| Country | United States |
| Volcanic Region | Yellowstone-Snake River Hotspot Volcano Group |
| Landform | Volc Type | Shield | Shield |
| Last Known Eruption | 300 BCE |
| Coordinates | 42.8859°N, 113.2166°W |
| Elevation | 1,597 m (5,240 ft) |
| Volcano Number | 324030 |
 Google Earth Placemark with Features
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 Cite Volcano Profile
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The Global Volcanism Program has no Weekly Volcanic Activity Reports available for Wapi Lava Field.
The Global Volcanism Program has no Bulletin Reports available for Wapi Lava Field.
The Global Volcanism Program has no Weekly Reports available for Wapi Lava Field.
The Global Volcanism Program has no Bulletin Reports available for Wapi Lava Field.
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There is data available for 1 confirmed eruptive period.
0300 BCE (?) Confirmed Eruption (Explosive / Effusive) VEI: 2 (?)
| Episode 1 | Eruption (Explosive / Effusive) | Kings Bowl Rift, Wapi Lava Field | |||||||||||||||||||||||
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| 0300 BCE (?) - Unknown | Evidence from Correlation: Tephrochronology | |||||||||||||||||||||||
| The Kings Bowl Rift flows and the massive Wapi Lava Field flows are placed at 2,250 BP based on stratigraphic position relative to flows from Craters of the Moon eruptive period A (Kuntz et al., 1982). Earlier 14C dates were 2,360 ± 150 and 2,130 ± 130 BP. | ||||||||||||||||||||||||
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List of 3 Events for Episode 1 at Kings Bowl Rift, Wapi Lava Field
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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 |
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| Feature Name | Feature Type | Elevation | Latitude | Longitude |
| Pillar Butte | Shield volcano | 1604 m | 42° 53' 7.00" N | 113° 12' 57.00" W |
Craters |
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| Feature Name | Feature Type | Elevation | Latitude | Longitude |
| Cottrells Blowout | Crater | 1582 m | 42° 59' 30.00" N | 113° 11' 24.00" W |
| Horse Butte | Crater | 1617 m | 43° 0' 33.00" N | 113° 11' 36.00" W |
| King's Bowl Rift | Fissure vent | 1500 m | 42° 57' 1.00" N | 113° 12' 58.00" W |
| Split Butte | Maar | 1400 m | 42° 53' 54.00" N | 113° 22' 22.00" W |
Other |
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| Feature Name | Feature Type | Elevation | Latitude | Longitude |
| Wapi Lava Field | Lava Flows | 1450 m | 42° 49' 40.00" N | 113° 13' 20.00" W |
Dark lava flows extend from the 6-km-long Kings Bowl Rift SE of Craters of the Moon. These flows were erupted at the same time as the much more massive Wapi lava field flows immediately to the south that covered about 300 km2, forming a broad, low shield volcano about 2250 years ago. The light-colored area overlying the lava flows at the lower center of the photo is an ash deposit produced by explosions from Kings Bowl crater.
The dramatic Kings Bowl rift cutting diagonally across the top of the photo produced a small 6-sq-km lava field about 2250 years ago immediately north of the much larger Wapi lava field. Kings Bowl itself is the small elongated crater on the right-center side of the rift in this photo; it formed during a phreatic explosion that deposited lighter-colored tephra to the east (upper right). The massive Wapi lava field, located out of view south (right) of Kings Bowl, covers an area of about 325 km2 and originated from Pillar Butte, a small shield volcano. There are no samples for Wapi Lava Field 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. |
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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. |
| EarthScope Consortium SAGE seismic stations/networks | EarthScope Consortium operates the NSF Geodetic Facility for the Advancement of Geoscience (GAGE) and NSF Seismological Facility for the Advancement of Geoscience (SAGE). The linked map shows 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 Wapi Lava Field. 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. |
| Large Eruptions of Wapi Lava Field | 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). |
