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The thermal signature of Aso Volcano during unrest episodes detected from space and ground-based measurements
The thermal signature of Aso Volcano (Nakadake) during unrest episodes has been analyzed by combining the MODIS-MIROVA data set (2000–2017) with high-resolution images (LANDSAT 8 OLI and Sentinel 2) and ground-based thermal observations (2013–2017). The site of major activity (crater 1) is located a...
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Published in: | Earth, planets, and space planets, and space, 2018-04, Vol.70 (1), p.1-15, Article 67 |
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description | The thermal signature of Aso Volcano (Nakadake) during unrest episodes has been analyzed by combining the MODIS-MIROVA data set (2000–2017) with high-resolution images (LANDSAT 8 OLI and Sentinel 2) and ground-based thermal observations (2013–2017). The site of major activity (crater 1) is located at the summit of the volcano and is composed by a fumarole field (located in the South Area) and an acidic lake (replaced by a Central Pit during Strombolian phases). The volcanic radiative power (VRP) obtained by nighttime satellite data during the reference period was mainly below 3 MW. This thermal threshold marks the transition from high fumarole activity (HFA) to Strombolian eruptions (SE). However, periods characterized by sporadic phreatic eruptions (PE, eventually bearing phreatomagmatic episodes), which is the prevalent phase during unrest episodes, exhibit very low VRP values, being around 0.5 MW, or below. The statistical analysis of satellite data shows that the transition from HFA to Strombolian activity (which started on August 2014 and ceased in May 2015) occurs when VRP values are above the cited 3 MW threshold. In particular during marked Strombolian phases (November–December 2014), the radiative power was higher than 4 MW, reaching peak values up to 15.6 MW (on December 7, 2014, i.e., 10 days after the major Strombolian explosion of November 27). Conversely, ground-based measurements show that heat fluxes recorded by FLIR T440 Thermo-camera on the fumarole field of the South Area has been relatively stable around 2 MW until February 2015. Their apparent temperatures were fluctuating around 490–575 °C before the major Strombolian explosive event, whereas those recorded at the active vent, named Central Pit, reached their maxima slightly above 600 °C; then both exhibited a decreasing trend in the following days. During the Strombolian activity, the crater lake dried out and was then replenished by early July, 2016. Then, volcanic activity shifted back to phreatic–phreatomagmatic and the eruptive cycle was completed. During this period, the MIROVA system detected very few thermal alerts and the ground-based measurements were fluctuating around 1 MW. The most violent explosion occurred on October 8, 2016, and within the following weeks measured VRP were moderately above 2 MW. This is coeval with a thermal increase at the fumarole field of the South Area, with temperatures well above 300 °C. Thermal monitoring at Aso Volcano is an additional tool in |
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The site of major activity (crater 1) is located at the summit of the volcano and is composed by a fumarole field (located in the South Area) and an acidic lake (replaced by a Central Pit during Strombolian phases). The volcanic radiative power (VRP) obtained by nighttime satellite data during the reference period was mainly below 3 MW. This thermal threshold marks the transition from high fumarole activity (HFA) to Strombolian eruptions (SE). However, periods characterized by sporadic phreatic eruptions (PE, eventually bearing phreatomagmatic episodes), which is the prevalent phase during unrest episodes, exhibit very low VRP values, being around 0.5 MW, or below. The statistical analysis of satellite data shows that the transition from HFA to Strombolian activity (which started on August 2014 and ceased in May 2015) occurs when VRP values are above the cited 3 MW threshold. In