Search Results - "Teanby, N."
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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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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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3
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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4
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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5
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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6
Bolide Airbursts as a Seismic Source for the 2018 Mars InSight Mission
Published in Space science reviews (01-10-2017)“…In 2018, NASA will launch InSight, a single-station suite of geophysical instruments, designed to characterise the martian interior. We investigate the…”
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Largest recent impact craters on Mars: Orbital imaging and surface seismic co-investigation
Published in Science (American Association for the Advancement of Science) (28-10-2022)“…Two >130-meter-diameter impact craters formed on Mars during the later half of 2021. These are the two largest fresh impact craters discovered by the Mars…”
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Structure and dynamics of the Martian lower and middle atmosphere as observed by the Mars Climate Sounder: Seasonal variations in zonal mean temperature, dust, and water ice aerosols
Published in Journal of Geophysical Research: Planets (01-12-2010)“…The first Martian year and a half of observations by the Mars Climate Sounder aboard the Mars Reconnaissance Orbiter has revealed new details of the thermal…”
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9
Flexible Mode Modelling of the InSight Lander and Consequences for the SEIS Instrument
Published in Space science reviews (01-12-2018)“…We present an updated model for estimating the lander mechanical noise on the InSight seismometer SEIS, taking into account the flexible modes of the InSight…”
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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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Near-Field Seismic Propagation and Coupling Through Mars’ Regolith: Implications for the InSight Mission
Published in Space science reviews (01-08-2018)“…NASA’s InSight Mission will deploy two three-component seismometers on Mars in 2018. These short period and very broadband seismometers will be mounted on a…”
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The Marsquake Service: Securing Daily Analysis of SEIS Data and Building the Martian Seismicity Catalogue for InSight
Published in Space science reviews (01-12-2018)“…The InSight mission expects to operate a geophysical observatory on Mars for at least two Earth years from late 2018. InSight includes a seismometer package,…”
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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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Spatial variations in Titan’s atmospheric temperature: ALMA and Cassini comparisons from 2012 to 2015
Published in Icarus (New York, N.Y. 1962) (01-06-2018)“…•Retrieved temperature profiles between ∼ 50 and 550 km from 2012 to 2015 are presented.•First spatially resolved measurements of Titan using ground-based…”
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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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Predicted detection rates of regional-scale meteorite impacts on Mars with the InSight short-period seismometer
Published in Icarus (New York, N.Y. 1962) (01-08-2015)“…•Scaling relations for peak seismic ground velocity from impacts are derived.•InSight’s SP seismometer should detect 0.1–30impacts/yr, nominally…”
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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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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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Seismic Coupling of Short-Period Wind Noise Through Mars’ Regolith for NASA’s InSight Lander
Published in Space science reviews (01-10-2017)“…NASA’s InSight lander will deploy a tripod-mounted seismometer package onto the surface of Mars in late 2018. Mars is expected to have lower seismic activity…”
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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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