The horizontal distribution of water in the stratospheres of Jupiter and Saturn with Herschel/PACS
HARTOGH, P.
Max-Planck-Institut für Sonnensystemforschung = Max Planck Institute for Solar System Research [MPS]
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Max-Planck-Institut für Sonnensystemforschung = Max Planck Institute for Solar System Research [MPS]
Language
en
Communication dans un congrès
This item was published in
EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. p.878, 2011, EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. p.878, 2011, EPSC-DPS Joint Meeting 2011,, 2011, Nantes. 2011-10p. 878
English Abstract
In this paper, we will present disk-resolved observations in the strong water line at 66.4 μm in the stratospheres of Jupiter and Saturn, recorded with the PACS (Photodetector Array Camera and Spectrometer) instrument [12] ...Read more >
In this paper, we will present disk-resolved observations in the strong water line at 66.4 μm in the stratospheres of Jupiter and Saturn, recorded with the PACS (Photodetector Array Camera and Spectrometer) instrument [12] of the Herschel Space Observatory [13] on December 15th, 2010, and January 11th, 2011, respectively. The resulting telescope beam was 900 wide allowing mapping the horizontal distribution of water in the planets' stratospheres with a good resolution for Jupiter and a more limited one for Saturn. Thesemaps enable us to draw new conclusions on the origin of water in the upper atmospheres of these planets.Read less <
Origin
Hal imported