Search Results - "Teanby, N. A."
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Estimates of seismic activity in the Cerberus Fossae region of Mars
Published in Journal of geophysical research. Planets (01-12-2013)“…The 2016 NASA InSight lander is the first planetary mission designed to study the deep interior of Mars. InSight's Seismic Experiment for Interior Structure…”
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Seasonal Evolution of Titan's Stratosphere During the Cassini Mission
Published in Geophysical research letters (28-03-2019)“…Titan's stratosphere exhibits significant seasonal changes, including breakup and formation of polar vortices. Here we present the first analysis of…”
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Phosphine on Jupiter and Saturn from Cassini/CIRS
Published in Icarus (New York, N.Y. 1962) (01-08-2009)“…The global distribution of phosphine (PH 3) on Jupiter and Saturn is derived using 2.5 cm −1 spectral resolution Cassini/CIRS observations. We extend the…”
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Automatic measurement of shear wave splitting and applications to time varying anisotropy at Mount Ruapehu volcano, New Zealand
Published in Journal of Geophysical Research: Solid Earth (01-12-2010)“…We present an automatic shear wave splitting measurement tool for local earthquakes, with the sole manual step of choosing an S arrival time. We apply the…”
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Temperature and Composition of Saturn's Polar Hot Spots and Hexagon
Published in Science (American Association for the Advancement of Science) (04-01-2008)“…Saturn's poles exhibit an unexpected symmetry in hot, cyclonic polar vortices, despite huge seasonal differences in solar flux. The cores of both vortices are…”
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Methane and its isotopologues on Saturn from Cassini/CIRS observations
Published in Icarus (New York, N.Y. 1962) (01-02-2009)“…High spectral resolution observations from the Cassini Composite Infrared Spectrometer [Flasar, F.M., and 44 colleagues, 2004. Space Sci. Rev. 115, 169–297]…”
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EVOLUTION OF THE STRATOSPHERIC TEMPERATURE AND CHEMICAL COMPOSITION OVER ONE TITANIAN YEAR
Published in The Astrophysical journal (20-12-2013)“…Since the Voyager 1 (V1) flyby in 1980, Titan's exploration from space and the ground has been ongoing for more than a full revolution of Saturn around the Sun…”
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THERMAL AND CHEMICAL STRUCTURE VARIATIONS IN TITAN'S STRATOSPHERE DURING THE CASSINI MISSION
Published in The Astrophysical journal (01-12-2012)“…We have developed a line-by-line Atmospheric Radiative Transfer for Titan code that includes the most recent laboratory spectroscopic data and haze…”
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Titan's winter polar vortex structure revealed by chemical tracers
Published in Journal of Geophysical Research - Planets (01-12-2008)“…The winter polar vortex on Saturn's largest moon Titan has profound effects on atmospheric circulation and chemistry and for the current northern midwinter…”
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ISOTOPIC RATIOS IN TITAN's METHANE: MEASUREMENTS AND MODELING
Published in The Astrophysical journal (20-04-2012)“…The existence of methane in Titan's atmosphere (~6% level at the surface) presents a unique enigma, as photochemical models predict that the current inventory…”
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Latitudinal Variations in Uranus' Vertical Cloud Structure from UKIRT UIST Observations
Published in The Astrophysical journal (10-08-2007)“…Prior to Uranus' northern spring equinox in 2007 December, near-infrared spectra and images of Uranus were obtained in 2006 August and September using the UIST…”
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Multispectral imaging observations of Neptune’s cloud structure with Gemini-North
Published in Icarus (New York, N.Y. 1962) (01-11-2011)“…► Neptune found to have two thin clouds, one at ∼2 bar and the other at between 0.05 and 0.2 bar. ► Single-scattering albedo of particles in the upper cloud…”
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Characterising Saturn's vertical temperature structure from Cassini/CIRS
Published in Icarus (New York, N.Y. 1962) (01-08-2007)“…Thermal infrared spectra of Saturn from 10–1400 cm −1 at 15 cm −1 spectral resolution and a spatial resolution of 1°–2° latitude have been obtained by the…”
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Oxygen compounds in Titan's stratosphere as observed by Cassini CIRS
Published in Icarus (New York, N.Y. 1962) (01-02-2007)“…We have investigated the abundances of Titan's stratospheric oxygen compounds using 0.5 cm−1 resolution spectra from the Composite Infrared Spectrometer on the…”
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Neptune and Uranus: ice or rock giants?
Published in Philosophical transactions of the Royal Society of London. Series A: Mathematical, physical, and engineering sciences (25-12-2020)“…Existing observations of Uranus and Neptune's fundamental physical properties can be fitted with a wide range of interior models. A key parameter in these…”
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Revised vertical cloud structure of Uranus from UKIRT/UIST observations and changes seen during Uranus’ Northern Spring Equinox from 2006 to 2008: Application of new methane absorption data and comparison with Neptune
Published in Icarus (New York, N.Y. 1962) (01-08-2010)“…Long-slit spectroscopy observations of Uranus by the United Kingdom InfraRed Telescope UIST instrument in 2006, 2007 and 2008 have been used to monitor the…”
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Characteristics of Titan's stratospheric aerosols and condensate clouds from Cassini CIRS far-infrared spectra
Published in Icarus (New York, N.Y. 1962) (01-11-2007)“…Four broad spectral features were identified in far-infrared limb spectra from the Cassini Composite Infrared Spectrometer (CIRS), two of which have not been…”
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Global and temporal variations in hydrocarbons and nitriles in Titan's stratosphere for northern winter observed by Cassini/CIRS
Published in Icarus (New York, N.Y. 1962) (01-02-2008)“…Mid-infrared spectra measured by Cassini's Composite InfraRed Spectrometer (CIRS) between July 2004 and January 2007 ( L s = 293 ° – 328 ° ) have been used to…”
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Far-infrared opacity sources in Titan’s troposphere reconsidered
Published in Icarus (New York, N.Y. 1962) (01-10-2010)“…We use Cassini far-infrared limb and nadir spectra, together with recent Huygens results, to shed new light on the controversial far-infrared opacity sources…”
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Further seasonal changes in Uranus’ cloud structure observed by Gemini-North and UKIRT
Published in Icarus (New York, N.Y. 1962) (01-03-2012)“…► Uranus’ zone at 45°N has brightened and counterpart zone at 45°S has faded during 2006–2010. ► H-band spectra (1.4–1.8μm) have similar sensitivity to main…”
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