The relationship between magnetic field strength and loop lengths in solar coronal active regions

By assuming that coronal active regions are made up of many loops, we investigate the relationship between the average magnetic field strength and loop length for a sample of active regions observed by the Soft X-ray Telescope aboard Yohkoh. We use photospheric magnetic data from the Michelson Doppl...

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Detalles Bibliográficos
Publicado: 2006
Materias:
Sun: corona
Sun: magnetic fields
Michelson Doppler Imager
Soft X-ray emission
Extrapolation
Magnetic field effects
Mathematical models
Space telescopes
Sun
X ray analysis
Solar energy
Acceso en línea:https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00046361_v450_n1_p375_Jain
http://hdl.handle.net/20.500.12110/paper_00046361_v450_n1_p375_Jain
Aporte de:
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires
id paper:paper_00046361_v450_n1_p375_Jain
record_format dspace
spelling paper:paper_00046361_v450_n1_p375_Jain2023-06-08T14:27:40Z The relationship between magnetic field strength and loop lengths in solar coronal active regions Sun: corona Sun: magnetic fields Michelson Doppler Imager Soft X-ray emission Sun: corona Sun: magnetic fields Extrapolation Magnetic field effects Mathematical models Space telescopes Sun X ray analysis Solar energy By assuming that coronal active regions are made up of many loops, we investigate the relationship between the average magnetic field strength and loop length for a sample of active regions observed by the Soft X-ray Telescope aboard Yohkoh. We use photospheric magnetic data from the Michelson Doppler Imager and compute extrapolated field lines that match the observed soft X-ray emission. We compare our results with a previous study and find them to be consistent and a logical extension of such work. Such studies have important implications for solar coronal heating models. © ESO 2006. 2006 https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00046361_v450_n1_p375_Jain http://hdl.handle.net/20.500.12110/paper_00046361_v450_n1_p375_Jain
institution Universidad de Buenos Aires
institution_str I-28
repository_str R-134
collection Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA)
topic Sun: corona
Sun: magnetic fields
Michelson Doppler Imager
Soft X-ray emission
Sun: corona
Sun: magnetic fields
Extrapolation
Magnetic field effects
Mathematical models
Space telescopes
Sun
X ray analysis
Solar energy
spellingShingle Sun: corona
Sun: magnetic fields
Michelson Doppler Imager
Soft X-ray emission
Sun: corona
Sun: magnetic fields
Extrapolation
Magnetic field effects
Mathematical models
Space telescopes
Sun
X ray analysis
Solar energy
The relationship between magnetic field strength and loop lengths in solar coronal active regions
topic_facet Sun: corona
Sun: magnetic fields
Michelson Doppler Imager
Soft X-ray emission
Sun: corona
Sun: magnetic fields
Extrapolation
Magnetic field effects
Mathematical models
Space telescopes
Sun
X ray analysis
Solar energy
description By assuming that coronal active regions are made up of many loops, we investigate the relationship between the average magnetic field strength and loop length for a sample of active regions observed by the Soft X-ray Telescope aboard Yohkoh. We use photospheric magnetic data from the Michelson Doppler Imager and compute extrapolated field lines that match the observed soft X-ray emission. We compare our results with a previous study and find them to be consistent and a logical extension of such work. Such studies have important implications for solar coronal heating models. © ESO 2006.
title The relationship between magnetic field strength and loop lengths in solar coronal active regions
title_short The relationship between magnetic field strength and loop lengths in solar coronal active regions
title_full The relationship between magnetic field strength and loop lengths in solar coronal active regions
title_fullStr The relationship between magnetic field strength and loop lengths in solar coronal active regions
title_full_unstemmed The relationship between magnetic field strength and loop lengths in solar coronal active regions
title_sort relationship between magnetic field strength and loop lengths in solar coronal active regions
publishDate 2006
url https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00046361_v450_n1_p375_Jain
http://hdl.handle.net/20.500.12110/paper_00046361_v450_n1_p375_Jain
_version_ 1768543014362284032

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