MARCH 1963 EDWARD N. LORENZ 141

must be unstable, in the sense that solutions temporarily approximating it do not continue to do so. A nonperiodic solution with a transient component is sometimes stable, but in this case its stability is one of its transient properties, which tends to die out.
To verify the existence of deterministic nonperiodic flow, we have obtained numerical solutions of a system of three ordinary differential equations designed to represent a convective process. These equations possess three steady-state solutions and a denumerably infinite set of periodic solutions. All solutions, and in particular the periodic solutions, are found to be unstable. The remaining solutions therefore cannot in general approach the periodic solutions asymptotically, and so are nonperiodic.
When our results concerning the instability of nonperiodic flow are applied to the atmosphere, which is ostensibly nonperiodic, they indicate that prediction of the sufficiently distant future is impossible by any method, unless the present conditions are known exactly. In view of the inevitable inaccuracy and incompleteness of weather observations, precise very-long-range forecasting would seem to be non-existent.
There remains the question as to whether our results really apply to the atmosphere- One does not usually regard the atmosphere as either deterministic or finite, and the lack of periodicity is not a mathematical certainty, since the atmosphere has not been observed forever.
The foundation of our principal result is the eventual necessity for any bounded system of finite dimensionality to come arbitrarily close to acquiring a state which it has previously assumed. If the system is stable, its future development will then remain arbitrarily close to its past history, and it will be quasi-periodic.
In the case of the atmosphere, the crucial point is then whether analogues must have occurred since the state of the atmosphere was first observed. By analogues, we mean specifically two or more states of the atmosphere, together with its environment, which resemble each other so closely that the differences may be ascribed to errors in observation. Thus, to be analogues, two states must be closely alike in regions where observations are accurate and plentiful, while they need not be at all alike in regions where there are no observations at all, whether these be regions of the atmosphere or the environment. If, however, some unobserved features are implicit in a succession of observed states, two successions of states must be nearly alike in order to be analogues.
If it is true that two analogues have occurred since atmospheric observation first began, it follows, since the atmosphere has not been observed to be periodic, that the successions of states following these analogues must eventually have differed, and no forecasting scheme could have given correct results both times. If, instead,

analogues have not occurred during this period, some accurate very-long-range prediction scheme, using observations at present available, may exist. But, if it does exist, the atmosphere will acquire a quasi-periodic behavior, never to be lost, once an analogue occurs. This quasi-periodic behavior need not be established, though, even if very-long-range forecasting is feasible, if the variety of possible atmospheric states is so immense that analogues need never occur. It should be noted that these conclusions do not depend upon whether or not the atmosphere is deterministic.
There remains the very important question as to how long is "very-long-range." Our results do not give the answer for the atmosphere; conceivably it could be a few days or a few centuries. In an idealized system, whether it be the simple convective model described here, or a complicated system designed to resemble the atmosphere as closely as possible, the answer may be obtained by comparing pairs of numerical solutions having nearly identical initial conditions. In the case of the real atmosphere, if all other methods fail, we can wait for an analogue.
Acknowledgments. The writer is indebted to Dr. Barry Saltzman for bringing to his attention the existence of nonperiodic solutions of the convection equations. Special thanks are due to Miss Ellen Fetter for handling the many numerical computations and preparing the graphical presentations of the numerical material. 

REFERENCES

- Birkhoff, G. O., 1927: Dynamical systems. New York, Amer. Math. Soc., Colloq Publ., 295 pp.
- Ford, L. R., 1933: Differentia1 equations. New York, McGraw-Hill, 264 pp.
- Fultz, D., R. R. Long, G. V. Owens, W. Bohan, R. Kaylor and J- Weil, 1959: Studies of thermal convection in a rotating cylinder with some implications for large-scale atmospheric motions. Meteor. Monog, 4(21), Amer. Meteor. Soc., 104 pp.
- Gibbs, J. W., 1902: Elementary principles in statistical mechanics. New York, Scribner, 207 pp.
- Hide, R., 1958: An experimental study of thermal convection in a rotating liquid. Phil. Trans. Roy. Soc. Lontlon, (A), 250, 441--478.
- Lorenz, E. N., 1960: Maximum simplification of the dynamic equations. Tellus, 12, 243-254.
___________, 1962a: Simplified dynamic equations applied to the rotating basin experiments. J. atmos. Sei., 19, 39-.51.
___________, 1962b: The statistical prediction of solutions of dynamic equations. Proc. Internat. Symposium Numerical Weather
Prediction, Tokyo, 629-635.
- Nemytskii, V. V., and V. V. Stepanov, 1960: Qualitative theory of
differential equations. Princeton, Princeton Univ. Press, 523 pp.
- Poincaré, H., 1881: Mémoire  sur les courbes définies par une équation différentielle.
J. de Math., 7, 375-442.
- Rayleigh, Lord, 1916: On convective currents in a horizontal layer of fluid when the higher temperature is on the under side.
Phil. Mag.,
32, 529-546.
- Saltzman, B., 1962: Finite amplitude free convection as an initial
value problem-I. J. atmos. Sci., 19, 329-341.

 
     
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