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Autor:
M. D. Smith, Frank Daerden, James Holmes, Stephen R. Lewis, C. Marriner, Alain Khayat, Ann Carine Vandaele, Yannick Willame, Manish R. Patel, Mark Leese, Séverine Robert, J. J. Lopez-Moreno, M.A.J. Brown, M. J. Wolff, Shohei Aoki, Cédric Depiesse, B. Hathi, Arianna Piccialli, Ian Thomas, Bojan Ristic, Kylash Rajendran, Paul Streeter, Giancarlo Bellucci, Jon Mason, G. Sellers, D.J. Slade
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
Journal of Geophysical Research: Planets
instname
Journal of Geophysical Research: Planets
This is an open access article under the terms of the Creative Commons Attribution License, which permits use, distribution and reproduction in any medium, provided the original work is properly cited.
We present ∼1.5 Mars Years (MY) of ozone
We present ∼1.5 Mars Years (MY) of ozone
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8f9a84b18c1884f33bf4fa8e876ce8ab
http://oro.open.ac.uk/79931/16/79931VOR.pdf
http://oro.open.ac.uk/79931/16/79931VOR.pdf
Autor:
Shohei Aoki, Mark Leese, Michael J. Wolff, Alain Khayat, J. Mason, Stephen R. Lewis, Graham Sellers, Charlotte Marriner, Frank Daerden, B. Hathi, Yannick Willame, James Holmes, Paul Streeter, Ian Thomas, Manish R. Patel, Séverine Robert, Cédric Depiesse, David Slade, Bojan Ristic, Giancarlo Bellucci, Arianna Piccialli, Ann Carine Vandaele, Megan Brown, Kylash Rajendran, Michael D. Smith, Jose-Juan Lopez-Moreno
We present ~1.5 Mars Years (MY) of ozone vertical profiles, covering Ls = 163deg; in MY34 to Ls = 320deg; in MY35, a period which includes the 2018 global dust storm. Since April 2018, the Ultravio...
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::46e8ec2a97c8ddfbeb2d01225453b195
https://doi.org/10.1002/essoar.10505984.1
https://doi.org/10.1002/essoar.10505984.1
This paper describes the radiation environment and radiation damage analysis performed for the Nadir and Occultation for MArs Discovery (NOMAD) Ultraviolet and Visible Spectrometer (UVIS) channel launched onboard the ExoMars Trace Gas Orbiter (TGO) i
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b4388002e08306ecd24d111b5c927713
Autor:
Philip M Daniell, Mark Leese, Ralph D. Lorenz, James Garry, Marek Banaszkiewicz, B. Hathi, Andrew J. Ball, John C. Zarnecki, Axel Hagermann, Martin C. Towner, Phil Rosenberg
Publikováno v:
Icarus. 197:579-584
Thermal conductivity measurements, presented in this paper (Fig. 3), were made during the descent of the Huygens probe through the atmosphere of Titan below the altitude of 30 km. The measurements are broadly consistent with reference values derived
Autor:
B. Hathi, Andrew J. Ball, Nadeem Ghafoor, Ralph D. Lorenz, Axel Hagermann, Mark Leese, Martin C. Towner, John C. Zarnecki
Publikováno v:
Planetary and Space Science. 55:1936-1948
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 some of which were excited by the Titan environment. Several sensors in the Huygens Surface
Autor:
B. Hathi, Philip D. Rosenberg, Mark Leese, Håkan Svedhem, John C. Zarnecki, Axel Hagermann, Martin C. Towner, Ralph D. Lorenz, James Garry
Publikováno v:
Icarus
Icarus, Elsevier, 2007, 189 (2), pp.538. ⟨10.1016/j.icarus.2007.02.004⟩
Icarus, Elsevier, 2007, 189 (2), pp.538. ⟨10.1016/j.icarus.2007.02.004⟩
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 speed-of-sound sensor. We present the first detailed description of the SSP speed of sound me
Publikováno v:
Journal of Thermal Analysis and Calorimetry. 87:585-590
This paper outlines the method of measurement and analysis of the thermal conductivity instrument (THP) that has successfully returned measurements from the atmosphere of Saturn’s moon Titan during the descent of the Huygens probe on 14th January 2
Autor:
Mark Leese, Axel Hagermann, Martin C. Towner, John C. Zarnecki, B. C. Clark, Håkan Svedhem, James Garry, Ralph D. Lorenz, B. Hathi
Publikováno v:
Icarus. 185:457-465
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 the implications of its data for the geomorphology and characteristics of the Huygens landi
Autor:
B. Hathi, Andrew J. Ball, Mark Leese, Ralph D. Lorenz, Philip D. Rosenberg, Axel Hagermann, Martin C. Towner, John C. Zarnecki
Publikováno v:
Advances in Space Research. 38:794-798
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 on Titan has become less popular over the last decade, though the possibility of lak