SIMBAD references

2003A&A...403L...7F - Astronomy and Astrophysics, volume 403, L7-10 (2003/5-3)

The infrared spectrum of Neptune at 3.5-4.1 microns: Search for H3+ and evidence for recent meteorological variations.

FEUCHTGRUBER H. and ENCRENAZ T.

Abstract (from CDS):

The infrared spectrum of Neptune at 3.5-3.75µm and 3.87-4.1µm has been measured at a spectral resolution of 1200. The observed flux is stronger by a factor ∼3 compared to previous measurements, suggesting important meteorological variations between 1997 and 2002. The flux is detected mostly from a bright belt at mid-southern latitudes. Strong absorptions, identified as methane, are observed over the L band. The observed CH4 spectrum can be fitted by a multilayer model assuming that the solar light is partly reflected above several layers, including the CH4 haze and stratospheric photochemical hazes. An upper limit to a disk averaged column density of H3+ of 2.9(+7.1-1.8)x1010.cm–2 is reported, consistent with present ionospheric models.

Abstract Copyright:

Journal keyword(s): line: formation - radiative transfer - planets and satellites: individual: Neptune - infrared: solar system

Simbad objects: 2

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