Activity in 1999; submarine eruption plume during January-February 2000
The submarine eruption that started on December 1998 (BGVN 24:01 and 24:03) from multiple vents along the Serreta Volcanic Ridge, about 10 km W of Terceira Island, Azores, continued through March 2000. Vents along the ridge were very active between December 1998 and September 1999. Activity then declined to very low levels with rare surface manifestations through December 1999. Activity increased again in late January 2000.
Several times during 1999 basaltic lava balloons were observed floating in the eruptive area. These "balloons" are very hot, gas-rich, lava fragments produced from small submarine lava lakes/fountains. During ascent to the surface, magmatic gas exsolves from the hot fragments, increasing the volume of the balloon while the crust is glassy and expansible. Once at the surface, interaction between the hot blocks and seawater produce white steam columns that can be seen from land when meteorological conditions are favorable (figure 5). The blocks eventually sink after the gas escapes.
Figure 5. Lava balloon from the Serreta Ridge off Terciera floating on the sea surface and producing white steam column. Courtesy of CVUA. |
An oceanographic mission supported by the national Foundation for Science and Technology was carried out in April 1999 to study the geological/geophysical characteristics of the eruption and its impact on local ecosystems. Scientists from the University of Azores, University of Lisbon, University of Algarve, Instituto do Mar, and Instituito Hidrográfico used a remotely operated vehicle that crossed an impressive submarine volcanic plume just above an active eruptive center at about 380 m depth. This plume was formed by volcanic particles of ash and lapilli size along with gas bubbles and lava balloons up to 2 m in diameter.
On 28 January 2000 a yellowish spot was observed at the sea surface above the eruptive area due to the dispersion of a volcanic plume that rose from a new vent located at about 250 m depth (figure 6). The area of water discoloration caused by the plume was visible almost continuously for about a month, reaching a maximum diameter of 8 km on 24 February. The plume was generated by multiple eruptive pulses from different eruptive centers located within a few hundred meters of each other.
Figure 6. Aerial view of the edge of a submarine volcanic ash plume spreading at the sea surface. Courtesy of CVUA. |
Seismicity along the ridge related to the eruption continued through the end of March, but at low levels. Since the beginning of this volcanic crisis the physical and chemical parameters of waters and fumarolic gases from Terceira Island have been monitored, with no changes detected. Another submarine eruption took place in this general location in June 1867. At that time five months of strong seismicity destroyed about 200 houses at Serreta.
Information Contacts: J.L. Gaspar, G. Queiroz, J.M. Pacheco, T. Ferreira, R. Coutinho, M.H. Almeida, and N. Wallenstein, Centre of Volcanology of the Azores University (CVUA), Departamento de Geociencias, Rua da Mae de Deus, 9502 Ponta Delgada, Azores, Portugal (URL: http://www.uac.pt/).
The Global Volcanism Program has no Weekly Reports available for Terceira.
Reports are organized chronologically and indexed below by Month/Year (Publication Volume:Number), and include a one-line summary. Click on the index link or scroll down to read the reports.
Submarine eruption west of Terceira produces floating lava blocks
A small seismic crisis during November 1998 was monitored by the Azores Seismological Surveillance System (SIVISA). It was centered W of Terceira Island on the E of the so-called Graciosa Trough [38.783°N, 27.483°W; submarine vent at -500 m]. After four days of major activity seismicity decreased and remained at normal levels until 18 December; then, a few microseisms were registered by SIVISA and white vapor columns were reported by fishermen to be rising from the sea 8 km W of Terceira island. These phenomena were discontinuous but persisted until the night of 23 December when local residents observed orange lights several miles W of Terceira.
Although no unusual seismicity was noticed in the following interval, on 8 January fishermen again reported white vapor columns on the sea. Scientists from the Center of Volcanology of Azores University (CVUA) using a helicopter of the Portuguese Air Force took the first pictures of the phenomenon (figure 1). Lava blocks reaching a maximum of 3 m in length rose gently to the surface where they floated for a few minutes. White steam columns resulting from contact between hot lava blocks and seawater were observed, rising about 10 m above the surface of the sea. During the night the same activity was observed from the W coast of Terceira island and six different areas of incandescent, dispersed lava blocks were identified along a NE-SW axis. Activity continued at the same level until 13 January after which only intermittent short-period events were observed.
