Relationships between CME's and prominences

B. Schmieder; L. van Driel-Gesztelyi; G. Aulanier; P. Démoulin; B. Thompson; C. De Forest; J. E. Wiik; C. Saint Cyr; J. C. Vial

doi:10.1016/S0273-1177(02)00211-9

Relationships between CME's and prominences

B. Schmieder
, L. van Driel-Gesztelyi
, G. Aulanier
, P. Démoulin
, B. Thompson
, C. De Forest
, J. E. Wiik
, C. Saint Cyr
, J. C. Vial

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

Abstract

We have studied the erupting prominces which were associated with coronal mass ejections during a series of campaigns involving both spacecraft and ground-based observatories. The evolution of the physical conditions within the prominences was established from Hα and magnetic field observations. Particular attention ahs been paid to the presence of mixed amgnetic polarity in the filament channel, the evolution of the shear of the large-scale magnetic field, and the existence of multiple magnetic inversion lines. We conclude that reconnection of large-scale coronal magnetic fields is responsible for both the CME and filament eruption.

Original language	English
Pages (from-to)	1451-1460
Number of pages	10
Journal	Advances in Space Research
Volume	29
Issue number	10
DOIs	https://doi.org/10.1016/S0273-1177(02)00211-9
Publication status	Published - 1 Jan 2002
Externally published	Yes

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10.1016/S0273-1177(02)00211-9

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title = "Relationships between CME's and prominences",

abstract = "We have studied the erupting prominces which were associated with coronal mass ejections during a series of campaigns involving both spacecraft and ground-based observatories. The evolution of the physical conditions within the prominences was established from Hα and magnetic field observations. Particular attention ahs been paid to the presence of mixed amgnetic polarity in the filament channel, the evolution of the shear of the large-scale magnetic field, and the existence of multiple magnetic inversion lines. We conclude that reconnection of large-scale coronal magnetic fields is responsible for both the CME and filament eruption.",

author = "B. Schmieder and \{van Driel-Gesztelyi\}, L. and G. Aulanier and P. D{\'e}moulin and B. Thompson and \{De Forest\}, C. and Wiik, \{J. E.\} and \{Saint Cyr\}, C. and Vial, \{J. C.\}",

year = "2002",

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doi = "10.1016/S0273-1177(02)00211-9",

language = "English",

volume = "29",

pages = "1451--1460",

journal = "Advances in Space Research",

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TY - JOUR

T1 - Relationships between CME's and prominences

AU - Schmieder, B.

AU - van Driel-Gesztelyi, L.

AU - Aulanier, G.

AU - Démoulin, P.

AU - Thompson, B.

AU - De Forest, C.

AU - Wiik, J. E.

AU - Saint Cyr, C.

AU - Vial, J. C.

PY - 2002/1/1

Y1 - 2002/1/1

N2 - We have studied the erupting prominces which were associated with coronal mass ejections during a series of campaigns involving both spacecraft and ground-based observatories. The evolution of the physical conditions within the prominences was established from Hα and magnetic field observations. Particular attention ahs been paid to the presence of mixed amgnetic polarity in the filament channel, the evolution of the shear of the large-scale magnetic field, and the existence of multiple magnetic inversion lines. We conclude that reconnection of large-scale coronal magnetic fields is responsible for both the CME and filament eruption.

AB - We have studied the erupting prominces which were associated with coronal mass ejections during a series of campaigns involving both spacecraft and ground-based observatories. The evolution of the physical conditions within the prominences was established from Hα and magnetic field observations. Particular attention ahs been paid to the presence of mixed amgnetic polarity in the filament channel, the evolution of the shear of the large-scale magnetic field, and the existence of multiple magnetic inversion lines. We conclude that reconnection of large-scale coronal magnetic fields is responsible for both the CME and filament eruption.

U2 - 10.1016/S0273-1177(02)00211-9

DO - 10.1016/S0273-1177(02)00211-9

M3 - Article

AN - SCOPUS:0036577528

SN - 0273-1177

VL - 29

SP - 1451

EP - 1460

JO - Advances in Space Research

JF - Advances in Space Research

IS - 10

ER -

Relationships between CME's and prominences

Abstract

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