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The Global Volcanism Program has no activity reports for Inyo Craters.
The Global Volcanism Program has no Weekly Reports available for Inyo Craters.
The Global Volcanism Program has no Bulletin Reports available for Inyo Craters.
Summary of Holocene eruption dates and Volcanic Explosivity Indices (VEI).
|Start Date||Stop Date||Eruption Certainty||VEI||Evidence||Activity Area or Unit|
|1380 ± 50 years||Unknown||Confirmed||4||Radiocarbon (corrected)||S Deadman, Obsidian Flow, Glass Creek|
|0290 ± 50 years||Unknown||Confirmed||4||Radiocarbon (corrected)||Wilson Butte|
|4050 BCE (?)||Unknown||Confirmed||Hydration Rind||North of Deadman Creek|
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.
|Feature Name||Feature Type||Elevation||Latitude||Longitude|
|Deadman Creek||Dome||2570 m||37° 43' 0" N||119° 1' 0" W|
|Glass Creek||Dome||2629 m||37° 45' 0" N||119° 1' 0" W|
|North Deadman Creek||Dome||2549 m||37° 43' 0" N||119° 1' 0" W|
|Obsidian||Dome||2622 m||37° 45' 0" N||119° 1' 0" W|
|Wilson Butte||Dome||2587 m||37° 47' 0" N||119° 1' 0" W|
|The Mono Craters volcanic field south of Mono Lake at the upper left, is a 17-km-long arcuate chain of rhyolitic lava domes and thick, viscous lava flows. Mono Craters has been frequently active throughout the Holocene, along with the Inyo Craters chain to the south. The Inyo Craters chain, which includes the Wilson Butte, Obsidian and Glass Creek domes, which are oriented diagonally along a N-S line from the left center to lower right of the photo. The latest eruptions of Mono Craters and Inyo Craters occurred nearly simultaneously around 600 years ago.
Photo by Roy Bailey, 1980 (U.S. Geological Survey).
|An aerial view from the south shows the North and South Inyo Craters phreatic explosion craters diagonally cutting forested Deer Mountain from the right center to lower right, and the unvegetated South Deadman lava dome and obsidian flow and the forested mound of North Deadman dome at the upper left. Eruption of magmatic tephra and the formation of the phreatic explosion craters preceded emplacement of the lava domes and flows about 600 years ago.
Photo by Larry Mastin, 1988 (U.S. Geological Survey).
|The Obsidian Flow, a lava flow with a hackly surface showing prominent flow banding, was erupted at the northern end of a chain of lava domes and flows during a dike-fed eruption about 600 years ago at Inyo Craters. The Obsidian Flow was the largest of four flows and domes emplaced during this eruption.
Photo by Larry Mastin, 1992 (U.S. Geological Survey).
|South Inyo Crater, one of a chain of small phreatic explosion craters at the southern end of the Inyo Craters chain of lava domes and flows, is partially filled by a shallow lake. The 200-m-wide South Inyo Crater was formed when groundwater interacted with magma from a shallow dike. That interaction fed a powerful explosive eruption that concluded with the emplacement of obsidian lava domes and flows to the north of this crater.
Photo by Larry Mastin, 1992 (U.S. Geological Survey).
|The pumice layers above the bottom of the pen originated from the South Deadman vent of Inyo Craters about 600 years ago. Interbedded finer layers record brief pauses during the course of the eruption.
Photo by Larry Mastin, 1986 (U.S. Geological Survey).
|The unvegetated Glass Creek lava flow on the left and Obsidian Flow on the right are among a group of obsidian lava flows and domes that were emplaced during a major eruption from the Inyo Craters about 600 years ago. The eruption, originating from a shallow dike, began with powerful explosive activity, pyroclastic flows, and a series of phreatic explosions, and ended with effusion of the lava domes and flows.
Photo by Larry Mastin, 1991 (U.S. Geological Survey).
|Wilson Butte, the northermost lava dome of the Inyo Craters, is seen from the Obsidian Flow lava dome to the south. The Inyo Craters are a 12-km-long chain of silicic lava domes, lava flows, and explosion craters along the eastern margin of Sierra Nevada south of Mono Craters near the town of Mammoth. Inyo Craters overtop the NW rim of the Pleistocene Long Valley caldera and extend onto the caldera floor, but are chemically and magmatically part of a different volcanic system. The latest eruptions at Inyo Craters took place about 600 years ago.
Photo by Lee Siebert, 1998 (Smithsonian Institution).
A listing of samples from the Smithsonian collections will be available soon.
|Large Eruptions of Inyo Craters||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).|
|WOVOdat||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.|
|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).|
|MODVOLC - HIGP MODIS Thermal Alert System||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.|
|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.|