particular during marked Strombolian phases (November–December 2014), the radiative power was higher than 4 MW, reaching peak values up to 15.6 MW (on December 7, 2014, i.e., 10 days after the major Strombolian explosion of November 27). Conversely, ground-based measurements show that heat fluxes recorded by FLIR T440 Thermo-camera on the fumarole field of the South Area has been relatively stable around 2 MW until February 2015. Their apparent temperatures were fluctuating around 490–575 °C before the major Strombolian explosive event, whereas those recorded at the active vent, named Central Pit, reached their maxima slightly above 600 °C; then both exhibited a decreasing trend in the following days. During the Strombolian activity, the crater lake dried out and was then replenished by early July, 2016. Then, volcanic activity shifted back to phreatic–phreatomagmatic and the eruptive cycle was completed. During this period, the MIROVA system detected very few thermal alerts and the ground-based measurements were fluctuating around 1 MW. The most violent explosion occurred on October 8, 2016, and within the following weeks measured VRP were moderately above 2 MW. This is coeval with a thermal increase at the fumarole field of the South Area, with temperatures well above 300 °C. Thermal monitoring at Aso Volcano is an additional tool in volcano surveillance that may contribute to near-real-time hazard assessment.</description><identifier>ISSN: 1880-5981</identifier><identifier>ISSN: 1343-8832</identifier><identifier>EISSN: 1880-5981</identifier><identifier>DOI: 10.1186/s40623-018-0831-7</identifier><language>eng</language><publisher>Berlin/Heidelberg: Springer Berlin Heidelberg</publisher><subject>5. Volcanology ; Acidic lakes ; Advancement of our knowledge on Aso volcano: Current activity and background ; Aso Volcano ; Earth and Environmental Science ; Earth Sciences ; Eruptions ; Fumarolic activity ; Geology ; Geophysics/Geodesy ; Ground-based observation ; Hazard assessment ; Heat flux ; Image resolution ; Lakes ; Landsat ; Landsat satellites ; Major explosions ; Methods ; Remote sensing ; Satellite data ; Satellite imagery ; Satellites ; Statistical analysis ; Statistical analysis of data ; Strombolian activity ; Temperature measurement ; Unrest episodes ; Variations ; Volcanic activity ; Volcanoes</subject><ispartof>Earth, planets, and space, 2018-04, Vol.70 (1), p.1-15, Article 67</ispartof><rights>The Author(s) 2018</rights><rights>COPYRIGHT 2018 Springer</rights><rights>Earth, Planets and Space is a copyright of Springer, (2018). All Rights Reserved.</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-a686t-6da884e35d5f15117046e16a182e9a135f532eb6603486dfee89a67d0c8657063</citedby><cites>FETCH-LOGICAL-a686t-6da884e35d5f15117046e16a182e9a135f532eb6603486dfee89a67d0c8657063</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://www.proquest.com/docview/2031246235/fulltextPDF?pq-origsite=primo$$EPDF$$P50$$Gproquest$$Hfree_for_read</linktopdf><linktohtml>$$Uhttps://www.proquest.com/docview/2031246235?pq-origsite=primo$$EHTML$$P50$$Gproquest$$Hfree_for_read</linktohtml><link.rule.ids>314,780,784,25753,27924,27925,37012,44590,75126</link.rule.ids></links><search><creatorcontrib>Cigolini, Corrado</creatorcontrib><creatorcontrib>Coppola, Diego</creatorcontrib><creatorcontrib>Yokoo, Akihiko</creatorcontrib><creatorcontrib>Laiolo, Marco</creatorcontrib><title>The thermal signature of Aso Volcano during unrest episodes detected from space and ground-based measurements</title><title>Earth, planets, and space</title><addtitle>Earth Planets Space</addtitle><description>The thermal signature of Aso Volcano (Nakadake) during unrest episodes has been analyzed by combining the MODIS-MIROVA data set (2000–2017) with high-resolution images (LANDSAT 8 OLI and Sentinel 2) and ground-based thermal observations (2013–2017). The site of major activity (crater 1) is located at the summit of the volcano and is composed by a fumarole field (located in the South Area) and an acidic lake (replaced by a Central Pit during Strombolian phases). The volcanic radiative