The HATS sonic array permitted finite difference estimates of vertical gradients to be made from the spatially-filtered measurements at two heights, which are applicable at the vertical mid-point of the two horizontal lines of sonics. On the other hand, finite difference estimates of crosswind gradients were made from the spatially-filtered measurements made at 5 crosswind distances by the nine sonic array at one of the heights. Thus the vertical and crosswind gradient estimates apply at two different heights, the vertical mid-point of the two horizontal lines of sonics and the height of the nine-sonic line. An improvement was made for the OHATS project by using nine sonics in both of the vertically-displaced lines of sonics. Thus crosswind (and streamwise) gradient estimates can be made at both heights and averaged to provide horizontal gradient estimates at the same height as the vertical gradient estimates, the vertical mid-point of the two horizontal lines of sonics.
Secondly, the vertical spacing between the two lines of sonics during the HATS field project was equal to the sonic spacing for the first sonic array geometry, but increased to twice the sonic spacing for the other three array geometries. It was found that the equal spacing of the first HATS array provided a better match between the spatial response of the vertical and horizontal gradient estimates. Thus for OHATS, the vertical spacing of the two lines of sonics was made equal to the horizontal sonic spacing, 58 cm.
The possibility of flow distortion by the sonic arrays was monitered during the HATS field project by deploying two sonics at the same heights as the horizontal sonic arrays, but on an independent tower separated by 10 m from the horizontal arrays. The turbulence statistics measured by each of the sonics within the sonic arrays were then compared to the measurements by the independent sonics. For all four of the HATS sonic array geometries, the turbulence statistics within the array agreed with those measured by the independent sonics.
However, the proposed OHATS array has a closer vertical spacing and more sonics than used during any of the HATS arrays Therefore a pre-project test was made at the Marshall, CO, field site to examine the possibility of flow distortion by the OHATS array. The Marshall array consisted of two horizontal ASTER masts at nominal heights of 4.75 m and 5.27 m. (Because of interference between the cross-bracing of the vertical ASTER masts and the attachment hardware, we could not separate the horizontal masts by the desired 58 cm and had to settle for 52 cm.) The horizontal masts are oriented east-west so that winds from the south are perpendicular to them. About 6 m to the west, we erected a reference tower. Nine sonic yokes were placed on each of the two horizontal masts, with a spacing of 58 cm, and CSAT electronics were mounted on the back of the masts in the intervening spaces. Sonics were mounted at the center three locations on both horizontal masts and at the same two heights on the reference tower. Photos of the Marshall array can be seen at the bottom of the OHATS photo page.
The sonics are designated as, e.g. u3, l2, etc, with u and l referring to the upper and lower arrays and the ordinal number increasing from west to east. Thus u1 and l1 are the reference sonics and u3 and l3 are the center sonics in the horizontal arrays. The specific sonics are:
Data were collected from May 1-12 and the results are summarized below as linear fits of the flow statistics from the horizontal array sonics to the reference sonics. The data used for the comparisons were restricted to wind directions within ±45° of normal to the array (nominally SW to SE). Here nmr denotes the mean absolute deviation from the linear fit, normalized by the standard deviation of data. The conclusion is that the flow distortion caused by the sonic array is minimal.
Wind Speed (942 5-min averages):
Spdu2 = 0.987 Spdu1 + 0 cm/s; nmr = 0.042
Spdu3 = 0.983 Spdu1 + 1 cm/s; nmr = 0.044
Spdu4 = 0.988 Spdu1 + 3 cm/s; nmr = 0.043
Spdl2 = 0.994 Spdl1 + 0 cm/s; nmr = 0.045
Spdl3 = 0.992 Spdl1 - 1 cm/s; nmr = 0.044
Spdl4 = 0.984 Spdl1 + 1 cm/s; nmr = 0.044
Turbulent Kinetic Energy (942 5-min averages; TKE < 5 m^2/s^2):
TKEu2 = 0.984 TKEu1 + 1e-3 m^2/s^2; nmr = 0.069
TKEu3 = 0.978 TKEu1 + 2e-3 m^2/s^2; nmr = 0.070
TKEu4 = 0.993 TKEu1 + 1e-3 m^2/s^2; nmr = 0.071
TKEl2 = 0.994 TKEl1 + 0e-3 m^2/s^2; nmr = 0.072
TKEl3 = 0.995 TKEl1 + 0e-3 m^2/s^2; nmr = 0.073
TKEl4 = 0.984 TKEl1 + 0e-3 m^2/s^2; nmr = 0.074
Friction velocity (359 15 min averages):
u*u2 = 0.999 u*u1 + 1 cm/s; nmr = 0.202
u*u3 = 0.995 u*u1 + 1 cm/s; nmr = 0.209
u*u4 = 0.965 u*u1 + 1 cm/s; nmr = 0.215
u*l2 = 1.01 u*l1 + 1 cm/s; nmr = 0.204
u*l3 = 0.986 u*l1 + 1 cm/s; nmr = 0.222
u*l4 = 0.960 u*l1 + 1 cm/s; nmr = 0.208 [an error occurred while processing this directive]
This page was prepared by Tom Horst, NCAR Earth Observing Laboratory.