- Info & Contacts
The Global Volcanism Program has no activity reports for Isla San Luis.
The Global Volcanism Program has no Weekly Reports available for Isla San Luis.
The Global Volcanism Program has no Bulletin Reports available for Isla San Luis.
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.
|Encantada Mayor, La | Salvatierra|
|Feature Name||Feature Type||Elevation||Latitude||Longitude|
|Plaza de Toros||Tuff ring||50 m||29° 58' 0" N||114° 24' 0" W|
|Poma, Isla||Tuff ring||29° 59' 0" N||114° 23' 0" W|
The Global Volcanism Program is not aware of any Holocene eruptions from Isla San Luis. If this volcano has had large eruptions (VEI >= 4) prior to 10,000 years ago, information might be found on the Isla San Luis page in the LaMEVE (Large Magnitude Explosive Volcanic Eruptions) database, a part of the Volcano Global Risk Identification and Analysis Project (VOGRIPA).
There is no Deformation History data available for Isla San Luis.
There is no Emissions History data available for Isla San Luis.
|Isla San Luis, viewed here from the SW with a large rhyolitic lava dome at the left center, is the largest of the seven Encantada islands in the northern part of the Gulf of California. The roughly 180-m-high island lies 3 km off the eastern shore of Baja California. An older lava dome forms the NE tip of the island, and a dissected tuff ring lies at the SE tip. The lava dome seen here in the center of the island was constructed within a tuff cone and is the youngest volcanic product of Isla San Luis.
Photo by Brian Hausback, 1997 (California State University, Sacramento).
|Isla San Luis is seen here from the south with a 2-km-long spit (at low tide) at the lower left. Three major vents, a rhyolitic lava dome forming the NW tip of the island, the central rhyolitic obsidian dome, and a dissected dacitic tuff ring at the SE tip of the island, were erupted along a trend parallel to a transform fault in the Gulf of California. Another tuff ring, Isla Poma, lies 1 km NE of Isla San Luis and is visible at the upper right.
Photo by Brian Hausback, 2000 (California State University, Sacramento).
|Isla San Luis lies across a narrow channel from the NE coast of Baja California (visible in the background). The center of the small island is dominated by a dramatic dark-colored rhyolitic obsidian dome. An older dome, partially mantled by ash and pumice from the central dome, forms the northern part of the island (foreground). A dissected tuff ring, Plaza de Toros, occupies the SE end of the island. A sequence of rocks ranging from initial basaltic-andesite and andesitic palagonite tuffs to rhyolitic lava domes was erupted during a short time interval.
Photo by Keith Sutter, 2000.
|The Plaza de Toros tuff ring on the SE side of Isla San Luis, seen here from the east, has been partially dissected by wave erosion. Remnants of dacitic lava flows are visible in the upper walls of the crater. Only a third of the tuff ring is still standing; the remainder subsided along normal faults or was removed by wave erosion. Longshore currents have redistributed friable volcanic ejecta from the cone to produce the dramatic tombolo at the upper right that forms the SW tip of the island and is 2 km long at low tide.
Photo by Keith Sutter, 2000.
|A dramatic youthful obsidian dome occupies the center of Isla San Luis off the NE coast of Baja California. The dome was constructed within a tuff cone whose rim is visible immediately in front of the dome. As growth of the dome continued in the central vent (left foreground), a thick coulee advanced to the south and overflowed the SE rim of the tuff cone, forming the broad lobe behind it. The age of the extremely youthful rhyolitic dome is not known. The dissected Plaza de Toros tuff ring in the left background forms the SE tip of the island.
Photo by Keith Sutter, 2000.
There are no samples for Isla San Luis in the Smithsonian's NMNH Department of Mineral Sciences Rock and Ore collection.
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.|
|Large Eruptions of Isla San Luis||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).|
|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.|
|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).|