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dc.contributor.authorcarrasco, VMS
dc.contributor.authorBertolin, Chiara
dc.contributor.authordominguez castro, fernando
dc.contributor.authorDe Ferri, Lavinia
dc.contributor.authorgallego, mc
dc.contributor.authorvaquero, JM
dc.date.accessioned2021-10-21T07:51:03Z
dc.date.available2021-10-21T07:51:03Z
dc.date.created2020-09-17T09:16:31Z
dc.date.issued2020
dc.identifier.citationSolar Physics. 2020, 295 1-12.en_US
dc.identifier.issn0038-0938
dc.identifier.urihttps://hdl.handle.net/11250/2824348
dc.description.abstractAntonio Colla was a meteorologist and astronomer who made sunspot observations at the Meteorological Observatory of the Parma University (Italy). He carried out his sunspot observations from 1830 to 1843, just after the Dalton Minimum. We have recovered 71 observation days for this observer. Unfortunately, many of these records are qualitative and we could only obtain the number of sunspot groups and/or single sunspots from 25 observations. However, we highlight the importance of these records because Colla is not included in the sunspot group database as an observer and, therefore, neither are his sunspot observations. With regards to the number of groups, the sunspot observations made by Colla are similar to those of several observers of his time. For common observation days, only Stark recorded significantly more groups than Colla. Moreover, we have calculated the sunspot areas and positions from Colla’s sunspot drawings concluding that both areas and positions recorded by this observer seem unreal. Therefore, Colla’s drawings can be interpreted such as sketches showing reliable information on the number of groups but the information on sunspot areas and positions should not be used for scientific purposes.en_US
dc.language.isoengen_US
dc.publisherSpringeren_US
dc.titleSunspot Records by Antonio Colla Just After the Dalton Minimumen_US
dc.typePeer revieweden_US
dc.typeJournal articleen_US
dc.description.versionpublishedVersionen_US
dc.rights.holderThe published version of the article will not be available due to copyright restrictions by Springeren_US
dc.source.pagenumber1-12en_US
dc.source.volume295en_US
dc.source.journalSolar Physicsen_US
dc.identifier.doi10.1007/s11207-020-01678-0
dc.identifier.cristin1830697
cristin.ispublishedtrue
cristin.fulltextoriginal
cristin.qualitycode1


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