Search Results - "Hathi, B"
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A soft solid surface on Titan as revealed by the Huygens Surface Science Package
Published in Nature (08-12-2005)“…The surface of Saturn's largest satellite-Titan-is largely obscured by an optically thick atmospheric haze, and so its nature has been the subject of…”
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ExoMars TGO/NOMAD‐UVIS Vertical Profiles of Ozone: 1. Seasonal Variation and Comparison to Water
Published in Journal of geophysical research. Planets (01-11-2021)“…We present ∼1.5 Mars Years (MY) of ozone vertical profiles, covering LS = 163° in MY34 to LS = 320° in MY35, a period which includes the 2018 global dust…”
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Huygens HASI servo accelerometer: A review and lessons learned
Published in Planetary and space science (01-10-2009)“…The servo accelerometer constituted a vital part of the Huygens Atmospheric Structure Instrument (HASI): flown aboard the Huygens probe, it operated…”
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Speed of sound measurements and the methane abundance in Titan's atmosphere
Published in Icarus (New York, N.Y. 1962) (01-08-2007)“…Aboard the Huygens probe, which descended through Titan's atmosphere in January 2005, was the Surface Science Package (SSP), a set of 9 sensors, including a…”
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Physical properties of Titan's surface at the Huygens landing site from the Surface Science Package Acoustic Properties sensor (API-S)
Published in Icarus (New York, N.Y. 1962) (01-12-2006)“…We present the results from the first sonar to be deployed outside of Earth, and the first active acoustic instrument on Titan, onboard the Huygens probe, and…”
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Analysis of entry accelerometer data: A case study of Mars Pathfinder
Published in Planetary and space science (01-08-2003)“…Accelerometers are regularly flown on atmosphere-entering spacecraft. Using their measurements, the spacecraft trajectory and the vertical structure of…”
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In situ thermal conductivity measurements of Titan's lower atmosphere
Published in Icarus (New York, N.Y. 1962) (01-10-2008)“…Thermal conductivity measurements, presented in this paper (Fig. 3), were made during the descent of the Huygens probe through the atmosphere of Titan below…”
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Huygens' Surface Science Package
Published in Space science reviews (01-01-2002)“…The design and performance of the Surface Science Package (SSP) on the Huygens probe are discussed. This instrument consists of nine separate sensors that are…”
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Reconstruction of the trajectory of the Huygens probe using the Huygens Atmospheric Structure Instrument (HASI)
Published in Planetary and space science (01-04-2008)“…The Huygens probe returned scientific measurements from the atmosphere and surface of Titan on 14 January 2005. Knowledge of the trajectory of Huygens is…”
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Physical properties as indicators of liquid compositions: Derivation of the composition for Titan's surface liquids from the Huygens SSP measurements
Published in Monthly notices of the Royal Astronomical Society (11-05-2005)“…We present a method for inferring the relative molar abundance of constituents of a liquid mixture, in this case methane, ethane, nitrogen and argon, from a…”
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The Huygens scientific data archive: Technical overview
Published in Planetary and space science (01-04-2008)“…The Cassini/Huygens mission was launched in October 1997, and during the third orbit around Saturn, the Huygens probe was released on course to enter Titan's…”
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Inferring the composition of the liquid surface on Titan at the Huygens probe landing site from Surface Science Package measurements
Published in Advances in space research (2006)“…With Huygens’ descent into Titan’s atmosphere drawing nearer, the composition and state of Titan’s surface remained largely unknown. The idea of a global ocean…”
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A stratospheric balloon experiment to test the Huygens atmospheric structure instrument (HASI)
Published in Planetary and space science (01-08-2004)“…We developed a series of balloon experiments parachuting a 1:1 scale mock-up of the Huygens probe from an altitude just over 30 km to simulate at planetary…”
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In situ measurements of the physical characteristics of Titan's environment
Published in Nature (08-12-2005)“…On the basis of previous ground-based and fly-by information, we knew that Titan's atmosphere was mainly nitrogen, with some methane, but its temperature and…”
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The Huygens surface science package (SSP): Flight performance review and lessons learned
Published in Planetary and space science (01-09-2012)“…The Surface Science Package (SSP) was one of six instruments flown onboard the Huygens probe to Titan, the largest moon of Saturn, in the framework of the…”
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Angioimmunoblastic lymphadenopathy presenting as superior vena caval obstruction
Published in Chest (01-12-1991)“…A 60-year-old man presented with features of superior vena cava (SVC) obstruction. On evaluation, he was diagnosed as having angioimmunoblastic lymphadenopathy…”
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Silence on Shangri-La: Attenuation of Huygens acoustic signals suggests surface volatiles
Published in Planetary and space science (01-01-2014)“…Characterize and understand acoustic instrument performance on the surface of Titan. The Huygens probe measured the speed of sound in Titan's atmosphere with a…”
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Thermal Conductivity measurements of Titan's Lower Atmosphere
Published in Icarus (New York, N.Y. 1962) (22-03-2010)Get full text
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Descent motions of the Huygens probe as measured by the Surface Science Package (SSP): Turbulent evidence for a cloud layer
Published in Planetary and space science (01-11-2007)“…The Huygens probe underwent vigorous short-period motions during its parachute descent through the atmosphere of Saturn's moon Titan in January 2005, at least…”
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