Publication:
Transitions of Spherical Thermohaline Circulation to Multiple Equilibria

dc.contributor.authorSaadet, Özer
dc.contributor.authorTaylan, Şengül
dc.date.accessioned2026-01-25T10:56:44Z
dc.date.issued2017-06-19
dc.description.abstractThe main aim of the paper is to investigate the transitions of the thermohaline circulation in a spherical shell in a parameter regime which only allows transitions to multiple equilibria. We find that the first transition is either continuous (Type-I) or drastic (Type-II) depending on the sign of the transition number. The transition number depends on the system parameters and $l_c$, which is the common degree of spherical harmonics of the first critical eigenmodes, and it can be written as a sum of terms describing the nonlinear interactions of various modes with the critical modes. We obtain the exact formulas of this transition number for $l_c=1$ and $l_c=2$ cases. Numerically, we find that the main contribution to the transition number is due to nonlinear interactions with modes having zero wave number and the contribution from the nonlinear interactions with higher frequency modes is negligible. In our numerical experiments we encountered both types of transition for $Le<1$ but only continuous transition for $Le>1$. In the continuous transition scenario, we rigorously prove that an attractor in the phase space bifurcates which is homeomorphic to the 2$l_c$ dimensional sphere and consists entirely of degenerate steady state solutions.
dc.description.urihttps://doi.org/10.1007/s00021-017-0331-8
dc.description.urihttp://arxiv.org/pdf/1706.02115
dc.description.urihttps://dx.doi.org/10.48550/arxiv.1706.02115
dc.description.urihttp://arxiv.org/abs/1706.02115
dc.description.urihttps://zbmath.org/6908398
dc.description.urihttps://dx.doi.org/10.1007/s00021-017-0331-8
dc.description.urihttps://hdl.handle.net/11424/241967
dc.identifier.doi10.1007/s00021-017-0331-8
dc.identifier.eissn1422-6952
dc.identifier.endpage515
dc.identifier.issn1422-6928
dc.identifier.openairedoi_dedup___::84034d7b302b0444d67a038e8c22b166
dc.identifier.orcid0000-0003-4841-7326
dc.identifier.startpage499
dc.identifier.urihttps://hdl.handle.net/11527/49957
dc.identifier.volume20
dc.language.isoeng
dc.publisherSpringer Science and Business Media LLC
dc.relation.ispartofJournal of Mathematical Fluid Mechanics
dc.rightsOPEN
dc.sdg.typeGoal 10: Reduced Inequality
dc.subjectThermohaline circulation
dc.subjectHydrology, hydrography, oceanography
dc.subjectBifurcation
dc.subjectphase space attractor
dc.subjectdynamic transition theory
dc.subjectspherical harmonics
dc.subjectPrincipal of exchange of stabilities
dc.subjectDynamic transition theory
dc.subjectMathematics - Analysis of PDEs
dc.subjectDynamic transitions
dc.subjectDynamical systems in fluid mechanics, oceanography and meteorology
dc.subjectConvection
dc.subjectStability and instability of geophysical and astrophysical flows
dc.subjectFOS: Mathematics
dc.subjectLinear stability
dc.subjectSpherical harmonics
dc.subjectlinear stability
dc.subjectexchange of stabilities
dc.subjectAnalysis of PDEs (math.AP)
dc.titleTransitions of Spherical Thermohaline Circulation to Multiple Equilibria
dc.typeArticle
dspace.entity.typePublication

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