NCAR global General Circulation Model of the atmosphere

This paper describes a model of the general circulation of the earth’s atmosphere which has been developed and experimented with, since 1964, at the National Center for Atmospheric Research (NCAR), Boulder, Colo. A distinguishing feature of the NCAR model is that the vertical coordinate is height rather than pressure, though hydrostatic equilibrium is maintained in the system. In fact, the dynamical framework of the model is very similar to the one proposed by L. F. Richardson in 1922. Various physical processes in the atmosphere, such as energy transfer due to solar and terrestrial radiation, small-scale turbulence and convection, etc., are incorporated in the model. An explicit prediction of the moisture field is avoided. Instead, it is assumed that the atmosphere is completely saturated by water vapor. Thus, the release of latent heat of condensation can be computed. In addition to a description of the model, the equations for the zonal mean and eddy energy are presented. Finally, a baroclinic stability analysis of the model is made in order to gain an insight into the finite-difference formulation of the present model. Long term (over 100 days) numerical integrations are being performed successfully with a two-layer version of the present model. Details of finite-difference schemes and the results of numerical calculations will be described in a separate article. “Perhaps some day in the dim future it will be possible to advance the computations faster than the weather advances and at a cost less than the saving to mankind due to the information gained. But that is a dream.” [From Weather Prediction by Numerical Process by L. F. Richardson, 1922.1

[1]  A. Arakawa Computational design for long-term numerical integration of the equations of fluid motion: two-dimen , 1997 .

[2]  Norman A. Phillips,et al.  The Equations of Motion for a Shallow Rotating Atmosphere and the “Traditional Approximation” , 1966 .

[3]  J. Deardorff,et al.  The Counter-Gradient Heat Flux in the Lower Atmosphere and in the Laboratory , 1966 .

[4]  Syukuro Manabe,et al.  NUMERICAL RESULTS FROM A NINE-LEVEL GENERAL CIRCULATION MODEL OF THE ATMOSPHERE1 , 1965 .

[5]  Syukuro Manabe,et al.  SIMULATED CLIMATOLOGY OF A GENERAL CIRCULATION MODEL WITH A HYDROLOGIC CYCLE II. ANALYSIS OF THE TROPICAL ATMOSPHERE , 1965 .

[6]  J. S. Winston,et al.  COMPUTATIONS OF ATMOSPHERIC ENERGY AND ITS TRANSFORMATION FOR THE NORTHERN HEMISPHERE FOR A RECENT FIVE-YEAR PERIOD , 1965 .

[7]  R. F. Strickler,et al.  Thermal Equilibrium of the Atmosphere with a Convective Adjustment , 1964 .

[8]  A. Wiin-nielsen,et al.  On Atmospheric Energy Conversions Between the Zonal Flow and the Eddies , 1963 .

[9]  J. Smagorinsky,et al.  GENERAL CIRCULATION EXPERIMENTS WITH THE PRIMITIVE EQUATIONS , 1963 .

[10]  A. Wiin-nielsen On baroclinic instability in filtered and non‐filtered numerical prediction models , 1963 .

[11]  A. H. Murphy,et al.  Numerical Weather Analysis and Prediction. , 1962 .

[12]  D. Richtmyer,et al.  A Survey of Difference Methods for Non-Steady Fluid Dynamics , 1962 .

[13]  Caskey,et al.  GENERAL CIRCULATION EXPERIMENTS WITH THE PRIMITIVE EQUATIONS I . THE BASIC EXPERIMENT , 1962 .

[14]  Syukuro Manabe,et al.  On the Radiative Equilibrium and Heat Balance of the Atmosphere , 1961 .

[15]  B. Saltzman,et al.  Further statistics on the modes of release of available potential energy , 1961 .

[16]  A. Kasahara,et al.  A NUMERICAL EXPERIMENT ON THE DEVELOPMENT OF A TROPICAL CYCLONE , 1961 .

[17]  J. E. McDonald,et al.  DIRECT ABSORPTION OF SOLAR RADIATION BY ATMOSPHERIC WATER VAPOR , 1960 .

[18]  J. S. A. Green,et al.  A problem in baroclinic stability , 1960 .

[19]  Walter M. Elsasser,et al.  Atmospheric radiation tables , 1960 .

[20]  A. Wiin-nielsen,et al.  A STUDY OF ENERGY CONVERSION AND MERIDIONAL CIRCULATION FOR THE LARGE-SCALE MOTION IN THE ATMOSPHERE ' , 2022 .

[21]  N. A. Phillips,et al.  A COORDINATE SYSTEM HAVING SOME SPECIAL ADVANTAGES FOR NUMERICAL FORECASTING , 1957 .

[22]  Robert M. White,et al.  On Conversions between Potential and Kinetic Energy in the Atmospher , 1956 .

[23]  Norman A. Phillips,et al.  The general circulation of the atmosphere: A numerical experiment , 1956 .

[24]  J. V. Mieghem The energy available in the atmosphere for conversion into kinetic energy , 1956 .

[25]  Edward N. Lorenz,et al.  Available Potential Energy and the Maintenance of the General Circulation , 1955 .

[26]  F. S. Johnson,et al.  THE SOLAR CONSTANT , 1954 .

[27]  Norman A. Phillips,et al.  Energy Transformations and Meridional Circulations associated with simple Baroclinic Waves in a two-level, Quasi-geostrophic Model , 1954 .

[28]  V. Starr Commentaries Concerning Research on the General Circulation , 1954 .

[29]  V. Starr Note Concerning the Nature of the Large-Scale Eddies in the Atmosphere , 1953 .

[30]  H. Kuo THE STABILITY PROPERTIES AND STRUCTURE OF DISTURBANCES IN A BAROCLINIC ATMOSPHERE , 1953 .

[31]  P. D. Thompson On the theory of large‐scale disturbances in a two‐dimensional baroclinic equivalent of the atmosphere , 1953 .

[32]  J. V. Mieghem Energy Conversions in the Atmosphere on the Scale of the General Circulation , 1952 .

[33]  H. Kuo A Note on the Kinetic Energy Balance of the Zonal Wind Systems , 1951 .

[34]  J. Miller ENERGY TRANSFORMATION FUNCTIONS , 1950 .

[35]  E. T. Eady,et al.  Long Waves and Cyclone Waves , 1949 .

[36]  J. G. Charney,et al.  THE DYNAMICS OF LONG WAVES IN A BAROCLINIC WESTERLY CURRENT , 1947 .

[37]  H. Panofsky METHODS OF COMPUTING VERTICAL MOTION IN THE ATMOSPHERE , 1946 .

[38]  Lewis F. Richardson,et al.  Weather Prediction by Numerical Process , 1922 .