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The total solar eclipse of March 2006: Overview

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dc.contributor.author Gerasopoulos, E en
dc.contributor.author Zerefos, CS en
dc.contributor.author Tsagouri, I en
dc.contributor.author Founda, D en
dc.contributor.author Amiridis, V en
dc.contributor.author Bais, AF en
dc.contributor.author Belehaki, A en
dc.contributor.author Christou, N en
dc.contributor.author Economou, G en
dc.contributor.author Kanakidou, M en
dc.contributor.author Karamanos, A en
dc.contributor.author Petrakis, M en
dc.contributor.author Zanis, P en
dc.date.accessioned 2014-06-06T06:48:47Z
dc.date.available 2014-06-06T06:48:47Z
dc.date.issued 2008 en
dc.identifier.issn 16807316 en
dc.identifier.uri http://62.217.125.90/xmlui/handle/123456789/4265
dc.relation.uri http://www.scopus.com/inward/record.url?eid=2-s2.0-51349158822&partnerID=40&md5=fbcb7e0c27420f8a611f7b11a3791381 en
dc.subject.other air quality en
dc.subject.other boundary layer en
dc.subject.other environmental effect en
dc.subject.other ionosphere en
dc.subject.other ozone en
dc.subject.other photochemistry en
dc.subject.other solar eclipse en
dc.subject.other solar radiation en
dc.subject.other stratosphere en
dc.subject.other troposphere en
dc.subject.other turbulence en
dc.title The total solar eclipse of March 2006: Overview en
heal.type journalArticle en
heal.publicationDate 2008 en
heal.abstract This paper provides the overview of an integrated, multi-disciplinary effort to study the effects of the 29 March 2006 total solar eclipse on the environment, with special focus on the atmosphere. The eclipse has been visible over the Eastern Mediterranean, and on this occasion several research and academic institutes organised co-ordinated experimental campaigns, at different distances from eclipse totality and at various environments in terms of air quality. Detailed results and findings are presented in a number of component scientific papers included in a Special Issue of Atmospheric Chemistry and Physics. The effects of the eclipse on meteorological parameters, though very clear, were shown to be controlled by local factors rather than the eclipse magnitudes, and the turbulence activity near surface was suppressed causing a decrease in the Planetary Boundary Layer. In addition to the above, the decrease in solar radiation has caused change to the photochemistry of the atmosphere, with night time chemistry dominating. The abrupt ""switch off"" of the sun, induced changes also in the ionosphere (140 up to 220 km) and the stratosphere. In the ionosphere, both photochemistry and dynamics resulted to changes in the reflection heights and the electron concentrations. Among the most important scientific findings from the experiments undertaken has been the experimental proof of eclipse induced thermal fluctuations in the ozone layer (Gravity Waves), due to the supersonic movement of the moon's shadow, for the first time with simultaneous measurements at three altitudes namely the troposphere, the stratosphere and the ionosphere. Within the challenging topics of the experiments has been the investigation of eclipse impacts on ecosystems (field crops and marine plankton). The rare event of a total solar eclipse provided the opportunity to evaluate 1 dimensional (1-D) and three dimensional (3-D) radiative transfer (in the atmosphere and underwater), mesoscale meteorological, regional air quality and photochemical box models, against measurements. en
heal.journalName Atmospheric Chemistry and Physics en
dc.identifier.issue 17 en
dc.identifier.volume 8 en
dc.identifier.spage 5205 en
dc.identifier.epage 5220 en


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