“…Different radiometer models were used by the participating institutions: (i) CIMEL CE318 sun/sky-radiometer, the standard instrument of the AERONET network (Holben et al, 1998) and its sub-networks AEROCAN, PHOTONS and RIMA; (ii) PREDE POM02 sun/sky-radiometer, adopted by the SKYNET network (Kim et al, 2004); (iii) Precision Filter Radiometer (PFR), designed by the Swiss PhysikalischMeteorologisches Observatorium Davos World Radiation Center (PMOD/WRC) and used in the World Meteorological Organization Global Atmospheric Watch (WMO/GAW) network (Wehrli, 2000); (iv) CartereScott SP01A and SP02 models, used by the Australian Bureau of Meteorology in its national network (Mitchell and Forgan, 2003) and by the National Oceanic & Atmospheric Administration/Global Monitoring Division (NOAA/GMD); (v) SP1A sun photometer, manufactured by Dr. Schulz & Partner GmbH and operated by the Alfred Wegener Institute for Polar and Marine Research (AWI) at their Antarctic and Arctic stations (Herber et al, 2002); (vi) ASP-15WL, designed at the Institute of Atmospheric Sciences and Climate (ISAC) of the Italian National Research Council (CNR), and deployed at the Italian Terra Nova Bay station (Antarctica) during summer campaigns (Tomasi et al, 2007). Alongside the above fully automated instruments, some hand-held MICROTOPS II sun photometers of Solar Light Company Inc. were operated during the two campaigns, this instrument being particularly suitable for itinerant campaigns or harsh environmental conditions, since it does not require the use of solar trackers and data acquisition systems (Smirnov et al, 2011). Their results were evaluated separately from that of the sun-tracking instruments, and were not utilized in the final evaluations of uncertainty parameters, because, as will be shown, precision achievable with this kind of instruments is not sufficiently high for AOD retrievals in polar regions.…”