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Journal articles on the topic 'Gravità intermedia'

Author: Grafiati

Published: 9 March 2023

Last updated: 31 July 2025

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1

Bronner, R., F. Dreger-Jauffret, and E. Pfirsch. "Lack of gravitropic response of tumour roots of Forsythia intermedia: cytological evidence for this behaviour." Canadian Journal of Botany 65, no. 1 (1987): 143–49. http://dx.doi.org/10.1139/b87-020.

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Tumours of Forsythia intermedia Zab. consist of clusters of roots characterized by limited growth. These roots are agravitropic and have a nontypical cap without starch. Placed in moisture, the roots elongate in the same direction as they had on the plant, without any gravitropic curvature. Elongated roots have a caplike area, the cells of which exhibit amyloplasts. The absence of gravitropic response of the elongated roots was confirmed experimentally. Amyloplasts of the columella cells do not sediment in the direction of gravity, even after modification of the position of the root with respe

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2

Pethő, Ágnes. "The Vertigo of the Single Image: From the Classic Narrative “Glitch” to the Post-Cinematic Adaptations of Paintings." Acta Universitatis Sapientiae, Film and Media Studies 6, no. 1 (2013): 65–90. http://dx.doi.org/10.2478/ausfm-2014-0005.

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Abstract As a possible cross section of cinematic narratology and the theory of intermediality the following essay assesses some of the effects of foregrounding the single, intermedial image within film. Specific figurations of intermediality that are experienced via the consciousness of single images, or some kind of “imageness” (i.e. as “intermedial references”) are presented as well as the modes in which they can interact with the narrative structure of a film. This interaction ranges from a momentary interference with the narrative structure of a film to disrupting it altogether; it may co

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3

Jang, Sujin, and E. Young Song. "Gravity with Intermediate Goods Trade." East Asian Economic Review 21, no. 4 (2017): 295–315. http://dx.doi.org/10.11644/kiep.eaer.2017.21.4.332.

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4

Conconi, Paola, Glenn Magerman, and Afrola Plaku. "The Gravity of Intermediate Goods." Review of Industrial Organization 57, no. 2 (2020): 223–43. http://dx.doi.org/10.1007/s11151-020-09762-2.

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5

Angenent, S. B., and D. G. Aronson. "Intermediate asymptotics for convergent viscous gravity currents." Physics of Fluids 7, no. 1 (1995): 223–25. http://dx.doi.org/10.1063/1.868722.

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6

Jamil, Mubasher, Davood Momeni, and Ratbay Myrzakulov. "Warm Intermediate Inflation in F(T) Gravity." International Journal of Theoretical Physics 54, no. 4 (2014): 1098–112. http://dx.doi.org/10.1007/s10773-014-2303-6.

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7

Rameli, Nabilah, Marini Ramli, Zefarina Zulkafli, et al. "Challenges in the Diagnosis of Beta-thalassemia Syndrome: The Importance of Molecular Diagnosis." Oman Medical Journal 37, no. 1 (2022): e331-e331. http://dx.doi.org/10.5001/omj.2021.48.

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Patients with heterozygous β-thalassemia are generally asymptomatic. However, the intermediate phenotype is uncommon, and patients require further investigation to confirm the diagnosis. We describe a 32-year-old woman (gravida 3, para 2) with heterozygous β-thalassemia who presented with symptomatic anemia and had a history of frequent blood transfusion in each pregnancy. Physical examination was unremarkable. Laboratory results at presentation showed hypochromic microcytic anemia with reticulocytosis. Molecular study revealed intermedia phenotypes resulting from coinheritance of heterozygous

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8

Greaney, Theresa M., and Kozo Kiyota. "The gravity model and trade in intermediate inputs." World Economy 43, no. 8 (2020): 2034–49. http://dx.doi.org/10.1111/twec.12947.

