Shallow magma convection evidenced by excess degassing and thermal radiation during the dome-forming Sabancaya eruption (2012–2020)

We used a large set of satellite- (visible, infrared, and radar images from Planetscope, MODIS, VIIRS, Sentinel2, Landsat 8, and Sentinel 1) and ground-based data (optical images, SO2 flux, shallow seismicity) to describe and characterize the activity of the Sabancaya volcano during the unrest and eruption phases that occurred between 2012 and 2020. The unrest phase (2012–2016) was characterized by increasing gas and thermal flux, sourced by a convective magma column rising along with the remnants of a buried plug still permeable to fluid flow. Conversely, a new conduit, adjacent to the previo... Mehr ...

Verfasser: Coppola D.
Valade S.
Masias P.
Laiolo M.
Massimetti F.
Campus A.
Aguilar R.
Anccasi R.
Apaza F.
Ccallata B.
Cigolini C.
Cruz L. F.
Finizola A.
Gonzales K.
Macedo O.
Miranda R.
Ortega M.
Paxi R.
Taipe E.
Valdivia D.
Dokumenttyp: Artikel
Erscheinungsdatum: 2022
Schlagwörter: Dome-forming-eruption / Excess degassing / Excess radiation / Sabancaya / Shallow magma convection
Sprache: Englisch
Permalink: https://search.fid-benelux.de/Record/base-26882910
Datenquelle: BASE; Originalkatalog
Powered By: BASE
Link(s) : http://hdl.handle.net/2318/1850099