Figure 1. Two views of the eruption site as photographed by João Gaspar from a helicopter during an overflight on 8 January 1999. Courtesy of CVUA. |
On the morning of 10 February three spots of white steam suddenly rose ~70 m into the air at a point 8 km from the coast. The steam was seen from land. That afternoon scientists from CVUA with personnel of the Azores Civil Protection Force retrieved the first rock sample from the eruption.
Lava produced by this submarine fissure eruption was basaltic, showing phenocrysts of olivine, pyroxene, and plagioclase in a highly vesicular groundmass. Analysis of the sample suggested that material rose from the sea bottom as hot lava balloons, lost gas from their interiors at the surface, and then sank. Seismic activity and physical and chemical parameters of waters and fumarolic gases continue to be monitored.
Another submarine eruption took place in this general location in June 1867, but closer to land. This is thought to be the first submarine eruption in the Atlantic in more than 30 years that has brought products to the sea surface. The name "Serrata" has been tentatively given to this feature.
Information Contacts: João Luís Gaspar and Nicolau Wallenstein, Center of Volcanology of the Azores University (CVAU), Departamento de Geociencias, Rua da Mae de Deus, 9502 Ponta Delgada, Azores, Portugal (URL: http://www.uac.pt/).
Migrating vents; floating blocks with large internal cavities ("lava balloons")
During February and March 1999 the submarine eruption that began late 1998 continued at the Serreta volcanic ridge, ~9-14 km W of Terceira island (BGVN 23:01; Luis and others, 1999). The activity decreased slightly until the end of February, but eruptive areas clearly defined two main volcanic trends in both NE-SW and NW-SE directions (figure 2). In March, activity became less vigorous and observers saw sea surface manifestations only during intermittent short periods.
The eruption of Serreta is interpreted as being a fissure-style vent that started along a NE-SW fracture system over 5 km long. During the eruption, the regional NW-SE fracture system also reactivated and eruptive vents developed on these two main trends. Plotting vent locations on published bathymetric maps made by the Instituto Hidrográfico puts them at depths of 300-800 m. However, bathymetric surveys carried out by the Portuguese Navy between January and March detected big anomalies in the area, perhaps due to gas bubbles, volcanic particles, and sharp thermal boundaries. Well-constrained depths for the active vents remain unknown and construction of a new bathymetric map of the area was planned for April.
This eruption involved basaltic, and probably very gas-rich, magma. Petrographic studies of the collected rock samples revealed olivine, pyroxene, and feldspars phenocrysts in a glassy groundmass with similar microlites that also include oxides. Chemical analysis made by colleagues from the Nordic Volcanological Institute showed that it is an alkaline magma with a composition along the magmatic trend defined by the Azores oceanic island basalts.
Floating blocks were seen on the surface (BGVN 23:01) and some were collected (figures 3 and 4). The scientific team attributed their seismic observations coupled with the floating blocks to the following mechanism. The magma, being low in viscosity, moves very easily through the already opened fractures and was thought to escape without producing high seismic signals. Floating lava blocks could result from the detachment of pillow-lava edges followed by the ascent of blocks with sufficient gas content. It is also possible that hot, gas-rich lava fragments result from small submarine lava lakes or fountains. A thin frozen skin of lava seals the gas cavity, and the block might then rise as a hot lava balloon. During ascent, the gas exsolves and nucleates inside the hot fragment while the blocks expand. Once at the surface the interaction between the hot blocks and the seawater produces white steam columns. At the same time, while cooling at the surface, the blocks crack slowly, lose their magmatic gas and sink. Sometimes when water enters inside the hot blocks, they blow up, violently throwing fragments several meters high.
Figure 4. A sub-spherical floating block (a "lava balloon") from the Serreta eruption collected on an undisclosed day. Taken from Radiotelevisão Portuguesa (April 1999); URL: http://www.rtp.pt/. |
Since the beginning of this volcanic crisis the physical and chemical parameters of waters and fumarolic gases from the Terceira Island have been monitored and no changes have been detected. Azores Civil Protection (SRPCA) devised a series of emergency plans.
