Zobrazeno 1 - 10
of 30
pro vyhledávání: '"Carlos Frederico Mendonça Raupp"'
Publikováno v:
Tellus: Series A, Dynamic Meteorology and Oceanography, Vol 72, Iss 1, Pp 1-17 (2020)
Here we have investigated the possibility of an inertio-acoustic wave-mode to be unstable with regards to gravity mode perturbations through non-linear triad interactions in the context of a shallow non-hydrostatic model. We have considered highly tr
Externí odkaz:
https://doaj.org/article/e6b8f7fe3ca6452589ef063d29aa137a
Publikováno v:
Biblioteca Digital de Teses e Dissertações da USPUniversidade de São PauloUSP.
A teoria da perturbação baseada em múltiplas escalas temporais é usada neste trabalho para estudar as interações não lineares entre ondas na atmosfera no contexto das equações primitivas no plano beta-equatorial em coordenadas isobáricas. A
Autor:
Breno Raphaldini, P. L. Silva-Dias, Daniel Y. Takahashi, Carlos Frederico Mendonça Raupp, André Seiji Teruya
Publikováno v:
The European Physical Journal Special Topics. 230:2999-3007
The geomagnetic field is generated by a dynamo process in the Earth’s core and is characterized by a predominant dipole component that has been steadily decreasing in the last few centuries. The physical drivers behind the fluctuations of the geoma
Autor:
Carlos Frederico Mendonça Raupp, Daniel Y. Takahashi, André Seiji Teruya, P. L. Silva-Dias, Breno Raphaldini
Publikováno v:
The European Physical Journal Special Topics. 230:3009-3017
The complex network approach has proved to be a valuable tool for climate and atmospheric sciences in recent years. Here, we show an application of causality ideas in complex networks to infer properties of equatorial wave interactions associated wit
Publikováno v:
Repositório Institucional da USP (Biblioteca Digital da Produção Intelectual)
Universidade de São Paulo (USP)
instacron:USP
Universidade de São Paulo (USP)
instacron:USP
Here the theory of global nonhydrostatic normal modes has been further developed with the analysis of both linear and weakly nonlinear energetics of inertia–acoustic (IA) and inertia–gravity (IG) modes. These energetics are analyzed in the contex
Autor:
Victor C. Mayta, Pedro Leite da Silva Dias, Carlos Frederico Mendonça Raupp, Breno Raphaldini, André Seiji Teruya
The study of tropical tropospheric disturbances has led to important challenges from both observational and theoretical points of view. In particular, the observed wavenumber-frequency spectrum of tropical oscillations, also known as Wheeler-Kiladis
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3428f701c12a1bc452d0923ab6dec84c
https://wcd.copernicus.org/preprints/wcd-2021-21/
https://wcd.copernicus.org/preprints/wcd-2021-21/
Publikováno v:
Repositório Institucional da USP (Biblioteca Digital da Produção Intelectual)
Universidade de São Paulo (USP)
instacron:USP
Universidade de São Paulo (USP)
instacron:USP
Atmospheric blockings are persistent large-scale climate patterns that lock in a geographic position for days and even weeks. In principle, blockings might involve a large number of waves interacting non-linearly, and a conclusive description for the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7aa833f336165ff5a318f540ae699c74
Publikováno v:
Repositório Institucional da USP (Biblioteca Digital da Produção Intelectual)
Universidade de São Paulo (USP)
instacron:USP
Universidade de São Paulo (USP)
instacron:USP
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::fadd2a4dc2752feaa55d11139d584019
Publikováno v:
Proc Math Phys Eng Sci
Repositório Institucional da USP (Biblioteca Digital da Produção Intelectual)
Universidade de São Paulo (USP)
instacron:USP
Repositório Institucional da USP (Biblioteca Digital da Produção Intelectual)
Universidade de São Paulo (USP)
instacron:USP
The geomagnetic field presents several stationary features that are thought to be linked to inhomogeneities at the core–mantle boundary. Particularly important stationary structures of the geomagnetic field are the flux lobes, which appear in pairs
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::78f70988ff7abfcd812fdc985faac81d
Publikováno v:
Repositório Institucional da USP (Biblioteca Digital da Produção Intelectual)
Universidade de São Paulo (USP)
instacron:USP
Universidade de São Paulo (USP)
instacron:USP
The Schwabe cycle of solar activity exhibits modulations and frequency fluctuations on slow time scales of centuries and millennia. Plausible physical explanations for the cause of these long-term variations of the solar cycle are still elusive, with
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6bc15bd1faac40473f36ceaec7bb0325