Large Aperture Scintillometer (LAS) data at location no. 16 in CASES99 network of flux towers version 1.0 1. Authors and data source: Wageningen University (the Netherlands) Oscar Hartogensis, Bas van de Wiel 2. Description of the sensor 2.1. Sensor type Large Aperture Scintillometer, built by Wageningen University 2.2. Theory in a nutshell: The Large Aperture Scintillometer (LAS) consists of a transmitter and receiver. The transmitter emits a near parallel 15 cm beam of near infra red light. The light intensity of this beam is determined at the receiver placed at a distance of 300m to 5000m from the transmitter. Following wave propagation theory for strong turbulence intensity fluctuations caused by turbulent fields along the path can be evaluated into a value of Cn2, the structure parameter of the refractive index. To distinguish the scintillometer emitted infra red radiation from ambient radiation, it is modulated at 7kHz. The scintillometer is designed such that it outputs both the average received intensity signal (the demodulated signal) and Cn2. 2.3. Location: Location no. 16 in CASES99 network of flux towers; co-ordinates N37’38.611’ W096’44.233’ 2.4. Set-up: Receiver was installed at 5.17m height in the flux tower at location no. 16. Transmitter was installed at 3.40m height on a tri-pod. Scintillometer path was 420m in a NNE – SSW direction. A small field survey had been conducted to establish the extend of the sloping terrain along the scintillometer path. In the table below the heights are given relative to the surface at the scintillometer transmitter, which is indicated by (*); the receiver is indicated by (**). The table represents a grid around the scintillometer path with intervals of 75 m between the points. -1.2 0.05 1.45 2.35 -0.25 -0.6 0 (*) 1.4 2.7 1.65 0.9 0.9 1.9 2.7 2.65 1.55 1.4 2.45 3.7 4.05 2.2 1.25 2.25 3.05 4.1 1.5 1.65 (**) 1.6 2.85 4.2 3 2.5 2.3 2.9 4 3.1 3.75 3 2.95 Data was logged with a micro-world G2 datalogger (12 bits) built-in in the receiver. 3. Description of derived variables A crude quality control test has been performed based on the following criteria: error code is set to 0 (bad data) if demodulated signal is more than –200mV, standard deviation of the demodulated signal is more than 25 mV, if Cn2 < 10^-17 m^-2/3 or more than 0.5*10^-11. These are rule of thumb estimations to rule out a distorted signal due to misalignment, dew formation on the windows, rain, or any intensity fluctuations in the signal caused by something else then turbulence (e.g. tower movement, birds flying through the path etc.). Invalid or no data are given as a dummy “-9999”. The columns in the data files are labelled; here follows an overview of all the variables with their label names and units: YYYYMMDDHHMMSS : Time in CASES99 standard time format [UTC] DOY : Day of Year [CDS] HH,MMSS : Decimal time, where minutes and seconds are expressed as a fraction of an hour [CDS] error : Flag which is set to 1 for good data, and 0 for bad data; description of error is given above [-] demod: average received demodulated signal intensity [mV] sd(demod): standard deviation of demod [mV] Cn2: Structure parameter of the refractive index, scaled with a factor of 10^15 [10^15m^-2/3] sd(Cn2): standard deviation of Cn2 [10^15m^-2/3] 4. Sample period Sample period = 1s Averaging period = 1 minute averaged data were stored. All data for the whole experiment are given in one plain ASCII file; the columns are space separated 5. Data availability The LAS has been in continuous operation between 1002 17:30 and 1028 14:00 local (CDS) time.