The Global Volcanism Program has no activity reports for Bayuda Volcanic Field.
The Global Volcanism Program has no Weekly Reports available for Bayuda Volcanic Field.
The Global Volcanism Program has no Bulletin Reports available for Bayuda Volcanic Field.
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.
|Baiyuda Volcanic Field|
|Feature Name||Feature Type||Elevation||Latitude||Longitude|
|Abour, Jebel El||Cone|
|Bararumbo||Cone||18° 28' 0" N||32° 47' 0" E|
|Goan||Cone||18° 23' 0" N||32° 52' 0" E|
|Hiwaish Abu Siba||Cone|
|Hosh Umm Araysh, Jebel||Cone|
|Mazrub, Jebel||Cone||18° 30' 0" N||32° 26' 0" E|
|Mersidat||Cone||18° 29' 0" N||32° 45' 0" E|
|Miraibta, Jebel El||Cone|
|Sergein||Cone||18° 32' 0" N||32° 40' 0" E|
|Tebel Qurein||Cone||18° 24' 0" N||32° 38' 0" E|
|Umm Khandag, Jebel||Cone||18° 31' 0" N||32° 23' 0" E|
|Umm Qureinat||Cone||18° 24' 0" N||32° 36' 0" E|
|Uruf, Jebel||Cone||18° 30' 0" N||32° 21' 0" E|
|Zein Umm Araysh, Jebel||Cone|
|Feature Name||Feature Type||Elevation||Latitude||Longitude|
|Bihadi||Crater||18° 18' 0" N||32° 47' 0" E|
|Hosh Ed Dalan||Crater||18° 23' 0" N||32° 38' 0" E|
|Hosh Es Siddig||Crater||18° 15' 0" N||33° 0' 0" E|
|Tebel Hebeish||Crater||18° 30' 0" N||32° 29' 0" E|
There is data available for 1 Holocene eruptive periods.
|Start Date||Stop Date||Eruption Certainty||VEI||Evidence||Activity Area or Unit|
|0850 ± 50 years||Unknown||Confirmed||Radiocarbon (uncorrected)|
There is no Deformation History data available for Bayuda Volcanic Field.
There is no Emissions History data available for Bayuda Volcanic Field.
|The Bayuda volcanic field is located near the center of the Bayuda desert of NE Sudan. The numerous small scoria cones that trend horizontally across the center of the volcanic field in this Space Shuttle image were erupted along a WNW-trending line. Lava flows, one of which was erupted about 1,100 years ago, are visible in this image, but about 10% of the vents are craters. Bayuda was constructed over Precambrian and Paleozoic granitic rocks, which form the darker areas at the lower right.
NASA Space Shuttle image ISS004-711-20, 2002 (http://eol.jsc.nasa.gov/).
The maps shown below have been scanned from the GVP map archives and include the volcano on this page. Clicking on the small images will load the full 300 dpi map. Very small-scale maps (such as world maps) are not included. The maps database originated over 30 years ago, but was only recently updated and connected to our main database. We welcome users to tell us if they see incorrect information or other problems with the maps; please use the Contact GVP link at the bottom of the page to send us email.
Title: Persian Gulf
Publisher: Aeronautical Chart and Information Center U.S. Air Force
Map Type: Geographic
There are no samples for Bayuda Volcanic Field in the Smithsonian's NMNH Department of Mineral Sciences Rock and Ore collection.
|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.|
Sentinel Hub Playground
Sentinel Hub EO Browser
|The Sentinel Hub Playground provides a quick look at any Sentinel-2 image in any combination of the bands and enhanced with image effects; Landsat 8, DEM and MODIS are also available. Sentinel Hub is an engine for processing of petabytes of satellite data. It is opening the doors for machine learning and helping hundreds of application developers worldwide. It makes Sentinel, Landsat, and other Earth observation imagery easily accessible for browsing, visualization and analysis. Sentinel Hub is operated by Sinergise|
|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 Bayuda Volcanic 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.|
|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 Bayuda Volcanic Field. 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.|
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 Bayuda Volcanic 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).|