Geoscience Reference
In-Depth Information
Ohlsen, D. R., and J. E. Hart (1989a), The transition to baro-
clinic chaos on the
β
-plane,
J. Fluid Mech.
,
203
, 23-50.
Ohlsen, D. R., and J. E. Hart (1989b), Nonlinear interference
vacillation,
Geophys. Astrophys. Fluid Dyn.
,
45
, 213-235.
Pedlosky, J. (1970), Finite-amplitude baroclinic waves,
J. Atmos.
Sci.
,
27
, 15-30.
Pedlosky, J. (1971), Finite-amplitude baroclinic waves with small
dissipation,
J. Atmos. Sci.
,
28
, 587-597.
Pedlosky, J. (1982a), Finite-amplitude baroclinic waves at mini-
mum critical shear,
J. Atmos. Sci.
,
39
, 555-562.
Pedlosky, J. (1982b), A simple model for nonlinear critical layers
in an unstable baroclinic waves,
J. Atmos. Sci.
,
39
, 2119-2127.
Pedlosky, J. (1987),
Geophysical Fluid Dynamics
, Springer,
Berlin.
Pedlosky, J., and C. Frenzen (1980), Chaotic and periodic behav-
ior of finite-amplitude baroclinic waves,
J. Atmos. Sci.
,
37
,
1177-1196.
Pérez, E. P. (2006), Heat transport by baroclinic eddies: Eval-
uating eddy parameterizations for numerical models, Ph.D.
thesis, Univ. of Oxford.
Pérez, E. P., P. L. Read, and I. M. Moroz (2010), Assessing eddy
parameterization schemes in a differentially heated rotating
annulus experiment,
Ocean Modelling
,
32
, 118-131.
Pfeffer, R. L., and A. Barcilon (1978), Determination of eddy
fluxes of heat and eddy temperature variances using weakly
nonlinear theory,
J. Atmos. Sci.
,
35
, 2099-2110.
Pfeffer, R. L., G. Buzyna, and R. Kung (1980), Time depen-
dent modes of behavior of thermally-driven rotating fluid,
J. Atmos. Sci.
,
37
, 2129-2149.
Phillips, N. A. (1954), Energy transformations and merid-
ional circulation associated with simple baroclinic waves in a
two-level quasi-geostrophic model,
Tellus
,
6
, 273-286.
Pierrehumbert, R. T. (2010),
Principles of Planetary Climate
,
Cambridge Univ. Press, Cambridge, UK.
Plumb, R., and J. Mahlman (1987), The zonally-averaged
transport characteristics of the GFDL general circual-
tion/transport model,
J. Atmos., Sci.
,
44
, 298-327.
Randriamampianina, A., W.-G. Früh, P. L. Read, and
P. Maubert (2006), Direct numerical simulations of bifur-
cations in an air-filled rotating baroclinic annulus,
J. Fluid
Mech.
,
561
, 359-389.
Ravela, S., J. Marshall, C. Hill, A. Wong, and S. Stransky (2010),
A realtime observatory for laboratory simulation of planetary
flows,
Exp. Fluids
,
48
, 915-925.
Read, P. L. (1986), Regimes of axisymmetric flow in an internally
heated rotating fluid,
J. Fluid Mech.
,
168
, 255-289.
Read, P. L. (1988), On the scale of baroclinic instability in deep,
compressible atmospheres,
Quart. J. R. Meteor. Soc.
,
114
,
421-437.
Read, P. L. (1992), Dynamics and instabilities of Ekman and
Stewartson layers, in
Rotating Fluids in Geophysical and
Industrial Applications
, edited by E. J. Hopfinger, pp. 49-84,
Springer-Verlag, Vienna and New York.
Read, P. L. (2003), A combined laboratory and numerical study
of heat transport by baroclinic eddies and axisymmetric flows,
J. Fluid Mech.
,
489
, 301-323.
Read, P. L. (2011), Dynamics and circulation regimes of terres-
trial planets,
Plan. Space Sci.
