Large and small solar coronal mass ejections

The large and small Coronal Mass Ejections (CMEs) and mini-CMEs are observed by the Extreme Ultra Violet Imager (EUVI) on the Solar Terrestrial Relation Observatory (STEREO). These eruption events are usually associated with dimming and wave-like brightenings. Here, the images of the full sun on 26...

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Main Authors: N Alipour Rad, H Safari
Format: Article
Language:English
Published: Isfahan University of Technology 2012-06-01
Series:Iranian Journal of Physics Research
Subjects:
Online Access:http://ijpr.iut.ac.ir/browse.php?a_code=A-10-1-562&slc_lang=en&sid=1
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author N Alipour Rad
H Safari
author_facet N Alipour Rad
H Safari
author_sort N Alipour Rad
collection DOAJ
description The large and small Coronal Mass Ejections (CMEs) and mini-CMEs are observed by the Extreme Ultra Violet Imager (EUVI) on the Solar Terrestrial Relation Observatory (STEREO). These eruption events are usually associated with dimming and wave-like brightenings. Here, the images of the full sun on 26 Apr 2008 with STEREO spacecraft (behind) with the cadences of 10 minutes and 150 seconds and pixel size of 1.59 arcsecond in pass band 195 and 171 Å were analyzed. The velocities of the large and small wave-like brightening were 221 km.s-1 and 6 km.s-1, respectively. The zernike moments of events and non-events were computed and these features were fed to the Support Vector Machine (SVM) classifier. Using this method, 697 mini-CMEs on three different regions of solar corona were detected. The number of mini-CMEs was increased when the CMEs occurred. The average velocity of mini-dimmings was 13.8 km.s-1.
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spelling doaj.art-606e5cdde47f4c08ac3a00924e05a46e2022-12-22T01:45:13ZengIsfahan University of TechnologyIranian Journal of Physics Research1682-69572012-06-011212936Large and small solar coronal mass ejectionsN Alipour RadH SafariThe large and small Coronal Mass Ejections (CMEs) and mini-CMEs are observed by the Extreme Ultra Violet Imager (EUVI) on the Solar Terrestrial Relation Observatory (STEREO). These eruption events are usually associated with dimming and wave-like brightenings. Here, the images of the full sun on 26 Apr 2008 with STEREO spacecraft (behind) with the cadences of 10 minutes and 150 seconds and pixel size of 1.59 arcsecond in pass band 195 and 171 Å were analyzed. The velocities of the large and small wave-like brightening were 221 km.s-1 and 6 km.s-1, respectively. The zernike moments of events and non-events were computed and these features were fed to the Support Vector Machine (SVM) classifier. Using this method, 697 mini-CMEs on three different regions of solar corona were detected. The number of mini-CMEs was increased when the CMEs occurred. The average velocity of mini-dimmings was 13.8 km.s-1.http://ijpr.iut.ac.ir/browse.php?a_code=A-10-1-562&slc_lang=en&sid=1sunCMEsmall scale events
spellingShingle N Alipour Rad
H Safari
Large and small solar coronal mass ejections
Iranian Journal of Physics Research
sun
CME
small scale events
title Large and small solar coronal mass ejections
title_full Large and small solar coronal mass ejections
title_fullStr Large and small solar coronal mass ejections
title_full_unstemmed Large and small solar coronal mass ejections
title_short Large and small solar coronal mass ejections
title_sort large and small solar coronal mass ejections
topic sun
CME
small scale events
url http://ijpr.iut.ac.ir/browse.php?a_code=A-10-1-562&slc_lang=en&sid=1
work_keys_str_mv AT nalipourrad largeandsmallsolarcoronalmassejections
AT hsafari largeandsmallsolarcoronalmassejections