power (VRP) obtained by nighttime satellite data during the reference period was mainly below 3 MW. This thermal threshold marks the transition from high fumarole activity (HFA) to Strombolian eruptions (SE). However, periods characterized by sporadic phreatic eruptions (PE, eventually bearing phreatomagmatic episodes), which is the prevalent phase during unrest episodes, exhibit very low VRP values, being around 0.5 MW, or below. The statistical analysis of satellite data shows that the transition from HFA to Strombolian activity (which started on August 2014 and ceased in May 2015) occurs when VRP values are above the cited 3 MW threshold. In particular during marked Strombolian phases (November–December 2014), the radiative power was higher than 4 MW, reaching peak values up to 15.6 MW (on December 7, 2014, i.e., 10 days after the major Strombolian explosion of November 27). Conversely, ground-based measurements show that heat fluxes recorded by FLIR T440 Thermo-camera on the fumarole field of the South Area has been relatively stable around 2 MW until February 2015. Their apparent temperatures were fluctuating around 490–575 °C before the major Strombolian explosive event, whereas those recorded at the active vent, named Central Pit, reached their maxima slightly above 600 °C; then both exhibited a decreasing trend in the following days. During the Strombolian activity, the crater lake dried out and was then replenished by early July, 2016. Then, volcanic activity shifted back to phreatic–phreatomagmatic and the eruptive cycle was completed. During this period, the MIROVA system detected very few thermal alerts and the ground-based measurements were fluctuating around 1 MW. The most violent explosion occurred on October 8, 2016, and within the following weeks measured VRP were moderately above 2 MW. This is coeval with a thermal increase at the fumarole field of the South Area, with temperatures well above 300 °C. Thermal monitoring at Aso Volcano is an additional tool in volcano surveillance that may contribute to near-real-time hazard assessment.</description><subject>5. Volcanology</subject><subject>Acidic lakes</subject><subject>Advancement of our knowledge on Aso volcano: Current activity and background</subject><subject>Aso Volcano</subject><subject>Earth and Environmental Science</subject><subject>Earth Sciences</subject><subject>Eruptions</subject><subject>Fumarolic activity</subject><subject>Geology</subject><subject>Geophysics/Geodesy</subject><subject>Ground-based observation</subject><subject>Hazard assessment</subject><subject>Heat flux</subject><subject>Image resolution</subject><subject>Lakes</subject><subject>Landsat</subject><subject>Landsat satellites</subject><subject>Major explosions</subject><subject>Methods</subject><subject>Remote sensing</subject><subject>Satellite data</subject><subject>Satellite imagery</subject><subject>Satellites</subject><subject>Statistical analysis</subject><subject>Statistical analysis of data</subject><subject>Strombolian activity</subject><subject>Temperature measurement</subject><subject>Unrest episodes</subject><subject>Variations</subject><subject>Volcanic activity</subject><subject>Volcanoes</subject><issn>1880-5981</issn><issn>1343-8832</issn><issn>1880-5981</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2018</creationdate><recordtype>article</recordtype><sourceid>PIMPY</sourceid><sourceid>DOA</sourceid><recordid>eNp1kUtv1TAQhSNEJUrLD2BniRWLFDt-xFleVTyuVAkJ2m6taTxOfXVjB9uR4N_jSxDQBfLC1vicTzNzmuY1o1eMafUuC6o63lKmW6o5a_tnzTnTmrZy0Oz5P-8XzcucD5RyKhQ_b-bbRyTlEdMMR5L9FKCsCUl0ZJcjuY_HEUIkdk0-TGQNCXMhuPgcLWZiseBY0BKX4kzyAiMSCJZMKa7Btg-Q69-MkCtyxlDyZXPm4Jjx1e_7orn78P72-lN78_nj_np304LSqrTKgtYCubTSMclYX3tFpoDpDgdgXDrJO3xQinKhlXWIegDVWzpqJXuq-EWz37g2wsEsyc-QfpgI3vwqxDQZSMWPRzTSDU5ZAQNXTsjR6Q56LajomJR9L3llvdlYS4rf1jq_OcQ1hdq-6Shnnah7l1V1takmqFAfXCwJxnoszn6MAZ2v9Z2UlSy5GKrh7RND1RT8XiZYczb7r1-eatmmHVPMOaH7MxKj5hS_2eI3NX5zit_01dNtnrycssP0t-3_m34CR12wRQ</recordid><startdate>20180426</startdate><enddate>20180426</enddate><creator>Cigolini, Corrado</creator><creator>Coppola, Diego</creator><creator>Yokoo, Akihiko</creator><creator>Laiolo, Marco</creator><general>Springer Berlin Heidelberg</general><general>Springer</general><general>Springer Nature B.V</general><general>SpringerOpen</general><scope>C6C</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>ISR</scope><scope>7TG</scope><scope>8FD</scope><scope>8FE</scope><scope>8FG</scope><scope>ABUWG</scope><scope>AFKRA</scope><scope>ARAPS</scope><scope>AZQEC</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>BHPHI</scope><scope>BKSAR</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>H8D</scope><scope>HCIFZ</scope><scope>KL.