中大機構典藏-NCU Institutional Repository-提供博碩士論文、考古題、期刊論文、研究計畫等下載:Item 987654321/33037
English  |  正體中文  |  简体中文  |  Items with full text/Total items : 80990/80990 (100%)
Visitors : 41773786      Online Users : 2235
RC Version 7.0 © Powered By DSPACE, MIT. Enhanced by NTU 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://ir.lib.ncu.edu.tw/handle/987654321/33037


    Title: Growth and form of planetary seedlings: Results from a microgravity aggregation experiment
    Authors: Blum,J;Wurm,G;Kempf,S;Poppe,T;Klahr,H;Kozasa,T;Rott,M;Henning,T;Dorschner,J;Schrapler,R;Keller,HU;Markiewicz,WJ;Mann,I;Gustafson,BAS;Giovane,F;Neuhaus,D;Fechtig,H;Grun,E;Feuerbacher,B;Kochan,H;Ratke,L;El Goresy,A
    Contributors: 太空科學研究所
    Keywords: PREPLANETARY DUST AGGREGATION;BROWNIAN-MOTION
    Date: 2000
    Issue Date: 2010-07-07 10:26:30 (UTC+8)
    Publisher: 中央大學
    Abstract: The outcome of the first stage of planetary formation, which is characterized by ballistic agglomeration of preplanetary dust grains due to Brownian motion in the free molecular flow regime of the solar nebula, is still somewhat speculative. We performed
    Relation: PHYSICAL REVIEW LETTERS
    Appears in Collections:[Graduate Institute of Space Science] journal & Dissertation

    Files in This Item:

    File Description SizeFormat
    index.html0KbHTML503View/Open


    All items in NCUIR are protected by copyright, with all rights reserved.

    社群 sharing

    ::: Copyright National Central University. | 國立中央大學圖書館版權所有 | 收藏本站 | 設為首頁 | 最佳瀏覽畫面: 1024*768 | 建站日期:8-24-2009 :::
    DSpace Software Copyright © 2002-2004  MIT &  Hewlett-Packard  /   Enhanced by   NTU Library IR team Copyright ©   - 隱私權政策聲明