English  |  正體中文  |  简体中文  |  Items with full text/Total items : 54367/62174 (87%)
Visitors : 14184566      Online Users : 71
RC Version 6.0 © Powered By DSPACE, MIT. Enhanced by NTHU Library IR team.
Scope Tips:
  • please add "double quotation mark" for query phrases to get precise results
  • please goto advance search for comprehansive author search
  • Adv. Search
    HomeLoginUploadHelpAboutAdminister Goto mobile version

    Please use this identifier to cite or link to this item: http://nthur.lib.nthu.edu.tw/dspace/handle/987654321/81009

    Authors: CUZZI, J.N.;LISSAUER, J.J.;SHU, F.H.
    教師: 徐遐生
    Date: 1981
    Publisher: Nature Publishing Group
    Relation: NATURE, Nature Publishing Group, Volume 292, Issue 5825, 1981, Pages 703-707
    Keywords: SATURNS RINGS
    Abstract: Certain radial brightness variations in the outer Cassini division of Saturn's rings may be spiral density waves driven by Saturn's large moon Iapetus, in which case a value of ~16 g cm−2 for the surface density is calculated in the region where the waves are seen. The kinematic viscosity in the same region is ~170 cm2 s−1 and the vertical scale height of the ring is estimated to be a maximum of ~40 m.
    Relation Link: http://www.nature.com/npg_/index_npg.html
    URI: http://nthur.lib.nthu.edu.tw/dspace/handle/987654321/81009
    Appears in Collections:[ 徐遐生 (2002-2006)] 期刊論文
    [物理系] 期刊論文

    Files in This Item:

    File SizeFormat


    SFX Query


    DSpace Software Copyright © 2002-2004  MIT &  Hewlett-Packard  /   Enhanced by   NTU Library IR team Copyright ©   - Feedback