S. ; Farrugia, C. J. ; Southwood, D. J. ; Paschmann, G. ; Sckopke, N. ; Russell, C. T. / Energy flow inside a reconnection layer containing slow shocks. в: Advances in Space Research. 1988 ; Том 8, № 9-10. стр. 239-244.

BibTeX

@article{92b86f5b2a544241ad6d3c5c379d90d1,
title = "Energy flow inside a reconnection layer containing slow shocks",
abstract = "In the Petschek-type reconnection model the main energy conversion process occurs inside the layer of MHD wave modes- the reconnection layer. Here we analyse the flow and distribution of energy inside this layer for a specific combination of MHD wave modes, which includes slow shocks. To illustrate the energy flow at the Earth's dayside magnetopause, we compare the predicted structure of the reconnection layer with a data example and use the measured parameter values in the magnetosheath and magnetosphere inflow regions to infer the energy flow inside the reconnection layer.",
author = "Heyn, {M. F.} and Rijnbeek, {R. P.} and Biernat, {H. K.} and Semenov, {V. S.} and Farrugia, {C. J.} and Southwood, {D. J.} and G. Paschmann and N. Sckopke and Russell, {C. T.}",
year = "1988",
doi = "10.1016/0273-1177(88)90136-6",
language = "English",
volume = "8",
pages = "239--244",
journal = "Advances in Space Research",
issn = "0273-1177",
publisher = "Elsevier",
number = "9-10",

}

RIS

TY - JOUR

T1 - Energy flow inside a reconnection layer containing slow shocks

AU - Heyn, M. F.

AU - Rijnbeek, R. P.

AU - Biernat, H. K.

AU - Semenov, V. S.

AU - Farrugia, C. J.

AU - Southwood, D. J.

AU - Paschmann, G.

AU - Sckopke, N.

AU - Russell, C. T.

PY - 1988

Y1 - 1988

N2 - In the Petschek-type reconnection model the main energy conversion process occurs inside the layer of MHD wave modes- the reconnection layer. Here we analyse the flow and distribution of energy inside this layer for a specific combination of MHD wave modes, which includes slow shocks. To illustrate the energy flow at the Earth's dayside magnetopause, we compare the predicted structure of the reconnection layer with a data example and use the measured parameter values in the magnetosheath and magnetosphere inflow regions to infer the energy flow inside the reconnection layer.

AB - In the Petschek-type reconnection model the main energy conversion process occurs inside the layer of MHD wave modes- the reconnection layer. Here we analyse the flow and distribution of energy inside this layer for a specific combination of MHD wave modes, which includes slow shocks. To illustrate the energy flow at the Earth's dayside magnetopause, we compare the predicted structure of the reconnection layer with a data example and use the measured parameter values in the magnetosheath and magnetosphere inflow regions to infer the energy flow inside the reconnection layer.

UR - http://www.scopus.com/inward/record.url?scp=45549117752&partnerID=8YFLogxK

U2 - 10.1016/0273-1177(88)90136-6

DO - 10.1016/0273-1177(88)90136-6

M3 - Article

AN - SCOPUS:45549117752

VL - 8

SP - 239

EP - 244

JO - Advances in Space Research

JF - Advances in Space Research

SN - 0273-1177

IS - 9-10

ER -

ID: 53096078