yesThis paper presents a new method that provides the means to detect sunspots on full-disk solar images recorded by the Solar Diameter Imager and Surface Mapper (SODISM) on the PICARD satellite. The method is a totally automated detection process that achieves a sunspot recognition rate of 97.6%. The number of sunspots detected by this method strongly agrees with the NOAA catalogue. The sunspot areas calculated by this method have a 99% correlation with SOHO over the same period, and thus help to calculate the filling factor for wavelength (W.L.) 607nm
37 pages, 14 figures, more information at http://picard.projet.latmos.ipsl.fr/International audience...
37 pages, 14 figures, more information at http://picard.projet.latmos.ipsl.fr/International audience...
This research modifies and expands previous work by Spahr in 2014 to automatically identify and clas...
International audienceThe calculated filling factors (FFs) for a feature reflect the fraction of the...
Solar images are one of the most important sources of available information on the current state and...
yesThe surface of the sun often shows visible sunspots which are located in magnetically active reg...
International audienceThe calculated filling factors (FFs) for a feature reflect the fraction of the...
International audienceThe calculated filling factors (FFs) for a feature reflect the fraction of the...
International audienceThe Solar Diameter Imager and Surface Mapper’s (SODISM) recording of data on t...
International audienceThe Solar Diameter Imager and Surface Mapper’s (SODISM) recording of data on t...
International audienceThe Solar Diameter Imager and Surface Mapper’s (SODISM) recording of data on t...
37 pages, 14 figures, more information at http://picard.projet.latmos.ipsl.fr/International audience...
37 pages, 14 figures, more information at http://picard.projet.latmos.ipsl.fr/International audience...
A new robust technique is presented for automated identification of sunspots on full-disk white-lig...
37 pages, 14 figures, more information at http://picard.projet.latmos.ipsl.fr/International audience...
37 pages, 14 figures, more information at http://picard.projet.latmos.ipsl.fr/International audience...
37 pages, 14 figures, more information at http://picard.projet.latmos.ipsl.fr/International audience...
This research modifies and expands previous work by Spahr in 2014 to automatically identify and clas...
International audienceThe calculated filling factors (FFs) for a feature reflect the fraction of the...
Solar images are one of the most important sources of available information on the current state and...
yesThe surface of the sun often shows visible sunspots which are located in magnetically active reg...
International audienceThe calculated filling factors (FFs) for a feature reflect the fraction of the...
International audienceThe calculated filling factors (FFs) for a feature reflect the fraction of the...
International audienceThe Solar Diameter Imager and Surface Mapper’s (SODISM) recording of data on t...
International audienceThe Solar Diameter Imager and Surface Mapper’s (SODISM) recording of data on t...
International audienceThe Solar Diameter Imager and Surface Mapper’s (SODISM) recording of data on t...
37 pages, 14 figures, more information at http://picard.projet.latmos.ipsl.fr/International audience...
37 pages, 14 figures, more information at http://picard.projet.latmos.ipsl.fr/International audience...
A new robust technique is presented for automated identification of sunspots on full-disk white-lig...
37 pages, 14 figures, more information at http://picard.projet.latmos.ipsl.fr/International audience...
37 pages, 14 figures, more information at http://picard.projet.latmos.ipsl.fr/International audience...
37 pages, 14 figures, more information at http://picard.projet.latmos.ipsl.fr/International audience...
This research modifies and expands previous work by Spahr in 2014 to automatically identify and clas...