  The distribution of ultraviolet (UV) radiation field provides critical
constraints on the physical environments of molecular clouds. Within 1 kpc of
our solar system and fostering protostars of different masses, the giant
molecular clouds in the Gould Belt present an excellent opportunity to resolve
the UV field structure in star forming regions. We performed spectral energy
distribution (SED) fitting of the archival data from the Herschel Gould Belt
Survey (HGBS). Dust radiative transfer analysis with the DUSTY code were
applied to 23 regions in 14 molecular complexes of the Gould Belt, resulting in
the spatial distribution of radiation field in these regions. For 10 of 15
regions with independent measurements of star formation rate, their star
formation rate and UV radiation intensity largely conform to a linear
correlation found in previous studies.
