Théorie mathématique des phénomènes thermiques produits par la radiation solaire

E538060
book climatology treatise scientific work

Théorie mathématique des phénomènes thermiques produits par la radiation solaire is a foundational scientific work by Milutin Milanković that mathematically analyzes how variations in solar radiation drive Earth’s climate and long-term temperature changes.

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Théorie mathématique des phénomènes thermiques produits par la radiation solaire canonical 1

Statements (42)

Predicate Object
instanceOf book ⓘ
climatology treatise ⓘ
scientific work ⓘ
academicDiscipline geophysics ⓘ
planetary science ⓘ
aim to explain climate variations from solar radiation changes ⓘ
associatedWith Milankovitch cycles NERFINISHED ⓘ
author Milutin Milanković NERFINISHED ⓘ
consequence provided theoretical basis for orbital-climate links ⓘ
contributor Milutin Milanković NERFINISHED ⓘ
describes influence of solar radiation on climate ⓘ
long-term climate variations ⓘ
mathematical analysis of insolation ⓘ
thermal phenomena on Earth ⓘ
field astronomy ⓘ
climatology ⓘ
mathematical physics ⓘ
focusesOn Earth’s temperature distribution ⓘ
climate forcing by orbital factors ⓘ
variations in solar radiation ⓘ
genre scientific monograph ⓘ
hasAuthorNationality Serbian ⓘ
impact shaped understanding of long-term climate change ⓘ
influenced Milankovitch theory of climate ⓘ
paleoclimate studies ⓘ
language French ⓘ
mainSubject Earth climate ⓘ
long-term temperature changes ⓘ
solar radiation ⓘ
originalTitle Théorie mathématique des phénomènes thermiques produits par la radiation solaire NERFINISHED ⓘ
publicationCentury 20th century ⓘ
relatedTo insolation curves ⓘ
orbital mechanics ⓘ
paleoclimatology ⓘ
status foundational work in climate theory ⓘ
topic energy balance of Earth ⓘ
solar forcing of climate ⓘ
temperature response to radiation changes ⓘ
typeOfWork foundational climate science work ⓘ
usesMethod differential equations ⓘ
mathematical modeling ⓘ
quantitative analysis of insolation ⓘ

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Milutin Milanković → notableWork → Théorie mathématique des phénomènes thermiques produits par la radiation solaire ⓘ