Zobrazeno 1 - 10
of 40
pro vyhledávání: '"Santiago Andrés Triana"'
Publikováno v:
Revista de la Academia Colombiana de Ciencias Exactas, Físicas y Naturales, Vol 23, Iss 86 (2024)
Desarrollamos aquí un algoritmo para realizar experimentos numéricos con el billar de Sinai en su versión clásica, junto con una breve discusión de la precisión y limitaciones de tal algoritmo. Algunos resultados de estos experimentos se presen
Externí odkaz:
https://doaj.org/article/ccc356e1c68e4615b86753e39f7625bb
Publikováno v:
AIP Advances, Vol 13, Iss 7, Pp 075025-075025-14 (2023)
The energy dissipation in a uniform vorticity flow, such as the flow in a precessing spheroid or the one associated with the earth’s free core nutation, is mainly confined to the boundary layers. However, the thinness of the boundary layer renders
Externí odkaz:
https://doaj.org/article/cf72353cbb4a4b028c7cefdc0aea9946
Autor:
Santiago Andrés Triana, Daniel S Zimmerman, Henri-Claude Nataf, Aurélien Thorette, Vedran Lekic, Daniel P Lathrop
Publikováno v:
New Journal of Physics, Vol 16, Iss 11, p 113005 (2014)
Measurement of the differential rotation of the Sunʼs interior is one of the great achievements of helioseismology, providing important constraints for stellar physics. The technique relies on observing and analyzing rotationally-induced splittings
Externí odkaz:
https://doaj.org/article/dbbef55423d546d18f8a3777a8024b2c
Autor:
A. Trinh, Jérémie Vidal, Jérémy Rekier, Felix Gerick, David Cébron, Mathieu Dumberry, Santiago Andrés Triana
Publikováno v:
Surveys in Geophysics
Abstract Changes in the Earth’s rotation are deeply connected to fluid dynamical processes in the outer core. This connection can be explored by studying the associated Earth eigenmodes with periods ranging from nearly diurnal to multi-decadal. It
Publikováno v:
Journal of Geodesy
Journal of Geodesy, Vol. 95, no. 5 (2021) (2021)
Journal of Geodesy, Vol. 95, no. 5 (2021) (2021)
The attempt to quantify the corrections of lunisolar nutation components was made after analysis of six sets of Earth’s orientation parameters (EOP). The deviations of the long-term nutation components about IAU2006/IAU2000A precession–nutation m
Publikováno v:
Journal of Geophysical Research. Solid Earth
Journal of Geophysical Research: Solid Earth
Journal of Geophysical Research: Solid Earth, Vol. 126, no. 4 (2021) (2021)
Journal of Geophysical Research: Solid Earth
Journal of Geophysical Research: Solid Earth, Vol. 126, no. 4 (2021) (2021)
The cause for the damping of the Earth's free core nutation (FCN) and the free inner core nutation eigenmodes has been a matter of debate since the earliest reliable estimations from nutation observations were made available. Numerical studies are di
The cause for the damping of the Earth's Free Core Nutation (FCN) and the Free Inner Core Nutation (FICN) eigenmodes has been a matter of debate since the earliest reliable estimations from nutation observations were made available. Numerical studies
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::df6805c4d67e79d49d559181e43c6488
https://doi.org/10.5194/egusphere-egu21-12492
https://doi.org/10.5194/egusphere-egu21-12492
Magnetic fields inside planetary objects can influence their rotation. This is true, in particular, of terrestrial objects with a metallic liquid core and a self-sustained dynamo such as the Earth, Mercury, Ganymede, etc. and also, to a lesser extent
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::a19bef7ea35a8242abd583a5f81a9f3d
https://doi.org/10.5194/egusphere-egu21-11936
https://doi.org/10.5194/egusphere-egu21-11936
Inertial modes are global oscillations that take place inside rotating objects, such as stars and planets with a fluid core and/or liquid ocean, which result from the restoring effect of the Coriolis force. Experimental studies in laboratory have sho
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::b772aba6a32b8495e13671562e292eb5
https://doi.org/10.5194/epsc2020-853
https://doi.org/10.5194/epsc2020-853
Publikováno v:
The Planetary Science Journal
The Planetary Science Journal, Vol. 1, no. 1, p. 20 (2020)
The Planetary Science Journal, Vol. 1, no. 1, p. 20 (2020)
We compute the inertial modes of a freely rotating two-layer planetary model with an ellipsoidal inviscid fluid core and a perfectly rigid mantle. We present a method to derive analytical formulae for the frequencies of the Free Core Nutation (FCN) a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::bbc605a5440f19b8f754dca3a17f8a7a
http://arxiv.org/abs/2004.08218
http://arxiv.org/abs/2004.08218