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Please use this identifier to cite or link to this item: https://research.matf.bg.ac.rs/handle/123456789/2886
DC FieldValueLanguage
dc.contributor.authorŠegan, Stevoen_US
dc.contributor.authorMarčeta, Dušanen_US
dc.date.accessioned2025-11-05T11:36:08Z-
dc.date.available2025-11-05T11:36:08Z-
dc.date.issued2010-
dc.identifier.urihttps://research.matf.bg.ac.rs/handle/123456789/2886-
dc.description.abstractIn this paper we have examined possibilities for preserving and improving the total density model of the Earth’s neutral thermosphere TD88 (Sehnal and Pospíšilová 1988) via modelling differences between TD88 and NRLMSISE-00 (Picone et al. 2002), which is used as a control model. It is shown that these residuals can be approximated with polyharmonic function. Starting from this we have developed the mathematical model of the residuals to identify their origin and possibilities to improve the TD88 model itself.en_US
dc.language.isoenen_US
dc.publisherBeograd : Matematički fakulteten_US
dc.relation.ispartofSerbian Astronomical Journalen_US
dc.subjectEarthen_US
dc.titlePossibilities of improving the TD88 atmospheric total density modelen_US
dc.typeArticleen_US
dc.identifier.doi10.2298/saj1081057s-
dc.identifier.scopus2-s2.0-78650438085-
dc.identifier.urlhttp://dx.doi.org/10.2298/saj1081057s-
dc.contributor.affiliationAstronomyen_US
dc.relation.issn1450-698Xen_US
dc.description.rankM24en_US
dc.relation.firstpage57en_US
dc.relation.lastpage61en_US
dc.relation.issue181en_US
item.openairetypeArticle-
item.fulltextNo Fulltext-
item.languageiso639-1en-
item.cerifentitytypePublications-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.grantfulltextnone-
crisitem.author.deptAstronomy-
crisitem.author.orcid0000-0003-4706-4602-
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