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9

LI, GUANGYU, and HAIBIN ZHAO. "CONSTRAINT ON INTERMEDIATE-RANGE GRAVITY FROM EARTH–SATELLITE AND LUNAR ORBITER MEASUREMENTS, AND LUNAR LASER RANGING." International Journal of Modern Physics D 14, no. 10 (2005): 1657–66. http://dx.doi.org/10.1142/s0218271805007176.

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In the experimental tests of gravity, there have been considerable interests in the possibility of intermediate-range gravity. In this paper, we use the earth–satellite measurement of earth gravity, the lunar orbiter measurement of lunar gravity, and lunar laser ranging measurement to constrain the intermediate-range gravity from λ = 1.2 × 107 m –3.8 × 108 m . The limits for this range are α = 10-8–5 × 10-8, which improve previous limits by about one order of magnitude in the range λ = 1.2 × 107 m –3.8 × 108 m .

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10

Brito, Francisco A., Carlos H. A. B. Borges, Jose A. V. Campos, and Francisco G. Costa. "Intermediate Coupling Regime in Dilatonic f(R,T) Inflationary Universe." Universe 11, no. 2 (2025): 65. https://doi.org/10.3390/universe11020065.

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In the present work, we study cosmology in dilatonic f(R,T) gravity to address the inflationary phase of the early universe. As usual, in dilatonic gravity, the scalar potential assumes the exponential form. However, this potential is not good enough to be in accordance with the Planck 2018 data. More strikingly, the generalized β-exponential cannot take this into account either. It is just only presence of the dilatonic sector, in the intermediate coupling regime, that can help the theory to be in full accordance with the observational data.

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11

Van Beeck, J., V. Prat, T. Van Reeth, et al. "Detecting axisymmetric magnetic fields using gravity modes in intermediate-mass stars." Astronomy & Astrophysics 638 (June 2020): A149. http://dx.doi.org/10.1051/0004-6361/201937363.

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Context. Angular momentum (AM) transport models of stellar interiors require improvements to explain the strong extraction of AM from stellar cores that is observed with asteroseismology. One of the frequently invoked mediators of AM transport are internal magnetic fields, even though their properties, observational signatures, and influence on stellar evolution are largely unknown. Aims. We study how a fossil, axisymmetric internal magnetic field affects period spacing patterns of dipolar gravity mode oscillations in main sequence stars with masses of 1.3, 2.0, and 3.0 M⊙. We assess the influ

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12

Zaninović, Vinko. "Facilitating trade in intermediate goods." Pomorstvo 36, no. 2 (2022): 271–78. http://dx.doi.org/10.31217/p.36.2.11.

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A side effect of economic globalisation and new information and communication technologies is the increasing fragmentation of the production process across different countries and continents, contributing to the rise of trade in intermediate goods, which has increased to almost 2/3 of total world trade. Most of this trade, i.e., intermediate goods, are transported by sea. Maritime trade is one of the most economical but also complex ways of trading and transporting goods, requiring good coordination, various stops and controls, transhipments, storage, ICT technology to track the cargo, etc. Th

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13

Barton, Bruce. "Still Ringing: Sounds Collaborative." Canadian Theatre Review 129 (January 2007): 25–29. http://dx.doi.org/10.3138/ctr.129.005.

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In CTR 126, I began a series of three linked articles that consider aspects of the relationship between theatricality and performativity in the work of the Toronto / New York intermedia performance ensemble, Bluemouth Inc. The first article explored the impact of the unanticipated relocation of the company’s 2005 recreation of American Standard from Pat’s Barber Shop on Toronto’s D’Arcy Street to the cavernous rehearsal space of Zero Gravity Circus in the same city’s industrial East End. The second article (in CTR 127) profiled Bluemouth Inc’.s 2005 reimaging of the performance Lenz in the evo

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14

Rabaey, G. F., and H. A. Hill. "The observed properties of the intermediate-degree gravity modes." Astrophysical Journal 362 (October 1990): 734. http://dx.doi.org/10.1086/169311.

