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Images of brightness-temperature difference between two thermal infrared channels (10.3-11.3μm and 11.5-12.5μm) were applied for detecting distribution of the eruption clouds. The results show that the eruption cloud migrated to the southeast along the line connecting between Mt. Asama and Katsuura-city on the Boso peninsula through the central part of Tokyo. The eruption cloud elongated toward the direction of the migration and the total length increased with time. The speed of the head and tail of the eruption cloud was estimated to be 135km/h and 51km/h, respectively. This relative speed difference could cause elongation of the total length. According to the meteorological data, at the altitude of 4900-5700m, wind was blowing to the southeast at the speed of 119km/h, and at 2700-3100m to the same direction at 50km/h. 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  1. 防災科研関係論文

MTSATで捉えた浅間山2009年2月2日噴火に伴う噴煙

https://nied-repo.bosai.go.jp/records/5376
https://nied-repo.bosai.go.jp/records/5376
e5ede2ee-de4c-4752-bb16-379fc4c460ae
Item type researchmap(1)
公開日 2023-03-30
タイトル
言語 ja
タイトル MTSATで捉えた浅間山2009年2月2日噴火に伴う噴煙
タイトル
言語 en
タイトル MTSAT Observation of the Eruption Cloud Occurred at the February 2, 2009 Eruption of Mt. Asama, Central Japan
言語
言語 jpn
著者 金子 隆之

× 金子 隆之

ja 金子 隆之

en KANEKO Takayuki

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田 寛之

× 田 寛之

ja 田 寛之

en DEN Hiroyuki

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高崎 健二

× 高崎 健二

ja 高崎 健二

en TAKASAKI Kenji

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安田 敦

× 安田 敦

ja 安田 敦

en YASUDA Atsushi

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前野 深

× 前野 深

ja 前野 深

en MAENO Fukashi

Search repository
小山 悦郎

× 小山 悦郎

ja 小山 悦郎

en KOYAMA Etsuro

Search repository
中田 節也

× 中田 節也

ja 中田 節也

en NAKADA Setsuya

Search repository
抄録
内容記述タイプ Other
内容記述 Mt. Asama (2568m a.s.l.) erupted on 2<sup>nd</sup> February 2009 at 1:51am (JST). Although it was a small-scale eruption, involving a eruption plume rising 2000m high from the summit, the ashes accidentally fell in the Tokyo metropolitan area, due to strong seasonal wind, which draw public concern. We observed migration and enlargement processes of the eruption cloud, using infrared images from Multi-functional Transport Satellite (MTSAT), and analyzed its relationship to distribution of ash-fall deposits and meteorological conditions. MTSAT is a gestational meteorological satellite of Japan Meteorological Agency and Civil Aviation Bureau and has five observation channels in the visible to infrared regions (visible: 1 and infrared: 4). Although the resolution is low (4km in infrared), the observation cycle is very high (every 30 to 60 minutes), which is preferable characteristics to eruption cloud studies. We used four MTSAT images taken on 2<sup>nd</sup> February at 2:30am, 3:30am, 4:30am and 5:30am. Images of brightness-temperature difference between two thermal infrared channels (10.3-11.3μm and 11.5-12.5μm) were applied for detecting distribution of the eruption clouds. The results show that the eruption cloud migrated to the southeast along the line connecting between Mt. Asama and Katsuura-city on the Boso peninsula through the central part of Tokyo. The eruption cloud elongated toward the direction of the migration and the total length increased with time. The speed of the head and tail of the eruption cloud was estimated to be 135km/h and 51km/h, respectively. This relative speed difference could cause elongation of the total length. According to the meteorological data, at the altitude of 4900-5700m, wind was blowing to the southeast at the speed of 119km/h, and at 2700-3100m to the same direction at 50km/h. These values roughly coincided with the estimated speed of the head and tail, respectively, indicating the difference in the wind speed was the main cause of the elongation. Distribution area of the ash-fall deposits on the ground did not well much the area where the eruption cloud flew over, but was located 0-40km south of it. Unlike the higher altitude, in the regions lower than ~2000m, wind was roughly blowing to the south at somewhat lower speed. When falling ashes from the eruption cloud entered this region, they could be blown to the further south, which could cause the wide and biased distribution of the ash-fall deposits, as observed.
言語 ja
抄録
内容記述タイプ Other
内容記述 Mt. Asama (2568m a.s.l.) erupted on 2<sup>nd</sup> February 2009 at 1:51am (JST). Although it was a small-scale eruption, involving a eruption plume rising 2000m high from the summit, the ashes accidentally fell in the Tokyo metropolitan area, due to strong seasonal wind, which draw public concern. We observed migration and enlargement processes of the eruption cloud, using infrared images from Multi-functional Transport Satellite (MTSAT), and analyzed its relationship to distribution of ash-fall deposits and meteorological conditions. MTSAT is a gestational meteorological satellite of Japan Meteorological Agency and Civil Aviation Bureau and has five observation channels in the visible to infrared regions (visible: 1 and infrared: 4). Although the resolution is low (4km in infrared), the observation cycle is very high (every 30 to 60 minutes), which is preferable characteristics to eruption cloud studies. We used four MTSAT images taken on 2<sup>nd</sup> February at 2:30am, 3:30am, 4:30am and 5:30am. Images of brightness-temperature difference between two thermal infrared channels (10.3-11.3μm and 11.5-12.5μm) were applied for detecting distribution of the eruption clouds. The results show that the eruption cloud migrated to the southeast along the line connecting between Mt. Asama and Katsuura-city on the Boso peninsula through the central part of Tokyo. The eruption cloud elongated toward the direction of the migration and the total length increased with time. The speed of the head and tail of the eruption cloud was estimated to be 135km/h and 51km/h, respectively. This relative speed difference could cause elongation of the total length. According to the meteorological data, at the altitude of 4900-5700m, wind was blowing to the southeast at the speed of 119km/h, and at 2700-3100m to the same direction at 50km/h. These values roughly coincided with the estimated speed of the head and tail, respectively, indicating the difference in the wind speed was the main cause of the elongation. Distribution area of the ash-fall deposits on the ground did not well much the area where the eruption cloud flew over, but was located 0-40km south of it. Unlike the higher altitude, in the regions lower than ~2000m, wind was roughly blowing to the south at somewhat lower speed. When falling ashes from the eruption cloud entered this region, they could be blown to the further south, which could cause the wide and biased distribution of the ash-fall deposits, as observed.
言語 en
書誌情報 ja : 火山
en : BULLETIN OF THE VOLCANOLOGICAL SOCIETY OF JAPAN

巻 55, 号 2, p. 119-128
出版者
言語 ja
出版者 特定非営利活動法人 日本火山学会
出版者
言語 en
出版者 The Volcanological Society of Japan
ISSN
収録物識別子タイプ ISSN
収録物識別子 0453-4360
DOI
関連識別子 10.18940/kazan.55.2_119
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