Standard

Acceleration processes in the course of dayside solar wind-magnetopause interaction. / Semenov, V. S.

в: Advances in Space Research, Том 21, № 4, 01.01.1998, стр. 583-590.

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

Harvard

Semenov, VS 1998, 'Acceleration processes in the course of dayside solar wind-magnetopause interaction', Advances in Space Research, Том. 21, № 4, стр. 583-590. https://doi.org/10.1016/S0273-1177(97)00967-8

APA

Semenov, V. S. (1998). Acceleration processes in the course of dayside solar wind-magnetopause interaction. Advances in Space Research, 21(4), 583-590. https://doi.org/10.1016/S0273-1177(97)00967-8

Vancouver

Semenov VS. Acceleration processes in the course of dayside solar wind-magnetopause interaction. Advances in Space Research. 1998 Янв. 1;21(4):583-590. https://doi.org/10.1016/S0273-1177(97)00967-8

Author

Semenov, V. S. / Acceleration processes in the course of dayside solar wind-magnetopause interaction. в: Advances in Space Research. 1998 ; Том 21, № 4. стр. 583-590.

BibTeX

@article{c1a93468de7349ae86893eca7405e270,
title = "Acceleration processes in the course of dayside solar wind-magnetopause interaction",
abstract = "Magnetic reconnection is believed to be the dominant coupling process at the Earth's magnetopause. The main features which characterise this process are the conversion of magnetic field energy into plasma energy, an associated change in the magnetic field topology, and the emission of high-energy (suprathermal) charged particles. A review is presented of the development of theoretical concepts of reconnection, starting with steady-state Petschek model. The topics covered include extension of Petschek's model for the time-dependent case, the switch-on and switch-off phases of reconnection, models of flux transfer events (FTEs), steady-state and time-dependent reconnection in compressible plasma, acceleration of plasma through the system of large-amplitude MHD waves, acceleration of charged particles in the diffusion region, the role of the surface waves.",
author = "Semenov, {V. S.}",
year = "1998",
month = jan,
day = "1",
doi = "10.1016/S0273-1177(97)00967-8",
language = "English",
volume = "21",
pages = "583--590",
journal = "Advances in Space Research",
issn = "0273-1177",
publisher = "Elsevier",
number = "4",

}

RIS

TY - JOUR

T1 - Acceleration processes in the course of dayside solar wind-magnetopause interaction

AU - Semenov, V. S.

PY - 1998/1/1

Y1 - 1998/1/1

N2 - Magnetic reconnection is believed to be the dominant coupling process at the Earth's magnetopause. The main features which characterise this process are the conversion of magnetic field energy into plasma energy, an associated change in the magnetic field topology, and the emission of high-energy (suprathermal) charged particles. A review is presented of the development of theoretical concepts of reconnection, starting with steady-state Petschek model. The topics covered include extension of Petschek's model for the time-dependent case, the switch-on and switch-off phases of reconnection, models of flux transfer events (FTEs), steady-state and time-dependent reconnection in compressible plasma, acceleration of plasma through the system of large-amplitude MHD waves, acceleration of charged particles in the diffusion region, the role of the surface waves.

AB - Magnetic reconnection is believed to be the dominant coupling process at the Earth's magnetopause. The main features which characterise this process are the conversion of magnetic field energy into plasma energy, an associated change in the magnetic field topology, and the emission of high-energy (suprathermal) charged particles. A review is presented of the development of theoretical concepts of reconnection, starting with steady-state Petschek model. The topics covered include extension of Petschek's model for the time-dependent case, the switch-on and switch-off phases of reconnection, models of flux transfer events (FTEs), steady-state and time-dependent reconnection in compressible plasma, acceleration of plasma through the system of large-amplitude MHD waves, acceleration of charged particles in the diffusion region, the role of the surface waves.

UR - http://www.scopus.com/inward/record.url?scp=0001428717&partnerID=8YFLogxK

U2 - 10.1016/S0273-1177(97)00967-8

DO - 10.1016/S0273-1177(97)00967-8

M3 - Article

AN - SCOPUS:0001428717

VL - 21

SP - 583

EP - 590

JO - Advances in Space Research

JF - Advances in Space Research

SN - 0273-1177

IS - 4

ER -

ID: 53088300