</scope><scope>L7M</scope><scope>P5Z</scope><scope>P62</scope><scope>PCBAR</scope><scope>PIMPY</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>PRINS</scope><scope>DOA</scope></search><sort><creationdate>20180426</creationdate><title>The thermal signature of Aso Volcano during unrest episodes detected from space and ground-based measurements</title><author>Cigolini, Corrado ; Coppola, Diego ; Yokoo, Akihiko ; Laiolo, Marco</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a686t-6da884e35d5f15117046e16a182e9a135f532eb6603486dfee89a67d0c8657063</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2018</creationdate><topic>5. Volcanology</topic><topic>Acidic lakes</topic><topic>Advancement of our knowledge on Aso volcano: Current activity and background</topic><topic>Aso Volcano</topic><topic>Earth and Environmental Science</topic><topic>Earth Sciences</topic><topic>Eruptions</topic><topic>Fumarolic activity</topic><topic>Geology</topic><topic>Geophysics/Geodesy</topic><topic>Ground-based observation</topic><topic>Hazard assessment</topic><topic>Heat flux</topic><topic>Image resolution</topic><topic>Lakes</topic><topic>Landsat</topic><topic>Landsat satellites</topic><topic>Major explosions</topic><topic>Methods</topic><topic>Remote sensing</topic><topic>Satellite data</topic><topic>Satellite imagery</topic><topic>Satellites</topic><topic>Statistical analysis</topic><topic>Statistical analysis of data</topic><topic>Strombolian activity</topic><topic>Temperature measurement</topic><topic>Unrest episodes</topic><topic>Variations</topic><topic>Volcanic activity</topic><topic>Volcanoes</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Cigolini, Corrado</creatorcontrib><creatorcontrib>Coppola, Diego</creatorcontrib><creatorcontrib>Yokoo, Akihiko</creatorcontrib><creatorcontrib>Laiolo, Marco</creatorcontrib><collection>Springer Nature OA Free Journals</collection><collection>CrossRef</collection><collection>Gale In Context: Science</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>Technology Research Database</collection><collection>ProQuest SciTech Collection</collection><collection>ProQuest Technology Collection</collection><collection>ProQuest Central (Alumni)</collection><collection>ProQuest Central</collection><collection>Advanced Technologies & Aerospace Collection</collection><collection>ProQuest Central Essentials</collection><collection>ProQuest Central</collection><collection>Technology Collection</collection><collection>ProQuest Natural Science Collection</collection><collection>Earth, Atmospheric & Aquatic Science Collection</collection><collection>ProQuest One Community College</collection><collection>ProQuest Central Korea</collection><collection>Aerospace Database</collection><collection>SciTech Premium Collection</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><collection>Advanced Technologies Database with Aerospace</collection><collection>Advanced Technologies & Aerospace Database</collection><collection>ProQuest Advanced Technologies & Aerospace Collection</collection><collection>Earth, Atmospheric & Aquatic Science Database</collection><collection>Publicly Available Content Database</collection><collection>ProQuest One Academic Eastern Edition (DO NOT USE)</collection><collection>ProQuest One Academic</collection><collection>ProQuest One Academic UKI Edition</collection><collection>ProQuest Central China</collection><collection>DOAJ Directory of Open Access Journals</collection><jtitle>Earth, planets, and