Articles | Volume 11, issue 3
Nonlin. Processes Geophys., 11, 363–370, 2004
https://doi.org/10.5194/npg-11-363-2004
Nonlin. Processes Geophys., 11, 363–370, 2004
https://doi.org/10.5194/npg-11-363-2004

  02 Aug 2004

02 Aug 2004

Nonlinear instability of baroclinic atmosphere with reference to planetary scale disturbances

I. A. Pisnichenko I. A. Pisnichenko
  • Center for Weather Forecasting and Climate Studies/Brazilian National Institute for Space Research, Brazil, on leave from A. M. Obukhov Institute of Atmospheric Physics, Russian Academy of Sciences, Moscow, Russia

Abstract. In this paper we investigate the stability of zonal flow in a baroclinic atmosphere with respect to finite-amplitude planetary-scale disturbances by applying Arnold's method. Specifically, we examine the sign of the second variation of a conserved functional for the case of a polytropic atmosphere (i.e. one with a linear lapse rate) and with a linear profile of zonal wind. Sufficient stability conditions for an infinite atmosphere (i.e. with a temperature lapse rate equal to zero) are satisfied only for an atmosphere in solid body rotation. For a polytropic atmosphere of finite extent (a lapse rate is not equal zero) the sufficient conditions of stability can be satisfied if a lid is placed below min (Zmax, polytropic atmospheric height). The dependence of height Zmax on values of the vertical gradient of the zonal wind and the zonal temperature distribution is calculated.