English  |  正體中文  |  简体中文  |  Items with full text/Total items : 66984/66984 (100%)
Visitors : 22656129      Online Users : 263
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/987654321/39305


    Title: STOKES PARAMETERS FOR THOMSON SCATTERING IN A COLD MAGNETIZED PLASMA
    Authors: CHOU,CK;CHEN,HH
    Contributors: 物理研究所
    Keywords: COMPTON-SCATTERING;FIELDS;RADIATION;PULSARS;GAPS;ENERGETICS
    Date: 1994
    Issue Date: 2010-07-08 14:11:30 (UTC+8)
    Publisher: 中央大學
    Abstract: The effect of a strong magnetic field on neutron stars or white dwarfs is calculated for Thomson scattering in a fully ionized collisionless plasma. The Stokes parameters for the scattered radiation are computed explicitly in terms of the state of polarization of the incident wave, the electron-cyclotron frequency, the plasma frequency, the angle of incidence, and the angle of scattering. The effects of the plasma are very insensitive to specific values of V(V = omega(p)2/omega2, omega(p) denotes the electron plasma frequency) so long as V much less than 1, whereas the criterion for the magnetic field to substantially affect the Stokes parameters is that the photon frequency be less than the electron-cyclotron frequency. The effects of classical radiation damping and natural line broadening are briefly mentioned.
    Relation: ASTROPHYSICS AND SPACE SCIENCE
    Appears in Collections:[物理研究所] 期刊論文

    Files in This Item:

    File Description SizeFormat
    index.html0KbHTML269View/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 ©   - Feedback  - 隱私權政策聲明