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  • Express Letter
  • Open Access

Temporal variations of plume activities before the 8 October 2016 eruption of Aso volcano, Japan, detected by ground-based and satellite measurements

Earth, Planets and Space201971:7

https://doi.org/10.1186/s40623-019-0986-x

  • Received: 31 March 2018
  • Accepted: 8 January 2019
  • Published:

Abstract

At many volcano observatories, measurements of the plume height are frequently applied. On the other hand, the recent development of the satellite measurements enables the monitoring of the SO2 mass emitted by the passive degassing at sufficient temporal resolution. Using these two techniques, this study focuses on the degassing activity before the 8 October 2016 phreatomagmatic eruption of Aso volcano, Japan. Here we show the temporal variations of the plume height, the SO2 mass, and ground-based SO2 flux during 6 months before the eruption. Our result shows similar temporal changes of them, especially for the maxima and the increase, respectively, in about 2 months and 6 days before the eruption. This result indicates that the degassing system had been stable during the whole study period, but the accumulation of volcanic gas in the conduit since August might trigger the phreatomagmatic eruption. These techniques can be sufficient to monitor the degassing activity and to detect its precursory change.
Graphical Abstract image

Keywords

  • Aso volcano
  • Volcanic eruption
  • Monitoring camera
  • Volcanic plume
  • Plume height
  • SO2
  • OMPS

Introduction

Phreatomagmatic eruptions are triggered by an interaction of magma with shallow hydrothermal systems (Rouwet et al. 2014). Related to the interaction of ascending magma with the hydrothermal systems, precursory changes of gas geochemistry and fumarolic activity have been documented at some volcanoes (Barberi et al. 1992; de Moor et al. 2015; Sano et al. 2015). Along with the observations of gas geochemistry, visual monitoring of volcanic plumes using cameras is also conducted at many volcanoes (Fukui 1995; Terada et al. 2003, 2005; Behncke et al. 2009; Arason et al. 2011; Fukui and Terada 2013; Shimbori and Fukui 2013). At many Japanese volcanoes, plume height is monitored as an indicator of the apparent intensity of the volcanic plume (Volcanological Division, Seismological and Volcanological Department, JMA 2014). However, the visibility of the plume is highly affected by atmospheric conditions (Matsushima and Shinohara 2006), and the plume height is also influenced by wind conditions (Bursik 2001). Therefore, to monitor the plume activity, the apparent intensity of the plume has rarely been treated quantitatively.

The supply of magma and volcanic gas is frequently monitored as the emission rate of sulfur dioxide (SO2) using ground-based (Stoiber et al. 1983; Galle et al. 2002) and satellite remote sensing techniques (Krueger 1983). Concerning the satellite remote sensing, satellite measurements of SO2 emissions to date are not limited in volcanic plumes of large explosions but also applied to those of passive degassing (Carn et al. 2008; Campion 2014). These previous studies have revealed that the satellite measurements of SO2 emissions have sufficient precision and temporal resolution to be used for the monitoring. Although the satellite measurements have a potential to monitor the passive degassing activity, the application of them is still rare at many volcano observatories.

This study focuses on the precursory changes of the plume activity before the phreatomagmatic eruptions using the ground-based monitoring of the plume intensity and the satellite measurements of SO2 emissions. We evaluate the plume intensity as the plume height and compare it with the SO2 mass estimated by the satellite measurements. Comparing a semiquantitative value (plume height) with a quantitative value (SO2 mass), we appraise an efficiency of the plume monitoring. As a case study, we choose the phreatomagmatic explosion of Aso volcano, Japan, on 8 October 2016. We show the temporal variations of the plume height and SO2 mass during 7 months before and after the explosion.

Aso volcano

Aso volcano is one of the most active volcanoes in Japan and consists of a caldera with diameters of 25 km in north–south and 18 km in east–west and post-caldera central cones. The only active cone is the Nakadake Volcano with compositions ranging from basalt to basaltic andesite (Ono and Watanabe 1985). Among seven craters of the volcano, only the northernmost crater (the Nakadake first crater, Fig. 1) has been active in the past 80 years (Ono and Watanabe 1985). The crater is filled with hot (40–80 °C) and hyper-acidic (pH < 1) lake water during calm periods (Miyabuchi and Terada 2009; Ohsawa et al. 2010; Terada et al. 2012; Shinohara et al. 2015), and the crater lake is maintained by a continuous supply of volcanic fluids from depth (Terada et al. 2012; Terada and Hashimoto 2017). Volcanic gas is persistently emitted from the lake surface and a fumarolic area on the southern wall of the crater. The SO2 flux in calm periods ranges in approximately 200–400 tons day−1 (JMA 2017).
Fig. 1
Fig. 1

