Abstract

Hawai’i Island often receives extreme (UV Index ≥ 11) solar ultraviolet radiation (UVR). While the UV Index (UVI) has been measured since 1997 at Hawai’i’s high-altitude Mauna Loa Observatory (MLO), measurements where people live and recreate are rare. We measured UVI on the face of a rotating mannequin head with UVR sensors at its eyes, ears and cheeks while simultaneously measuring the UVI with a zenith-facing sensor at MLO and seven sites at or near sea level from 19 July to 14 August 2018. The mannequin sensors received higher UVR at midmorning and midafternoon than at noon. For example, at sea level the peak UVI at the left cheek was 5.2 at midmorning and 2.9 at noon, while the horizontal UVI at noon was 12.7. Our measurements were supplemented with wide-angle (190° and 360°) sky photographs and UV images of the mannequin head. Because the UVI applies to horizontal surfaces, people in tropical and temperate latitudes should be informed that their face may be more vulnerable to UVR at midmorning and midafternoon than at noon. Finally, our instruments provided opportunities to measure unexpected UVR-altering events, including rare biomass smoke over MLO and spectroscopic measurements of substantial UVR-absorbing sulfur dioxide in the eruption plume of the Kilauea volcano.

Highlights

  • Solar ultraviolet radiation (UVR) has been measured by a suite of well-maintained instruments atHawai’i Island’s high-altitude (3400 m) Mauna Loa Observatory (MLO) for over 20 years [1]

  • While the UVR measured at and near sea level was significantly modulated by clouds and vog during many days, sky conditions allowed mannequin head deployments during some or all of 14 days

  • The global UVR measured by the PMA1102 is superimposed over the mannequin head data in Figure 5, which makes the very significant reduction in the UV Index (UVI) at solar noon especially obvious

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Summary

Introduction

Solar ultraviolet radiation (UVR) has been measured by a suite of well-maintained instruments at. This report describes a 13-month field study on Hawai’i Island between December 1994 and January 1996, during which UVR was measured from near sea level at Hilo and along traverses to and from the summit of Mauna Kea (4205 m) and MLO (3400 m) on the north slope of Mauna Loa. This study used. Robertson–Berger UVR radiometers (Model 501 A) [3] that measure the band of UVR wavelengths (280–400 nm) responsible for the reddening of human skin (erythema) and skin cancer. MLO to skies that alter the a wide variety of sky conditions These range from the pristine sky over MLO to skies that alterUVI the with clouds, smoke fromfrom dry season fires fires and vog, a haze of volcanic origin composed of gaseous.

Old Kona Airport
Health Effects of UVR
Instrumentation
Discussion
Methodology
Results and Discussion
Mannequin Head Results
UVI Noon Minimum
Horizontal
UVI Measurement Challenges
Ozone Error
Cosine Error
UVR and Volcanic Sulfur Dioxide
Kilauea of the Kilauea aerosols in the eruption plume fromfrom
Cameras used in in the the UVI
Conclusions
Full Text
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