Study of the Spacial and Temporal Structure of Turbulence in the Nocturnal Residual Layer

  • Frank R. Freedman
  • Robert D. Bornstein
Part of the NATO • Challenges of Modern Society book series (NATS, volume 22)


Of the planetary boundary layer (PBL) sublayers defined by Stull (1988, pp. 10–11), the nighttime residual layer (RL) may be the least understood. One reason for this is that, unlike the daytime convective boundary layer and surface based nocturnal boundary layer, the RL is in general decoupled from the surface. Consequently, turbulence in the RL does not scale with surface turbulent quantities, and derivation of accurate similarity relationships is difficult, if not impossible. Although qualitative success has been achieved in relating RL turbulence to the gradient Richardson number (Ri) (Mahrt et al., 1979; Lenschow et al., 1987; Kim and Mahrt, 1992), oftentimes these scalings quantitatively fail due to overly coarse vertical differencing in computing Ri (Padman and Jones, 1985). Study of RL turbulence is further complicated by the wide variety of atmospheric forcing mechanisms present during the night. Since nighttime turbulent intensities are small, forcing by radiation, baroclinity, topographic drainage flows, and gravity waves can become important. Variability in each of these leads to a seemingly infinite number of possible RL turbulent time/height structures (e. g., André et al., 1978; Garratt, 1985; Lenschow et al., 1978; Heilman and Takle, 1991; Weber and Kurzeja, 1991).


Turbulent Kinetic Energy Planetary Boundary Layer Wind Shear Geostrophic Wind Residual Layer 


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  1. André, J.C., De Moor, G., Lacarrère, P., Therry, G., and Du Vachat, R., 1978, Modeling the 24-hour evolution of the mean and turbulent structures of the planetary boundary layer,. J. Atmos. Sci. 35: 1861–1883.CrossRefGoogle Scholar
  2. Clarke, R.H., Dyer, A.J., Brook, R.R, Reid, D.G., Troup, A.J., 1971, The Wangara Experiment: Boundary Layer Data, Commonwealth Scientific and Industrial Research Organization, Australia.Google Scholar
  3. Freedman, F.R, 1996, Reevaluation of lower order turbulence closure prediction the PBL, M.S. thesis, San Jose State University.Google Scholar
  4. Garratt, J.R., 1985, The inland boundary layer at low altitudes, Bound. Layer Meteor. 42: 307–327.CrossRefGoogle Scholar
  5. —, and Brost, R.A., 1981, Radiative cooling effects within and above the nocturnal boundary layer, J. Atmos. Sci. 38: 2730–2746.CrossRefGoogle Scholar
  6. Heilman, W.E., Takle, ES., 1991, Numerical simulation of the nocturnal turbulence characteristics over Rattlesnake Mountain, J. Appl Meteor. 30: 1106–1116.CrossRefGoogle Scholar
  7. Kim, J., and Mahrt, L., 1992, Simple formulation of turbulent mixing in the stable free atmosphere and nocturnal boundary layer, Tellus 44A: 381–394.Google Scholar
  8. Lenschow, D.H., Li, X.S., Zhu, C.J., and Stankov, B.B., The stably stratified boundary layer over the Great Plains, Bound. Layer Meteor. 42: 95-121.Google Scholar
  9. Mahrt, L., Heald, R.C., Lenschow, D.H., and Stankov, B.B., 1979, An observational study of the structure of the nocturnal boundary layer, Bound. Layer Meteor. 17: 247–264.CrossRefGoogle Scholar
  10. Miles, J.W., 1961, On the stability of heterogeneous shear flows, J. Fluid Mech. 10: 496–508.CrossRefGoogle Scholar
  11. Neu, U., Künzle, T., and Wanner, H., 1994, On the relation between ozone storage in the residual layer and daily variation in near-surface concentration-a case study, Bound. Layer Meteor. 69: 221–247.CrossRefGoogle Scholar
  12. Padman, L., and Jones, I.S.F., 1985, Richardson number statistics in the seasonal thermocline, J. Phys. Oceanogr. 15(7): 844–854.CrossRefGoogle Scholar
  13. Schayes, G., Thunis, P., and Bornstein, R.D., 1996, Topographic vorticity-mode mesoscale-β (TVM) model: Part I-formulation, J. Appl. Meteor. 35: 1815–1823.CrossRefGoogle Scholar
  14. Stull, R. B., 1988, An Introduction to Boundary Layer Meterology, Kluwer Academic Pub., Dordrecht.Google Scholar
  15. Therry, G., and Lacarrère, P., 1983, Improving the eddy kinetic energy model for planetary boundary layer description, Bound Layer Meteor. 25: 63–88.CrossRefGoogle Scholar
  16. Weber, A.H., and Kurzeja, R.J., 1991, Nocturnal planetary boundary layer structure and turbulence episodes during the project STABLE field program, J. Appl. Meteor. 30: 1117–1133.CrossRefGoogle Scholar
  17. Yamada, T., and Mellor, G., 1975, A simulation of the Wangara atmospheric boundary layer data, J. Atmos. Sci. 32: 2309–2329.CrossRefGoogle Scholar

Copyright information

© Springer Science+Business Media New York 1998

Authors and Affiliations

  • Frank R. Freedman
    • 1
    • 2
  • Robert D. Bornstein
    • 2
  1. 1.Department of Civil EngineeringStanford UniversityStanfordUSA
  2. 2.Department of MeteorologySan Jose State UniversitySan JoseUSA

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