Location of monitoring camera and the crater of Aso volcano. Location of Aso volcano is depicted with the red triangle in the inset. Data of the base map are from Geospatial Information Authority of Japan

After a series of intermittent ash emissions and Strombolian explosions from November 2014 to May 2015, a phreatomagmatic explosion occurred on 14 September 2015 (Miyabuchi et al. 2018). It was followed by a small phreatomagmatic explosion on 23 October 2015 and some minor phreatic explosions from December 2015 to March 2016 (JMA 2017). In March 2016, the lake water started to refill the crater bottom, and the surface area of the lake increased to 70% of the crater bottom in July 2016. During March and September 2016, quite minor wet ash emissions from the crater bottom were frequently observed (JMA 2017). A minor explosion occurred at 21:52 JST (UTC + 09:00) on 7 October 2016 followed by a large phreatomagmatic explosion at 01:46 JST on 8 October 2016 (JMA 2017). For the latter explosion, the top of the plume height observed by a geostationary meteorological satellite Himawari-8 was estimated to be 13–14 km asl (Ishii et al. 2018). The total eruptive mass of the 7–8 October explosions was estimated to be 6.0–6.5 × 106 tons, and the juvenile magma erupted by the explosions accounted for 20% of the deposits (Miyabuchi et al. 2017).

Analysis method

To estimate the plume height between April and October 2016, we used the monitoring video camera that was maintained by JMA (WV-E850, Panasonic Corp.) and located at 3.1 km west of the crater (Fig. 1). The 30-Hz video was captured every 2 s, and the captured image was compressed and saved into a jpeg file with a size of 640 × 480 pixels. To dismiss short-term (from seconds to minutes) disturbances by wind and other meteorological conditions, the images of an hour (1800 images at maximum) were first composited into one image. Then, based on the composite image, the plume height was estimated manually. In this study, the plume height is presented in meters above the crater rim (1270 m asl at the western side of the crater where the crater rim is visible in the image). From April to October 2016, the crater had always been filled with the lake water, and the volcanic plume had persistently risen from the lake surface and the fumarolic area on the southern wall of the crater (JMA 2017). This approximately constant geometry of the source of the volcanic plume hardly affects the estimation of the plume height.

The analysis of SO2 mass between April and October 2016 was performed using the Ozone Mapping and Profiler Suite (OMPS) nadir mapper instrument (Flynn et al. 2014; Seftor et al. 2014) onboard the NASA/NOAA Suomi National Polar-orbiting Partnership (Suomi-NPP) satellite. Suomi-NPP is in a polar orbit with a local equator crossing time of 13:30. The instrument measures UV (300–380 nm) backscatter radiances and provides daily global mapping data of ozone, SO2, and other trace gases. The spatial resolution of the instrument is 50 × 50 km at nadir. The SO2 vertical column densities (VCDs) retrieved by the algorithm of Li et al. (2013, 2017) are provided by NASA Goddard Space Flight Center (https://avdc.gsfc.nasa.gov/pub/data/satellite/Suomi_NPP/L2/NMSO2-PCA-L2/). In this study, to analyze the SO2 mass of the passive degassing, the SO2 VCDs assuming an SO2 profile centered in the planetary boundary layer (PBL, a center of mass altitude of 0.9 km asl) and the lower troposphere (TRL, a center of mass altitude of 3 km asl) were normally used, whereas those in the upper troposphere (TRU, a center of mass altitude of 13 km asl) were used only in the analysis of the SO2 mass emitted by the 8 October 2016 eruption. Although SO2 PBL might overestimate the SO2 mass considering of an altitude of the crater rim (1270 m asl), the main topic in this study is passive degassing and thus we will mainly focus on SO2 PBL in the following sections. The SO2 VCDs are presented in DU (Dobson units, 1 DU = 2.69 × 1016 molecules cm−2).

