| Country | Saudi Arabia |
| Volcanic Region | Western Arabia Volcanic Province |
| Landform | Volc Type | Cluster | Volcanic field |
| Last Known Eruption | Pleistocene |
| Coordinates | 27.408°N, 37.279°E |
| Elevation | 1,700 m (5,577 ft) |
| Volcano Number | 231015 |
 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 Harrat ar Rahah-'Uwayrid.
The Global Volcanism Program has no Bulletin Reports available for Harrat ar Rahah-'Uwayrid.
The Global Volcanism Program has no Weekly Reports available for Harrat ar Rahah-'Uwayrid.
The Global Volcanism Program has no Bulletin Reports available for Harrat ar Rahah-'Uwayrid.
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There is data available for 0 confirmed eruptive period.
[ 0640 (?) ] Uncertain Eruption
| Episode 1 | Eruption (Explosive / Effusive) | Hala-'l-Bedr, Hala-'l-'Ishqua or both | ||||||||||||||||||||||||||||||||||||||
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| 0640 (?) - Unknown | Evidence from Correlation: Anthropology | ||||||||||||||||||||||||||||||||||||||
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List of 6 Events for Episode 1 at Hala-'l-Bedr, Hala-'l-'Ishqua or both
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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 |
| Harrat al 'Uwayrid
Harrat el-'Uweirizh Harrat el-'Awayridh Harrat en-Nar |
Volcanic field | 1600 m | 27° 0' 0.00" N | 37° 33' 0.00" E |
| Harrat ar Rahah
Harrat er-Raha |
Volcanic field | 1700 m | 27° 40' 0.00" N | 36° 45' 0.00" E |
The large dark wedge-shaped area near the center of this Space Shuttle image is Harrat 'Uwayrid, a major volcanic field in NW Saudi Arabia that contains basaltic scoria and tuff cones. Bedouin legends say that Hala-'l-Bedr erupted fire and stones in 640 CE, killing herdsmen and their cattle and sheep. Another volcanic field, Harrat ar Rahah (top-left), lies to the NW.
The darker-colored area extending diagonally down the center of this Space Shuttle image is Harrat ar Rahah, the northernmost of a series of Quaternary volcanic fields paralleling the Red Sea coast of Saudi Arabia. The geometrical outlines of the historical town of Tabuk (top center), located on the road leading from Hijr to Damascus, can be seen to the N. There are fewer young volcanoes in Harrat ar Rahah than in other harrats (lava fields) to the S.
Harrat ar Rahah-'Uwayrid is the northernmost of a series of Quaternary volcanic fields paralleling the Red Sea coast of Saudi Arabia, south of the city of Tabuk. The olivine basaltic field extends NW-SE about 240 km overall, and contains numerous scoria cones, tuff cones, and associated lava fields.There are no samples for Harrat ar Rahah-'Uwayrid 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. |
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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. |
| 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 Harrat ar Rahah-'Uwayrid. 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 Harrat ar Rahah-'Uwayrid | 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). |
