Titan's meridional wind profile and Huygens' orientation and swing inferred from the geometry of DISR imaging

被引:14
|
作者
Karkoschka, Erich [1 ]
机构
[1] Univ Arizona, Lunar & Planetary Lab, Tucson, AZ 85721 USA
关键词
Titan; surface; atmosphere; Atmospheres; dynamics; Rotational dynamics; MIDLATITUDE CLOUDS; LANDING SITE; PROBE; ATMOSPHERE; DESCENT; SURFACE; TEMPERATURES; ENVIRONMENT; DYNAMICS; MIDDLE;
D O I
10.1016/j.icarus.2015.06.012
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The altitude and zonal motion of the Huygens probe descending through Titan's atmosphere was determined early under the assumption of no meridional motion (Bird et al. [2005]. Nature 438, 800-802). By comparing images taken during the descent, Karkoschka et al. (Karkoschka et al. [2007]. Planet. Space Sci. 55, 1895-1935) determined the meridional motion of Huygens, which was generally much smaller than its zonal motion. Here, we present a comprehensive geometrical analysis of all images taken during the descent that is four times more accurate than the previous study. The result is a meridional wind profile across Titan's troposphere with northward winds by up to 0.4 m/s with an average of 0.1 m/s above 1 km altitude, and southward winds below, peaking at 0.9 m/s near 0.4 km altitude. The imaging data extend down to 0.22 km altitude, although additional information came from the horizontal impact speed near 0.8 m/s southward (Schroder et al. [2012]. Planet. Space Sci. 73, 327-340). There is a region between 5 and 8 km altitude with no significant meridional wind. In the stratosphere, the average meridional wind was 1.2 +/- 1.5 m/s northward, and zero meridional motion is possible down to 15 km altitude. We present the difference between the zonal speeds of Huygens and the wind that was ignored in previous publications and amounts to up to 7 m/s. We determined the three rotational angles of Huygens for the times of each exposure that showed surface features. During 26 exposures, the swing speed of Huygens was fast enough to smear images. Inferred swing speeds were up to 20 degrees/s during the calm phase of the descent, consistent with up to 40 degrees/s swings reported before during the rough phase. The improved geometric calibration of images allowed identification of many features also seen in Cassini radar images. This comparison yields the location of the Huygens Landing Site as 192.34 +/- 02 degrees West and 10.47 +/- 0.02 degrees South. (C) 2015 Elsevier Inc. All rights reserved.
引用
收藏
页码:326 / 338
页数:13
相关论文
共 6 条
  • [1] DISR imaging and the geometry of the descent of the Huygens probe within Titan's atmosphere
    Karkoschka, Erich
    Tomaskoa, Martin G.
    Doose, Lyn R.
    See, Chuck
    McFarlane, Elisabeth A.
    Schroeder, Stefan E.
    Rizk, Bashar
    [J]. PLANETARY AND SPACE SCIENCE, 2007, 55 (13) : 1896 - 1935
  • [2] The properties of Titan's surface at the Huygens landing site from DISR observations
    Keller, H. U.
    Grieger, B.
    Kueppers, M.
    Schroeder, S. E.
    Skorov, Y. V.
    Tomasko, M. G.
    [J]. PLANETARY AND SPACE SCIENCE, 2008, 56 (05) : 728 - 752
  • [3] Eight-color maps of Titan's surface from spectroscopy with Huygens' DISR
    Karkoschka, Erich
    Schroeder, Stefan E.
    [J]. ICARUS, 2016, 270 : 260 - 271
  • [4] The methane mole fraction in Titan's stratosphere from DISR measurements during the Huygens probe's descent
    Bezard, Bruno
    [J]. ICARUS, 2014, 242 : 64 - 73
  • [5] Simultaneous retrieval of optical depths and scattering phase functions in Titan's atmosphere from Huygens/DISR data
    Grieger, B
    Rodin, A
    Salinas, S
    Keller, HU
    [J]. PLANETARY AND SPACE SCIENCE, 2003, 51 (14-15) : 991 - 1001
  • [6] New insights on Titan's plasma-driven Schumann resonance inferred from Huygens and Cassini data
    Beghin, C.
    Canu, P.
    Karkoschka, E.
    Sotin, C.
    Bertucci, C.
    Kurth, W. S.
    Berthelier, J. J.
    Grard, R.
    Hamelin, M.
    Schwingenschuh, K.
    Simoes, F.
    [J]. PLANETARY AND SPACE SCIENCE, 2009, 57 (14-15) : 1872 - 1888