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Ritmos e ciclos no clima local de Cuiabá/Várzea Grande - MT : uma análise secular (1912 a 2012)
(Universidade Federal de Mato GrossoBrasilInstituto de Ciências Humanas e Sociais (ICHS) – RondonópolisUFMT CUR - RondonopólisPrograma de Pós-Graduação em Geografia – Rondonópolis, 2015-11-13)
The main objective was to analyze trends and climatic oscillations in Cuiabá / Várzea
Grande. The specific objectives were: to analyze the climate pace in Cuiabá / Várzea Grande in
the period 1912-2012; study the ...
Possible effects of secular resonances in Phobos and Triton
(Elsevier B.V., 2014)
Secular effects of ultralight dark matter on binary pulsars
(American Physical Society, 2020-03)
Dark matter (DM) can consist of very light bosons behaving as a classical scalar field that experiences coherent oscillations. The presence of this DM field would perturb the dynamics of celestial bodies, either because ...
New historical archeointensity data from Brazil: Evidence for a large regional non-dipole field contribution over the past few centuries
(ELSEVIER SCIENCE BV, 2011)
We report new archeointensity data obtained from the analyses of baked clay elements (architectural and kiln brick fragments) sampled in Southeast Brazil and historically and/or archeologically dated between the end of the ...
Archeointensity in Northeast Brazil over the past five centuries
(ELSEVIER SCIENCE BV, 2010)
This study presents the first archeointensity results from Northeast Brazil obtained from 14 groups of architectural brick fragments sampled in the city of Salvador, Bahia State (13 degrees S, 38.5 degrees W) and dated ...
New historical archeointensity data from Brazil: Evidence for a large regional non-dipole field contribution over the past few centuries
(2011-06)
We report new archeointensity data obtained from the analyses of baked clay elements (architectural and kiln
brick fragments) sampled in Southeast Brazil and historically and/or archeologically dated between the end of
the ...
Sobre a dinâmica de rotação de um planeta através de um sistema médio
(Universidade Estadual Paulista (Unesp), 2013)
Let us consider a non-spherical body (usually a planet C1) which is in a keplerian orbit around C3 (Sun). We still consider a massive satellite (C2) around the target planet (C1). Our main task is to investigate the secular ...
Epidemiology of holoprosencephaly: Prevalence and risk factors
(Wiley-Liss, 2020)