This paper describes a model of the general circulation of the earth's atmosphere which has been developed at the Computing Center of the Siberian Branch of the USSR Academy of Sciences. Formulated in spherical coordinates, the vertical coordinate being the Phillips' coordinate sigma , the primitive hydrothermodynamics equations are reduced to a symmetrized semidivergent form. Methods of parameterization of subgrid scale processes are outlined briefly. The method of solution is based on the partition method. The results of a numerical experiment on the modeling of the average January atmosphere circulation for given average January ocean surface temperature and sun declination are presented.
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Texas A&M Univ, Dept Atmospher Sci, College Stn, TX 77843 USATexas A&M Univ, Dept Atmospher Sci, College Stn, TX 77843 USA
Gu, Boyan
Ren, Tong
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Texas A&M Univ, Dept Atmospher Sci, College Stn, TX 77843 USATexas A&M Univ, Dept Atmospher Sci, College Stn, TX 77843 USA
Ren, Tong
Kuo, Chia-Pang
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Texas A&M Univ, Dept Atmospher Sci, College Stn, TX 77843 USA
Cooperat Inst Res Atmosphere, Ft Collins, CO USATexas A&M Univ, Dept Atmospher Sci, College Stn, TX 77843 USA
Kuo, Chia-Pang
Yang, Ping
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Texas A&M Univ, Dept Atmospher Sci, College Stn, TX 77843 USATexas A&M Univ, Dept Atmospher Sci, College Stn, TX 77843 USA
Yang, Ping
Bowman, Kenneth
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Texas A&M Univ, Dept Atmospher Sci, College Stn, TX 77843 USATexas A&M Univ, Dept Atmospher Sci, College Stn, TX 77843 USA
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Russian Acad Sci, Space Res Inst, Moscow, Russia
State Univ, Moscow Inst Phys & Technol, Moscow, RussiaRussian Acad Sci, Space Res Inst, Moscow, Russia
Shaposhnikov, D. S.
Rodin, A. V.
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Russian Acad Sci, Space Res Inst, Moscow, Russia
State Univ, Moscow Inst Phys & Technol, Moscow, RussiaRussian Acad Sci, Space Res Inst, Moscow, Russia
Rodin, A. V.
Medvedev, A. S.
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Max Planck Inst Solar Syst Res, Gottingen, GermanyRussian Acad Sci, Space Res Inst, Moscow, Russia