Another submarine eruption took place near the current one in mid-1867 (figure 1). Five months of strong seismicity around the time of the eruption destroyed about 200 houses on Terceira in the coastal settlement of Serreta. Websites associated with Azores civil defense and a local TV station have more photos of the eruption, including floating blocks.
References. Azores civil defense website, April 1999, Açores crise sismovulcania: URL:.
Luis, J.F., Lourenço, N., Miranda, J.M., Gaspar, J.L., and G. Queiroz, 1999, A submarine eruption W of Terceira Island (Azores Archipelao): InterRidge News, Initiative for international cooperation in ridge-crest studies, vol. 8, no. 1, Spring 1999, p. 13-14.
Machado, F., 1967, Active volcanoes of the Azores, in Neumann Van Padang, M., and others, 1967, Catalogue of the Active Volcanoes of the World: International Assoc. of Volcanology, Part XXI, p. 28-30.
Information Contacts: J.L. Gaspar, T. Ferreira, G. Queiroz, R. Coutinho, M.H. Almeida, N. Wallenstein, and J.M. Pacheco, Centre of Volcanology of the Azores University (CVUA), Departamento de Geociencias, Rua da Mae de Deus, 9502 Ponta Delgada, Azores, Portugal (URL: http://www.uac.pt/).
Activity in 1999; submarine eruption plume during January-February 2000
The submarine eruption that started on December 1998 (BGVN 24:01 and 24:03) from multiple vents along the Serreta Volcanic Ridge, about 10 km W of Terceira Island, Azores, continued through March 2000. Vents along the ridge were very active between December 1998 and September 1999. Activity then declined to very low levels with rare surface manifestations through December 1999. Activity increased again in late January 2000.
Several times during 1999 basaltic lava balloons were observed floating in the eruptive area. These "balloons" are very hot, gas-rich, lava fragments produced from small submarine lava lakes/fountains. During ascent to the surface, magmatic gas exsolves from the hot fragments, increasing the volume of the balloon while the crust is glassy and expansible. Once at the surface, interaction between the hot blocks and seawater produce white steam columns that can be seen from land when meteorological conditions are favorable (figure 5). The blocks eventually sink after the gas escapes.
Figure 5. Lava balloon from the Serreta Ridge off Terciera floating on the sea surface and producing white steam column. Courtesy of CVUA. |
An oceanographic mission supported by the national Foundation for Science and Technology was carried out in April 1999 to study the geological/geophysical characteristics of the eruption and its impact on local ecosystems. Scientists from the University of Azores, University of Lisbon, University of Algarve, Instituto do Mar, and Instituito Hidrográfico used a remotely operated vehicle that crossed an impressive submarine volcanic plume just above an active eruptive center at about 380 m depth. This plume was formed by volcanic particles of ash and lapilli size along with gas bubbles and lava balloons up to 2 m in diameter.
On 28 January 2000 a yellowish spot was observed at the sea surface above the eruptive area due to the dispersion of a volcanic plume that rose from a new vent located at about 250 m depth (figure 6). The area of water discoloration caused by the plume was visible almost continuously for about a month, reaching a maximum diameter of 8 km on 24 February. The plume was generated by multiple eruptive pulses from different eruptive centers located within a few hundred meters of each other.
Figure 6. Aerial view of the edge of a submarine volcanic ash plume spreading at the sea surface. Courtesy of CVUA. |
Seismicity along the ridge related to the eruption continued through the end of March, but at low levels. Since the beginning of this volcanic crisis the physical and chemical parameters of waters and fumarolic gases from Terceira Island have been monitored, with no changes detected. Another submarine eruption took place in this general location in June 1867. At that time five months of strong seismicity destroyed about 200 houses at Serreta.
Information Contacts: J.L. Gaspar, G. Queiroz, J.M. Pacheco, T. Ferreira, R. Coutinho, M.H. Almeida, and N. Wallenstein, Centre of Volcanology of the Azores University (CVUA), Departamento de Geociencias, Rua da Mae de Deus, 9502 Ponta Delgada, Azores, Portugal (URL: http://www.uac.pt/).
