Surface deformation of the Barren Island volcano, Andaman Sea (2007–2017) constrained by InSAR measurements: Evidence for shallow magma reservoir and lava field subsidence
Introduction
The Sunda arc, formed by the subduction of the Indian plate below the SE Asian plate, hosts more than 80 volcanoes from eastern Java to the Andaman Island (Fig. 1). Barren Island, situated in the Andaman Sea, is the northernmost active volcano of this arc. The volcano rises from a depth of 2000 m to a maximum height of 354 m above the mean sea level. The diameter of the island is about 3 km. The volcano consists of a cinder cone surrounded by caldera wall, which opens towards the west (Fig. 1).
Barren Island volcano is built of prehistoric lava flows along with volcanoclastic deposits (Sheth et al., 2009). Geochemical and isotopic studies suggest that the volcano became sub-aerial at about 1.6 Ma and had major eruptions at 71, 62, 23, 17, 12 and 8 Ka (Ray et al., 2013, Ray et al., 2015; Awasthi et al., 2014). According to historical records, the formation of the cinder cone at the centre of the pre-historical caldera occurred as a result of a series of violent volcanic eruptions during 1787–1832 (Shanker et al., 2001; Luhr and Haldar, 2006). After about 150 years of quiescence, the second phase of volcanic activity resumed around 1991 and several eruption episodes have been recorded since then. Violent eruptions with lava flows were observed during 1991, 1994–95, 2005–2006 and 2008–2010 (Pal et al., 2010; Sheth et al., 2010). After 2010, the volcanic activity has subsided and strombolian activity with ash and occasional lava eruptions continues until the present.
Measurement of surface deformation caused by volcanic activity can provide vital insights into the magma plumbing system and eruption mechanisms. Volcanic systems of the west Sunda and Java regions are well studied using InSAR data (Philibosian and Simons, 2011; Chaussard and Amelung, 2012; Chaussard et al., 2013). However, despite the long eruption history, Barren Island volcano is poorly studied using InSAR and its magma reservoir characteristics are largely unknown. Previous satellite based studies are restricted to optical/thermal image analysis for construing the surface and atmospheric process associated with the volcanic eruptions (Reddy et al., 1993; Vinod Kumar et al., 2006; Martha et al., 2018). We present, for the first time, comprehensive surface deformation data of the Barren Island volcano from InSAR measurements during 2007–2011 and 2015–2017 epochs. We also present a source model for the volcanic deformation using inversion of the InSAR data.
Section snippets
InSAR analysis and results
We use ALOS Sentinel-1 and ALOS-2 data during epochs 2007–2011 and 2015–2017 for interferometric analysis (Fig. S1). SAR imagery cropped to an area of 5 × 5 km2 covering Barren Island were co-registered and corrected for flat-earth using ISCE software (Gurrola et al., 2016). Interferograms are generated and unwrapped using GMTSAR (Sandwell et al., 2011) and SNAPHU (Chen and Zebker, 2002) software, respectively. Topographic phases are removed using re-processed version of Shuttle Radar
Deformation of the cinder cone and source modelling
We detect significant deformation around the cinder cone with an average rate of −50 mm/yr during 2007–2011 (Fig. 2, Fig. 3). However, the cinder cone, also imaged by the ALOS-2 data during 2015–2017, showed very little to almost no discernible deformation pattern (Figs. 2c and S6a-b). However, concentric fringes observed for some of the ALOS2 interferograms that correlate with the topography of cinder cone (e.g. ALOS220160722_20170721, Fig. S2) appears to be atmospheric related signals. We
Subsidence of the lava field
The nearly circular caldera wall of the Barren Island is filled with lava flows that erupted from the central cone during 1789–1832. Lava flows from recent eruptions (1991, 1994–95, 2005–06 and 2008–2010) initially covered the 1789–1832 flows and subsequently breached the western caldera wall to form a lava delta before reaching the sea (Sheth et al., 2010). We observe distinct deformation patterns along the lava delta for both 2007–2011 and 2015–2017 epochs. ALOS time-series suggests that the
Measurement of topographic changes
We compare the topographic map of Barren Island prepared in 1979 by the Survey of India with the SRTM data of the year 2000 (Fig. 5). We infer that between 1979 and 2000 the western boundary of the lava delta was extended seawards upto ~450 m. The topography between these boundaries inferred from the SRTM data essentially suggest the thicknesses of lava flow including volcanic deposits such as pyroclastic and lahar accumulated during 1979–2000 period. Further east, difference of topographic
Magma ascent beneath the Barren Island volcano
The Intra-arc stress regime can influence the depth of magma reservoirs for subduction zone volcanoes (Chaussard and Amelung, 2014). Volcanoes close to the extensional stress regime, as in the case of the west Sunda region, develop shallow magma reservoirs at 1500 to 4500 m below the summit of the volcano (Chaussard and Amelung, 2012). Interestingly, the magma reservoir depth estimated in the present study (~578 m) is significantly shallower than that of other volcanoes of the western Sunda arc
Conclusions
We report on the comprehensive surface deformation of Barren Island volcano measured using the InSAR technique during 2007–2011 and 2015–2017 periods. Major conclusions of the study are as follows:
- 1)
InSAR analysis revealed that the cinder cone of Barren Island volcano experienced LOS deformation rate of −50 mm/yr during 2007–2011, while its caldera rim remained stable.
- 2)
Modelling of the InSAR data suggest the presence of a shallow magma reservoir at 578−100+300 m.
- 3)
The depth of the magma reservoir is
Declaration of Competing Interest
The authors declare that they have no known competing financial interests or personal relationships that could have appeared to influence the work reported in this paper.
Acknowledgments
Sentinel-1 data used for the analysis are available at Copernicus Open Hub. ALOS PALSAR images archived at the Alaska Satellite Facility (https://search.asf.alaska.edu). ALOS-2 PALSAR data were provided by JAXA through RA-6, PI NO. 3053. This work was carried out jointly by SAC-ISRO and JPL as a part of the NISAR-Solid Earth Science program. D. K. Das, Raj Kumar, and Paul Rosen have supported the collaborative study. KMS, RA and ASR are also supported by GAP program of SAC. We thank Paul
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