Active Region-Based Full-Disc Solar Image Hashing

dc.contributorCzȩstochowa University of Technology
dc.contributorUniversidade Estadual Paulista (UNESP)
dc.date.accessioned2022-04-28T19:29:47Z
dc.date.accessioned2022-12-20T01:13:44Z
dc.date.available2022-04-28T19:29:47Z
dc.date.available2022-12-20T01:13:44Z
dc.date.created2022-04-28T19:29:47Z
dc.date.issued2020-01-01
dc.identifierLecture Notes in Computer Science (including subseries Lecture Notes in Artificial Intelligence and Lecture Notes in Bioinformatics), v. 12416 LNAI, p. 19-30.
dc.identifier1611-3349
dc.identifier0302-9743
dc.identifierhttp://hdl.handle.net/11449/221614
dc.identifier10.1007/978-3-030-61534-5_2
dc.identifier2-s2.0-85096534236
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/5401743
dc.description.abstractThe main components of the Solar activity are solar flares, coronal mass ejections, high-speed solar wind, and solar energetic particles. Solar flares impact the Earth when they occur on the side facing our planet.
dc.languageeng
dc.relationLecture Notes in Computer Science (including subseries Lecture Notes in Artificial Intelligence and Lecture Notes in Bioinformatics)
dc.sourceScopus
dc.subjectCBIR
dc.subjectSolar activity analysis
dc.subjectSolar hash
dc.subjectSolar image description
dc.titleActive Region-Based Full-Disc Solar Image Hashing
dc.typeActas de congresos


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