This compilation of synonyms and subsidiary features may not be comprehensive. Features are organized into four major categories: Cones, Craters, Domes, and Thermal Features. Synonyms of features appear indented below the primary name. In some cases additional feature type, elevation, or location details are provided.
Cones |
||||
Feature Name | Feature Type | Elevation | Latitude | Longitude |
Alto, Pico | Stratovolcano | 38° 45' 0" N | 27° 12' 0" W | |
Brasil, Monte | Cone | |||
Cinco Picos | Shield volcano | 545 m | 38° 42' 0" N | 27° 10' 0" W |
Guilherme Moniz
Macico da Agualva Serra do Moriao |
Stratovolcano | 632 m | 38° 44' 0" N | 27° 12' 0" W |
Santa Barbara | Stratovolcano | 1023 m | 38° 44' 0" N | 27° 19' 0" W |
Craters |
||||
Feature Name | Feature Type | Elevation | Latitude | Longitude |
Serreta Ridge | Submarine crater | -500 m | 38° 47' 0" N | 27° 29' 0" W |
Domes |
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Feature Name | Feature Type | Elevation | Latitude | Longitude |
Agualva | Dome | 798 m | 38° 44' 0" N | 27° 13' 0" W |
Farol | Dome | |||
Lagoinha | Dome |
|
|
There is data available for 15 confirmed Holocene eruptive periods.
1998 Nov 25 (?) - 2000 Mar 16 (?) ± 15 days Confirmed Eruption VEI: 0
Episode 1 | Eruption | Serreta Ridge (submarine vent W of Terceira) | ||||||||||||||||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
1998 Nov 25 (?) - 2000 Mar 16 (?) ± 15 days | Evidence from Observations: Reported | ||||||||||||||||||||||||
List of 3 Events for Episode 1 at Serreta Ridge (submarine vent W of Terceira)
|
1867 Jun 1 - 1867 Jun 8 Confirmed Eruption VEI: 3
Episode 1 | Eruption | Submarine vent 3-6 WNW of Terceira | |||||||||||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
1867 Jun 1 - 1867 Jun 8 | Evidence from Observations: Reported | |||||||||||||||||||
List of 2 Events for Episode 1 at Submarine vent 3-6 WNW of Terceira
|
1761 Apr 17 - 1761 Apr 28 (?) Confirmed Eruption VEI: 2
Episode 1 | Eruption | Fissure zone (east of Santa Barbara) | |||||||||||||||||||||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
1761 Apr 17 - 1761 Apr 28 (?) | Evidence from Observations: Reported | |||||||||||||||||||||||||||||
List of 4 Events for Episode 1 at Fissure zone (east of Santa Barbara)
|
1400 ± 50 years Confirmed Eruption
Episode 1 | Eruption | Farol I dome (Santa Barbara) | ||||||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
1400 ± 50 years - Unknown | Evidence from Correlation: Tephrochronology | ||||||||||||||
List of 1 Events for Episode 1 at Farol I dome (Santa Barbara)
|
1200 ± 300 years Confirmed Eruption
Episode 1 | Eruption | Guilherme Moniz (Pico Alto) | ||||||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
1200 ± 300 years - Unknown | Evidence from Correlation: Tephrochronology | ||||||||||||||
List of 1 Events for Episode 1 at Guilherme Moniz (Pico Alto)
|
0920 ± 50 years Confirmed Eruption
Episode 1 | Eruption | Guilherme Moniz (Quinta da Madalena) | |||||||||||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
0920 ± 50 years - Unknown | Evidence from Isotopic: 14C (uncalibrated) | |||||||||||||||||||
List of 2 Events for Episode 1 at Guilherme Moniz (Quinta da Madalena)
|
0820 ± 40 years Confirmed Eruption