In each daily map of the SO2 VCDs, the volcanic SO2 signal was basically weak, and the volcano was sometimes covered with cloud. Therefore, the daily SO2 mass was not basically estimated in this study. Instead, the averaged SO2 mass for PBL and TRL in certain periods (10 days and 1 month) was calculated following the method presented by Carn et al. (2008) and Campion (2014). The daily SO2 VCDs in each period were first gridded in a step of 0.1°, and then, they were stacked and averaged by the number of days. The time-averaged volcanic SO2 mass was calculated by summing the SO2 VCDs in a volcanic region (4° in longitude × 2° in latitude, red rectangle in Figs. 3 and 4) that were higher than a threshold value (mean + standard deviation of the SO2 VCDs in an SO2-free region for each period, blue rectangle in Figs. 3 and 4). Further details on the analysis method of SO2 mass and the influence of cloud cover are provided in the supporting information of this article (Additional file 1: Sections 1 and 2).

Results

Time series of the estimated plume height and representative examples of the composite image are shown in Fig. 2. We were not able to estimate the plume height for dilute plumes or plumes surrounded by clouds, especially when the plume flew near the ground. This difficulty is the reason that the plume height values shown in Fig. 2 are almost more than 100 m. However, in some cases, the plume height was successfully estimated for dilute plumes (examples shown in Fig. 2; 13:00 JST, 12 May, and 00:00 JST, 12 August). The influence of wind and atmospheric conditions on the plume height is discussed in detail in the supporting information (Additional file 1: Section 3 and Figures S1 and S2). As a brief conclusion of the supporting information, variations of the plume height in a week–month scale are represented by an envelope of the maximum plume height in that scale in Fig. 2.
Fig. 2
Fig. 2

Time series of the plume height estimated by the monitoring camera and representative examples of the composite camera image. The dotted lines in the images correspond to the top of the plume

In Fig. 2, some maxima of the plume height in a week–month scale were found at 10 April, 12 May, 3 June, 10 August, 6 September, and 7 October. Especially at 16:00 JST, 7 October (the image shown in Fig. 2), the plume height was 1010 m, which was the maximum value in this study. Looking closely before the 8 October eruption, the plume height increased on 1 and 2 October to 720 m, then decreased to 160 m on 4 October, and increased again to 740 m on 6 October and 1010 m on 7 October.

The maps of 10-day and monthly averaged SO2 PBL VCDs are shown in Figs. 3 and 4, respectively. Those of 10-day and monthly averaged SO2 TRL VCDs are shown in Additional file 1: Figures S3 and S4, respectively. In many maps shown in Figs. 3 and 4, high SO2 VCDs around the volcano were observed clearly through the whole study period. In the case of SO2 TRL, though the SO2 VCDs in the volcanic region were often comparable to those in the SO2-free region, high SO2 VCDs were sometimes found around the volcano (Additional file 1: Figures S3 and S4).
Fig. 3
Fig. 3

Maps of the 10-day averaged SO2 PBL VCDs measured by OMPS from 1 April to 27 October 2016. The period for each map is shown at the right bottom of the map (DD.MM–DD.MM). Location of Aso volcano is depicted with the triangle. The volcanic and SO2-free regions for the SO2 mass calculation (see text) are shown with red and blue rectangles, respectively. The high SO2 VCDs around 140°E in longitude found in 8.10–17.10 map correspond to the SO2 cloud by the 8 October explosion

Fig. 4
Fig. 4

Maps of the monthly averaged SO2 PBL VCDs measured by OMPS from April to October 2016. The triangle and the red and blue rectangles are as same as those in Fig. 3. The high SO2 VCDs around 140°E in longitude found in October map correspond to the SO2 cloud by the 8 October explosion

The time series of the 10-day and monthly averaged SO2 PBL and TRL mass are shown in Fig. 5a and Additional file 1: Figure S5a, respectively. The 10-day averaged SO2 mass showed more fluctuations than the monthly one for both PBL and TRL. In the 10-day and monthly averaged SO2 PBL mass, the maximum value was found in early October and August, respectively. The maxima of the 10-day averaged value were also found in middle April, early June, late July, and middle August. Some of these maxima coincide with those of the plume height shown in Fig. 5b, but the detail will be discussed in the supporting information related to cloud fraction (Fig. 5c and Additional file 1: Section 4). The SO2 mass after the explosion was much lower than that before the explosion. The time series of the SO2 TRL mass (Additional file 1: Figure S5a) showed similar trends to that of the SO2 PBL mass with an exception that the maximum 10-day averaged SO2 mass was observed in middle August.
Fig. 5
Fig. 5

