Standard

Temporal evolution of the convective plasma flow during a reconnection process. / Semenov, V. S.; Kubyshkin, I. V.; Heyn, M. F.; Biernat, H. K.

In: Advances in Space Research, Vol. 4, No. 2-3, 1984, p. 471-474.

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

Harvard

Semenov, VS, Kubyshkin, IV, Heyn, MF & Biernat, HK 1984, 'Temporal evolution of the convective plasma flow during a reconnection process', Advances in Space Research, vol. 4, no. 2-3, pp. 471-474. https://doi.org/10.1016/0273-1177(84)90347-8

APA

Semenov, V. S., Kubyshkin, I. V., Heyn, M. F., & Biernat, H. K. (1984). Temporal evolution of the convective plasma flow during a reconnection process. Advances in Space Research, 4(2-3), 471-474. https://doi.org/10.1016/0273-1177(84)90347-8

Vancouver

Semenov VS, Kubyshkin IV, Heyn MF, Biernat HK. Temporal evolution of the convective plasma flow during a reconnection process. Advances in Space Research. 1984;4(2-3):471-474. https://doi.org/10.1016/0273-1177(84)90347-8

Author

Semenov, V. S. ; Kubyshkin, I. V. ; Heyn, M. F. ; Biernat, H. K. / Temporal evolution of the convective plasma flow during a reconnection process. In: Advances in Space Research. 1984 ; Vol. 4, No. 2-3. pp. 471-474.

BibTeX

@article{9b9f93da836a4ec08e9a983372bacfd1,
title = "Temporal evolution of the convective plasma flow during a reconnection process",
abstract = "Following the initial suggestion of Petschek that the efficiency of the energy conversion from magnetic into kinetic energy of the plasma may be essentially enhanced by shock waves, we investigate the temporal evolution of these shocks in a reconnection configuration.",
author = "Semenov, {V. S.} and Kubyshkin, {I. V.} and Heyn, {M. F.} and Biernat, {H. K.}",
year = "1984",
doi = "10.1016/0273-1177(84)90347-8",
language = "English",
volume = "4",
pages = "471--474",
journal = "Advances in Space Research",
issn = "0273-1177",
publisher = "Elsevier",
number = "2-3",

}

RIS

TY - JOUR

T1 - Temporal evolution of the convective plasma flow during a reconnection process

AU - Semenov, V. S.

AU - Kubyshkin, I. V.

AU - Heyn, M. F.

AU - Biernat, H. K.

PY - 1984

Y1 - 1984

N2 - Following the initial suggestion of Petschek that the efficiency of the energy conversion from magnetic into kinetic energy of the plasma may be essentially enhanced by shock waves, we investigate the temporal evolution of these shocks in a reconnection configuration.

AB - Following the initial suggestion of Petschek that the efficiency of the energy conversion from magnetic into kinetic energy of the plasma may be essentially enhanced by shock waves, we investigate the temporal evolution of these shocks in a reconnection configuration.

UR - http://www.scopus.com/inward/record.url?scp=48749139199&partnerID=8YFLogxK

U2 - 10.1016/0273-1177(84)90347-8

DO - 10.1016/0273-1177(84)90347-8

M3 - Article

AN - SCOPUS:48749139199

VL - 4

SP - 471

EP - 474

JO - Advances in Space Research

JF - Advances in Space Research

SN - 0273-1177

IS - 2-3

ER -

ID: 53096955