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

Abstract

Abstract.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 O 3 , NO 2 and NO concentrations can be deduced from the observations while there is no correlation of observed O 3 , NO 2 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 O 3 , NO 2 and NO concentrations are revealed from both the measurements and modeling with the net effect being a decrease in O 3 and NO and an increase in NO 2 as NO 2 formedCorrespondence to: P. Zanis (zanis@auth.gr) from the reaction of O 3 with NO while at the same time NO 2 is not efficiently photolysed. This result is also supported by a positive correlation of observed global radiation with O 3 and NO and a negative correlation with NO 2 . It is evident from the 3-D air quality modeling over Greece that the maximum effects of the eclipse on O 3 , NO 2 and NO are reflected on the large urban agglomerations of Athens, and Thessaloniki where the maximum of the emissions occur.

基于半导体激光云高仪的合肥日全食期间边界层高度的判决和演变

“…4, where the structure of the ABL is stable all the time from 09:20 to 10:10 BJT. As reported by Eaton et al, during the maximum phase of an eclipse, the sensible heat and radiation fluxes are affected, turbulence is reduced, and the air refractive index structure constant is dramatically decreased [9,10] This resembles the phenomenon recorded during nighttime where the residual layer coexists with the nocturnal boundary layer.…”

The effects of a solar eclipse on photo-oxidants in different areas of China

“…In the same event, the partitioning of NO x between NO and NO 2 was determined almost exclusively by variations in J NO 2 (Fabian et al, 2001). More recently in the total solar eclipse of 29 March 2006, observations and modeling show that there was a significant decrease in O 3 and NO and an increase in NO 2 at polluted sites, but no clear impact on these pollutants at unpolluted sites (Zanis et al, 2007). The decrease in the surface ozone concentration that was observed after the beginning of the eclipse lasted two hours, probably due to the decreased efficiency of photochemical ozone formation (Tzanis et al, 2008).…”

Contrasting behavior of slow and fast photoreactive gases during the August 21, 2017, solar eclipse

“…Similar conclusions were derived in a comparison of eclipse data from four sites in Greece. At two relatively unpolluted sites there was no clear signal in O 3 , NO, and NO 2 , while at two urban sites, decreases in O 3 and NO, and an increase in NO 2 (Zanis et al, 2007) were observed. Evidently, under eclipse conditions, in environments with higher NO x emission, there is a higher rate of NO x buildup from the loss of turbulent mixing, increase in NO 2 from the NO + O 3 -> NO 2 reaction, and conversely a higher rate of O 3 loss.…”