@inproceedings{oai:jaxa.repo.nii.ac.jp:00003122,
 author = {高羽, 幸 and 金田, 英宏 and 石原, 大助 and 深川, 美里 and 安田, 晃子 and 小林, 宙 and 大坪, 貴文 and Takaba, Sachi and Kaneda, Hidehiro and Ishihara, Daisuke and Fukagawa, Misato and Yasuda, Akiko and Kobayashi, Hiroshi and Otsubo, Takafumi},
 book = {宇宙航空研究開発機構特別資料, JAXA Special Publication: The Cosmic Wheel and the Legacy of the AKARI archive: from galaxies and stars to planets and life},
 month = {Mar},
 note = {第4回「あかり」国際会議 (2017年10月17-20日. 東京大学), 文京区, 東京, The 4th AKARI International Conference: The Cosmic Wheel and the Legacy of the AKARI archive: from galaxies and stars to planets and life (October 17-20, 2017. The University of Tokyo), Bunkyo-ku, Tokyo, Japan, The zodiacal cloud in our solar system emits thermal radiation from the interplanetary dust (IPD), which is the dominant foreground emission for mid-IR observations in space. The zodiacal cloud has small-scale spatial structures called ''dust bands'', which are formed by dust grains originating in the asteroidal main belt. It also has the smooth cloud, a dominant component of a several au scale. In the previous study, based on the AKARI 9 and 18 micrometers mid-IR all-sky survey data, the zodiacal cloud standard model (Kelsall et al. 1998) has been re-examined and improved especially for the smooth cloud (Kondo et al. 2016a). However, the improved model still does not well reproduce the observational data on small spatial structures. In this study, we further improve the Kelsall model for the dust bands, using the AKARI mid-IR all-sky survey data., 形態: カラー図版あり, Physical characteristics: Original contains color illustrations, 資料番号: AA1730026048, レポート番号: JAXA-SP-17-009E},
 pages = {265--268},
 publisher = {宇宙航空研究開発機構(JAXA), Japan Aerospace Exploration Agency (JAXA)},
 title = {A Study of the Dust Bands in the Zodiacal Cloud using AKARI Mid-Infrared All-sky Survey Data},
 volume = {JAXA-SP-17-009E},
 year = {2018}
}