日本地球惑星科学連合2019年大会

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[J] 口頭発表

セッション記号 M (領域外・複数領域) » M-IS ジョイント

[M-IS09] 最新の大気科学:ダスト

2019年5月30日(木) 13:45 〜 15:15 102 (1F)

コンビーナ:石塚 正秀(香川大学)、黒崎 泰典(鳥取大学乾燥地研究センター)、関山 剛(気象庁気象研究所)、長島 佳菜(海洋研究開発機構 地球環境観測研究開発センター)、座長:関山 剛

15:00 〜 15:15

[MIS09-05] Dust layer captured by an inversion layer over the Gobi Desert on 29–30 April 2015

*河合 慶1西尾 優汰2甲斐 憲次1,3能田 淳4Erdenebadrakh Munkhjargal1,5篠田 雅人1杉本 伸夫6清水 厚6Enkhbaatar Davaanyam5,7Dashdondog Batdorj8 (1.名古屋大学、2.気象庁、3.茨城大学、4.酪農学園大学、5.モンゴル気象水文環境情報研究所、6.国立環境研究所、7.筑波大学、8.モンゴル気象環境監視庁)

キーワード:黄砂・アジアダスト、砂塵嵐・ダストストーム、長距離輸送、シーロメーター、ライダー、ゴビ砂漠

Asian dust originates in arid and semi-arid regions of East Asia, such as the Gobi Desert and the Taklimakan Desert. If the dust emitted from the ground surface reaches the free troposphere, it can be transported toward the Pacific Ocean over a long range by the westerlies. Therefore, the vertical distribution of dust over the source region is a key factor of the long-range transport of dust. In the Gobi Desert, a ceilometer (compact lidar) observation has been conducted at Dalanzadgad, Mongolia, since the end of April 2013. The ceilometer observed a developed dust storm over the ground and a dust layer at a height of 1.2–1.8 km on 29–30 April 2015. According to SYNOP reports, this dust storm had already developed in the upwind region before arriving at Dalanzadgad. This feature was consistent with the sudden increase of the ceilometer observation values. Then, the dust was lifted to a height of 1.2–1.8 km, and the dust layer was observed at almost the same height for 12 hours by the ceilometer. During this dust event, radiosonde observation at Dalanzadgad showed an inversion layer at a height of 1.2–1.5 km over cold air. These results suggest that the dust layer was captured by the inversion layer, which prevented the dust from reaching the free troposphere and restrained the long-range transport of the dust by the westerlies. This study was supported by Research Fellowships of Japan Society for the Promotion of Science (JSPS) for Young Scientists and by Grants-in-Aid for Scientific Research from the JSPS (16H02703, 17H01616, and 18J12795).