JpGU-AGU Joint Meeting 2017

講演情報

[EJ] 口頭発表

セッション記号 P (宇宙惑星科学) » P-PS 惑星科学

[P-PS06] [EJ] あかつき金星周回1.5年とその科学成果

2017年5月20日(土) 10:45 〜 12:15 コンベンションホールB (国際会議場 2F)

コンビーナ:佐藤 毅彦(宇宙航空研究開発機構・宇宙科学研究本部)、堀之内 武(北海道大学地球環境科学研究院)、山本 勝(九州大学応用力学研究所)、Kevin McGouldrick(University of Colorado Boulder)、座長:McGouldrick Kevin(University of Colorado Boulder)

10:45 〜 11:05

[PPS06-06] Characteristic features in cloud-top temperature of Venus

★招待講演

*田口 真1福原 哲哉1神山 徹2今村 剛3佐藤 隆雄4二口 将彦10高村 真央1山田 武尊1岩上 直幹5鈴木 睦4上野 宗孝6佐藤 光輝7はしもと じょーじ8高木 聖子9中村 正人4 (1.立教大学、2.産業技術総合研究所、3.東京大学、4.宇宙科学研究所、5.専修大学、6.神戸大学、7.北海道大学、8.岡山大学、9.東海大学、10.東邦大学)

The Longwave Infrared Camera (LIR) onboard Akatsuki has obtained more than 4000 images during the first year after the Venus orbit insertion (VOI-R1) in December 2015. Temperature distributions at the cloud-top altitudes have been retrieved from them. A large bow-shaped thermal structure was discovered in the very first image taken after VOI-R1, and it is concluded by a numerical simulation that the bow-shaped structure is temperature perturbation associated with passage of a gravity wave generated in the equatorial lower atmosphere. More than 15 bows have been found in the images obtained in the subsequent eight months, and we found that most of their center positions locate above the highlands of Venus surface. Local time dependence, topographical distribution, and amplitude of the bows are being investigated. Since Akatsuki is orbiting a highly elongated elliptical orbit almost in the equatorial plane, both northern and southern polar regions can be observed by LIR. It has been known that characteristic thermal features called as polar dipoles and polar collars exist in the polar regions of Venus atmosphere. Rotation periods of the polar vortices have been derived from the cloud-top temperature distributions to be slightly longer than the previous results by Pioneer Venus and Venus Express. Limb darkening is apparent in the Venus disks obtained by LIR, and vertical distributions of cloud particles can be retrieved form the limb darkening profiles combined with a vertical temperature distribution obtained by the radio occultation technique. In the close-up images obtained while Akatsuki passes periapsis cell-like structures with a horizontal scale of ~100 km are found in the low latitudes, and they may correspond to those known in the UV images. Relationship between the cell-like structures seen in the IR and UV images is being studied in detail.