Search Results - "Romani, Paul"
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Fresh clouds: A parameterized updraft method for calculating cloud densities in one-dimensional models
Published in Icarus (New York, N.Y. 1962) (01-01-2015)“…•Fixes the cloud density calculation in models like Weidenschilling and Lewis (1973).•Updraft length scale (or speed and duration) determines cloud…”
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The composition of Titan's stratosphere from Cassini/CIRS mid-infrared spectra
Published in Icarus (New York, N.Y. 1962) (01-07-2007)“…We have analyzed data recorded by the Composite Infrared Spectrometer (CIRS) aboard the Cassini spacecraft during the Titan flybys T0–T10 (July 2004–January…”
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Vertical abundance profiles of hydrocarbons in Titan's atmosphere at 15° S and 80° N retrieved from Cassini/CIRS spectra
Published in Icarus (New York, N.Y. 1962) (01-05-2007)“…Limb spectra recorded by the Composite InfraRed Spectrometer (CIRS) on Cassini provide information on abundance vertical profiles of C 2H 2, C 2H 4, C 2H 6, CH…”
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Detection of C2HD and the D/H ratio on Titan
Published in Icarus (New York, N.Y. 1962) (01-10-2008)“…We report here the first detection of mono-deuterated acetylene (acetylene-d1, C 2HD) in Titan's atmosphere from the presence of two of its emission bands at…”
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Observations of C2H6 and C2H2 in the stratosphere of Saturn
Published in Icarus (New York, N.Y. 1962) (01-02-2005)“…We have performed high-resolution spectral observations at mid-infrared wavelengths of C2H6 (12.16 microns) and C2H2 (13.45 microns) on Saturn. These emission…”
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Temporally varying ethylene emission on Jupiter
Published in Icarus (New York, N.Y. 1962) (01-12-2008)“…Ethylene (C 2H 4) emission has been measured in the poles and equator of Jupiter. The 949 cm −1 spectra were recorded with a high resolution spectrometer at…”
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Rate constant for the reaction CH3 + CH3 → C2H6 at T = 155 K and model calculation of the CH3 abundance in the atmospheres of Saturn and Neptune
Published in Journal of Geophysical Research - Planets (15-11-2003)“…The column abundances of CH3 observed by the Infrared Space Observatory (ISO) satellite on Saturn and Neptune were lower than predicted by atmospheric…”
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Cassini Composite Infrared Spectrometer (CIRS) Observations of Titan 2004-2017
Published in The Astrophysical journal (11-09-2019)“…From 2004 to 2017, the Cassini spacecraft orbited Saturn, completing 127 close flybys of its largest moon, Titan. Cassini’s Composite Infrared Spectrometer…”
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Titan trace gaseous composition from CIRS at the end of the Cassini–Huygens prime mission
Published in Icarus (New York, N.Y. 1962) (01-05-2010)“…This paper reports on the results from an extensive study of all nadir-looking spectra acquired by Cassini/CIRS during the 44 flybys performed in the course of…”
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Stratospheric Ammonia on Jupiter after the SL9 Collision
Published in Icarus (New York, N.Y. 1962) (01-06-1996)“…We report results from measurements of NH3emission lines from the stratosphere of Jupiter following the impacts of fragments of Comet P/Shoemaker–Levy 9…”
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Titan's Atmospheric Temperatures, Winds, and Composition
Published in Science (American Association for the Advancement of Science) (13-05-2005)“…Temperatures obtained from early Cassini infrared observations of Titan show a stratopause at an altitude of 310 kilometers (and 186 kelvin at$15\textdegree…”
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Titan's Surface Brightness Temperatures
Published in The Astrophysical journal (01-02-2009)Get full text
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Exploring The Saturn System In The Thermal Infrared: The Composite Infrared Spectrometer
Published in Space science reviews (01-01-2004)“…The Composite Infrared Spectrometer (CIRS) is a remote-sensing Fourier Transform Spectrometer (FTS) on the Cassini orbiter that measures thermal radiation over…”
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Temperatures, Winds, and Composition in the Saturnian System
Published in Science (American Association for the Advancement of Science) (25-02-2005)“…Stratospheric temperatures on Saturn imply a strong decay of the equatorial winds with altitude. If the decrease in winds reported from recent Hubble Space…”
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Meridional variations of C2H2 and C2H6 in Jupiter's atmosphere from Cassini CIRS infrared spectra
Published in Icarus (New York, N.Y. 1962) (01-05-2007)“…Hydrocarbons such as acetylene (C 2H 2) and ethane (C 2H 6) are important tracers in Jupiter's atmosphere, constraining our models of the chemical and…”
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Upper limits for undetected trace species in the stratosphere of Titan
Published 01-03-2011“…Faraday Discuss., 2010, Vol. 147, pp. 65-81 In this paper we describe a first quantitative search for several molecules in Titan's stratosphere in Cassini CIRS…”
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An intense stratospheric jet on Jupiter
Published in Nature (08-01-2004)“…The Earth's equatorial stratosphere shows oscillations in which the east-west winds reverse direction and the temperatures change cyclically with a period of…”
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Isotopic Ratios in Titan's Atmosphere from Cassini CIRS Limb Sounding: HC3N in the North
Published in The Astrophysical journal (10-07-2008)Get full text
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12C/13C Ratio in Ethane on Titan and Implications for Methane’s Replenishment
Published in The journal of physical chemistry. A, Molecules, spectroscopy, kinetics, environment, & general theory (22-10-2009)“…The 12C/13C abundance ratio in ethane in the atmosphere of Titan has been measured at 822 cm−1 from high spectral resolution ground-based observations. The…”
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