Standard

Physical Processes of Meso-Scale, Dynamic Auroral Forms. / Forsyth, C.; Sergeev, V. A.; Henderson, M. G.; Nishimura, Y.; Gallardo-Lacourt, B.

в: Space Science Reviews, Том 216, № 4, 46, 20.04.2020.

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

Harvard

Forsyth, C, Sergeev, VA, Henderson, MG, Nishimura, Y & Gallardo-Lacourt, B 2020, 'Physical Processes of Meso-Scale, Dynamic Auroral Forms', Space Science Reviews, Том. 216, № 4, 46. https://doi.org/10.1007/s11214-020-00665-y

APA

Forsyth, C., Sergeev, V. A., Henderson, M. G., Nishimura, Y., & Gallardo-Lacourt, B. (2020). Physical Processes of Meso-Scale, Dynamic Auroral Forms. Space Science Reviews, 216(4), [46]. https://doi.org/10.1007/s11214-020-00665-y

Vancouver

Forsyth C, Sergeev VA, Henderson MG, Nishimura Y, Gallardo-Lacourt B. Physical Processes of Meso-Scale, Dynamic Auroral Forms. Space Science Reviews. 2020 Апр. 20;216(4). 46. https://doi.org/10.1007/s11214-020-00665-y

Author

Forsyth, C. ; Sergeev, V. A. ; Henderson, M. G. ; Nishimura, Y. ; Gallardo-Lacourt, B. / Physical Processes of Meso-Scale, Dynamic Auroral Forms. в: Space Science Reviews. 2020 ; Том 216, № 4.

BibTeX

@article{269b154010eb4294a379c8fbeeafde25,
title = "Physical Processes of Meso-Scale, Dynamic Auroral Forms",
abstract = "Meso-scale auroral forms, such as poleward boundary intensifications, streamers, omega bands, beads and giant undulations, are manifestations of dynamic processes in the magnetosphere driven, to a large part, by plasma instabilities in the magnetotail. New observations from ground- and space-based instrumentation and theoretical treatments are giving us a clearer view of some of the physical processes behind these auroral forms. However, questions remain as to how some of these observations should be interpreted, given uncertainties in mapping auroral features to locations in the magnetotatil and due to the significant overlap in the results from a variety of models of different plasma instabilities. We provide an overview of recent results in the field and seek to clarify some of the remaining questions with regards to what drives some of the largest and most dynamic auroral forms.",
keywords = "Auroral beads, Auroral streamers, Giant undulations, Magnetic mapping, Magnetosphere ionosphere coupling, Magnetotail, Meso-scale aurora, Omega bands, Plasma instabilities, Poleward boundary intensifications, Torches, LARGE-SCALE UNDULATIONS, POLAR-CAP FLOWS, PLASMA SHEET FLOW, POLEWARD BOUNDARY INTENSIFICATIONS, HIGH-SPEED FLOWS, SUBSTORM CURRENT WEDGE, FIELD CURRENT INSTABILITY, MAGNETIC-FIELD, KINETIC BALLOONING/INTERCHANGE INSTABILITY, EARTHWARD FLOW BURSTS",
author = "C. Forsyth and Sergeev, {V. A.} and Henderson, {M. G.} and Y. Nishimura and B. Gallardo-Lacourt",
year = "2020",
month = apr,
day = "20",
doi = "10.1007/s11214-020-00665-y",
language = "English",
volume = "216",
journal = "Space Science Reviews",
issn = "0038-6308",
publisher = "Springer Nature",
number = "4",

}

RIS

TY - JOUR

T1 - Physical Processes of Meso-Scale, Dynamic Auroral Forms

AU - Forsyth, C.

AU - Sergeev, V. A.

AU - Henderson, M. G.

AU - Nishimura, Y.

AU - Gallardo-Lacourt, B.

PY - 2020/4/20

Y1 - 2020/4/20

N2 - Meso-scale auroral forms, such as poleward boundary intensifications, streamers, omega bands, beads and giant undulations, are manifestations of dynamic processes in the magnetosphere driven, to a large part, by plasma instabilities in the magnetotail. New observations from ground- and space-based instrumentation and theoretical treatments are giving us a clearer view of some of the physical processes behind these auroral forms. However, questions remain as to how some of these observations should be interpreted, given uncertainties in mapping auroral features to locations in the magnetotatil and due to the significant overlap in the results from a variety of models of different plasma instabilities. We provide an overview of recent results in the field and seek to clarify some of the remaining questions with regards to what drives some of the largest and most dynamic auroral forms.

AB - Meso-scale auroral forms, such as poleward boundary intensifications, streamers, omega bands, beads and giant undulations, are manifestations of dynamic processes in the magnetosphere driven, to a large part, by plasma instabilities in the magnetotail. New observations from ground- and space-based instrumentation and theoretical treatments are giving us a clearer view of some of the physical processes behind these auroral forms. However, questions remain as to how some of these observations should be interpreted, given uncertainties in mapping auroral features to locations in the magnetotatil and due to the significant overlap in the results from a variety of models of different plasma instabilities. We provide an overview of recent results in the field and seek to clarify some of the remaining questions with regards to what drives some of the largest and most dynamic auroral forms.

KW - Auroral beads

KW - Auroral streamers

KW - Giant undulations

KW - Magnetic mapping

KW - Magnetosphere ionosphere coupling

KW - Magnetotail

KW - Meso-scale aurora

KW - Omega bands

KW - Plasma instabilities

KW - Poleward boundary intensifications

KW - Torches

KW - LARGE-SCALE UNDULATIONS

KW - POLAR-CAP FLOWS

KW - PLASMA SHEET FLOW

KW - POLEWARD BOUNDARY INTENSIFICATIONS

KW - HIGH-SPEED FLOWS

KW - SUBSTORM CURRENT WEDGE

KW - FIELD CURRENT INSTABILITY

KW - MAGNETIC-FIELD

KW - KINETIC BALLOONING/INTERCHANGE INSTABILITY

KW - EARTHWARD FLOW BURSTS

UR - http://www.scopus.com/inward/record.url?scp=85083642526&partnerID=8YFLogxK

UR - https://www.mendeley.com/catalogue/247c7cdc-de84-3ccb-8f01-414a22131885/

U2 - 10.1007/s11214-020-00665-y

DO - 10.1007/s11214-020-00665-y

M3 - Review article

AN - SCOPUS:85083642526

VL - 216

JO - Space Science Reviews

JF - Space Science Reviews

SN - 0038-6308

IS - 4

M1 - 46

ER -

ID: 53464636