Erupting flux rope, rising x-ray source and a slow CME on 16 april 2002

A long-duration event (LDE) linked to a slow coronal mass ejection (CME) was observed at the NW solar limb on 16 April 2002. A multiwavelength analysis involving TRACE, RHESSI, SOHO/EIT, CDS and LASCO observations as well as magnetic modelling (SOHO/MDI) provided several new pieces of evidence suppo...

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Detalles Bibliográficos
Publicado: 2005
Materias:
Magnetic field effects
Mathematical models
X ray analysis
CDS spectrograph
Mass motions
X-ray source
Astrophysics
Acceso en línea:https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_03796566_v_n600_p785_Goff
http://hdl.handle.net/20.500.12110/paper_03796566_v_n600_p785_Goff
Aporte de:
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires
id paper:paper_03796566_v_n600_p785_Goff
record_format dspace
spelling paper:paper_03796566_v_n600_p785_Goff2023-06-08T15:40:45Z Erupting flux rope, rising x-ray source and a slow CME on 16 april 2002 Magnetic field effects Mathematical models X ray analysis CDS spectrograph Mass motions X-ray source Astrophysics A long-duration event (LDE) linked to a slow coronal mass ejection (CME) was observed at the NW solar limb on 16 April 2002. A multiwavelength analysis involving TRACE, RHESSI, SOHO/EIT, CDS and LASCO observations as well as magnetic modelling (SOHO/MDI) provided several new pieces of evidence supporting the classical LDE/CME scenario: the event started with the eruption of a filament, which was found to have helical mass motions when crossing the CDS spectrograph slit situated 50" above the limb. Rising with the filament, a coronal X-ray source was identified as a plasmoid originating from the interaction between upward reconnection outflow and the closed magnetic structure of the erupting filament. We also found down-flows of plasma in hot, newly reconnected flare loops and an exponential acceleration of the erupting filament between the TRACE and LASCO/C2 fields of view. 2005 https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_03796566_v_n600_p785_Goff http://hdl.handle.net/20.500.12110/paper_03796566_v_n600_p785_Goff
institution Universidad de Buenos Aires
institution_str I-28
repository_str R-134
collection Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA)
topic Magnetic field effects
Mathematical models
X ray analysis
CDS spectrograph
Mass motions
X-ray source
Astrophysics
spellingShingle Magnetic field effects
Mathematical models
X ray analysis
CDS spectrograph
Mass motions
X-ray source
Astrophysics
Erupting flux rope, rising x-ray source and a slow CME on 16 april 2002
topic_facet Magnetic field effects
Mathematical models
X ray analysis
CDS spectrograph
Mass motions
X-ray source
Astrophysics
description A long-duration event (LDE) linked to a slow coronal mass ejection (CME) was observed at the NW solar limb on 16 April 2002. A multiwavelength analysis involving TRACE, RHESSI, SOHO/EIT, CDS and LASCO observations as well as magnetic modelling (SOHO/MDI) provided several new pieces of evidence supporting the classical LDE/CME scenario: the event started with the eruption of a filament, which was found to have helical mass motions when crossing the CDS spectrograph slit situated 50" above the limb. Rising with the filament, a coronal X-ray source was identified as a plasmoid originating from the interaction between upward reconnection outflow and the closed magnetic structure of the erupting filament. We also found down-flows of plasma in hot, newly reconnected flare loops and an exponential acceleration of the erupting filament between the TRACE and LASCO/C2 fields of view.
title Erupting flux rope, rising x-ray source and a slow CME on 16 april 2002
title_short Erupting flux rope, rising x-ray source and a slow CME on 16 april 2002
title_full Erupting flux rope, rising x-ray source and a slow CME on 16 april 2002
title_fullStr Erupting flux rope, rising x-ray source and a slow CME on 16 april 2002
title_full_unstemmed Erupting flux rope, rising x-ray source and a slow CME on 16 april 2002
title_sort erupting flux rope, rising x-ray source and a slow cme on 16 april 2002
publishDate 2005
url https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_03796566_v_n600_p785_Goff
http://hdl.handle.net/20.500.12110/paper_03796566_v_n600_p785_Goff
_version_ 1768544599098261504

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