Three-dimensional reconstruction of eccrine poroma vessels seen under reflectance confocal microscopy

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dc.article.number065005
dc.contributor.authorHidalgo L.
dc.contributor.authorHanlon K.L.
dc.contributor.authorCorrea-Selm L.
dc.contributor.authorVillaseca M.A.
dc.contributor.authorCarrasco K.
dc.contributor.authorPeirano D.
dc.contributor.authorDonoso F.
dc.contributor.authorUribe P.
dc.contributor.authorNavarrete-Dechent C.
dc.date.accessioned2025-05-01T10:31:27Z
dc.date.available2025-05-01T10:31:27Z
dc.date.issued2023
dc.description.abstract© 2023 IOP Publishing Ltd.Because solar light, from Earth perspective, a curve is drawn in Moon’s surface that separates its dark side from the illuminated one. This curve is known as the terminator curve. In this article we prove, using direct and indirect methods, that the terminator curve corresponds to an ellipse. This is demonstrated using mathematical concepts and photographs of the Moon that are analysed with a geometrical software. Using this information, we also show how to calculate the illuminated fraction area of the Moon depending on its day of rotation. We obtain excellent approximations regarding the values given by computational systems. We discuss the results of considering the Moon as a flat disk or like a sphere. We analyse the technical difficulties of the process and the mathematical tools needed for more precise calculations. We also put in context this demonstration of the ellipticity of the terminator curve for any interior planet illuminated by a central star of any planetary system, seen from a outsider planet, the case in which the phases are more noticeable. Finally we extend the previous calculations to analyse the illuminated percentage of the inner planets Mercury and Venus, obtaining excellent results in the case of Venus.
dc.description.funderANID-Millennium Science Initiative Program
dc.format.extent13 páginas
dc.fuente.origenScopus
dc.identifier.doi10.1111/exd.14936
dc.identifier.eisbn978-1-5106-5352-8
dc.identifier.eissn2641-435X
dc.identifier.isbn978-1-5106-5351-1
dc.identifier.issn16000625 09066705
dc.identifier.pubmedid40243597
dc.identifier.scieloidS0718-69242020000300109
dc.identifier.scopusidSCOPUS_ID:85173057277
dc.identifier.urihttps://doi.org/10.1111/exd.14936
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/103757
dc.identifier.wosidWOS:001082877200001
dc.information.autorucEscuela de Medicina; Navarrete Dechent Cristian Patricio; 0000-0003-4040-3640; 156251
dc.issue.numero3
dc.language.isoen
dc.nota.accesoContenido parcial
dc.pagina.final1393
dc.pagina.inicio1385
dc.publisherSpringer International Publishing
dc.relation.ispartofInternational Conference on Intelligent User Interfaces (30a. : 2025)
dc.revistaExperimental Dermatology
dc.rightsacceso restringido
dc.subjectellipse
dc.subjectilluminated area
dc.subjectMoon’s terminator
dc.subject.ddc510
dc.subject.deweyMatemática física y químicaes_ES
dc.subject.ods03 Good health and well-being
dc.subject.odspa03 Salud y bienestar
dc.titleThree-dimensional reconstruction of eccrine poroma vessels seen under reflectance confocal microscopy
dc.typeartículo
dc.volumen70
sipa.codpersvinculados156251
sipa.indexScopus
sipa.trazabilidadCarga WOS-SCOPUS;01-05-2025
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