Zodiacal Cloud Complexes

• Mann Ingrid

  MPI für Aeronomie

抄録

We discuss some aspects of the study of the Zodiacal cloud based on brightness observations. The discussion of optical properties as well as the spatial distribution of the dust cloud show that the description of the dust cloud as a homogeneous cloud is reasonable for the regions near the Earth orbit, but fails in the description of the dust in the inner solar system. The reasons for this are that different components of the dust cloud may have different types of orbital evolution depending on the parameters of their initial orbits. Also the collisional evolution of dust in the inner solar system may have some influence. As far as perspectives for future observations are concerned, the study of Doppler shifts of the Fraunhofer lines in the Zodiacal light will provide further knowledge about the orbital distribution of dust particles, as well as advanced infrared observations will help towards a better understanding of the outer solar system dust cloud beyond the asteroid belt.

収録刊行物

• Ｅａｒｔｈ，　Ｐｌａｎｅｔｓ　ａｎｄ　Ｓｐａｃｅ

  Ｅａｒｔｈ，　Ｐｌａｎｅｔｓ　ａｎｄ　Ｓｐａｃｅ 50 (6-7), 465-471, 1998

  地球電磁気・地球惑星圏学会 、公益社団法人 日本地震学会、特定非営利活動法人 日本火山学会、日本測地学会、日本惑星科学会

キーワード

• Space and Planetary Science
• Geology

詳細情報

• CRID: 1390001206508845312
• NII論文ID: 10002206803
• NII書誌ID: AA11211921
• DOI: 10.1186/bf03352135
• ISSN: 18805981
• ISSN: 13438832
• NDL書誌ID: 4552196
• Web Site: https://ndlsearch.ndl.go.jp/books/R000000004-I4552196
• Web Site: https://link.springer.com/content/pdf/10.1186/BF03352135.pdf
• Web Site: https://link.springer.com/article/10.1186/BF03352135/fulltext.html
• Web Site: http://link.springer.com/content/pdf/10.1186/BF03352135
• 本文言語コード: en
• データソース種別:
  • JaLC
  • NDL
  • Crossref
  • CiNii Articles
• 抄録ライセンスフラグ: 使用不可