The DOI matches its Crossref record.
Convection in a rotating, laterally heated annulus the wave number transitions
Abstract
The radial temperature differences at which the transitions from one wave number to the next occur have been measured with either increasing or decreasing positive radial temperature gradients, at five different rotation rates, with the fluid being always in thermal equilibrium and being in contact with an upper rigid lid. Hysteresis has been observed in all wave number transitions, and also in the transition to upper symmetry. There are, nevertheless, regions in the stability diagram where the wave number is unique. There is an excluded region where the wave number four cannot be obtained through quasi-steady procedure. There is a reversal of the sense of the hysteresis of the transitions. At low ΔT, a wave number transition with increasing radial temperature difference occurs at a higher ΔT, than the same transition with decreasing temperature difference. On the other hand, at large values of ΔT, a wave number transition with increasing radial temperature difference occurs at a lower ΔT, than the same transition with decreasing temperature difference. Wave number transitions with increasing ΔT, occur spontaneously out of amplitude oscillations. Wave number transitions with decreasing ΔT, occur via slow wave splitting in association with phase modulations of the waves. The uniqueness of the wave number in the unique areas of the stability diagram has been confirmed by sudden start experiments.
Overview
Integrity signals
Registry
Cites
Statistics
Verification
Claims the paper makes
Claims other papers make about this one
Each is checked against this paper’s own text: does it say what the citing paper says it does?
In the citing paper
“Previous studies have also shown how baroclinic instabilities can equilibrate into meanders in such pro fi les ( Koschmieder & White 1981; Bastin & Read 1997; Sutyrin et al. 2001 ) .”
From MEANDERING SHALLOW ATMOSPHERIC JET AS A MODEL OF SATURNʼS NORTH-POLAR HEXAGON (2015) · cites this paper as Koschmieder & White 1981
Citations
Cites
No references could be resolved yet.
Research works printed but not linked: 14
- Buzyna G., 1978, J. Atmos. Sci., 35, 859, 10.1175/1520-0469(1978)035<0859:CVOTIT>2.0.CO;2 · DOI
- Cole R. J., 1971, Q.J.R. Meteorol. Soc., 97, 506, 10.1002/qj.49709741410 · DOI
- Dietrich D. E., 1973, Pure & Appl. Geophys., 109, 1826, 10.1007/BF00876109 · DOI
- Fein J. S., 1973, Geophys. Fluid Dyn., 5, 213, 10.1080/03091927308236118 · DOI
- Fowlis W. W., 1965, J. Atmos. Sci., 22, 541, 10.1175/1520-0469(1965)022<0541:TCIARA>2.0.CO;2 · DOI
- Fultz D., 1959, Met. Monographs, 4, 21
- Hide R., 1975, Adv. Phys., 24, 47, 10.1080/00018737500101371 · DOI
- Kaiser J. A. C., 1970, Tellus, 22, 275, 10.1111/j.2153-3490.1970.tb00495.x · DOI
- Koschmieder E. L., 1972, J. Fluid Mech., 51, 637, 10.1017/S0022112072001284 · DOI
- Koschmieder E. L., 1978, Geophys. & Astrophys. Fluid Dyn., 10, 157, 10.1080/03091927808242635 · DOI
- Lorenz E. N., 1962, J. Atmos. Sci., 19, 39, 10.1175/1520-0469(1962)019<0039:SDEATT>2.0.CO;2 · DOI
- Mason P. J., 1975, Philos. Trans. R. Soc. London, 278, 397, 10.1098/rsta.1975.0032 · DOI
- White H. D., 1981, Geophys. & Astrophys. Fluid Dyn., 18, 301, 10.1080/03091928108208842 · DOI
- Williams G. P., 1967, J. Atmos Sci., 24, 144, 10.1175/1520-0469(1967)024<0144:TCIARF>2.0.CO;2 · DOI
Cited by
Sorted by citations
MEANDERING SHALLOW ATMOSPHERIC JET AS A MODEL OF SATURNʼS NORTH-POLAR HEXAGON
Morales-Juberías, R., Sayanagi, K. M., Simon, A. A., Fletcher, L. N., & Cosentino, R. G. (2015) · The Astrophysical Journal · doi:10.1088/2041-8205/806/1/l18 · Cited by 35
Metadata
- Authors
- Koschmieder, E. L., & White, H. D.
- Affiliations
- The University of Texas at Austin (US)
- Venue
- Geophysical & Astrophysical Fluid Dynamics
- Publisher
- Informa UK Limited
- Published
- 1981-12
- Volume
- 18
- Issue
- 3-4
- Pages
- 279-299
- ISSN
- 0309-1929 (ISSN-L)
- 1029-0419
- OpenAlex
- W2118772935
- Cited by
- 15
- References
- 0
- Citations by year
- 2015: 2 · 2014: 2
- FWCI
- 1.11
- Type
- journal article
- Language
- en
- Open access
- closed
- Locations
- Geophysical & Astrophysical Fluid Dynamics (publishedVersion)
- Topics
- Physical Sciences › Engineering › Computational Mechanics › Fluid Dynamics and Turbulent Flows
- Physical Sciences › Earth and Planetary Sciences › Oceanography › Oceanographic and Atmospheric Processes
- Physical Sciences › Physics and Astronomy › Statistical and Nonlinear Physics › Nonlinear Dynamics and Pattern Formation
- Keywords
- rotating convection, hysteresis, radial temperature gradient, stability diagram, amplitude oscillations, wave splitting, phase modulation, thermal equilibrium
About these checks
Registry, retraction, Cites and statistics results are computed, not judged, with one exception: a printed reference that no index lists is read once by a model before it counts as a citation error. Claims are extracted by a model and kept only when their quote appears verbatim in the text; each cited source is then checked, with a model’s help, for whether it says what the claim relies on. Those verdicts can be wrong — read the claim’s quote and the cited source before relying on one.
Statistics and arithmetic are recomputed, not judged.
Confidence bands are shown only for fields calibrated on our annotated test set. None is calibrated yet, so no band is shown.
What counts as a claim ›How we measure confidence ›How we check this ›
Are you an author, or do you see a problem with this page? Request a review