a The time-averaged (10-days and monthly) SO2 PBL mass emitted by the passive degassing of Aso volcano estimated by OMPS. b Time series of the plume height (black line, from Fig. 2) and SO2 flux (orange point). The SO2 flux data are measured by car traverses by JMA (http://www.data.jma.go.jp/svd/vois/data/fukuoka/rovdm/Asosan_rovdm/gas/gas.html). The error bars correspond to maximum and minimum SO2 fluxes obtained by multiple traverses. The text “15,000 ton day−1” shown in the upper part corresponds to the SO2 flux measured on 7 October 2016. c The time-averaged (10-days and monthly) and spatial-averaged cloud fraction of the OMPS data in the volcanic region (red rectangle in Figs. 3 and 4). d Correlation plot of the 10-days averaged SO2 PBL mass against the fourth power of the maximum plume height for the corresponding period. The plume height values are converted to those above the crater bottom (= plume height in Fig. 2 + 100 m, see text). A number on the right shoulder of each point correspond to the period number shown in Fig. 3. e Correlation plot of the 10-days averaged SO2 PBL mass against the SO2 flux for the corresponding period. A number on the right shoulder of each point correspond to the SO2 flux number shown in Fig. 5b. fi Daily map of SO2 VCDs of f TRL on 2 October, g TRL on 6 October, h TRL on 7 October, and i TRU on 8 October 2016. The triangle and the red and blue rectangles in f–i are as same as those in Fig. 3

To clarify the similar temporal variations between the plume height (Fig. 5b) and the SO2 mass, we compare the 10-day averaged SO2 mass with the fourth power of the maximum plume height in the corresponding period (Fig. 5d and Additional file 1: Figure S5b). We used the fourth power of the plume height because it is proportional to heat discharge rate assuming that the plume is maintained from the steady source (Morton et al. 1956). We added 100 m to the plume height because the crater rim was 100 m higher than the crater bottom (Fig. 1). Although some points are plotted far from the fitted line, positive correlation was roughly found between the SO2 mass and the fourth power of the plume height (R2 = 0.37 for PBL and 0.28 for TRL; Fig. 5d and Additional file 1: Figure S5b). The points far from the fitted line can be dismissed because they are influenced by the cloud fraction problem (details are written in Additional file 1: Section 4). The influence of the wind speed on the plume height was not found in these plots (Additional file 1: Figure S7). A rough positive correlation was also found between the SO2 mass and the SO2 flux measured by car traverses (R2 = 0.41 for PBL and 0.23 for TRL; Fig. 5b, e; Additional file 1: Figure S6 and Section 5).

The daily SO2 mass on 2, 6, and 7 October was so high that it was able to be calculated (Fig. 5f–h), when the plume height was also high as mentioned above. The daily SO2 TRL mass on 2, 6, and 7 October was calculated to be 769, 434, and 1120 tons, respectively. The erupted SO2 of the 8 October phreatomagmatic explosion was captured on the daily map on the same day (Fig. 5i). Location of the SO2 cloud detected by OMPS is almost the same as that detected by a meteorological satellite Himawari-8 (Ishii et al. 2018). The SO2 mass emitted by the explosion was estimated to be 10,810 tons.

Discussion and concluding remarks

By comparing Fig. 5a and b, the time series of the plume height, the averaged SO2 mass, and the SO2 flux showed similar temporal variations. Although the correlation between the plume height and the SO2 mass was not good as shown in Fig. 5d and Additional file 1: Figure S5b, the rough positive correlation was found. A similar positive correlation was also found between the SO2 mass and the SO2 flux observed by JMA (Fig. 5e and Additional file 1: Figure S6). These correlations likely indicate that, although the correlations were rough, the degassing system represented by the heat discharge rate and SO2 flux (= SO2 mass) had been stable during the whole study period, except for some data in middle May, middle August, and early October (points far from the fitted line in Fig. 5d, details are written in Additional file 1: Section 4).