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15

Sanyal, Abhik Kumar. "Intermediate Inflation or Late Time Acceleration?" Advances in High Energy Physics 2008 (2008): 1–16. http://dx.doi.org/10.1155/2008/630414.

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The expansion rate of “intermediate inflation” lies between the exponential and power law expansion but corresponding accelerated expansion does not start at the onset of cosmological evolution. Present study of “intermediate inflation” reveals that it admits scaling solution and has got a natural exit form it at a later epoch of cosmic evolution, leading to late time acceleration. The corresponding scalar field responsible for such feature is also found to behave as a tracker field for gravity with canonical kinetic term.

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16

Oikonomou, V. K. "On the expanding phase of a singular bounce and intermediate inflation: The modified gravity description." Modern Physics Letters A 32, no. 10 (2017): 1750067. http://dx.doi.org/10.1142/s0217732317500675.

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We demonstrate that the intermediate inflation scenario is a singular inflation cosmology, with the singularity at the origin t = 0 being a pressure and energy density singularity and particularly a Type III singularity. Also, we show that the expanding phase of a singular bounce can be identical to the intermediate inflation scenario, if the singular bounce has a Type III singularity at the origin. For the intermediate inflation scenario we examine the cosmological implications on the power spectrum in the context of various forms of modified gravity. Particularly, we calculate the power spec

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17

de Mello-Sampayo, Felipa. "Competing-destinations gravity model applied to trade in intermediate goods." Applied Economics Letters 24, no. 19 (2017): 1378–84. http://dx.doi.org/10.1080/13504851.2017.1282109.

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18

Aerts, C., M. G. Pedersen, and T. Van Reeth. "Measuring and Decoding Gravito-Inertial Modes in Intermediate- and High-Mass Stars." Proceedings of the International Astronomical Union 14, S339 (2017): 98–103. http://dx.doi.org/10.1017/s1743921318002314.

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AbstractThis talk discussed the basics of gravito-inertial asteroseismology as recently developed for stars born with a convective core. Photometric space missions originally built for exoplanet hunting, notably Kepler, have opened up the low-frequency regime of stellar oscillations and revealed a larger diversity in variability than anticipated prior to the era of high-precision space photometry. The talk explained the basics of forward seismic modelling based on gravito-inertial modes, which probe the deep stellar interior. It described how a hierarchical fitting approach allows us to derive

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19

Janssen, Peter A. E. M., and Miguel Onorato. "The Intermediate Water Depth Limit of the Zakharov Equation and Consequences for Wave Prediction." Journal of Physical Oceanography 37, no. 10 (2007): 2389–400. http://dx.doi.org/10.1175/jpo3128.1.

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Abstract Finite-amplitude deep-water waves are subject to modulational instability, which eventually can lead to the formation of extreme waves. In shallow water, finite-amplitude surface gravity waves generate a current and deviations from the mean surface elevation. This stabilizes the modulational instability, and as a consequence the process of nonlinear focusing ceases to exist when kh &lt; 1.363. This is a well-known property of surface gravity waves. Here it is shown for the first time that the usual starting point, namely the Zakharov equation, for deriving the nonlinear source ter

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20

Ratnasingam, R. P., P. V. F. Edelmann, and T. M. Rogers. "Onset of non-linear internal gravity waves in intermediate-mass stars." Monthly Notices of the Royal Astronomical Society 482, no. 4 (2018): 5500–5512. http://dx.doi.org/10.1093/mnras/sty3086.

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21

Silverman, M. P. "Satellite test of intermediate-range deviation from Newton's law of gravity." General Relativity and Gravitation 19, no. 5 (1987): 511–14. http://dx.doi.org/10.1007/bf00760655.

