AMSR-E Algorithm for Snowmelt Onset Detection in Subarctic Heterogeneous Terrain

Snowmelt onset in the upper Yukon River basin, Canada, can be derived from brightness temperatures (Tb) obtained by the Advanced Microwave Scanning Radiometer for EOS (AMSRE) on NASA’s Aqua satellite. This sensor, with a resolution of 14 x 8 km for the 36.5 GHz frequency and two to four observations per day, improves upon the twice-daily coverage and 37 x 28 km spatial resolution of the Special Sensor Microwave Imager (SSM/I). The onset of melt within a snowpack causes an increase in the average daily 36.5 GHz vertically polarized Tb as well as a shift to high diurnal amplitude variations (DAV) as the snow melts during the day and refreezes at night. The higher temporal and spatial resolution makes AMSR-E more sensitive to sub-daily Tb oscillations, resulting in DAV that often show a greater daily range compared to SSM/I. Therefore, thresholds of Tb > 246 K and DAV > ±10 K developed for use with SSM/I have been adjusted for detecting melt onset with AMSR-E using ground-based surface temperature and snowpack wetness relationships. Using newly developed thresholds of Tb > 252 K and DAV > ±18 K, AMSR-E determined snowmelt onset correlates well with SSM/I observations in the small subarctic Wheaton River basin through the 2004 and 2005 winter/spring transition. In addition, snowmelt onset derived from AMSR-E data gridded at a higher resolution than the SSM/I data indicates that finer-scale differences in elevation and land cover affect snowmelt onset and are detectable with the AMSR-E sensor. Based on these observations, the enhanced resolution of AMSR-E is more effective than SSM/I at delineating spatial and temporal snowmelt dynamics in the heterogeneous terrain of the upper Yukon River basin.