Faculae Cancel out on the Surfaces of Active Suns (vol 934, L23, 2022)

Basit Öğe Kaydı
dc.authoridIsik, Emre/0000-0001-6163-0653
dc.authoridKrishnamurthy, Sowmya/0000-0002-3243-1230
dc.authoridShapiro, Alexander/0000-0002-8842-5403
dc.authoridNemec, Nina-Elisabeth/0000-0001-6090-1247
dc.contributor.authorNemec, N. -E.
dc.contributor.authorShapiro, A. I.
dc.contributor.authorIsik, E.
dc.contributor.authorSowmya, K.
dc.contributor.authorSolanki, S. K.
dc.contributor.authorKrivova, N. . A.
dc.contributor.authorCameron, R. H.
dc.date.accessioned2025-02-20T08:42:13Z
dc.date.available2025-02-20T08:42:13Z
dc.date.issued2022
dc.departmentTürk-Alman Üniversitesien_US
dc.description.abstractIn Figures 1 and 2(a) the values given on the x- and y-axes, as well as the values on the x-axis given in Figure 2(b), do not correspond to the disk area coverage in percent. The values must be multiplied by 10 in order to be in units of percent of the solar/stellar disk. These plots were solely for demonstration purposes of the change in the area coverages with increasing stellar activity and do not affect the following results and conclusions.en
dc.identifier.doi10.3847/2041-8213/ac8b70
dc.identifier.issn2041-8205
dc.identifier.issn2041-8213
dc.identifier.issue1en_US
dc.identifier.scopus2-s2.0-85139076503
dc.identifier.scopusqualityQ1
dc.identifier.urihttps://doi.org/10.3847/2041-8213/ac8b70
dc.identifier.urihttps://hdl.handle.net/20.500.12846/1559
dc.identifier.volume936en_US
dc.identifier.wosWOS:000849098400001
dc.identifier.wosqualityQ1
dc.indekslendigikaynakWeb of Science
dc.indekslendigikaynakScopus
dc.language.isoen
dc.publisherIop Publishing Ltd
dc.relation.ispartofAstrophysical Journal Letters
dc.relation.publicationcategoryDiğer
dc.rightsinfo:eu-repo/semantics/openAccess
dc.snmzKA_WOS_20250220
dc.titleFaculae Cancel out on the Surfaces of Active Suns (vol 934, L23, 2022)
dc.typeCorrection

Dosyalar

Koleksiyon

WoS İndeksli Yayınlar Koleksiyonu
Scopus İndeksli Yayınlar Koleksiyonu