http://www.cnr.it/ontology/cnr/individuo/prodotto/ID216555
Analysis of VIMS near-IR spectra in Titan's upper atmosphere: Evidence for heavy and abundant aromatic hydrocarbons (Comunicazione a convegno)
- Type
- Label
- Analysis of VIMS near-IR spectra in Titan's upper atmosphere: Evidence for heavy and abundant aromatic hydrocarbons (Comunicazione a convegno) (literal)
- Anno
- 2013-01-01T00:00:00+01:00 (literal)
- Alternative label
M. López-Puertas (1), B. M. Dinelli (2), A. Adriani (3), B. Funke (1), M. García-Comas (1), M. L. Moriconi(4), E. D'Aversa
(3), C. Boersma (5) and L. J. Allamandola (5) (2013)
Analysis of VIMS near-IR spectra in Titan's upper atmosphere: Evidence for heavy and abundant aromatic hydrocarbons
in European Planetary Science Congress 2013, London, UK
(literal)
- Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#autori
- M. López-Puertas (1), B. M. Dinelli (2), A. Adriani (3), B. Funke (1), M. García-Comas (1), M. L. Moriconi(4), E. D'Aversa
(3), C. Boersma (5) and L. J. Allamandola (5) (literal)
- Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#affiliazioni
- 1. Instituto de Astrofísica de Andalucía (CSIC), Granada, Spain
2. ISAC-CNR, Bologna, Italy
3. IAPS-INAF, Rome, Italy
4. ISAC-CNR, Rome, Italy
5. NASA Ames Research Center, Moffett Field, CA 94035-1000, USA (literal)
- Titolo
- Analysis of VIMS near-IR spectra in Titan's upper atmosphere: Evidence for heavy and abundant aromatic hydrocarbons (literal)
- Abstract
- Observations of Titan atmosphere made with the
VIMS instrument on board the Cassini satellite show
a strong limb emission around 3.3 ?m at high atmospheric
altitudes (above 700 km). This emission exhibits
the spectral signatures of the strong CH4 bands.
A detailed analysis of the spectra reveals an additional
strong emission centered at 3.28 ?m and peaking at
about 950 km. Here we present an analysis of this
residual spectra and show that it attributed to emission
from heavy aromatic hydrocarbon compounds. (literal)
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- Autore CNR
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