Episode 1 | Eruption | Santa Barbara | |||||||||||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
0820 ± 40 years - Unknown | Evidence from Isotopic: 14C (uncalibrated) | |||||||||||||||||||
List of 2 Events for Episode 1 at Santa Barbara
|
0190 ± 40 years Confirmed Eruption
Episode 1 | Eruption | Guilherme Moniz (Pico Alto) | ||||||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
0190 ± 40 years - Unknown | Evidence from Isotopic: 14C (uncalibrated) | ||||||||||||||
List of 1 Events for Episode 1 at Guilherme Moniz (Pico Alto)
|
0070 ± 40 years Confirmed Eruption
Episode 1 | Eruption | Fissure zone (east of Santa Barbara) | ||||||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
0070 ± 40 years - Unknown | Evidence from Isotopic: 14C (uncalibrated) | ||||||||||||||
List of 1 Events for Episode 1 at Fissure zone (east of Santa Barbara)
|
0060 BCE (?) Confirmed Eruption
Episode 1 | Eruption | Fissure zone (south of Pico Alto) | |||||||||||||||||||||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
0060 BCE (?) - Unknown | Evidence from Isotopic: 14C (uncalibrated) | |||||||||||||||||||||||||||||
List of 4 Events for Episode 1 at Fissure zone (south of Pico Alto)
|
0090 BCE ± 100 years Confirmed Eruption
Episode 1 | Eruption | Fissure zone (east of Santa Barbara) | |||||||||||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
0090 BCE ± 100 years - Unknown | Evidence from Isotopic: 14C (uncalibrated) | |||||||||||||||||||
List of 2 Events for Episode 1 at Fissure zone (east of Santa Barbara)
|
0670 BCE ± 300 years Confirmed Eruption
Episode 1 | Eruption | Guilherme Moniz, Biscoito Rachado deposit | ||||||||||||||||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
0670 BCE ± 300 years - Unknown | Evidence from Isotopic: 14C (uncalibrated) | ||||||||||||||||||||||||
List of 3 Events for Episode 1 at Guilherme Moniz, Biscoito Rachado deposit
|
0940 BCE ± 50 years Confirmed Eruption
Episode 1 | Eruption | Santa Barbara NW flank (Lagoinha dome) | |||||||||||||||||||||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
0940 BCE ± 50 years - Unknown | Evidence from Isotopic: 14C (uncalibrated) | |||||||||||||||||||||||||||||
List of 4 Events for Episode 1 at Santa Barbara NW flank (Lagoinha dome)
|
2530 BCE ± 40 years Confirmed Eruption
Episode 1 | Eruption | Fissure zone (east of Santa Barbara) | |||||||||||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
2530 BCE ± 40 years - Unknown | Evidence from Isotopic: 14C (uncalibrated) | |||||||||||||||||||
List of 2 Events for Episode 1 at Fissure zone (east of Santa Barbara)
|
6720 BCE ± 50 years Confirmed Eruption
Episode 1 | Eruption | Guilherme Moniz (Pico das Pardelas) | ||||||||||||||||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
6720 BCE ± 50 years - Unknown | Evidence from Isotopic: 14C (uncalibrated) | ||||||||||||||||||||||||
List of 3 Events for Episode 1 at Guilherme Moniz (Pico das Pardelas)
|
There is no Deformation History data available for Terceira.
There is no Emissions History data available for Terceira.
Maps are not currently available due to technical issues.
There are no samples for Terceira in the Smithsonian's NMNH Department of Mineral Sciences Rock and Ore collection.
