The unusual dynamics of northern Dark Spots on Neptune

被引:21
|
作者
Sromovsky, LA [1 ]
Fry, PM
Baines, KH
机构
[1] Univ Wisconsin, Space Sci & Engn Ctr, Madison, WI 53706 USA
[2] CALTECH, Jet Prop Lab, Pasadena, CA 91109 USA
基金
美国国家航空航天局;
关键词
Neptune; dynamics; atmosphere;
D O I
10.1006/icar.2001.6761
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Hubble Space Telescope (HST) and ground-based observations of Neptune from 1991 to 2000 show that Neptune's northern Great Dark Spots (NGDS) remained remarkably stable in latitude and longitudinal drift rate, in marked contrast to the 1989 southern Great Dark Spot (GDS), which moved continuously equatorward during 1989 and dissipated unseen during 1990. NGDS-32, discovered in October 1994 HST images, (H. B. Hammel et al., 1995, Science 268, 1740-1742), stayed at similar to32degreesN from 1994 through at least 1996, and possibly through 2000. The second northern GDS (NGDS-15), discovered in August 1996 HST images, (L. A. Sromovsky et al. 2001, Icarus 146, 459-488), appears to have existed as early as 8 March 1996 and remained near 15degreesN for the 16 months over which it was observed. NGDS-32 had a very uniform longitudinal drift rate averaging -36.28+/-0.04degrees/day from 10 October 1994 to 2 November 1995, and -35.84+/-0.02degrees/day from I September 1995 through 24 November 1995. A single circulation feature certainly exists during each of the first two periods, though it is not certain that it is the same feature. It is probable, but less certain, that only a single circulation feature was tracked during the 1996-1998 period, during which positions are consistent with a modulated drift rate averaging -35.401+/-0.001degrees/day, but with a peak-to-peak modulation of 1.5degrees/day with an similar to760-day period. If NDS-32 varied its drift rate in accord with the local latitudinal shear in the zonal wind, then all its drift-rate changes might be due to only similar to0.4degrees of latitudinal motion. The movement of NGDS-15 is also not consistent with a uniform longitudinal drift rate, but the nature of its variation cannot be estimated from the limited set of observations. The relatively stable latitudinal positions of both northern dark spots are not consistent with current numerical model calculations treating them as anticyclonic vortices in a region of uniform potential vorticity gradient (R. P. Lebeau and T. E. Dowling 1998, Icarus 132, 239-265). Possible explanations include unresolved latitudinal structure in the zonal wind background or unaccounted-for variations in vertical stability structure. (C) 2002 Elsevier Science (USA).
引用
收藏
页码:16 / 36
页数:21
相关论文
共 50 条
  • [21] The dynamics of inclined Neptune Trojans
    R. Dvorak
    Ch. Lhotka
    R. Schwarz
    Celestial Mechanics and Dynamical Astronomy, 2008, 102 : 97 - 110
  • [22] The dynamics of inclined Neptune Trojans
    Dvorak, R.
    Lhotka, Ch.
    Schwarz, R.
    CELESTIAL MECHANICS & DYNAMICAL ASTRONOMY, 2008, 102 (1-3): : 97 - 110
  • [23] Unusual Mucosal Spots in Adulthood
    Yilmaz, Kaan
    Anemueller, Waltraud
    DEUTSCHES ARZTEBLATT INTERNATIONAL, 2023, 119 (50): : 875 - 875
  • [24] Evolution of a dark vortex on Neptune with transient secondary features
    Wong, Michael H.
    Sromovsky, Lawrence A.
    Fry, Patrick M.
    Sanchez-Lavega, Agustin
    Hueso, Ricardo
    Legarreta, Jon
    Simon, Amy A.
    Morales-Juberias, Raul
    Tollefson, Joshua
    de Pater, Imke
    Irwin, Patrick G. J.
    ICARUS, 2022, 387
  • [25] Formation of a New Great Dark Spot on Neptune in 2018
    Simon, A. A.
    Wong, M. H.
    Hsu, A. I.
    GEOPHYSICAL RESEARCH LETTERS, 2019, 46 (06) : 3108 - 3113
  • [26] Role of bran particles in the formation of dark spots on fresh wet noodle sheets: what are the dark spots?
    Zhao, Yang
    Huang, Ze-Hua
    Zhou, Hui-Ming
    Ma, Liang
    An, Yan-Xia
    Abddollahi, Mehdi
    Zhang, Jian
    Yin, Gui-Hong
    JOURNAL OF THE SCIENCE OF FOOD AND AGRICULTURE, 2023, 103 (11) : 5560 - 5568
  • [27] Inhibition of hexose oxidase on the dark spots in fresh wet noodle sheets: A feasible prevention of dark spots
    Zhao, Yang
    Huang, Ze-Hua
    Zhou, Hui-Ming
    Zhu, Ke-Xue
    Guo, Xiao-Na
    Peng, Wei
    FOOD CHEMISTRY, 2021, 339
  • [28] SPECTRAL OBSERVATIONS OF IMPACT DARK SPOTS
    SUZUKI, B
    KURIHARA, H
    SASAKI, T
    WATANABE, J
    EARTH MOON AND PLANETS, 1994, 66 (01): : 19 - 27
  • [29] Cold spots in the Chamaeleon dark clouds
    Hotzel, S
    Lemke, D
    Tóth, LV
    Stickel, M
    Krause, O
    Klaas, U
    Bogun, S
    Kessler, MF
    Laureijs, RJ
    Burgdorf, M
    Beichman, CA
    Rowan-Robinson, M
    Efstathiou, A
    Richter, G
    Braun, M
    UNIVERSE AS SEEN BY ISO, VOLS I AND II, 1999, 427 : 675 - 678
  • [30] Episodic bright and dark spots on Uranus
    Sromovsky, L. A.
    Hammel, H. B.
    de Pater, I.
    Fry, P. M.
    Rages, K. A.
    Showalter, M. R.
    Merline, W. J.
    Tamblyn, P.
    Neyman, C.
    Margot, J. -L.
    Fang, J.
    Colas, F.
    Dauvergne, J. -L.
    Gomez-Forrellad, J. M.
    Hueso, R.
    Sanchez-Lavega, A.
    Stallard, Thomas
    ICARUS, 2012, 220 (01) : 6 - 22