As found in the time series of both the plume height and the SO2 mass, the degassing activity was intensified especially in middle August. Then, both values decreased in September, and some extremely high values were observed again in early October (Fig. 5a, b). The maxima in middle August coincides with the inflation timing of the deep magmatic source observed by GNSS networks (JMA 2017). Thus, the input of deep magma might have started since this period. Both values slightly decreased in September. In early October, the plume height started to increase since 1 October, and the SO2 mass also increased on 2 October as shown in the daily SO2 map (Fig. 5f). Both values temporally decreased, but the plume height and the SO2 mass started to increase again on 6 and 7 October, respectively. The decreasing trend from August to October is similar to the decreasing trend of the conduit pressure before Vulcanian explosions proposed by Iguchi et al. (2008). Although the duration of a decrease in this study is much longer than the precursory change in the case of Iguchi et al. (2008), similar accumulation of volcanic gas in the conduit might have occurred in the case of the 8 October eruption of Aso volcano. Following this model, the increase in early October might be explicable by leakage of the accumulated gas just before the explosion. This leakage might have contributed to a decrease of the conduit pressure. Consequently, an interaction of magma with infiltrating waters from the hydrothermal system into the conduit and/or a sudden outgassing of the magma might trigger the explosion.

As mentioned above, the erupted SO2 mass of the 8 October explosion was estimated to be 10,810 tons. According to a petrological study by Saito et al. (2018), sulfur content of the melt inclusions in plagioclases, clinopyroxenes, and olivines in scoriae from the 2014 eruption ranged from 0.008 to 0.036 wt% S. Assuming that the sulfur content in the pre-eruptive magma is 0.036 wt% that was the maximum value of the sulfur content, the amount of the pre-eruptive magma for this explosion is estimated to be 1.5 × 107 tons. The total eruptive mass of the 7–8 October explosions was estimated to be 6.0–6.5 × 106 tons with the juvenile magma accounting for 20% of the deposits (Miyabuchi et al. 2017). Therefore, most of the pre-eruptive magma associated with the explosion might reside in depth, and only the volcanic gas accumulated in depth might be emitted by the explosion. The presence of the accumulated gas is consistent with the model proposed above.

Finally, we emphasize the importance of plume monitoring. Although our result did not show a good correlation between the plume height and the SO2 mass, the plume height measurement can be sufficient to monitor the degassing activity. To reveal the relationship more clearly, accumulation of the data and the precise analysis of the SO2 mass from the passive degassing will be necessary. To the latter case, a recently launched instrument, the Tropospheric Monitoring Instrument (TROPOMI) that can detect the SO2 VCDs in low altitude at higher spatial resolutions (Theys et al. 2017), might contribute.

Abbreviations

asl: 

above sea level

DU: 

Dobson units

GNSS: 

global navigation satellite system

JMA: 

Japan Meteorological Agency

JST: 

Japan Standard Time

NASA: 

National Aeronautics and Space Administration

NOAA: 

National Oceanic and Atmospheric Administration

OMPS: 

Ozone Mapping and Profiler Suite

Suomi-NPP: 

Suomi National Polar-orbiting Partnership

UTC: 

Coordinated Universal Time

UV: 

ultraviolet

VCDs: 

vertical column densities

Declarations

Authors’ contributions

MM performed the whole part of this study. The author read and approved the final manuscript.

Acknowledgements

The camera images were provided by JMA. The author is grateful to Drs. Akihiko Yokoo, Takehiko Mori, Toshiya Mori, Hiroshi Shinohara, Akihiko Terada, and Genji Saito for data acquisition and discussion. The author would like to thank Dr. Takahiro Ohkura and three anonymous reviewers for their constructive comments that significantly improved the manuscript.

Competing interests

The author declares that he has no competing interests.

Availability of data and materials

The satellite SO2 data are available at https://avdc.gsfc.nasa.gov/pub/data/satellite/Suomi_NPP/L2/NMSO2-PCA-L2/. The other datasets used in this study are available from the corresponding author on reasonable request.

Funding

This study received no specific grant from any funding agency.

Publisher’s Note

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Open AccessThis article is distributed under the terms of the Creative Commons Attribution 4.0 International License (http://creativecommons.org/licenses/by/4.0/), which permits unrestricted use, distribution, and reproduction in any medium, provided you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons license, and indicate if changes were made.

Authors’ Affiliations

(1)
Geological Survey of Japan, National Institute of Advanced Industrial Science and Technology, Central 7, Higashi 1-1-1, Tsukuba 305-8567, Japan

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