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 987654321/50411
English  |  正體中文  |  简体中文  |  Items with full text/Total items : 80990/80990 (100%)
Visitors : 43340742      Online Users : 1592
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/987654321/50411


    Title: Studying the Lunar Ionosphere with SELENE Radio Science Experiment
    Authors: Imamura,T;Iwata,T;Yamamoto,Z;Mochizuki,N;Kono,Y;Matsumoto,K;Liu,QH;Noda,H;Hanada,H;Oyama,K;Nabatov,A;Futaana,Y;Saito,A;Ando,H
    Contributors: 太空科學研究所
    Keywords: SOURCE 3C 273;GPS NETWORK;PHOTOELECTRON LAYER;GEOMAGNETIC TAIL;MAGNETIC-FIELDS;SOLAR-WIND;ATMOSPHERE;OCCULTATION;SURFACE;PROSPECTOR
    Date: 2010
    Issue Date: 2012-03-27 17:31:07 (UTC+8)
    Publisher: 國立中央大學
    Abstract: Radio occultation observations of the electron density near the lunar surface were conducted during the SELENE (Kaguya) mission using the Vstar and Rstar sub-satellites. Previous radio occultation measurements conducted in the Soviet lunar missions have indicated the existence of an ionosphere with peak densities of several hundreds of electrons per cubic centimeters above the dayside lunar surface. These densities are difficult to explain theoretically when the removal of plasma by the solar wind is considered, and thus the generation mechanism of the lunar ionosphere is a major issue, with even the validity of previous observations still under debate. The most serious error source in the measurement is the fluctuation of the terrestrial ionosphere which also exists along the ray path. To cope with this difficulty, about 400 observations were conducted using Vstar to enable statistical analysis of the weak signal of the lunar ionosphere. Another method is to utilize Vstar and Rstar with the second one being used to measure the terrestrial ionosphere contribution. The observations will establish the morphology of the lunar ionosphere and will reveal its relationship with various conditions to provide possible clues to the mechanism.
    Relation: SPACE SCIENCE REVIEWS
    Appears in Collections:[Graduate Institute of Space Science] journal & Dissertation

    Files in This Item:

    File Description SizeFormat
    index.html0KbHTML544View/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