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Neutralschichten und magnetfeldverschmelzung. / Semenov, V. S.; Kubyshkin, I. V.; Heyn, M. F.; Biernat, H.

In: STAR Protocols, Vol. 21, No. 9, 1982.

Research output: Contribution to journalArticlepeer-review

Harvard

Semenov, VS, Kubyshkin, IV, Heyn, MF & Biernat, H 1982, 'Neutralschichten und magnetfeldverschmelzung.', STAR Protocols, vol. 21, no. 9.

APA

Semenov, V. S., Kubyshkin, I. V., Heyn, M. F., & Biernat, H. (1982). Neutralschichten und magnetfeldverschmelzung. STAR Protocols, 21(9).

Vancouver

Semenov VS, Kubyshkin IV, Heyn MF, Biernat H. Neutralschichten und magnetfeldverschmelzung. STAR Protocols. 1982;21(9).

Author

Semenov, V. S. ; Kubyshkin, I. V. ; Heyn, M. F. ; Biernat, H. / Neutralschichten und magnetfeldverschmelzung. In: STAR Protocols. 1982 ; Vol. 21, No. 9.

BibTeX

@article{175c476c36b04eecaffa9f66bd805a55,
title = "Neutralschichten und magnetfeldverschmelzung.",
abstract = "The process of magnetic merging which is important in magnetic field topology in cosmic plasmas is discussed. In this process the energy which is stored in the magnetic field is converted into another form of energy. The occurrence of the reconnection process in the interplanetary space is examined. The importance of the stage of time dependent processes is shown. A curvilinear coordinate system is introduced which is a simple description of the ideal MHD-equations. The nonstationary line of flux fusion is examined and conditions for fusion processes are indicated.-from STAR, 21(9), 1983",
author = "Semenov, {V. S.} and Kubyshkin, {I. V.} and Heyn, {M. F.} and H. Biernat",
note = "Copyright: Copyright 2017 Elsevier B.V., All rights reserved.",
year = "1982",
language = "немецкий",
volume = "21",
journal = "STAR Protocols",
issn = "2666-1667",
publisher = "Cell Press",
number = "9",

}

RIS

TY - JOUR

T1 - Neutralschichten und magnetfeldverschmelzung.

AU - Semenov, V. S.

AU - Kubyshkin, I. V.

AU - Heyn, M. F.

AU - Biernat, H.

N1 - Copyright: Copyright 2017 Elsevier B.V., All rights reserved.

PY - 1982

Y1 - 1982

N2 - The process of magnetic merging which is important in magnetic field topology in cosmic plasmas is discussed. In this process the energy which is stored in the magnetic field is converted into another form of energy. The occurrence of the reconnection process in the interplanetary space is examined. The importance of the stage of time dependent processes is shown. A curvilinear coordinate system is introduced which is a simple description of the ideal MHD-equations. The nonstationary line of flux fusion is examined and conditions for fusion processes are indicated.-from STAR, 21(9), 1983

AB - The process of magnetic merging which is important in magnetic field topology in cosmic plasmas is discussed. In this process the energy which is stored in the magnetic field is converted into another form of energy. The occurrence of the reconnection process in the interplanetary space is examined. The importance of the stage of time dependent processes is shown. A curvilinear coordinate system is introduced which is a simple description of the ideal MHD-equations. The nonstationary line of flux fusion is examined and conditions for fusion processes are indicated.-from STAR, 21(9), 1983

UR - http://www.scopus.com/inward/record.url?scp=85040304981&partnerID=8YFLogxK

M3 - статья

AN - SCOPUS:85040304981

VL - 21

JO - STAR Protocols

JF - STAR Protocols

SN - 2666-1667

IS - 9

ER -

ID: 75945584