Overview of
Solar and Thermal Atmospheric Radiation (STAR)
STAR is a subdivision of the NOAA Climate
Monitoring and Diagnostics Laboratory. The STAR group's activities
involve empirical and theoretical research
of the Earth's surface radiation budget. The group specializes in
the investigation of climatically significant variations in long-term
radiation and meteorological measurements
made primarily at a globally diverse network
of surface sites. Our research interests are in the extent and cause
of observed variations, and in collaborating with other research
groups making satellite observations and climate model calculations.
In addition, we make some relative observations of spectral solar
radiation for the purpose of remote sensing of certain atmospheric
constituents. A relatively new program in the group is the absolute
measurement of spectral solar UV for the investigation of the interaction
of ozone and solar radiation.
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