Auswahl der wissenschaftlichen Literatur zum Thema „Sabra shell model“
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Zeitschriftenartikel zum Thema "Sabra shell model"
Biswas, Tania, und Sheetal Dharmatti. „Control problems and invariant subspaces for sabra shell model of turbulence“. Evolution Equations & Control Theory 7, Nr. 3 (2018): 417–45. http://dx.doi.org/10.3934/eect.2018021.
Der volle Inhalt der QuelleChen, Nan, Yuchen Li und Evelyn Lunasin. „An efficient continuous data assimilation algorithm for the Sabra shell model of turbulence“. Chaos: An Interdisciplinary Journal of Nonlinear Science 31, Nr. 10 (Oktober 2021): 103123. http://dx.doi.org/10.1063/5.0057421.
Der volle Inhalt der QuelleL'vov, V. S., E. Podivilov und I. Procaccia. „Hamiltonian structure of the Sabra shell model of turbulence: Exact calculation of an anomalous scaling exponent“. Europhysics Letters (EPL) 46, Nr. 5 (01.06.1999): 609–12. http://dx.doi.org/10.1209/epl/i1999-00307-8.
Der volle Inhalt der QuelleConstantin, Peter, Boris Levant und Edriss S. Titi. „Sharp Lower Bounds for the Dimension of the Global Attractor of the Sabra Shell Model of Turbulence“. Journal of Statistical Physics 127, Nr. 6 (05.05.2007): 1173–92. http://dx.doi.org/10.1007/s10955-007-9317-x.
Der volle Inhalt der QuelleShand, B. A., M. Lester und T. K. Yeoman. „Substorm associated radar auroral surges: a statistical study and possible generation model“. Annales Geophysicae 16, Nr. 4 (30.04.1998): 441–49. http://dx.doi.org/10.1007/s00585-998-0441-y.
Der volle Inhalt der QuelleShaikh, Muhammad Vaseem, Sabra K. Salim, Jeffrey Wei, William T. Maich, Alisha A. Anand, Oliver Young Tang, Minomi K. Subapanditha et al. „Abstract 5241: Generation of allogeneic CAR-T circumvents functional deficits in patient-derived autologous product for glioblastoma“. Cancer Research 84, Nr. 6_Supplement (22.03.2024): 5241. http://dx.doi.org/10.1158/1538-7445.am2024-5241.
Der volle Inhalt der QuelleChen, Nan, Aseel Farhat und Evelyn Lunasin. „Data assimilation with model error: Analytical and computational study for Sabra shell model“. Physica D: Nonlinear Phenomena, Oktober 2022, 133552. http://dx.doi.org/10.1016/j.physd.2022.133552.
Der volle Inhalt der QuelleFontaine, Côme, Malo Tarpin, Freddy Bouchet und Léonie Canet. „Functional renormalisation group approach to shell models of turbulence“. SciPost Physics 15, Nr. 5 (28.11.2023). http://dx.doi.org/10.21468/scipostphys.15.5.212.
Der volle Inhalt der QuelleBiswas, Tania, und Sheetal Dharmatti. „Interior and H ∞ feedback stabilization for sabra shell model of turbulence“. Mathematical Methods in the Applied Sciences, 10.08.2022. http://dx.doi.org/10.1002/mma.8615.
Der volle Inhalt der QuelleEvans, Alistair R., Tahlia I. Pollock, Silke G. C. Cleuren, William M. G. Parker, Hazel L. Richards, Kathleen L. S. Garland, Erich M. G. Fitzgerald, Tim E. Wilson, David P. Hocking und Justin W. Adams. „A universal power law for modelling the growth and form of teeth, claws, horns, thorns, beaks, and shells“. BMC Biology 19, Nr. 1 (30.03.2021). http://dx.doi.org/10.1186/s12915-021-00990-w.
Der volle Inhalt der QuelleDissertationen zum Thema "Sabra shell model"
Fontaine, Côme. „Etude de deux modèles simplifiés de turbulence à l'aide du groupe de renormalisation fonctionnel : l'équation de Burgers et le modèle de Sabra“. Electronic Thesis or Diss., Université Grenoble Alpes, 2023. http://www.theses.fr/2023GRALY083.
Der volle Inhalt der QuelleIn this thesis, we focus on two simplified models describing turbulent flows. In these two models, the turbulent state exhibits scale-invariance and universal statistical properties resembling those of true hydrodynamical turbulence. This type of behaviour is very familiar in physics: it corresponds to a critical system. In this work, we use a widely used tool in the study of criticality: the functional renormalisation group (FRG). The first model, named the Sabra shell model, describes effective interactions among a discrete number of velocity modes of a turbulent fluid. This schematic description captures many essential properties of turbulent flows. In particular, the velocity field is multifractal. The way in which the dynamics generates this multifractality is still poorly understood from a theoretical perspective. In this thesis, we formulate a reverse renormalisation flow, meaning that we integrate out the largest scales first. Using this method, we find a fixed point of the renormalisation flow with anomalous scale invariance, relatively close to the expected value for certain observables. We show that it is clearly distinct from the fixed point obtained when all scales are forced, through a forcing with a power-law spectrum, which corresponds to the fixed point of the RG obtained in perturbation theory. The second model studied is the Burgers equation, which describes the dynamics of a fluid in the absence of pressure. We focus on the effect of a conservative noise on the velocity field. We prove the existence of a scale invariant regime with a critical dynamical exponent z=1 using an exact closure of the renormalisation flow equation. This closure relies on the existence of certain symmetries of the Burgers equation. Indications of the existence of this new scaling regime were previously found in numerical solutions of the Burgers equation. We provide in this thesis a theoretical proof of its existence and calculate the associated universal properties
Buchteile zum Thema "Sabra shell model"
Rodriguez Carranza, Alexis, Obidio Rubio Mercedes und Elder Joel Varas Peréz. „Numerical Simulation of Energy Cascading in Turbulent Flows Using Sabra Shell Model“. In Vortex Simulation and Identification [Working Title]. IntechOpen, 2023. http://dx.doi.org/10.5772/intechopen.111468.
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