Ba. Bodhaine et al., NEW ULTRAVIOLET SPECTRORADIOMETER MEASUREMENTS AT MAUNA-LOA-OBSERVATORY, Geophysical research letters, 23(16), 1996, pp. 2121-2124
A research-grade scanning UV spectroradiometer was installed at Mauna
Loa Observatory (MLO), Hawaii, in July 1995. This instrument, built ar
ound a commercially available double monochromator, is interfaced with
a PC to provide automatic control and data acquisition. The spectral
range sampled by the instrument is 290-450 nn, and the bandpass is abo
ut 1 nm. A complete scan requires about 200 seconds and is performed e
very 5 degrees of solar zenith angle (SZA) during daylight hours. Cali
bration is performed on site at g-month intervals using a 1000-W stand
ard quartz-halogen FEL lamp with calibration traceable to NIST. The UV
irradiances measured at MLO are much more intense than at low altitud
e midlatitude locations. For observations at a SZA of 45 degrees, the
erythemally weighted UV can exceed 18 mu W cm(-2), which is approximat
ely 15-20% greater than the maxima seen at Lauder, New Zealand, for si
milar ozone amounts. The difference is primarily due to the higher alt
itude at MLO. For overhead sun conditions at MLO, erythemal UV can exc
eed 45 mu W cm(-2) which to our knowledge is the highest recorded anyw
here at the Earth's surface. UV irradiance is strongly correlated (inv
ersely) with Dobson spectrophotometer total ozone measurements at MLO,
with higher correlations at shorter wavelengths. The radiative amplif
ication factor (RAF) for erythema at MLO is about 1.44 +/- 0.46 at SZA
45 degrees. Using ozone retrievals from the UV spectra themselves, th
e deduced RAF for erythema is 1.26 +/- 0.38. The RAFs for erythema at
SZA 60 degrees are similar, and in agreement with other determinations
within the limits of experimental uncertainty.