AMIP II Diagnostic Subproject No. 15:
Atmospheric angular momentum and the planetary momentum balance
Project coordinators:
David A. Salstein1, Richard D. Rosen1
Jean O. Dickey2 and Steven L. Marcus2
 
1Atmospheric and Environmental Research, Inc., USA
2 Jet Propulsion Laboratory, California Institute of Technology, USA


Background

The behavior of atmospheric angular momentum (AAM) is important for any global circulation model to simulate because of its fundamental relationship to global climate variations on many time scales.  Fluctuations in AAM are also important to the angular momentum balance of the whole planet and are reflected in measurable planetary motions.  In AMIP-1, we examined the mean, seasonal, and interannual fluctuations of AAM relative to the Earth's mean rotation (Hide et al. 1997).  The annual cycle was captured very well by the models, and interannual fluctuations were reasonably well simulated, notably the global peaks and latitudinal anomalies associated with the El Nino/Southern Oscillation (Marcus and Dickey 1994). Nevertheless, not all features related to the ENSO cycle were successfully simulated; for example, the relative amplitudes of the ENSO peaks were generally not correct.

The AMIP-1 simulations of AAM were verified against data that extended up to the lower stratosphere.  Because the new NCEP reanalyses now incorporate the upper stratosphere, we will now be able to assess the simulation of important signals there, including elements of the quasi-biennial and semiannual oscillations (Salstein and Rosen 1997). In addition, the longer AMIP-2 period includes ENSO variability beyond that covered by AMIP-1, so that a larger number of ENSO-related AAM signals can be examined.  Newly available from analysis systems, too, are values of angular momentum exchanges between the atmosphere and other Earth components.  We can now assess how AMIP-2 models produce the friction and mountain torques that effect such exchanges (White 1991; Salstein and Rosen 1994; Madden and Speth 1995).

Besides the relative angular momentum highlighted in our AMIP-1 work, AMIP-2 allows us to assess the planetary portion of angular momentum, calculated from the surface pressure field.  Related as well are low-order harmonics of surface pressure (Chao and Au 1991; Dong et al. 1996), measures of the planetary mass distribution; interestingly, gravity anomalies from fluctuations in these harmonics can significantly perturb the orbits of Earth satellites, and observations are sensitive enough to detect such perturbations.

Changes in axial angular momentum, in particular, are mirrored by variations in the momentum of the solid Earth as measured independently by changes in length of day (Hide et al. 1997), while equatorial components of the AAM vector are associated with polar motion excitation. A full exposition of the AAM framework and its application to the global momentum balance is derived in Barnes et al.(1983); details of AAM calculations in an operational setting are given by Salstein et al. (1993).

The primary verification data that we intend to use for AMIP-2 are the relative and planetary atmospheric angular momentum values produced from the wind and surface pressure fields of the NCEP reanalysis system and other reanalyses and analysis systems (Salstein and Rosen 1997).  Although we will focus on monthly mean fields, we will also consider limited sets of daily values for the purpose of verifying statistics of high-frequency fluctuations.  We also plan to use other datasets to supplement reanalyses, such as satellite-based observations of the stresses over the ocean and of upper atmosphere winds, and geodetically-inferred variations in both the axial and equatorial components of global AAM.

Objectives

We will diagnose the mean climate and variability of the angular momentum of the atmosphere, and assess errors on mean, seasonal, and interannual time scales in the ensemble of AMIP-2 models.  To identify the sources of errors we will examine fields of the zonal wind and surface pressure simulations.  We will extend our diagnoses into the upper stratosphere to determine the ability of models to simulate signals in that layer, such as the quasi-biennial oscillation.  We will also determine the planetary component of angular momentum as well as torque mechanisms driving momentum changes in the atmosphere.

Approach
 
a.  Relative angular momentum and zonal winds

b.  Planetary angular momentum and mass field c. Torques Data Requirements
  References
For further information, contact David A. Salstein (salstein@aer.com), Richard D. Rosen  (rdrosen@aer.com) or the AMIP Project Office (amip@pcmdi.llnl.gov).


Last update: 5 January 1998.  This page is maintained by mccravy@pcmdi.llnl.gov

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