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22

Varghese, A., R. P. Ratnasingam, R. Vanon, P. V. F. Edelmann, and T. M. Rogers. "Chemical Mixing Induced by Internal Gravity Waves in Intermediate-mass Stars." Astrophysical Journal 942, no. 1 (2023): 53. http://dx.doi.org/10.3847/1538-4357/aca092.

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Abstract Internal gravity waves can cause mixing in the radiative interiors of stars. We study this mixing by introducing tracer particles into 2D hydrodynamic simulations. Following the work of Rogers & McElwaine, we extend our study to different masses (3, 7, and 20 M ⊙) and ages (ZAMS, midMS, and TAMS). The diffusion profiles of these models are influenced by various parameters such as the Brunt–Väisälä frequency, density, thermal damping, the geometric effect, and the frequencies of waves contributing to these mixing profiles. We find that the mixing profile changes dramatically across

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23

Lara, Martin. "LEO intermediary propagation as a feasible alternative to Brouwer’s gravity solution." Advances in Space Research 56, no. 3 (2015): 367–76. http://dx.doi.org/10.1016/j.asr.2014.12.023.

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24

Shelikhov, A. P. "DETERMINATION OF THE VARIABLE DENSITY OF THE INTERMEDIATE LAYER WITHIN THE GUBAKHA AREA (PERMSKIY KRAI)." Вестник Пермского университета. Геология 21, no. 4 (2022): 341–50. http://dx.doi.org/10.17072/psu.geol.21.4.341.

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Because of the improvement of instrumentation and technology progress in the conducting of gravity survey, there is a continuous increase in the accuracy of calculating the gravity Bouguer anomalies. At the same time, due to inadequate assessment of the intermediate layer density taken as a constant for reduction, the calculated anomalies may contain significant relative error. The article describes the experience of using the three-point formula of V.M. Berezkin to build a map of the areal distribution of the density of the intermediate layer and calculating, on its basis, anomalies in the Bo

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25

Zhao, Xing. "Sewing the self: Art, needlework and Liu Beili’s intersectional identity." Journal of Contemporary Chinese Art 9, no. 1 (2022): 113–31. http://dx.doi.org/10.1386/jcca_00058_1.

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As a Chinese-born woman living in the United States, Liu Beili is aware of the structurally, politically and representationally formulated intersectionality based on her national origin, ethnicity, language, gender and other factors. As a high-profile artist, Liu’s multimodal, polysemous and intermedial art reflects on the nuance that provides for understanding an intersectional immigrant’s sociocultural experience. Liu analogizes her femininity to water, which is resilient, and regards her art practices as the way to ‘better understand how migration and diaspora impact human experience throug

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26

Mizunuma, Hiroshi. "Intermediate viscosity in a gravity-driven flow and its application to simple viscometry." Journal of Rheology 69, no. 2 (2025): 131–38. https://doi.org/10.1122/8.0000879.

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In a capillary tube flow, if the wall shear stress τw and apparent shear rate 4V/R are given, the viscosity reduces to the viscosity τw/(4V/R) at a dimensionless intermediate radius ra* (≡ra/R) of approximately 0.8, where the shear rate is ra* × 4V/R. This known result is extended to the quasi-steady gravity-driven flow in a capillary tube, where the fluid head decreases from Hmax to H over a period of T seconds. Using a Carreau and power-law model, the intermediate viscosity for a gravity-driven flow is derived for the logarithmic middle fluid head between Hmax and H. This intermediate viscos

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27

Sivamohan, R., and E. Forssberg. "A review of the literature on intermediate and fine particle gravity concentration." International Journal of Mineral Processing 15, no. 3 (1985): 155. http://dx.doi.org/10.1016/0301-7516(85)90031-6.

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28

Hyun, Hea-Jung. "Institutional quality and trade in intermediate goods." Journal of Korea Trade 22, no. 2 (2018): 162–86. http://dx.doi.org/10.1108/jkt-02-2018-0009.

