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Introduction


The Puna of Atacama is a high altitude intertropical very dry desert region placed on the Andes mountains in the latitude-longitude range of about (12º - 24º S, 65º - 71º W). Since in the summer Southern Hemisphere the Earth-Sun actual distance is the lowest one (it pass at the minimum distance, in the beginning of January), the corresponding extraterrestrial solar irradiance, proportional to the inverse square of the ratio of this distance to the mean one, is 6.4 % higher than the Northern Hemisphere one (see for example, Iqbal, 1983). Due to all these circumstances, which determine naturally low intertropical ozone total column and low aerosol atmospheric content, the global as well as UV solar irradiances are within the highest in the world (Piacentini and Herman, 1996; Piacentini and Cede, 2000).

The detailed knowledge of the solar UV irradiance is of great importance in relation to its absolute value in each region of the Earth as well as in order to determine its variation due to ozone and aerosol changes by natural or antropogenic causes (see for example, Herman et al, 2000). Also it is related to different biological and material degradation actions (UNEP, 1998; Zerefos and Bais, 1997).


Table 1. Solar risk qualification for the different ranges of the UV Index.


 

UV Index

Solar risk qualification
0-2.9
Very low
3-4.9
Low
5-6.9
Moderate
7-9.9
High
10-13.9
Very high
14 or more
Extreme


The solar risk measured though the UV index, is directly related to the erythemal irradiance (in SI units) through the factor 40 (or 0.04 when the common mW/m2 unit of irradiance is used). This irradiance is obtained multiplying the spectral solar UV irradiance by the well established erythemal action spectra of McKinlay and Diffey and integrating the product in the UV (280 nm - 400 nm) range. This action spectra measures the effectiveness of the incident photons in reddening the normal reference skin and it is mainly concentrated in the UVB (280 nm -320 nm) range. So, it is an alarm signal for skin damage (Jagger, 1985). Table 1 gives the relation between the numbers related to the solar UV Index and the qualification adopted for describing the correspondent erythemal intensity.


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