The relatively large temperature response is related to positive feedbacks which enhance the initial impact of changed
snow grain size.
MODIS - based Mosaic of Antarctica (MOA) data sets: Continent - wide surface morphology and
snow grain size.
The relatively large temperature response is related to positive feedbacks which enhance the initial impact of changed
snow grain size.
But Dumont and her colleagues have found that, since 2009, there has been a darkening that can not be explained by larger
snow grain size alone.
Not exact matches
Two properties dominate reflectivity in dry
snow — the
size of
snow grains, which become larger and more absorbent as they melt, and the presence of dark impurities that absorb the sun's energy, predominantly black carbon and mineral dust, which also cause the
snow to melt faster.
Nakamura, T., Abe, O., Hasegawa, T., Tamura, R., Ohta, T. (2001) Spectral reflectance of
snow with a known
grain -
size distribution in successive metamorphism.
This is, however, a complex process: the reflection by
snow results from scattering of sunlight by numerous
snow grains with largely varying shapes and
sizes.
Freshly fallen
snow reflects up to 84 percent of incoming sunlight, but during the warm season the reflectivity declines as the ice
grains within the snowpack change shape and
size.
Smaller -
sized graupels are generally referred to as
snow grains.
The
snow albedo depends not only on
snow grain shapes but also their
sizes and other factors like impurities in
snow.
This is, however, a complex process: the reflection by
snow results from scattering of sunlight by numerous
snow grains with largely varying shapes and
sizes.
Soon after
snow falls, its
grains begin to change shape and
size.