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Purpose Recently published studies stress the importance of trade in intermediate goods. The literature on determinants of trade, however, have largely focused on the sources of comparative advantage in determining aggregate trade flows rather than trade in intermediate goods. The purpose of this paper is to examine the role of institutional quality and trade costs to explain the determinants of trade in intermediates. Design/methodology/approach The simple model is based on the model of comparative advantage in the gravity framework used by Eaton and Kortum (2002) and Chor (2010) to relate tr

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29

Quéno, Louis, Rebecca Mott, Paul Morin, Bertrand Cluzet, Giulia Mazzotti, and Tobias Jonas. "Snow redistribution in an intermediate-complexity snow hydrology modelling framework." Cryosphere 18, no. 8 (2024): 3533–57. http://dx.doi.org/10.5194/tc-18-3533-2024.

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Abstract. Snow hydrological regimes in mountainous catchments are strongly influenced by snowpack heterogeneity resulting from wind- and gravity-induced redistribution processes, requiring them to be modelled at hectometre and finer resolutions. This study presents a novel modelling approach to address this issue, aiming at an intermediate-complexity solution to best represent these processes while maintaining operationally viable computational times. To this end, the physics-based snowpack model FSM2oshd was complemented by integrating the modules SnowTran-3D and SnowSlide to represent wind-

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30

Toscani, Martina, Giuseppe Lodato, and Elena Maria Rossi. "Discovering intermediate massive black holes through tidally disrupted stars." International Journal of Modern Physics D 28, no. 14 (2019): 1944015. http://dx.doi.org/10.1142/s0218271819440152.

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Stars are spheres of gas held together by self-gravity. When flying by a black hole, however, the star self-binding force can be overwhelmed by the black hole tides and the star can be torn apart. This is a physically rich and fascinating event which will be described by first introducing the concept of black hole from a mathematical point of view. We will then dive into the physics of the tidal disruption and proceed describing the accompanying electromagnetic flare and gravitational wave burst in the frequency range of the Laser Interferometer Space Antenna. This empowers such events to disc

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31

Varghese, A., R. P. Ratnasingam, R. Vanon, P. V. F. Edelmann, S. Mathis, and T. M. Rogers. "Effect of Rotation on Wave Mixing in Intermediate-mass Stars." Astrophysical Journal 970, no. 2 (2024): 104. http://dx.doi.org/10.3847/1538-4357/ad54b5.

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Abstract Internal gravity waves are likely to cause mixing in stellar interiors. Studies show that the mixing by these waves changes drastically across age and mass. Here, we study the effect of rotation on this wave mixing by considering a 7 M ⊙ model at zero-age main sequence and mid-main sequence. We compare the mixing profiles at a range of rotation rates (1 × 10−5, 2 × 10−5, 3 × 10−5, 4 × 10−5, and 1 × 10−4 rad s−1) and observe that the mixing decreases with decreasing Rossby number. This can be attributed to the effect of rotation on convection, which influences the amplitude with which

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32

Miles-Páez, P. A., M. R. Zapatero Osorio, E. Pallé, and K. Peña Ramírez. "Optical and near-infrared linear polarization of low and intermediate-gravity ultracool dwarfs." Monthly Notices of the Royal Astronomical Society 466, no. 3 (2016): 3184–98. http://dx.doi.org/10.1093/mnras/stw3278.

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33

Rees, Julia M., and William B. Zimmerman. "An intermediate wavelength, weakly nonlinear theory for the evolution of capillary gravity waves." Wave Motion 48, no. 8 (2011): 707–16. http://dx.doi.org/10.1016/j.wavemoti.2011.03.006.

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34

Gondoin, P. "On the relation between rotation, convection and activity in intermediate-mass giants." Proceedings of the International Astronomical Union 2, S239 (2006): 154–56. http://dx.doi.org/10.1017/s1743921307000324.

