Vis enkel innførsel

dc.contributor.authorGirard, Lucas
dc.contributor.authorBerg, Torunn
dc.contributor.authorHole, Lars Robert
dc.date.accessioned2021-06-29T10:31:17Z
dc.date.available2021-06-29T10:31:17Z
dc.date.issued2005
dc.identifier.issn0807-7185
dc.identifier.urihttps://hdl.handle.net/11250/2761915
dc.description.abstractSince February 2000, gaseous elemental mercury (GEM) is continuously monitored at the Zeppelin station, close to Ny-Ålesund. The concentration of GEM remains quite constant throughout the year, around the background value, except for a three month period following the polar sunrise during which it encounters several rapid depletions, dropping down to very low levels, below the detection limit. These events are referred to as atmospheric mercury depletion events (AMDEs) and they are the result of the oxidation of GEM by bromine (BrO) free radicals. While most studies on AMDEs focus on the period with the most serious events (April in Ny-Ålesund), early and late spring 2003 (17/03 to 14/04 and 04/05 to 30/05) were examined in this study.
dc.language.isoeng
dc.publisherNILU
dc.relation.ispartofNILU TR
dc.relation.ispartofseriesNILU TR;01/2005
dc.subjectZeppelinobservatoriet
dc.subjectKvikksølv
dc.subjectPolare områder
dc.subjectAtmosfære og klima
dc.titleInvestigation of mercury depletion events recorded during early and late spring 2003 at Zeppelin/Ny-Ålesund, Svalbard (Norway).
dc.typeResearch report
dc.rights.holder© NILU
dc.source.issue01/2005


Tilhørende fil(er)

Thumbnail

Denne innførselen finnes i følgende samling(er)

Vis enkel innførsel