“…The upward pointing probe is equipped with a cosine receptor (PP-Systems) to correct sky irradiance measurements for varying solar altitudes. The downward looking probe measures canopy reflectance at a zenith angle of 62° to account for canopy clumping (Chen and Black, 1991) The sampling area for the eddy covariance measurements or "flux-footprint" depends on windspeed and atmospheric conditions (Leclerc and Thurtell, 1990), and can range from a few hectares to a few square-kilometres (Schmid and Lloyd, 1999). However, the area to which flux measurements are most sensitive, also referred to as peak footprint, is much smaller and covers a radius of only 100-300 m (Blanken et al, 2001, Kljun et al, 2004.…”