With the availability of multiple years of data from new and improved passive instruments launched as part of the Earth Observing System (EOS) and active instruments belonging to the A-Train constellation (L'Ecuyer and Jiang 2010), a more
complete observational record of ERB variations and the underlying processes is now possible.
Not exact matches
The more direct measure of global warming provided by measuring the energy content of the climate system avoids many of these problems, although the
observational record is shorter and less
complete (e.g. Church et al 2011).
Moreover, while there are other variants, we have this
observational record for the
complete area and we don't have to worry about sampling bias and homogenization.