X-Raying Neutral Density Disturbances in the Mesosphere and Lower Thermosphere induced by the 2022 Hunga-Tonga Volcano Eruption-Explosion

Fuente: arXiv
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Main Authors: Katsuda, Satoru, Shinagawa, Hiroyuki, Fujiwara, Hitoshi, Jin, Hidekatsu, Miyoshi, Yasunobu, Miyoshi, Yoshizumi, Motizuki, Yuko, Nakajima, Motoki, Nakazawa, Kazuhiro, Nobukawa, Kumiko K., Otsuka, Yuichi, Shinbori, Atsushi, Sori, Takuya, Tao, Chihiro, Tashiro, Makoto S., Wada, Yuuki, Yamawaki, Takaya
Format: Preprint
Published: 2024
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author Katsuda, Satoru
Shinagawa, Hiroyuki
Fujiwara, Hitoshi
Jin, Hidekatsu
Miyoshi, Yasunobu
Miyoshi, Yoshizumi
Motizuki, Yuko
Nakajima, Motoki
Nakazawa, Kazuhiro
Nobukawa, Kumiko K.
Otsuka, Yuichi
Shinbori, Atsushi
Sori, Takuya
Tao, Chihiro
Tashiro, Makoto S.
Wada, Yuuki
Yamawaki, Takaya
author_facet Katsuda, Satoru
Shinagawa, Hiroyuki
Fujiwara, Hitoshi
Jin, Hidekatsu
Miyoshi, Yasunobu
Miyoshi, Yoshizumi
Motizuki, Yuko
Nakajima, Motoki
Nakazawa, Kazuhiro
Nobukawa, Kumiko K.
Otsuka, Yuichi
Shinbori, Atsushi
Sori, Takuya
Tao, Chihiro
Tashiro, Makoto S.
Wada, Yuuki
Yamawaki, Takaya
contents We present X-ray observations of the upper atmospheric density disturbance caused by the explosive eruption of the Hunga Tonga-Hunga Ha'apai (HTHH) volcano on 15 January 2022. From 14 January to 16 January, the Chinese X-ray astronomy satellite, Insight-HXMT, was observing the supernova remnant Cassiopeia A. The X-ray data obtained during Earth's atmospheric occultations allowed us to measure neutral densities in the altitude range of ~90-150 km. The density profiles above 110 km altitude obtained before the major eruption are in reasonable agreement with expectations by both GAIA and NRLMSIS 2.0 models. In contrast, after the HTHH eruption, a severe density depletion was found up to ~1,000 km away from the epicenter, and a relatively weak depletion extending up to ~7,000 km for over 8 hr after the eruption. In addition, density profiles showed wavy structures with a typical length scale of either ~20 km (vertical) or ~1,000 km (horizontal). This may be caused by Lamb waves or gravity waves triggered by the volcanic eruption.
format Preprint
id arxiv_https___arxiv_org_abs_2410_09410
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle X-Raying Neutral Density Disturbances in the Mesosphere and Lower Thermosphere induced by the 2022 Hunga-Tonga Volcano Eruption-Explosion
Katsuda, Satoru
Shinagawa, Hiroyuki
Fujiwara, Hitoshi
Jin, Hidekatsu
Miyoshi, Yasunobu
Miyoshi, Yoshizumi
Motizuki, Yuko
Nakajima, Motoki
Nakazawa, Kazuhiro
Nobukawa, Kumiko K.
Otsuka, Yuichi
Shinbori, Atsushi
Sori, Takuya
Tao, Chihiro
Tashiro, Makoto S.
Wada, Yuuki
Yamawaki, Takaya
Geophysics
Earth and Planetary Astrophysics
Atmospheric and Oceanic Physics
We present X-ray observations of the upper atmospheric density disturbance caused by the explosive eruption of the Hunga Tonga-Hunga Ha'apai (HTHH) volcano on 15 January 2022. From 14 January to 16 January, the Chinese X-ray astronomy satellite, Insight-HXMT, was observing the supernova remnant Cassiopeia A. The X-ray data obtained during Earth's atmospheric occultations allowed us to measure neutral densities in the altitude range of ~90-150 km. The density profiles above 110 km altitude obtained before the major eruption are in reasonable agreement with expectations by both GAIA and NRLMSIS 2.0 models. In contrast, after the HTHH eruption, a severe density depletion was found up to ~1,000 km away from the epicenter, and a relatively weak depletion extending up to ~7,000 km for over 8 hr after the eruption. In addition, density profiles showed wavy structures with a typical length scale of either ~20 km (vertical) or ~1,000 km (horizontal). This may be caused by Lamb waves or gravity waves triggered by the volcanic eruption.
title X-Raying Neutral Density Disturbances in the Mesosphere and Lower Thermosphere induced by the 2022 Hunga-Tonga Volcano Eruption-Explosion
topic Geophysics
Earth and Planetary Astrophysics
Atmospheric and Oceanic Physics
url https://arxiv.org/abs/2410.09410