Probing the limits of sampling gaseous elemental mercury passively in the remote atmosphere

Author:

Hoang Christopher1,Magand Olivier2ORCID,Brioude Jérôme3ORCID,Dimuro Andrea4ORCID,Brunet Christophe4,Ah-Peng Claudine5,Bertrand Yann2,Dommergue Aurelien2ORCID,Lei Ying Duan1,Wania Frank1ORCID

Affiliation:

1. Department of Physical and Environmental Sciences, University of Toronto Scarborough, 1265 Military Trail, Toronto, Ontario, Canada M1C 1A4

2. Université Grenoble Alpes, CNRS, IRD, Grenoble INP, IGE, Grenoble, France

3. Laboratoire de l’Atmosphère et des Cyclones, UMR8105, CNRS, Université de La Réunion, 97744 Saint-Denis, France

4. Observatoire Volcanologique du Piton de la Fournaise, Institut de Physique du Globe de Paris, 97418 La Plaine des Cafres, Réunion, France

5. UMR PVBMT, Université de La Réunion, Saint-Pierre, France

Abstract

Deployment times of at least two months and dedicated efforts to limit contamination during transport and storage are recommended to obtain reliable results when using passive samplers for gaseous elemental mercury in the remote atmosphere.

Funder

Institut Polaire Français Paul Emile Victor

Institut national des sciences de l'Univers

Centre National de la Recherche Scientifique

University of Toronto

Publisher

Royal Society of Chemistry (RSC)

Subject

Pollution,Environmental Chemistry,Chemistry (miscellaneous),Analytical Chemistry

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