FN Archimer Export Format
PT J
TI MAP-IO, an atmospheric and marine observatory program onboard Marion Dufresne over the Southern Ocean
BT 
AF Tulet, Pierre
   Van Baelen, Joel
   Bosser, Pierre
   Brioude, Jérome
   Colomb, Aurelie
   Goloub, Philippe
   Pazmino, Andrea
   Portafaix, Thierry
   Ramonet, Michel
   Sellegri, Karine
   Thyssen, Melilotus
   Gest, Lea
   Marquestaut, Nicolas
   Mékiès, Dominique
   Metzger, Jean-Marc
   Athier, Gilles
   Blarel, Luc
   Delmotte, Marc
   Desprairies, Guillaume
   Dournaux, Meredith
   Dubois, Gaël
   Duflot, Valentin
   Lamy, Kevin
   Gardes, Lionel
   Guillemot, Jean-François
   Gros, Valérie
   Kolasinski, Joanna
   Lopez, Morgan
   Magand, Olivier
   Noury, Erwan
   Nunes-Pinharanda, Manuel
   Payen, Guillaume
   Pianezze, Joris
   Picard, David
   Picard, Olivier
   Prunier, Sandrine
   Rigaud-Louise, François
   Sicard, Michael
   Torres, Benjamin
AS 1:1;2:2;3:3;4:2;5:4;6:5;7:6;8:2;9:7;10:4;11:8;12:2;13:9;14:2;15:9;16:1;17:5;18:7;19:9;20:1;21:5;22:2;23:2;24:10;25:9;26:7;27:11;28:7;29:9;30:9;31:6;32:9;33:1;34:4;35:2;36:2;37:2;38:2;39:5;
FF 1:;2:;3:;4:;5:;6:;7:;8:;9:;10:;11:;12:;13:;14:;15:;16:;17:;18:;19:;20:;21:;22:;23:;24:;25:;26:;27:;28:;29:;30:;31:;32:;33:;34:;35:;36:;37:;38:;39:;
C1 LAERO, Laboratoire d’Aérologie (UMR 5560 CNRS, UT3, IRD), Toulouse, France
   LACY, Laboratoire de l’Atmosphère et des Cyclones (UMR 8105 CNRS, Université de La Réunion, Météo-France), Saint-Denis de La Réunion, France
   Lab-STICC (UMR 6285, CNRS, ENSTA-Bretagne), Brest, France
   LAMP, Laboratoire de Météorologie Physique (UMR 6016 Université Clermont Auvergne, CNRS), Aubière, France
   LOA, Laboratoire d’Optique Atmosphérique (UMR 8518 Université de Lille, CNRS), Villeneuve d’Ascq, France
   LATMOS,Laboratoire Atmosphères, Observations Spatiales, (UMR 8190 IPSL, UVSQ, Université Paris-Saclay, Sorbonne Université, CNRS), Guyancourt, France
   LSCE, Laboratoire des Sciences du Climat et de l’Environnement (UMR 8212 IPSL, CEA-CNRS-UVSQ, Université Paris-Saclay), Gif-sur-Yvette, France
   MIO, Institut Méditerranéen d’Océanologie (UMR 235 Aix Marseille Univ, Université de Toulon, CNRS, IRD) Marseille, France
   OSU-R, Observatoire des Sciences de l’Univers de La Réunion (UAR 3365 CNRS, Université de La Réunion, Météo-France), Saint-Denis de La Réunion, France
   TAAF, Terres australes et antarctiques françaises, Saint-Pierre de La Réunion, France
   ENTROPIE, Écologie Marine Tropicale des Océans Pacifique et Indien (UMR 250 Université de La Réunion, IFREMER, CNRS, IRD, Université de Nouvelle Calédonie), 97744, Saint-Denis, La Réunion
C2 CNRS, FRANCE
   UNIV LA REUNION, FRANCE
   ENSTA BRETAGNE, FRANCE
   UNIV CLERMONT AUVERGNE, FRANCE
   UNIV LILLE, FRANCE
   UNIV PARIS SACLAY, FRANCE
   UNIV PARIS SACLAY, FRANCE
   UNIV AIX MARSEILLE, FRANCE
   OSU-R, FRANCE
   TAAF, FRANCE
   UNIV LA REUNION, FRANCE
UM ENTROPIE
IN DOAJ
TC 0
UR https://archimer.ifremer.fr/doc/00879/99118/108964.pdf
LA English
DT Article
CR MAP-IO
   MAP-IO
   MD 241 / AMARYLLIS AMAGAS
   RESILIENCE
   SWINGS
   TRANSAMA
BO Marion Dufresne
AB This article is devoted to the presentation of the MAP-IO observation program. This program, launched in early 2021, has enabled the observation of nearly 700 days of measurements over the Indian and Southern Ocean thanks to the equipment of 17 meteorological and oceanographic scientific instruments on board the ship Marion Dufresne. Several observation techniques have been developed to respond to the difficulties of observations on board ships, in particular for passive remote sensing data, as well as quasi-autonomous data acquisition and transfer. The first measurements made it possible to draw up unprecedented climatological data of the Southern Ocean of the size distribution and optical thickness of aerosols, of the concentration of trace gases and greenhouse gases, of UV, and of integrated water vapor. High resolution observations of phytoplankton in surface waters have also shown a great variability in latitude, in terms of abundance and community structure (diversity). The operational success of this program and these unique scientific results all together establish a proof of concept and underline the need to transform this program into a permanent observatory. 
PY 2024
PD FEB
SO Earth System Science Data
SN 1866-3516
PU Copernicus GmbH
DI 10.5194/essd-2023-531
ID 99118
ER

EF