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AbstractI found evidence that the X-ray surface flux of intermediate-mass G and K giants is correlated with their rotation period and Rossby number. Confidence in the degree of correlation is significantly higher when stellar gravity is taken into account. An empirical relation is found that accounts for the X-ray luminosity evolution of single intermediate-mass giants and giants in close or long-period binary systems, such as RS CVn-type systems, as they evolve off the main sequence towards the top of red giant branch.

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35

Lathers, Claire M., Peter H. Diamandis, Jeanne M. Riddle, et al. "Acute and Intermediate Cardiovascular Responses to Zero Gravity and to Fractional Gravity Levels Induced by Head-Down or Head-Up Tilt." Journal of Clinical Pharmacology 30, no. 6 (1990): 494–523. http://dx.doi.org/10.1002/j.1552-4604.1990.tb03614.x.

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36

Joshi, M., M. Stringer, K. van der Wiel, A. O'Callaghan, and S. Fueglistaler. "IGCM4: a fast, parallel and flexible intermediate climate model." Geoscientific Model Development Discussions 7, no. 4 (2014): 5517–45. http://dx.doi.org/10.5194/gmdd-7-5517-2014.

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Abstract. The IGCM4 (Intermediate Global Circulation Model version 4) is a global spectral primitive equation climate model whose predecessors have extensively been used in fields such as climate dynamics, processes modelling, and atmospheric dynamics. The IGCM4's niche and utility lies in its parallel spectral dynamics and fast radiation scheme. Moist processes such as clouds, evaporation, and soil moisture are simulated in the model, though in a simplified manner compared to state-of-the-art GCMs. The latest version has been parallelised, which has led to massive speed-up and enabled much hi

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37

Nie, Deming, Limin Qiu, and Xiaobin Zhang. "Direct numerical simulation of multiple interacting particles at intermediate Reynolds numbers." International Journal of Numerical Methods for Heat & Fluid Flow 25, no. 2 (2015): 202–13. http://dx.doi.org/10.1108/hff-04-2013-0138.

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Purpose – The purpose of this paper is to study the flow patterns and particle-particle collisions during the sedimentation of multiple circular particles under gravity at intermediate Reynolds numbers through direct numerical simulations (DNS). Design/methodology/approach – The previously developed lattice Boltzmann-direct forcing/fictitious domain (LB-DF/FD) method is adopted in this work to conduct DNS. Findings – It is found that the number of particle-particle collisions display a linear growth at long times after an initial evolution, resulting in a constant collision rate, which also de

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38

Van Reeth, T., J. S. G. Mombarg, S. Mathis, et al. "Sensitivity of gravito-inertial modes to differential rotation in intermediate-mass main-sequence stars." Astronomy & Astrophysics 618 (October 2018): A24. http://dx.doi.org/10.1051/0004-6361/201832718.

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Context. While rotation has a major impact on stellar structure and evolution, its effects are not well understood. Thanks to high-quality and long-time base photometric observations obtained with recent space missions, we are now able to study stellar rotation more precisely.Aims. We aim to constrain radial differential rotation profiles inγDoradus (γDor) stars, and to develop new theoretical seismic diagnosis for such stars with rapid and potentially non-uniform rotation.Methods. We have derived a new asymptotic description which accounts for the impact of weak differential near-core rotatio

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Teh, Lip H., and Benoit P. Gilbert. "A buckling model for the stability design of steel columns with intermediate gravity loads." Journal of Constructional Steel Research 117 (February 2016): 243–54. http://dx.doi.org/10.1016/j.jcsr.2015.10.019.

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40

Aldarabseh, Safa Mohammad, and Parviz Merati. "An intermediate water gravity wavelength and wave height measurement inside a large wave flume tank." Journal of Applied Research and Technology 21, no. 3 (2023): 407–23. http://dx.doi.org/10.22201/icat.24486736e.2023.21.3.1757.

