Three-dimensional infrared models of the interplanetary dust distribution

DOI PDF Web Site Web Site Web Site 被引用文献1件 参考文献22件
  • Kwon S. M.
    Department of Science Education, Kangwon National University
  • Hong S. S.
    Department of Astronomy, Seoul National University

書誌事項

タイトル別名
  • Three-dimensional infrared models of th

この論文をさがす

抄録

We have calculated the brightness of zodiacal emission by using the three dimensional optical models of zodiacal cloud. By comparing the calculated brightness distribution with the IRAS observations, we found that the cosine model is the best out of the three for describing the helioecliptic latitude dependence of dust distribution. We also found best parameters for the heliocentric variations of the dust temperature and volumetric absorption cross-section. Inclination and ascending node of the symmetry plane were deduced from annual variations of i) the peak offset latitude and ii) the pole brightness difference. Longitudes of the ascending node derived from i) and ii) are shown to be significantly different from each other.

収録刊行物

被引用文献 (1)*注記

もっと見る

参考文献 (22)*注記

もっと見る

詳細情報 詳細情報について

問題の指摘

ページトップへ