Lu Li, Liu Shaomin, Xu Ziwei, et al. Results from measurements of large aperture scintillometer over different surfaces. J Appl Meteor Sci, 2009, 20(2): 171-178.
Citation: Lu Li, Liu Shaomin, Xu Ziwei, et al. Results from measurements of large aperture scintillometer over different surfaces. J Appl Meteor Sci, 2009, 20(2): 171-178.

Results from Measurements of Large Aperture Scintillometer over Different Surfaces

  • Received Date: 2008-06-03
  • Rev Recd Date: 2009-02-05
  • Publish Date: 2009-04-30
  • For surface flux measurements, large aperture scintillometer (LAS) has become more and more popular in recent years. Compared with traditional observation techniques, it can measure surface fluxes on a larger scale (500 m-10 km). At present, LAS observation is not common in China. Beijing Normal University, associated with other institutes, has carried out several short term measurements of LAS at Xiao tangshan (Beijing, 2002, 2004). A long-term LAS site has also been constructed at Miyun (Beijing) in June, 2006. Sensible heat flux (H) calculation with the LAS data of above measurements shows that the beam height of LAS and wind speed are sensitive factors for sensible heat flux measurement (HLAs), zeroplane displacement height is crucial unless the beam height is much lager than it, and Bowen ratio needs to be determined accurately over wet surface, while air temperature, air pressure and aerodynamic roughness length are not sensitive for HLAs. There are two key points of HLAS calculation under stable condition. First, there is much less agreement on the form which universal stability function fT should take. In this study, the fT function proposed by Andreas (as in the LAS manual) is used. Further more, since the iteration process of HLAS can not be convergence when low wind speed and very stable conditions appearing at night, ψm≥-5 is specified. Second, the scintillometer is unable to determine the sign of the heat flux. Richardson Number Ri can be used to determine atmospheric stability and fix the sign of HLAS. Besides, the sunrise-sunset time and net radiation could be used for this purpose if there is no wind and air temperature profiles. Therefore, a calculation scheme of 24-hour sensible heat flux observed by LAS is obtained after settling the above two key points. According to the observations mentioned above, LAS can measure surface fluxes both over homogeneous and heterogeneous surfaces. The daily and monthly variation of HLAs is analyzed. And the observation differences between eddy covariance system and LAS, need to be studied further combined with footprint model and energy unbalance of eddy covariance system observation.
  • Fig. 1  Daily variation of HLAS, HEC and Rn with the sign of HLAS determined by the measured HEC(HLAS1), Richardson number (HLAS2), sunrise-sunset time (HLAS3) and net radiation (HLAS4)

    Fig. 2  Daily variation of HLAS, HEC and Rn over homogeneous, heterogeneous surfaces

    Fig. 3  Monthly variation of HLAS and HEC in 2007 of Miyun

    Table  1  Statistics of HLAS flux estimated with different β against the reference value

    Table  2  Statistics of HLAS estimated under different conditions of u and T against the reference value

    Table  3  Statistics of HLAS estimated under different conditions of d, z0m and zLAS against the reference value

    Table  4  Statistics of HLAS estimated with different fT_functions against the one with fT_Andreas under stable condition

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    • Received : 2008-06-03
    • Accepted : 2009-02-05
    • Published : 2009-04-30

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