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The Global Volcanism Program has no activity reports for Mono Craters.
The Global Volcanism Program has no Weekly Reports available for Mono Craters.
The Global Volcanism Program has no Bulletin Reports available for Mono Craters.
Summary of Holocene eruption dates and Volcanic Explosivity Indices (VEI).
|Start Date||Stop Date||Eruption Certainty||VEI||Evidence||Activity Area or Unit|
|1350 ± 20 years||Unknown||Confirmed||4||Dendrochronology||Panum Crater and nearby vents|
|1000 ± 200 years||Unknown||Confirmed||Hydration Rind||Dome on NW edge of NW Coulee|
|0620 ± 27 years||Unknown||Confirmed||4||Radiocarbon (corrected)||South Coulee|
|0490 ± 100 years||Unknown||Confirmed||Radiocarbon (uncorrected)||NW Coulee and Pumice Pit dome|
|0440 ± 100 years||Unknown||Confirmed||Radiocarbon (uncorrected)||Southern Mono Craters|
|0320 ± 200 years||Unknown||Confirmed||Radiocarbon (corrected)||South Coulee?|
|0010 ± 200 years||Unknown||Confirmed||Radiocarbon (corrected)||South Coulee?|
|0700 BCE ± 800 years||Unknown||Confirmed||Hydration Rind||Central Mono Craters|
|3850 BCE ± 1160 years||Unknown||Confirmed||Hydration Rind||Crater north of Punchbowl|
|6750 BCE ± 1740 years||Unknown||Confirmed||Hydration Rind||Punchbowl|
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|
|West Control Crater||Crater|
|Feature Name||Feature Type||Elevation||Latitude||Longitude|
|Crater Mountain||Dome||2796 m||37° 53' 0" N||119° 0' 0" W|
|Cratered Dome||Dome||2134 m||37° 55' 0" N||119° 2' 0" W|
|North Coulee||Dome||2583 m||37° 53' 28" N||119° 1' 0" W|
|Panum||Dome||2121 m||37° 56' 0" N||119° 3' 0" W|
|Pumice Pit Dome||Dome||2060 m||37° 55' 0" N||119° 2' 28" W|
|Punchbowl||Dome||2455 m||37° 49' 0" N||119° 2' 0" W|
|South Coulee||Dome||2691 m||37° 51' 0" N||119° 1' 0" W|
|Upper Dome||Dome||2390 m||37° 55' 0" N||119° 2' 0" W|
|The Mono Craters volcanic field, between Mono Lake in the foreground and Long Valley caldera at the upper left, is a 17-km-long chain of rhyolitic lava domes and thick, viscous lava flows. Mono Craters have been frequently active during the Holocene. Panum crater (the vent nearest to Mono Lake), is partially filled by a lava dome and was the site of the latest eruption from Mono Craters, about 600 years ago.
Photo by R. Von Huene, 1971 (U.S. Geological Survey).
|The hackly surfaced Panum lava dome, filling a tephra ring at the northern end of the Mono Craters chain, was one of five rhyolitic lava domes and flows emplaced at the end of a major eruption about 600 years ago. The eruption, which began with powerful plinian explosive eruptions accompanied by pyroclastic flows and surges, occurred just a year or two prior to another major eruption at Inyo Craters to the south.
Photo by Dan Dzurisin, 1982 (U.S. Geological Survey).
|Flow-banded rhyolitic obsidian of the Panum Crater lava dome was erupted about 600 years ago at the northern end of the Mono Craters. The greenish-yellow areas are lichens on the surface of the dome.
Photo by Lee Siebert, 1973 (Smithsonian Institution).
|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).
|The Mono Craters volcanic field, seen here from the NW, is a 17-km-long arcuate chain of lava domes, lava flows, and tephra rings. The latest eruptions took place about 600 years ago from several vents at the northern end of the chain, producing rhyolitic lava domes and flows.
Photo by Victoria Avery, 1992 (Smithsonian Institution).
The following 52 samples associated with this volcano can be found in the Smithsonian's NMNH Department of Mineral Sciences collections. Catalog number links will open a window with more information.
|Catalog Number||Sample Description|
|NMNH 111123-59||Rhyolitic pumice|
|NMNH 111123-60||Rhyolitic obsidian|
|NMNH 29631-5||Hyalo liparite|
|NMNH 29631-6||Hyalo liparite|
|NMNH 37216||Hypersthene andesite|
|Large Eruptions of Mono 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.|