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This paper discusses an intermediate water gravity wavelength and wave height measurement method. Three methods were used to obtain wave height, wavelength, and period. Firstly, conventional methods used two Honeywell pressure sensors mounted at the bottom of the wave tank at two different locations. Secondly, using the transfer function of the flap wavemaker (the relationship between wave height and the wave paddle stroke). Thirdly, the Laser Sheet technique (PIV image processing technique). The significant wave height and period from pressure reading sensors of regular gravity waves were obt

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41

Guzik, Joyce A., T. H. Morgan, N. J. Nelson, et al. "2-D and 3-D models of convective turbulence and oscillations in intermediate-mass main-sequence stars." Proceedings of the International Astronomical Union 11, A29B (2015): 540–43. http://dx.doi.org/10.1017/s1743921316006086.

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AbstractWe present multidimensional modeling of convection and oscillations in main-sequence stars somewhat more massive than the Sun, using three separate approaches: 1) Using the 3-D planar StellarBox radiation hydrodynamics code to model the envelope convection zone and part of the radiative zone. Our goals are to examine the interaction of stellar pulsations with turbulent convection in the envelope, excitation of acoustic modes, and the role of convective overshooting; 2) Applying the spherical 3-D MHD ASH (Anelastic Spherical Harmonics) code to simulate the core convection and radiative

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42

Heifetz, Eyal, and Brian F. Farrell. "Generalized Stability of Nongeostrophic Baroclinic Shear Flow. Part II: Intermediate Richardson Number Regime." Journal of the Atmospheric Sciences 64, no. 12 (2007): 4366–82. http://dx.doi.org/10.1175/2007jas2225.1.

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Abstract This work continues the generalized stability theory (GST) analysis of baroclinic shear flow in the primitive equations (PE), focusing on the regime in which the mean baroclinic shear and the stratification are of the same order. The Eady model basic state is used and solutions obtained using the PE are compared to quasigeostrophic (QG) solutions. Similar optimal growth is obtained in the PE and QG frameworks for eddies with horizontal scale equal to or larger than the Rossby radius, although PE growth rates always exceed QG growth rates. The primary energy growth mechanism is the con

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43

Joshi, M., M. Stringer, K. van der Wiel, A. O'Callaghan, and S. Fueglistaler. "IGCM4: a fast, parallel and flexible intermediate climate model." Geoscientific Model Development 8, no. 4 (2015): 1157–67. http://dx.doi.org/10.5194/gmd-8-1157-2015.

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Abstract. The IGCM4 (Intermediate Global Circulation Model version 4) is a global spectral primitive equation climate model whose predecessors have extensively been used in areas such as climate research, process modelling and atmospheric dynamics. The IGCM4's niche and utility lies in its speed and flexibility allied with the complexity of a primitive equation climate model. Moist processes such as clouds, evaporation, atmospheric radiation and soil moisture are simulated in the model, though in a simplified manner compared to state-of-the-art global circulation models (GCMs). IGCM4 is a para

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44

Jiang, Tong, Ning Dai, Yungui Gong, Dicong Liang, and Chao Zhang. "Constraint on Brans-Dicke theory from intermediate/extreme mass ratio inspirals." Journal of Cosmology and Astroparticle Physics 2022, no. 12 (2022): 023. http://dx.doi.org/10.1088/1475-7516/2022/12/023.

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Abstract Intermediate/Extreme mass ratio inspiral (I/EMRI) system provides a good tool to test the nature of gravity in strong field. Based on the method of osculating orbits, we compute the orbital evolutions of I/EMRIs on quasi-elliptic orbits in both Einstein's general relativity and Brans-Dicke theory. The extra monopolar and dipolar channels in Brans-Dicke theory accelerate the orbital decay, so it is important to consider the effects of monopolar and dipolar emissions on the waveform. With the help of accurate orbital motion, we generate waveform templates which include both monopolar an

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Yang, Yixin, and Zejiong Zhou. "The Impact of Competition Policy Provisions in Regional Trade Agreements on Intermediate Product Trade." Frontiers in Business, Economics and Management 6, no. 3 (2022): 7–12. http://dx.doi.org/10.54097/fbem.v6i3.3109.

