Author
Listed:
- G. Israël
(Service d'Aéronomie UMR 7620 CNRS, ISPL, Universities Paris 6 and Versailles-Saint Quentin)
- C. Szopa
(Service d'Aéronomie UMR 7620 CNRS, ISPL, Universities Paris 6 and Versailles-Saint Quentin)
- F. Raulin
(Laboratoire Interuniversitaire des Systèmes Atmosphériques, UMR 7583 CNRS, Universities Paris 12 and Paris 7)
- M. Cabane
(Service d'Aéronomie UMR 7620 CNRS, ISPL, Universities Paris 6 and Versailles-Saint Quentin)
- H. B. Niemann
(NASA Goddard Space Flight Centre)
- S. K. Atreya
(Oceanic and Space Sciences, University of Michigan)
- S. J. Bauer
(Institute for Meteorology and Geophysics, University of Graz)
- J.-F. Brun
(Service d'Aéronomie UMR 7620 CNRS, ISPL, Universities Paris 6 and Versailles-Saint Quentin)
- E. Chassefière
(Service d'Aéronomie UMR 7620 CNRS, ISPL, Universities Paris 6 and Versailles-Saint Quentin)
- P. Coll
(Laboratoire Interuniversitaire des Systèmes Atmosphériques, UMR 7583 CNRS, Universities Paris 12 and Paris 7)
- E. Condé
(Centre National d'Etudes Spatiales (CNES))
- D. Coscia
(Laboratoire Interuniversitaire des Systèmes Atmosphériques, UMR 7583 CNRS, Universities Paris 12 and Paris 7)
- A. Hauchecorne
(Service d'Aéronomie UMR 7620 CNRS, ISPL, Universities Paris 6 and Versailles-Saint Quentin)
- P. Millian
(Office National d'Etudes et de Recherches Aérospatiales)
- M. J. Nguyen
(Laboratoire Interuniversitaire des Systèmes Atmosphériques, UMR 7583 CNRS, Universities Paris 12 and Paris 7)
- T. Owen
(Institute for Astronomy, University of Hawaii at Manoa)
- W. Riedler
(Space Research Institute)
- R. E. Samuelson
(University of Maryland, College Park)
- J.-M. Siguier
(Office National d'Etudes et de Recherches Aérospatiales)
- M. Steller
(Institut für Weltraumforschung, Österreichische Akademie der Wissenschaften)
- R. Sternberg
(Laboratoire Interuniversitaire des Systèmes Atmosphériques, UMR 7583 CNRS, Universities Paris 12 and Paris 7)
- C. Vidal-Madjar
(Laboratoire de Recherche sur les Polymères, UMR 7581 CNRS)
Abstract
Biemann 1 calls into question our preliminary interpretations of our experimental results2. A comparison of laboratory and flight measurements should settle the uncertainties he raises. In addition to evaluating instrumental characteristics such as the 'piston effect', a technique we used for injecting oven-gas content for gas chromatography–mass spectrometry (GC–MS), such studies should enable a wide range of possible compositions for Titan's aerosols to be investigated. Our aerosol collection and pyrolysis (ACP) measurements in Titan's atmosphere can then be revisited.
Suggested Citation
G. Israël & C. Szopa & F. Raulin & M. Cabane & H. B. Niemann & S. K. Atreya & S. J. Bauer & J.-F. Brun & E. Chassefière & P. Coll & E. Condé & D. Coscia & A. Hauchecorne & P. Millian & M. J. Nguyen & , 2006.
"Complex organic matter in Titan's aerosols? (Reply),"
Nature, Nature, vol. 444(7118), pages 6-7, November.
Handle:
RePEc:nat:nature:v:444:y:2006:i:7118:d:10.1038_nature05418
DOI: 10.1038/nature05418
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