FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2044528902> ?p ?o ?g. }

• W2044528902 endingPage "351" @default.
• W2044528902 startingPage "337" @default.
• W2044528902 abstract "The atmospheric pressure effects on the Earth's Free Core Nutation (FCN) and some forced nutations are evaluated numerically from the global pressure field provided by the European Center for Medium Range Weather Forecast (ECMWF) on the Earth's solid surface using a 12-year long pressure data set sampled every 6 h on a (1.125°×1.125°) grid. Our model incorporates both the pressure and gravitational torques from the atmosphere as well as the elastic deformational effects induced by atmospheric loading. The pressure torque is computed from the surface pressure field acting on the Earth's topography and the antagonist gravitational torque is also dependent on this pressure field but acting on the gravitational equipotential surface (assuming vertical hydrostatic equilibrium between density and pressure). The response of the oceans to pressure excitation is approximated by the static ocean model which is different from the classical non-inverted barometer (NIBO) and the inverted barometer (IBO) hypotheses and depends on the degree of the spherical harmonic decomposition of the pressure field. The most efficient term in perturbing the nutations is the S1 solar barometric tide of thermal origin which induces a contribution to the prograde annual nutation of gravitational origin. Seasonal modulations of S1 also appear clearly which cause perturbations to other nutations. We show that the contributions to the nutation values are ranging from a few tenths of a milliarcsecond up to the milliarcsecond for the annual prograde term and therefore are close to the lower bounds of the values from a previous calculation by Dehant et al. [Dehant, V., Bizouard, Ch., Hinderer, J., Legros, H., Lefftz, M., 1996. On atmospheric pressure perturbation on precession and nutations. Phys. Earth Planet. Interiors 96, 25–39.] based on the 20-yr-old S1 pressure field from Haurwitz and Cowley [Haurwitz, B., Cowley, A.D., 1973. The diurnal and semidiurnal barometric oscillations, global distribution and annual variation. Pageoph. 102, 193–222.] and speculations on its amplitude modulation. These effects are therefore not negligible and this study points out the importance of atmospheric pressure corrections on the gravitational nutations of lunisolar origin. We also estimate the excitation power available from the atmospheric pressure, gravitational torques and elastic surface loading to explain the mean observed FCN amplitude as derived from VLBI (Very Long Baseline Interferometry) observations. It is suggested that the atmosphere is a good candidate for randomly exciting this free rotational mode." @default.
• W2044528902 created "2016-06-24" @default.
• W2044528902 creator A5007872270 @default.
• W2044528902 creator A5058767285 @default.
• W2044528902 creator A5063434251 @default.
• W2044528902 creator A5072665303 @default.
• W2044528902 creator A5083889308 @default.
• W2044528902 date "1998-04-01" @default.
• W2044528902 modified "2023-10-13" @default.
• W2044528902 title "Influence of atmospheric pressure on the Free Core Nutation, precession and some forced nutational motions of the Earth" @default.
• W2044528902 cites W1485286469 @default.
• W2044528902 cites W1618333098 @default.
• W2044528902 cites W1649249565 @default.
• W2044528902 cites W175872267 @default.
• W2044528902 cites W1968945990 @default.
• W2044528902 cites W1973567654 @default.
• W2044528902 cites W1974692522 @default.
• W2044528902 cites W1976132358 @default.
• W2044528902 cites W1982304204 @default.
• W2044528902 cites W1984676644 @default.
• W2044528902 cites W1988134363 @default.
• W2044528902 cites W2005144790 @default.
• W2044528902 cites W2008563135 @default.
• W2044528902 cites W2015466429 @default.
• W2044528902 cites W2024021891 @default.
• W2044528902 cites W2044793209 @default.
• W2044528902 cites W2046851173 @default.
• W2044528902 cites W2048442088 @default.
• W2044528902 cites W2050238048 @default.
• W2044528902 cites W2062226426 @default.
• W2044528902 cites W2073252683 @default.
