The 3B/X3 solar flare of 27 February 1992

Active region NOAA 7070 was related to a 3B/X3 solar flare that occurred on February 27, 1992. The soft X-ray flare observations were obtained by the SXT (Soft X-ray Telescope) on board the Yohkoh satellite, and those in Hα from the Udaipur Observatory. The location of the Hα kernels and ribbons, an...

Descripción completa

Guardado en:
Detalles Bibliográficos
Publicado: 2000
Materias:
Magnetohydrostatics (MHS)
Solar activity
Solar flares
Solar magnetic field
solar activity
Acceso en línea:https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00167169_v39_n1_p65_LopezFuentes
http://hdl.handle.net/20.500.12110/paper_00167169_v39_n1_p65_LopezFuentes
Aporte de:
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires
id paper:paper_00167169_v39_n1_p65_LopezFuentes
record_format dspace
spelling paper:paper_00167169_v39_n1_p65_LopezFuentes2023-06-08T14:38:47Z The 3B/X3 solar flare of 27 February 1992 Magnetohydrostatics (MHS) Solar activity Solar flares Solar magnetic field solar activity Active region NOAA 7070 was related to a 3B/X3 solar flare that occurred on February 27, 1992. The soft X-ray flare observations were obtained by the SXT (Soft X-ray Telescope) on board the Yohkoh satellite, and those in Hα from the Udaipur Observatory. The location of the Hα kernels and ribbons, and the shape of soft X-ray loops are compared with the magnetic field model of the AR. Both, observations and model, suggest that the coronal loops are highly sheared before the flare and that the configuration relaxes after energy release. We compute the magnetic free energy at 2x1032 erg; this value is typical for the energy released by solar flares. 2000 https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00167169_v39_n1_p65_LopezFuentes http://hdl.handle.net/20.500.12110/paper_00167169_v39_n1_p65_LopezFuentes
institution Universidad de Buenos Aires
institution_str I-28
repository_str R-134
collection Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA)
topic Magnetohydrostatics (MHS)
Solar activity
Solar flares
Solar magnetic field
solar activity
spellingShingle Magnetohydrostatics (MHS)
Solar activity
Solar flares
Solar magnetic field
solar activity
The 3B/X3 solar flare of 27 February 1992
topic_facet Magnetohydrostatics (MHS)
Solar activity
Solar flares
Solar magnetic field
solar activity
description Active region NOAA 7070 was related to a 3B/X3 solar flare that occurred on February 27, 1992. The soft X-ray flare observations were obtained by the SXT (Soft X-ray Telescope) on board the Yohkoh satellite, and those in Hα from the Udaipur Observatory. The location of the Hα kernels and ribbons, and the shape of soft X-ray loops are compared with the magnetic field model of the AR. Both, observations and model, suggest that the coronal loops are highly sheared before the flare and that the configuration relaxes after energy release. We compute the magnetic free energy at 2x1032 erg; this value is typical for the energy released by solar flares.
title The 3B/X3 solar flare of 27 February 1992
title_short The 3B/X3 solar flare of 27 February 1992
title_full The 3B/X3 solar flare of 27 February 1992
title_fullStr The 3B/X3 solar flare of 27 February 1992
title_full_unstemmed The 3B/X3 solar flare of 27 February 1992
title_sort 3b/x3 solar flare of 27 february 1992
publishDate 2000
url https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00167169_v39_n1_p65_LopezFuentes
http://hdl.handle.net/20.500.12110/paper_00167169_v39_n1_p65_LopezFuentes
_version_ 1768543403308482560

Ejemplares similares