“…Global measurements of W can be assessed from satellite observations [e.g., Smith, 1991] generally at low temporal resolution [Tobin et al, 2006]. To address such limitation a wide range of ground-based measurements of W are currently done through intense observational programs, including Sun photometry [e.g., Alexandrov et al, 2009], radiosondes [e.g., Durre et al, 2006], Raman lidar systems [e.g., Whiteman et al, 2010Whiteman et al, , 2012, Fourier transform spectrometers [e.g., Leblanc et al, 2011], microwave radiometers [e.g., Cadeddu et al, 2013], and Global Positioning System (GPS) receivers [e.g., Elgered et al, 1997;Ware et al, 2001].…”