Copernicus Browser | The Copernicus Browser replaced the Sentinel Hub Playground browser in 2023, to provide access to Earth observation archives from the Copernicus Data Space Ecosystem, the main distribution platform for data from the EU Copernicus missions. |
MIROVA | Middle InfraRed Observation of Volcanic Activity (MIROVA) is a near real time volcanic hot-spot detection system based on the analysis of MODIS (Moderate Resolution Imaging Spectroradiometer) data. In particular, MIROVA uses the Middle InfraRed Radiation (MIR), measured over target volcanoes, in order to detect, locate and measure the heat radiation sourced from volcanic activity. |
MODVOLC Thermal Alerts | Using infrared satellite Moderate Resolution Imaging Spectroradiometer (MODIS) data, scientists at the Hawai'i Institute of Geophysics and Planetology, University of Hawai'i, developed an automated system called MODVOLC to map thermal hot-spots in near real time. For each MODIS image, the algorithm automatically scans each 1 km pixel within it to check for high-temperature hot-spots. When one is found the date, time, location, and intensity are recorded. MODIS looks at every square km of the Earth every 48 hours, once during the day and once during the night, and the presence of two MODIS sensors in space allows at least four hot-spot observations every two days. Each day updated global maps are compiled to display the locations of all hot spots detected in the previous 24 hours. There is a drop-down list with volcano names which allow users to 'zoom-in' and examine the distribution of hot-spots at a variety of spatial scales. |
WOVOdat
Single Volcano View Temporal Evolution of Unrest Side by Side Volcanoes |
WOVOdat is a database of volcanic unrest; instrumentally and visually recorded changes in seismicity, ground deformation, gas emission, and other parameters from their normal baselines. It is sponsored by the World Organization of Volcano Observatories (WOVO) and presently hosted at the Earth Observatory of Singapore.
GVMID Data on Volcano Monitoring Infrastructure The Global Volcano Monitoring Infrastructure Database GVMID, is aimed at documenting and improving capabilities of volcano monitoring from the ground and space. GVMID should provide a snapshot and baseline view of the techniques and instrumentation that are in place at various volcanoes, which can be use by volcano observatories as reference to setup new monitoring system or improving networks at a specific volcano. These data will allow identification of what monitoring gaps exist, which can be then targeted by remote sensing infrastructure and future instrument deployments. |
Volcanic Hazard Maps | The IAVCEI Commission on Volcanic Hazards and Risk has a Volcanic Hazard Maps database designed to serve as a resource for hazard mappers (or other interested parties) to explore how common issues in hazard map development have been addressed at different volcanoes, in different countries, for different hazards, and for different intended audiences. In addition to the comprehensive, searchable Volcanic Hazard Maps Database, this website contains information about diversity of volcanic hazard maps, illustrated using examples from the database. This site is for educational purposes related to volcanic hazard maps. Hazard maps found on this website should not be used for emergency purposes. For the most recent, official hazard map for a particular volcano, please seek out the proper institutional authorities on the matter. |
IRIS seismic stations/networks | Incorporated Research Institutions for Seismology (IRIS) Data Services map showing the location of seismic stations from all available networks (permanent or temporary) within a radius of 0.18° (about 20 km at mid-latitudes) from the given location of Terceira. Users can customize a variety of filters and options in the left panel. Note that if there are no stations are known the map will default to show the entire world with a "No data matched request" error notice. |
UNAVCO GPS/GNSS stations | Geodetic Data Services map from UNAVCO showing the location of GPS/GNSS stations from all available networks (permanent or temporary) within a radius of 20 km from the given location of Terceira. Users can customize the data search based on station or network names, location, and time window. Requires Adobe Flash Player. |
DECADE Data | The DECADE portal, still in the developmental stage, serves as an example of the proposed interoperability between The Smithsonian Institution's Global Volcanism Program, the Mapping Gas Emissions (MaGa) Database, and the EarthChem Geochemical Portal. The Deep Earth Carbon Degassing (DECADE) initiative seeks to use new and established technologies to determine accurate global fluxes of volcanic CO2 to the atmosphere, but installing CO2 monitoring networks on 20 of the world's 150 most actively degassing volcanoes. The group uses related laboratory-based studies (direct gas sampling and analysis, melt inclusions) to provide new data for direct degassing of deep earth carbon to the atmosphere. |
Large Eruptions of Terceira | Information about large Quaternary eruptions (VEI >= 4) is cataloged in the Large Magnitude Explosive Volcanic Eruptions (LaMEVE) database of the Volcano Global Risk Identification and Analysis Project (VOGRIPA). |
EarthChem | EarthChem develops and maintains databases, software, and services that support the preservation, discovery, access and analysis of geochemical data, and facilitate their integration with the broad array of other available earth science parameters. EarthChem is operated by a joint team of disciplinary scientists, data scientists, data managers and information technology developers who are part of the NSF-funded data facility Integrated Earth Data Applications (IEDA). IEDA is a collaborative effort of EarthChem and the Marine Geoscience Data System (MGDS). |