space</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Cigolini, Corrado</au><au>Coppola, Diego</au><au>Yokoo, Akihiko</au><au>Laiolo, Marco</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>The thermal signature of Aso Volcano during unrest episodes detected from space and ground-based measurements</atitle><jtitle>Earth, planets, and space</jtitle><stitle>Earth Planets Space</stitle><date>2018-04-26</date><risdate>2018</risdate><volume>70</volume><issue>1</issue><spage>1</spage><epage>15</epage><pages>1-15</pages><artnum>67</artnum><issn>1880-5981</issn><issn>1343-8832</issn><eissn>1880-5981</eissn><abstract>The thermal signature of Aso Volcano (Nakadake) during unrest episodes has been analyzed by combining the MODIS-MIROVA data set (2000–2017) with high-resolution images (LANDSAT 8 OLI and Sentinel 2) and ground-based thermal observations (2013–2017). The site of major activity (crater 1) is located at the summit of the volcano and is composed by a fumarole field (located in the South Area) and an acidic lake (replaced by a Central Pit during Strombolian phases). The volcanic radiative power (VRP) obtained by nighttime satellite data during the reference period was mainly below 3 MW. This thermal threshold marks the transition from high fumarole activity (HFA) to Strombolian eruptions (SE). However, periods characterized by sporadic phreatic eruptions (PE, eventually bearing phreatomagmatic episodes), which is the prevalent phase during unrest episodes, exhibit very low VRP values, being around 0.5 MW, or below. The statistical analysis of satellite data shows that the transition from HFA to Strombolian activity (which started on August 2014 and ceased in May 2015) occurs when VRP values are above the cited 3 MW threshold. In particular during marked Strombolian phases (November–December 2014), the radiative power was higher than 4 MW, reaching peak values up to 15.6 MW (on December 7, 2014, i.e., 10 days after the major Strombolian explosion of November 27). Conversely, ground-based measurements show that heat fluxes recorded by FLIR T440 Thermo-camera on the fumarole field of the South Area has been relatively stable around 2 MW until February 2015. Their apparent temperatures were fluctuating around 490–575 °C before the major Strombolian explosive event, whereas those recorded at the active vent, named Central Pit, reached their maxima slightly above 600 °C; then both exhibited a decreasing trend in the following days. During the Strombolian activity, the crater lake dried out and was then replenished by early July, 2016. Then, volcanic activity shifted back to phreatic–phreatomagmatic and the eruptive cycle was completed. During this period, the MIROVA system detected very few thermal alerts and the ground-based measurements were fluctuating around 1 MW. The most violent explosion occurred on October 8, 2016, and within the following weeks measured VRP were moderately above 2 MW. This is coeval with a thermal increase at the fumarole field of the South Area, with temperatures well above 300 °C. Thermal monitoring at Aso Volcano is an additional tool in volcano surveillance that may contribute to near-real-time hazard assessment.</abstract><cop>Berlin/Heidelberg</cop><pub>Springer Berlin Heidelberg</pub><doi>10.1186/s40623-018-0831-7</doi><tpages>15</tpages><oa>free_for_read</oa></addata></record> |
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subjects | 5. Volcanology Acidic lakes Advancement of our knowledge on Aso volcano: Current activity and background Aso Volcano Earth and Environmental Science Earth Sciences Eruptions Fumarolic activity Geology Geophysics/Geodesy Ground-based observation Hazard assessment Heat flux Image resolution Lakes Landsat Landsat satellites Major explosions Methods Remote sensing Satellite data Satellite imagery Satellites Statistical analysis Statistical analysis of data Strombolian activity Temperature measurement Unrest episodes Variations Volcanic activity Volcanoes |
title | The thermal signature of Aso Volcano during unrest episodes detected from space and ground-based measurements |
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