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The deepening of the content of regional trade agreements has promoted the deep integration of global value chains. As an important part of the behind-the-border measures of regional trade agreements, competition policy provisions have an important impact on intermediate product trade. This paper constructs the depth index of competition policy provisions, uses the trade gravity model combined with Poisson's pseudo maximum likelihood estimation (PPML) and fixed effects to empirically analyze the impact of competition policy depth on the scale of intermediate product trade, and finally proposes

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Xu, Xingjian, Jiangbin Liu, Fenghua Wei, et al. "Specific gravity and dropping speed in eggs ofOncomelania hupensis, a snail intermediate host of Schistosomiasis." Molluscan Research 20, no. 2 (2000): 31–36. http://dx.doi.org/10.1080/13235818.2000.10673731.

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Ratnasingam, R. P., P. V. F. Edelmann, and T. M. Rogers. "Two-dimensional simulations of internal gravity waves in the radiation zones of intermediate-mass stars." Monthly Notices of the Royal Astronomical Society 497, no. 4 (2020): 4231–45. http://dx.doi.org/10.1093/mnras/staa2296.

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ABSTRACT Intermediate-mass main-sequence stars have large radiative envelopes overlying convective cores. This configuration allows internal gravity waves (IGWs) generated at the convective–radiative interface to propagate towards the stellar surface. The signatures of these waves can be observed in the photometric and spectroscopic data from stars. We have studied the propagation of these IGWs using two-dimensional (2D) fully non-linear hydrodynamical simulations with realistic stellar reference states from the 1D stellar evolution code, Modules for Stellar Astrophysics (mesa). When a single

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Barthelemy, X., M. L. Banner, W. L. Peirson, F. Fedele, M. Allis, and F. Dias. "On a unified breaking onset threshold for gravity waves in deep and intermediate depth water." Journal of Fluid Mechanics 841 (February 23, 2018): 463–88. http://dx.doi.org/10.1017/jfm.2018.93.

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We revisit the classical but as yet unresolved problem of predicting the breaking onset of 2D and 3D irrotational gravity water waves. Based on a fully nonlinear 3D boundary element model, our numerical simulations investigate geometric, kinematic and energetic differences between maximally tall non-breaking waves and marginally breaking waves in focusing wave groups. Our study focuses initially on unidirectional domains with flat bottom topography and conditions ranging from deep to intermediate depth (depth to wavelength ratio from 1 to 0.2). Maximally tall non-breaking (maximally recurrent)

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Boos, Jens, and Friedrich W. Hehl. "Gravity-Induced Four-Fermion Contact Interaction Implies Gravitational Intermediate W and Z Type Gauge Bosons." International Journal of Theoretical Physics 56, no. 3 (2016): 751–56. http://dx.doi.org/10.1007/s10773-016-3216-3.

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Merchalov, S. V., V. I. Pryadkin, V. I. Orobinsky, A. V. Vorokhobin, V. V. Voronin, and A. A. Smyshlyaev. "Construction for intermediate separation of ground grain in combined fodder production." IOP Conference Series: Earth and Environmental Science 1052, no. 1 (2022): 012022. http://dx.doi.org/10.1088/1755-1315/1052/1/012022.

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Abstract The article provides research on a conical gravity separator with wedge-shaped separating channels expanding in the processed material's direction. Separation of the crushed grain material occurs due to the influence of the gravitational field and does not require additional energy consumption for the process itself. Energy is required to lift the processed material to a particular technological height. The use of wedge-shaped calibrating channels in the separator eliminates expensive frames, crank mechanisms, bearing assemblies and shafts, suspension, and drive mechanisms as in sieve

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