References

ACP

Atmospheric Chemistry and Physics

ACP

1680-7324

Copernicus GmbH

Göttingen, Germany

10.5194/acp-7-6061-2007

Effects on surface atmospheric photo-oxidants over Greece during the total solar eclipse event of 29 March 2006

Zanis

¹ Katragkou

² Kanakidou

³ Psiloglou

B. E.

⁴ Karathanasis

⁵ Vrekoussis

³ ⁶ Gerasopoulos

⁴ Lisaridis

² Markakis

² Poupkou

² Amiridis

⁴ Melas

² Mihalopoulos

³ Zerefos

⁴

Department of Meteorology and Climatology, Aristotle University of Thessaloniki, Greece

Laboratory of Atmospheric Physics, Aristotle University of Thessaloniki, Greece

Environmental Chemical Processes Laboratory, Department of Chemistry, University of Crete, Greece

National Observatory of Athens, Athens, Greece

Region of Central Macedonia, Thessaloniki, Greece

now at: Institute of Environmental Physics and Remote Sensing IUP/IFE, University of Bremen, Germany

10 12 2007

7 23 6061 6073

This is an open-access article ditributed under the terms of the Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original author and source are credited.

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This study investigates the effects of the total solar eclipse of 29 March 2006 on surface air-quality levels over Greece based on observations at a number of sites in conjunction with chemical box modelling and 3-D air-quality modelling. Emphasis is given on surface ozone and other photooxidants at four Greek sites Kastelorizo, Finokalia (Crete), Pallini (Athens) and Thessaloniki, which are located at gradually increasing distances from the path of the eclipse totality and are characterized by different air pollution levels. The eclipse offered the opportunity to test our understanding of air pollution build-up and the response of the gas-phase chemistry of photo-oxidants during a photolytical perturbation using both a photochemical box model and a regional air-quality offline model based on the modeling system WRF/CAMx. At the relatively unpolluted sites of Kastelorizo and Finokalia no clear signal of the solar eclipse on surface O3, NO2 and NO concentrations can be deduced from the observations while there is no correlation of observed O3, NO2 and NO with observed global radiation. The box and regional model simulations for the two relatively unpolluted sites indicate that the calculated changes in net ozone production rates between eclipse and non eclipse conditions are rather small compared to the observed short-term ozone variability. Furthermore the simulated ozone lifetime is in the range of a few days at these sites and hence the solar eclipse effects on ozone can be easily masked by local and regional transport. At the polluted sites of Thessaloniki and Pallini, the solar eclipse effects on O3, NO2 and NO concentrations are revealed from both the measurements and modeling with the net effect being a decrease in O3 and NO and an increase in NO2 as NO2 formed from the reaction of O3 with NO while at the same time NO2 is not efficiently photolysed. This result is also supported by a positive correlation of observed global radiation with O3 and NO and a negative correlation with NO2. It is evident from the 3-D air quality modeling over Greece that the maximum effects of the eclipse on O3, NO2 and NO are reflected on the large urban agglomerations of Athens, and Thessaloniki where the maximum of the emissions occur.

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