Analysis of Jupiter north equatorial belt hot spots in the 4–5 μm range from Galileo/near‐infrared mapping spectrometer observations: Measurements of cloud opacity, water, and ammonia
M. Roos‐Serote(National Astronomical Observatory of Japan), Andrew Weir(University of Oxford), R. Mehlman(United States Geological Survey), S. B. Calcutt(University of Oxford), P. G. J. Irwin(University of Oxford), Glenn S. Orton(Jet Propulsion Laboratory), P. Drossart(Centre National de la Recherche Scientifique), F. W. Taylor(University of Oxford), E. Lellouch(Centre National de la Recherche Scientifique), R. W. Carlson, K. H. Baines(Jet Propulsion Laboratory), L. W. Kamp(Jet Propulsion Laboratory), Thérèse Encrenaz(Brown University)
Cited by 62
Related Papers
Global Mineralogical and Aqueous Mars History Derived from OMEGA/Mars Express Data
|Science|2006|1.6k
JUpiter ICy moons Explorer (JUICE): An ESA mission to orbit Ganymede and to characterise the Jupiter system
|Planetary and Space Science|2012|671
The NEMESIS planetary atmosphere radiative transfer and retrieval tool
|Journal of Quantitative Spectroscopy and Radiative Transfer|2007|549