Zobrazeno 1 - 10
of 785
pro vyhledávání: '"Atmosphere of Titan"'
Autor:
Marzio Rosi, Piergiorgio Casavecchia, Luca Mancini, Dimitrios Skouteris, Demian Marchione, Giacomo Pannacci, Pedro Recio, Nadia Balucani, Gianmarco Vanuzzo, Pengxiao Liang
Publikováno v:
The Journal of Physical Chemistry. a
The reaction of excited nitrogen atoms N(2D) with CH3CCH (methylacetylene) was investigated under single-collision conditions by the crossed molecular beams (CMB) scattering method with mass spectrometric detection and time-of-flight analysis at the
Autor:
Abeer A. Mahmoud, H. G. Abdelwahed
Publikováno v:
Journal of Taibah University for Science, Vol 15, Iss 1, Pp 679-684 (2021)
Nitrogen gas is considered one of the significant standard gases in stratosphere of Titan, Saturn's largest moon, which represents almost 98.4% of Titan atmosphere chemical composites. Hydrodynamics fluid model has been constructed to describe the Ni
Publikováno v:
LITHOSPHERE (Russia). 20:873-895
Research subject and methods. The paper presents a review of available information on the atmosphere of Titan and its surface, necessary for the development of concepts of hydrocarbon formation, including the natural hydrocarbon synthesis, formation
Publikováno v:
Atmospheric and Oceanic Optics. 33:439-442
General formulas for the extinction coefficient of laser radiation in an atmosphere are derived. They take into account nonlinear effects and significantly differ from the linear optics results. Specific calculations are carried out for the atmospher
Autor:
Athena Coustenis
Titan, Saturn’s largest satellite, is one of the most intriguing moons in our Solar System, in particular because of its dense and extended nitrogen-based and organic-laden atmosphere. Other unique features include a methanological cycle similar to
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::d39b55996e5fabc2db99a1c6671f071d
https://doi.org/10.1093/acrefore/9780190647926.013.120
https://doi.org/10.1093/acrefore/9780190647926.013.120
Autor:
Aatmik R. Patel, Samuel Kougias, Brian J. Esselman, Maria Zdanovskaia, Robert J. McMahon, R. Claude Woods
Publikováno v:
Molecular Physics. 119
The analysis of syn-2-cyano-1,3-butadiene (C5H5N, μa = 3.2 D, μb = 2.3 D) in its ground vibrational state and two lowest-energy excited vibrational states, ν27 (A″, 144 cm−1) and ν19 (A′, 163 cm−1)...
Autor:
Raymond P. LeBeau, Joshua Beltz
Publikováno v:
AIAA AVIATION 2021 FORUM.
Autor:
Nadia Balucani
How did life emerge from inanimate matter? The processes that led from complex organic molecules to the first self-replicating systems are no longer at play and we cannot easily reconstruct them because we do not have a geological record of the perio
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::9e1cbc23429ab1fa9e657a94693919fa
https://doi.org/10.5194/epsc2021-779
https://doi.org/10.5194/epsc2021-779
Publikováno v:
Icarus. 331:1-14
We report observations of Titan using 190 images from the Hubble Space Telescope WFPC2 and NICMOS over 4 oppositions of Titan 1994–1997. Analysis of these images yields maps of surface brightness at 0.67, 0.94, and 1.08 μm that compare well with C
Publikováno v:
Icarus
Icarus, Elsevier, 2019, 329, pp.55-71. ⟨10.1016/j.icarus.2019.03.024⟩
Icarus, Elsevier, 2019, 329, pp.55-71. ⟨10.1016/j.icarus.2019.03.024⟩
International audience; The photochemical processes at work in the atmosphere of Titan are very complex and lead to a great variety of compounds with aerosols as an end-product. One of the most complex molecules detected so far is benzene (C6H6). In