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3. The 0.0167 Hz residual gravity time series after reduction for tidal constituents of gravity time series at the SLV station between July 22 and 7 August 2008. The dateline is given in UTC. ( a ) Residuals after correction using models DDW and FES2004. ( b ) Residuals after reduction using the new precision model (Table 14.1). The spike in the time series on 23 July in (a) and (b) was induced by the operator. ( c ) RSME for 5 min data bins of the residual gravity time series. Note the sharp increase from background levels associated with the VE on 29 July 2008 described in detail in Gottsmann et al. (2011). 

3. The 0.0167 Hz residual gravity time series after reduction for tidal constituents of gravity time series at the SLV station between July 22 and 7 August 2008. The dateline is given in UTC. ( a ) Residuals after correction using models DDW and FES2004. ( b ) Residuals after reduction using the new precision model (Table 14.1). The spike in the time series on 23 July in (a) and (b) was induced by the operator. ( c ) RSME for 5 min data bins of the residual gravity time series. Note the sharp increase from background levels associated with the VE on 29 July 2008 described in detail in Gottsmann et al. (2011). 

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Gravimetric time series can provide vital clues about subsurface dynamics associated with active volcanism. Here, we report on continuous and campaign-style gravimetric observations on Montserrat between 2006 and 2009. More than 240 days of continuous gravimetric records enabled us to derive a first local joint solid Earth tides and ocean loading m...

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... Time-lapse gravity observations were successfully applied to monitor, e.g. subsurface water storage changes in general ( Naujoks et al., 2008;Pfeffer et al., 2013) and in karst regions Jacob et al., 2010;Cham- pollion et al., 2018), CO 2 storage changes ( Nooner et al., 2007;Wilkinson et al., 2017), or withdrawal or intrusions beneath volcanic edifices ( Jentzsch et al., 2004;Hautmann et al., 2014;Carbone et al., 2017). ...
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... Combining gravity and deformation measurements permits discrimination between gas, water, and magma intrusion (Bagnardi et al., 2014;Bonvalot et al., 1998;Hautmann et al., 2014), assessing voids opening (Carbone, 2003;Furuya et al., 2003), magma density changes associated with degassing (Bagnardi et al., 2014;Poland & Carbone, 2016) or overturn of resident magma in a reservoir (Rymer et al., 1998). Terrestrial gravity measurements can also support the investigation of dike growth and migration, which can be induced by vertical intrusion (Gudmundsson, 1995(Gudmundsson, , 1998Wright et al., 2012) or lateral outflow of magma (Einarsson & Brandsdottir, 1978;Gudmundsson et al., 2016;Sigmundsson et al., 2014) ( Figure 10). ...
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Les dômes de lave sont associés à des éruptions volcaniques violentes et des indices d’explosivité élevés. L’observation et la surveillance de dômes actifs (e.g. St. Helens, Unzen, Montserrat) ont mis en évidence des modes de croissance caractérisés par des phases d’extrusion, d’explosion et des phénomènes d’effondrement, impliquant une structure interne souvent complexe de ces édifices volcaniques. L’étude du Puy de Dôme (Massif Central français), un dôme trachytique âgé de 11 000 ans, grâce à l’apport de l’imagerie géophysique et à la modélisation des données, ainsi qu’à une analyse morpho-structurale détaillée, a permis d’établir un modèle précis de la structure interne du dôme et a fourni de nouvelles contraintes concernant sa croissance et son évolution. L’analyse du Modèle Numérique de Terrain haute résolution (0,5 m) a permis d’identifier différentes unités sur le dôme, morphologiquement distinctes, et associées à des dynamismes éruptifs différents, ainsi que des structures volcano-tectoniques remarquables sur les édifices volcaniques voisins (Petit Puy de Dôme et Puy des Grosmanaux). Différentes méthodes géophysiques (tomographie des résistivités électriques – ERT -, gravimétrie et magnétisme) ont été mises en oeuvre afin d’étudier la structure interne du dôme, et de caractériser la nature des mécanismes à l’origine des zones de déformations identifiées dans l’environnement du Puy de Dôme. L’utilisation de plusieurs méthodes a permis d’étudier des paramètres physiques différents mais complémentaires, bien que l’interprétation globale des résultats géophysiques ait parfois été délicate dans le cas d’un édifice volcanique aussi complexe. Les modèles géophysiques 2D et 3D obtenus montrent que le Puy de Dôme repose sur des édifices volcaniques préexistants, un ensemble de volcans stromboliens dont la présence et/ou l’extension exacte étaient partiellement méconnues jusqu’alors. La structure interne de l’édifice, très hétérogène, est constituée d’une partie centrale très massive, entourée d’une ceinture de brèches d’effondrement, la zone sommitale du conduit étant affectée de nombreuses évidences d’une forte altération hydrothermale, caractéristique des dômes volcaniques. La partie supérieure du dôme est définie par une carapace de roches consolidées, de quelques dizaines de mètres d’épaisseur au maximum, alors que la base de l’édifice forme un talus constitué des dépôts d’effondrements gravitaires et d’écoulements pyroclastiques associés à la croissance du dôme. Enfin, les données gravimétriques et magnétiques ont permis la mise en évidence de la présence d’intrusions sous les édifices du Petit Puy de Dôme et du Puy des Grosmanaux. La géométrie de ces intrusions, déterminées grâce à différentes approches de modélisation, ainsi que la nature des roches qui les composent indiquent des processus de mise en place complexes.