小郷原 一智
   所属   京都産業大学  理学部 宇宙物理・気象学科
   職種   准教授
発行・発表の年月 2018/12/01
形態種別 研究論文
査読 査読あり
標題 Initial products of Akatsuki 1-μm camera
執筆形態 その他
掲載誌名 Earth, Planets and Space
巻・号・頁 70(1)
著者・共著者 Iwagami N,Sakanoi T,Hashimoto G.L,Sawai K,Ohtsuki S,Takagi S,Uemizu K,Ueno M,Kameda S,Murakami S.-Y,Nakamura M,Ishii N,Abe T,Satoh T,Imamura T,Hirose C,Suzuki M,Hirata N,Yamazaki A,Sato T.M,Yamada M,Yamamoto Y,Fukuhara T,Ogohara K,Ando H,Sugiyama K.-I,Kashimura H,Kouyama T
概要 © 2018, The Author(s). The status and initial products of the 1-μm camera onboard the Akatsuki mission to Venus are presented. After the successful retrial of Venus’ orbit insertion on Dec. 2015 (5 years after the failure in Dec. 2010), and after a long cruise under intense radiation, damage in the detector seems small and fortunately insignificant in the final quality of the images. More than 600 dayside images have been obtained since the beginning of regular operation on Apr. 2016 although nightside images are less numerous (about 150 in total at three wavelengths) due to the light scattered from the bright dayside. However, data acquisition stopped after December 07, 2016, due to malfunction of the electronics and has not been resumed since then. The 0.90-µm dayside images are of sufficient quality for the cloud-tracking procedure to retrieve wind field in the cloud region. The results appear to be similar to those reported by previous 1-μm imaging by Galileo and Venus Express. The representative altitude sampled for such dayside images is estimated to be 51–55 km. Also, the quality of the nightside 1.01-µm images is sufficient for a search for active volcanism, since interference due to cloud inhomogeneity appears to be insignificant. The quality of the 0.97-µm images may be insufficient to achieve the expected spatial resolution for the near-surface H2O mixing ratio retrievals.[Figure not available: see fulltext.].
DOI 10.1186/s40623-017-0773-5
ISSN 1343-8832/1880-5981
Put Code(ORCID) 52343306
PermalinkURL http://orcid.org/0000-0001-7666-4442