The meeting covered the following areas:
By the time of the experiment:
Grossman and LeMone Will study diurnal variation of PBL for different surface evaporation conditions and gain confidence level in profilers. Special needs: raw profiler data (spectral data) should be recorded for five IOP's, synoptic-scale model analysis/prediction data plus synoptic surface data needed to determine forcing. Detailed satellite and model needs forthcoming.
Site-Selection and Instrumentation Issues discussed include (a) CO_2 fluxes at central site, Argonne site, ARL site, (b) Desire to have as many stations along flight track as possible, esp stations with CO_2 and/or ozone flux (c) 3 ASTER stations should have max 10-km spacing; desire over different land-use areas so can get time-series data over different types of surface.
Pielke and Zeng will use above instrumentation to (a) test and link surface flux scheme (BATS) to PBL scheme (that used in CCM2 or another), (b) use aircraft data to test feasibility of measuring impact of mesoscale eddies on fluxes, (c) aid Grossman/LeMone in defining surface characteristics. Special needs not already listed include: (a) Satellite: NDVI, skin temp, cloud fraction to derive other quantities (LAI, fractional vegetation cover (b)comparison satellite skin temp with that from surface and/or aircraft,
Careful launch procedures are critical; operators need special training, and will require a week to get up to speed.
Launch procedure: outdoor launch, insure LORAN lock, slow rise (3 m/s) wave sondes like pendulum to ventilate for good comparison to surface thermo. Must launch every day to keep operators up to speed (agreed that 2 p.m. good; if two/day 2nd sonde about sunrise). This should be possible with sondes we have. There should be 2 operators per launch; at least one must do this full time. Might try launches such that sondes are released and can record on the way down as well as the way up, a procedure tried successfully in Microfronts experiment.
Will be 3/4 mile N of highway 54, SW of Wichita and not too far from Wichita WSR-88D radar. This offers a clear horizon of the watershed. However. this location is 35 km from western boundary of CASES-97 triangle; thus beam about 600 m deep -- too deep for BL-depth determination but can perhaps use TREC to get some idea of horizontal wind variability; and use VAD-derived wind profiles.