Reference : The current budget of NOy above the Jungfraujoch as derived from IR solar observations
Scientific congresses and symposiums : Paper published in a book
Physical, chemical, mathematical & earth Sciences : Earth sciences & physical geography
http://hdl.handle.net/2268/95591
The current budget of NOy above the Jungfraujoch as derived from IR solar observations
English
Demoulin, Philippe mailto [Université de Liège - ULg > Département d'astrophys., géophysique et océanographie (AGO) > Groupe infra-rouge de phys. atmosph. et solaire (GIRPAS) >]
Mahieu, Emmanuel mailto [Université de Liège - ULg > Département d'astrophys., géophysique et océanographie (AGO) > Groupe infra-rouge de phys. atmosph. et solaire (GIRPAS) >]
Zander, Rodolphe [Université de Liège - ULg > Services généraux (Faculté des sciences) > Relations académiques et scientifiques (Sciences) >]
Roland, G. [> >]
Delbouille, L. [> >]
Servais, Christian [Université de Liège - ULg > Département d'astrophys., géophysique et océanographie (AGO) > Groupe infra-rouge de phys. atmosph. et solaire (GIRPAS) >]
De Mazière, M. [> >]
Van Roozendael, M. [> >]
1998
Polar stratospheric ozone 1997
Harris, N. R. P.
Kilbane-Dawe, I.
Amanatidis, G. T.
No
No
International
92-828-2365-2
The Fourth European Symposium on Polar Stratospheric Ozone Research
22-26 September 1997
Schliersee
Germany
[en] atmospheric composition and trends ; FTIR spectrometer ; Jungfraujoch ; nitrogen compounds in Earth's atmosphere
[en] This paper reports on an investigations of a series of compounds of the NOy family, based on high resolution infrared solar observations made at the ISSJ (International Scientific Station of the Jungfraujoch), Switzerland (46.55ºN, 7.99ºE, 3580 m a.s.l.). These observations are part of a long-term monitoring effort undertaken by the Liège group since the mid-1970s, and integrated more recently as a contribution to the Network for the Detection of Stratospheric Change (NDSC). Currently, vertical column abundances of over 20 molecules are retrieved from solar spectra recorded under clear sky conditions as regularly as possible, using two high resolution Fourier transform infrared (2 to 15 microns) spectrometers.
Researchers ; Professionals ; Students ; Others
http://hdl.handle.net/2268/95591
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