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dc.contributor.authorMamatsashvili, George-
dc.date.accessioned2016-06-14T10:51:30Z-
dc.date.available2016-06-14T10:51:30Z-
dc.date.issued2006-
dc.identifier.urihttp://dspace.nplg.gov.ge/handle/1234/161144-
dc.description.tableofcontents1. Introduction–– 1.1 Aim of the thesis–– 1.2 Plan of the thesis–– 2. Linear dynamics of non-symmetric perturbations in geostrophic horizontal shear flows–– 2.1 Mathematical formalism–– 2.2 Dynamics of non-symmetric perturbations–– 2.2.1 Ro<<1 regime. WKB analysis–– 2.2.2 Ro ~ 1 regime–– Numerical solution –– 2.3 Influence of viscosity–– 2.4 Bounded flows–– Summary–– 3. Linear dynamics of perturbations in astrophysical discs–– 3.1 Physical model and equations–– 3.2 SFH dynamics–– 3.2.1 Numerical integration–– 3.2.2 Reflection and transmission–– 3.2.3 Generation of spiral density waves by vortices–– 3.3 Dynamics of localized density wave packets–– Summary–– 4. Summary and Discussions–– Appendix A–– Appendix B–– References-
dc.format.extent115 გვ.en_US
dc.language.isoenen_US
dc.publisherთბილისიen_US
dc.sourceVelocity shear induced perturbation dynamics in atmospheric, oceanic and astrophysical flows / G. Mamatsashvili: Candidate Dissertation; 01.03.02 / Georgian E. Kharadze Abastumani National Astrophysical Observatory; Tb.-2006. 115p. bibliographi: p. - 93-115(საქართველოს პარლამენტის ეროვნული ბიბლიოთეკა, საარქივო ფონდი)en_US
dc.subjectმათემატიკაen_US
dc.subjectბუნების მეტყველებაen_US
dc.subjectასტროფიზიკაen_US
dc.titleVelocity shear induced perturbation dynamics in atmospheric, oceanic and astrophysical flowsen_US
dc.typeThesisen_US
dc.rights.holderსაქართველოს პარლამენტის ეროვნული ბიბლიოთეკაen_US
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