,
59
, 900-914.
Read, P. L., and S. H. Risch (2011), A laboratory study of global-
scale wave interactions in baroclinic flow with topography i:
Multiple flow regimes,
Geophys. Astrophys. Fluid Dyn.
,
105
,
128-160.
Read, P. L., M. J. Bell, D. W. Johnson, and R. M. Small (1992),
Quasi-periodic and chaotic flow regimes in a thermally driven,
rotating fluid annulus,
J. Fluid Mech.
,
238
, 599-632.
Read, P. L., N. P. J. Thomas, and S. H. Risch (2000), An evalu-
ation of Eulerian and semi-Lagrangian advection schemes in
simulations of rotating, stratified flows in the laboratory. Part
I: Axisymmetric low,
Mon. Weather Rev.
,
128
, 2835-2852.
Rhines, P. B. (1979), Geostrophic turbulence,
Ann. Rev. Fluid
Mech.
,
11
, 401-441.
Richardson, L. F. (1922),
Weather Prediction by Numerical Pro-
cess
, Dover Publications, New York.
Romea, R. D. (1977), The effects of friction and
β
on finite
amplitude baroclinic waves,
J. Atmos. Sci.
,
34
, 1689-1695.
Rossby, C. G. (1926), On the solution of problems of atmo-
spheric motion by means of model experiments,
Mon.
Weather Rev.
,
54
, 237-240.
Saffman, P. G. (1971), On the spectrum and decay of random
two-dimensional vorticity distributions of large Reynolds
number,
Stud. Appl. Math.
,
50
, 377-383.
Salmon, R. (1980), Baroclinic instability and geostrophic turbu-
lence,
Geophys. Astrophys. Fluid Dyn.
,
15
, 167-211.
Salmon, R. S. (1978), Two-layer quasi-geostrophic turbulence
in a simple special case,
Geophys. Astrophys. Fluid Dyn.
,
10
,
25-52.
Schneider, J., Dedieu, C., Le Sidaner, P., Savalle, R., and Zolo-
tukhin, I. (2011), Defining and cataloging exoplanets: The
exoplanet.eu database,
Astron. Astrophys.
,
532
, A79. doi:10.
1051/0004-6361/201116713.
Schneider, T., and C. C. Walker (2006), Self-organization of
atmospheric macroturbulence into critical states of weak non-
linear eddy-eddy interactions,
J. Atmos. Sci.
,
63
, 1569-1586.
Scott, R. B., and B. K. Arbic (2007), Spectral energy fluxes
in geostrophic turbulence: Implications for ocean energetics,
J. Phys. Oceanogr.
,
37
, 673-688.
Scott, R. B., and F. Wang (2005), Direct evidence of an
oceanic inverse energy cascade from satellite altimetry,
J. Phys.
Oceanogr.
,
35
, 1650-1666.
Showman, A. P., J. Cho, and K. Menou (2010), Atmospheric
circulation of extrasolar planets, in
Exoplanets
,editedby
S. Seager, pp. 471-516, Univ. of Arizona Press, Tueson, Ariz.
Sitte, B., and C. Egbers (2000), Higher order dynamics of
baroclinic waves, in
Physics of Rotating Fluids. Proc. 11th
Int. Couette-Taylor Workshop, July 20-23, 1999, Bremen,
Germany
. C. Egbers and G. Pfister (Eds), LNP 549, pp. 355-
375. Springer-Verlag, Berlin & Heidelberg.
Spence, T. W., and D. Fultz (1977), Experiments on wave-
transition spectra and vacillation in an open rotating cylinder,
J. Atmos. Sci.
,
34
, 1261-1285.
Stemler, T., and K. Judd (2009), A guide to using shadow-
ing filters for forecasting and state estimation,
Phys. D
,
238
,
1260-1273.
Stone, P. (1972), A simplified radiative-dynamical model for the
static stability of rotating atmospheres,
J. Atmos. Sci.
,
29
,
405-418.
