Zobrazeno 1 - 10
of 10
pro vyhledávání: '"Miyuu Uemura"'
Publikováno v:
Progress in Earth and Planetary Science, Vol 5, Iss 1, Pp 1-16 (2018)
Abstract Seismic interferometry is one of the most effective techniques for detecting temporal variations in seismic velocity caused by large earthquakes. Before the 2011 Tohoku-Oki earthquake (M w 9.0) near the Japan Trench, a slow slip event (SSE,
Externí odkaz:
https://doaj.org/article/0bfaf6bf18d346499011a26e440b2c86
The interactions of wind with the ocean surface, ocean wave with acoustic wave, acoustic wave with seismic wave below the sea bottom, and the interplay among them drive important energy flows from the atmosphere to the lithosphere. Uncertainty remain
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::0f0168715ed9d9d5c99edf6fcf854fe0
https://doi.org/10.5194/egusphere-egu2020-6159
https://doi.org/10.5194/egusphere-egu2020-6159
Temporal variations in seismic velocity at LS1. These figures show the temporal velocity changes calculated from the phase delays at each lapse time: from 10 to 20 s, 20–30 s, 30–40 s, 40–50 s, 50–60 s, and 60–70 s. The four colors of broke
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0469e34698e549326a6bff2ce7664fc4
Temporal variations in seismic velocity at S02. These figures show the temporal velocity changes calculated from the phase delays at each lapse time: from 10 to 20 s, 20–30 s, 30–40 s, 40–50 s, 50–60 s, and 60–70 s. The four colors of broke
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::95f45ce837f5b4dd741a940bd4861cb0
Temporal variations in 15-day ACFs at Station LS2. (a) 15-day ACFs calculated from OBS data over 15 continuous days, including the 7 days before and after the given date. The ACFs plotted in red are in the SSE period, and the bottom ACF is the refere
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::53ad7420af697eedfe6ac803579ed661
Temporal variations in seismic velocity at LS3. These figures show the temporal velocity changes calculated from the phase delays at each lapse time: from 10 to 20 s, 20–30 s, 30–40 s, 40–50 s, 50–60 s, and 60–70 s. The four colors of broke
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f5951f3cb5ec69d8fdf0d90cabea477f
Temporal variations in seismic velocity at LS2. These figures show the temporal velocity changes calculated from the phase delays at each lapse time: from 10 to 20 s, 20–30 s, 30–40 s, 40–50 s, 50–60 s, and 60–70 s. The four colors of broke
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6bdc7ff57ab6e4f8c3d9ca55e7f287f0
Temporal variations in seismic velocity at LS4. These figures show the temporal velocity changes calculated from the phase delays at each lapse time: from 10 to 20 s, 20–30 s, 30–40 s, 40–50 s, 50–60 s, and 60–70 s. The four colors of broke
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3aa0736864d4c519a44ac29b77303995
Temporal variations in 15-day ACFs at Station LS3. (a) 15-day ACFs calculated from OBS data over 15 continuous days, including the 7 days before and after the given date. The ACFs plotted in red are in the SSE period, and the bottom ACF is the refere
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::65202f8a2aa898cba48541fe877ae30d
Temporal variations in 15-day ACFs at Station S01. (a) 15-day ACFs calculated from OBS data over 15 continuous days, including the 7 days before and after the given date. The ACFs plotted in red are in the SSE period, and the bottom ACF is the refere
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5d7bcc80da72a98c4798eedf5a605923