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Ozone layer depletion on the west coast of South America, map of stratospheric ozone distribution obtained from NASA (Jan 31st, 2005). Notice the depletion of the ozone layer over the west coast FO South America. 

Ozone layer depletion on the west coast of South America, map of stratospheric ozone distribution obtained from NASA (Jan 31st, 2005). Notice the depletion of the ozone layer over the west coast FO South America. 

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UV absorption in Valparaíso, Chile, is analyzed during the passage of a smoke column from a nearby forest fire. Total solar absorption is measured, UVB and UVA radiation, UV nanometre to nanometre between 295 nm and 315 nm. With the purpose of seeing what factors intervene in this absorption, tropospheric ozone and PM10 particulate material are mea...

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... city of Valpara ́ ıso is located on the central coast of Chile, with the following geographic coordinates: 33 01 S; 71 ◦ 38 W. The climate is subtropical, similar to moderate Mediterranean, with an average maximum temperature of 20 ◦ C. The coolest months are July and August even though the winter is benign due to the influence of offshore marine breezes which penetrate the Aconcagua valley. The rainy season occurs in the months of May, June and July, during which periods of rain of great intensity are possible. Predominant winds blow mainly towards South-Southeast throughout the year. This condition is interrupted during the rainy winter months during which the winds blow predominantly North-Northwest. Valpara ́ ıso, being on the west coast of South America, is exposed to an increase of UV radiation during the summer as a result of the presence of a stratospheric ozone layer depletion which runs the length of Chile as can be appreci- ated in fig. 1 (see [1]). UVB irradiance values during the summer and winter solstice of 2006 were 33 . 3 μ W / m 2 and 6 . 2 μ W / m 2 , respectively. For more detailed UV climatology information on Valpara ́ ıso see [2]. The city of Valpara ́ ıso is surrounded by an extensive forest area and is prone to forest wildfires during the summer months. Wildfires dam- aged 5 157 . 7 hectares (51 . 58 km 2 ) only in the Valpara ́ ıso province in 2005, of which 3 472 . 23 hectares (34 . 72 km 2 ) were destroyed in January. These forest fires, apart from producing particulate material and smoke, produce allergenic and toxic compounds which affect the population. The area of this study has a population of approximately 800 000 people. The smoke and particulate produced by these forest fires has an effect on the UV radiation which at this time of year is high because it happens during the summer, in addition to the stratospheric ozone depletion in this region as previously mentioned. In this publication, results of the analysis done to determine the action of smoke and principally the PM 10 particulate material generated by forest fires in the region of Valpara ́ ıso and their effect upon UV radiation are shown. A forest fire was reported in Casablanca (33 19 S; 71 24 W) located approximately 30 km Southeast of Valpara ́ ıso in the morning of January 31st, 2005. At about 12:30 p.m. local time, a decrease in solar UVA and UVB irradiance was detected by the spectroradiometer EKO model MS-701, property of the Universidad Técnica Federico Santa Mar ́ ıa (UTFSM). In fig. 2, the wind direction from 03:00 to 21:00 is shown. In this graph, it can be observed the wind direction was variable, between 60 ◦ and 350 ◦ from 03:00 to 10:00. At 10:00, the wind shifted to 170 ◦ SE and remained at this direction until 21:00. This data was taken at the UTFSM meteorological station by the Wind Monitor model 05103 manufactured by Young Instruments. It also registered the wind speed throughout the day. Wind speed is low between 03:00 and 10:00, approximately 1 m / s. On the other hand, wind speed starts to increase at 10:00, 5.5 m / s and reaches a maximum of 7.0 m / s at 19:00, see fig. 3. This wind direction and wind speed data over Valpara ́ ıso establishes the fact that the smoke from this fire passed over Valpara ́ ıso and as a result generated low solar and UV irradiance. In addition, meteorological data for this day indicated clear skies over the area of Valpara ́ ıso, corroborated by satellite images. Solar radiation is measured once a minute using spectral piranometer from Eppley Lab model PSP series No. 32108F3, belonging to the Solar Evaluation Laboratory at UTFSM. When the decline of solar irradiance is analyzed in the graph in fig. 4, it can be observed that this decline commenced at approximately 12:30 and that it lasted until 20:00, this decline is relatively rapid, at 12:30 the irradiance value was 937 W / m 2 whereas the irradiance value at 14:40 was 437 . 9 W / m 2 which corresponds to a 53% decline. In fig. 5 the total irradiance graph is shown, direct plus diffused of the UVB band. The band’s irradiance value at 12:30 was 26 . 9 μ W / m 2 and at 14:40 it was 2 . 2 μ W / m 2 which is a 92% decrease. In the case of the UVA band, the decrease is on the order of 84%. Both UVB and UVA declines were greater than that of the Solar Spectrum as indicated previously. In fig. 6 the behaviour of UV irradiance for distinct wavelengths by the EKO spectroradiometer for every nm between 295 and 315 nm is shown. In all of the wavelengths, the behaviour is similar over time which indicates that all are altered in the same way, not noting any great absorption for any particular wavelength. During the afternoon, fluctuations of all bands can be noticed. This is due to the variation in the thickness of the layer smoke. This type of alteration suggests that the absorption is more the black-body ...

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