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Ethane ocean on Titan
It is proposed that Saturn's satellite Titan is covered by an ocean one to several kilometers
deep consisting mainly of ethane. If the ocean is in thermodynamic equilibrium with an …
deep consisting mainly of ethane. If the ocean is in thermodynamic equilibrium with an …
PAMPRE: A dusty plasma experiment for Titan's tholins production and study
C Szopa, G Cernogora, L Boufendi, JJ Correia… - Planetary and space …, 2006 - Elsevier
Organic aerosols play a significant role in the properties and evolution of Titan's
atmosphere. But our knowledge of them and their physico-chemical mechanisms of …
atmosphere. But our knowledge of them and their physico-chemical mechanisms of …
Experimental laboratory simulation of Titan's atmosphere: aerosols and gas phase
The discovery that Titan, the largest satellite of Saturn, has an atmosphere and that methane
is a significant constituent of it, was the starting point for a systematic study of Titan's …
is a significant constituent of it, was the starting point for a systematic study of Titan's …
Production and condensation of organic gases in the atmosphere of Titan
C Sagan, WR Thompson - Icarus, 1984 - Elsevier
The rates and altitudes for the dissociation of atmospheric constituents of Titan are
calculated for solar UV, solar wind protons, interplanetary electrons, Saturn magnetospheric …
calculated for solar UV, solar wind protons, interplanetary electrons, Saturn magnetospheric …
Precise ro-vibrational analysis of molecular bands forbidden in absorption: the ν8+ ν10 band of the 12C2H4 molecule
ON Ulenikov, OV Gromova, ES Bekhtereva… - Journal of Molecular …, 2015 - Elsevier
The highly accurate (experimental accuracy in line positions∼(1-2)× 10-4 cm− 1) ro-
vibrational spectrum of the ν 8+ ν 10 band of the 12 C 2 H 4 molecule was recorded for the …
vibrational spectrum of the ν 8+ ν 10 band of the 12 C 2 H 4 molecule was recorded for the …
Methane and ethane on the bright Kuiper belt object 2005 FY9
The spectrum of the bright Kuiper Belt object 2005 FY9 from 0.34 to 2.5 μm is dominated by
the red coloring of many outer solar system objects in the optical wavelength regime and by …
the red coloring of many outer solar system objects in the optical wavelength regime and by …
High resolution FTIR study of the ν7+ ν10− ν10 and ν10+ ν12− ν10 “hot” bands of C2H4
ON Ulenikov, OV Gromova, ES Bekhtereva… - Journal of Quantitative …, 2014 - Elsevier
Two weak “hot” absorption bands, ν 7+ ν 10− ν 10 and ν 10+ ν 12− ν 10, of ethylene, C 2 H
4, were analyzed for the first time with high resolution using the Fourier transform …
4, were analyzed for the first time with high resolution using the Fourier transform …
High resolution ro-vibrational analysis of interacting bands ν4, ν7, ν10, and ν12 of 13C2H4
ON Ulenikov, OV Gromova, ES Bekhtereva… - Journal of Quantitative …, 2015 - Elsevier
Abstract High accurate,~ 1× 10− 4 cm− 1, ro-vibrational spectra of the C 2 13 H 4 molecule
in the region of 600–1600 cm− 1 were recorded with Bruker IFS 120/125 HR Fourier …
in the region of 600–1600 cm− 1 were recorded with Bruker IFS 120/125 HR Fourier …
Nitrogen Incorporation in CH4-N2 Photochemical Aerosol Produced by Far Ultraviolet Irradiation
Nitrile incorporation into Titan aerosol accompanying hydrocarbon chemistry is thought to be
driven by extreme UV wavelengths (λ< 120 nm) or magnetospheric electrons in the outer …
driven by extreme UV wavelengths (λ< 120 nm) or magnetospheric electrons in the outer …
Study of the high resolution FTIR spectrum of CH2CD2 in the region of 1300–1450 cm− 1: The ν12 (A1) and 2ν10 (A1) bands
ON Ulenikov, OV Gromova, ES Bekhtereva… - Journal of Quantitative …, 2015 - Elsevier
The high resolution IR spectrum of the CH 2 CD 2 ethylene isotopomer was recorded and
analyzed in the region of 1300–1450 cm− 1, where the strongly interacting bands ν 12 (A 1) …
analyzed in the region of 1300–1450 cm− 1, where the strongly interacting bands ν 12 (A 1) …