• W2044528902 cites W2078559991 @default.
• W2044528902 cites W2081581591 @default.
• W2044528902 cites W2084247824 @default.
• W2044528902 cites W2090161055 @default.
• W2044528902 cites W2094767824 @default.
• W2044528902 cites W2096871726 @default.
• W2044528902 cites W2106915366 @default.
• W2044528902 cites W2117726877 @default.
• W2044528902 cites W2123530499 @default.
• W2044528902 cites W2125604824 @default.
• W2044528902 cites W2130827352 @default.
• W2044528902 cites W2141163948 @default.
• W2044528902 cites W2152353746 @default.
• W2044528902 cites W2157829102 @default.
• W2044528902 cites W2162761340 @default.
• W2044528902 cites W2163944757 @default.
• W2044528902 cites W3112703728 @default.
• W2044528902 cites W4242741598 @default.
• W2044528902 doi "https://doi.org/10.1016/s0031-9201(97)00100-3" @default.
• W2044528902 hasPublicationYear "1998" @default.
• W2044528902 type Work @default.
• W2044528902 sameAs 2044528902 @default.
• W2044528902 citedByCount "24" @default.
• W2044528902 countsByYear W20445289022014 @default.
• W2044528902 countsByYear W20445289022015 @default.
• W2044528902 countsByYear W20445289022020 @default.
• W2044528902 crossrefType "journal-article" @default.
• W2044528902 hasAuthorship W2044528902A5007872270 @default.
• W2044528902 hasAuthorship W2044528902A5058767285 @default.
• W2044528902 hasAuthorship W2044528902A5063434251 @default.
• W2044528902 hasAuthorship W2044528902A5072665303 @default.
• W2044528902 hasAuthorship W2044528902A5083889308 @default.
• W2044528902 hasConcept C100722585 @default.
• W2044528902 hasConcept C101677414 @default.
• W2044528902 hasConcept C107284991 @default.
• W2044528902 hasConcept C121332964 @default.
• W2044528902 hasConcept C127313418 @default.
• W2044528902 hasConcept C1276947 @default.
• W2044528902 hasConcept C13280743 @default.
• W2044528902 hasConcept C14257148 @default.
• W2044528902 hasConcept C153294291 @default.
• W2044528902 hasConcept C200239111 @default.
• W2044528902 hasConcept C37025601 @default.
• W2044528902 hasConcept C57879066 @default.
• W2044528902 hasConcept C72782756 @default.
• W2044528902 hasConcept C74650414 @default.
• W2044528902 hasConcept C8058405 @default.
• W2044528902 hasConcept C81502235 @default.
• W2044528902 hasConcept C98156149 @default.
• W2044528902 hasConceptScore W2044528902C100722585 @default.
• W2044528902 hasConceptScore W2044528902C101677414 @default.
• W2044528902 hasConceptScore W2044528902C107284991 @default.
• W2044528902 hasConceptScore W2044528902C121332964 @default.
• W2044528902 hasConceptScore W2044528902C127313418 @default.
• W2044528902 hasConceptScore W2044528902C1276947 @default.
• W2044528902 hasConceptScore W2044528902C13280743 @default.
• W2044528902 hasConceptScore W2044528902C14257148 @default.
• W2044528902 hasConceptScore W2044528902C153294291 @default.
• W2044528902 hasConceptScore W2044528902C200239111 @default.
• W2044528902 hasConceptScore W2044528902C37025601 @default.
• W2044528902 hasConceptScore W2044528902C57879066 @default.
• W2044528902 hasConceptScore W2044528902C72782756 @default.
• W2044528902 hasConceptScore W2044528902C74650414 @default.
• W2044528902 hasConceptScore W2044528902C8058405 @default.
• W2044528902 hasConceptScore W2044528902C81502235 @default.
• W2044528902 hasConceptScore W2044528902C98156149 @default.
• W2044528902 hasIssue "3-4" @default.

• next