Global Volcanism Program

The Global Volcanism Program has no activity reports for Halla.

The Global Volcanism Program has no Weekly Reports available for Halla.

The Global Volcanism Program has no Bulletin Reports available for Halla.

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.

Synonyms

Cheju-do | Jeju

Cones

Feature Name

Feature Type

Elevation

Latitude

Longitude

Dangsanbong

Tuff cone

148 m

Dansan

Tuff cone

Guduack

Cone

Huckack

Cone

Ilchulbong

Tuff cone

180 m

Jueockack

Cone

Sangumburi

Cone

308 m

33° 26' 0" N

126° 42' 0" E

Soengpanack

Vent

Songaksan

Tuff ring

104 m

33° 12' 0" N

126° 22' 30" E

Suwolbong

Tuff ring

78 m

33° 17' 0" N

126° 10' 0" E

Udo

Tuff cone

132 m

Yongmeori

Tuff ring

33° 14' 0" N

126° 19' 0" E

Craters

Feature Name

Feature Type

Elevation

Latitude

Longitude

Backlockdam

Crater

Domes

Feature Name

Feature Type

Elevation

Latitude

Longitude

Hodo

Dome

Rimdo

Dome

Sanbangsan

Dome

395 m

33° 14' 0" N

126° 19' 0" E

Basic Data

Volcano Number

Last Known Eruption

Elevation

Latitude
Longitude

306040

1007 CE

1919 m / 6296 ft

33.361°N
126.53°E

Volcano Types

Shield
Pyroclastic cone(s)
Lava dome(s)

Rock Types

Major
Basalt / Picro-Basalt
Trachybasalt / Tephrite Basanite
Trachyandesite / Basaltic Trachyandesite

Minor
Trachyte / Trachydacite

Tectonic Setting

Intraplate
Continental crust (> 25 km)

Population

Within 5 km
Within 10 km
Within 30 km
Within 100 km

134
2,653
482,766
543,082

Geological Summary

The massive Halla shield volcano forms much of the 40 x 80 km Cheju (Jeju) Island, which lies 90 km S of the Korean Peninsula. Eruptions during the Pliocene and Pleistocene built a lava plateau above the roughly 100-m-deep continental shelf on which the basaltic-to-trachytic edifice was constructed. A 400-m-wide crater truncates the summit. About 360 late-Pleistocene and Holocene basaltic parasitic cones dotting the flanks of the low-angle volcano were erupted primarily along the long axis of the ENE-WSW-trending island. Most of these are scoria cones, but about 20 along the coast of the island or offshore are Pleistocene-to-Holocene tuff rings and tuff cones; lava domes also occur. Flank eruptions continued into historical time, with the final two taking place during the 11th century.

This volcano is located within the Jeju Island, a UNESCO Global Geopark property.

References

The following references have all been used during the compilation of data for this volcano, it is not a comprehensive bibliography.

Chough S K, Sohn Y K, 1990. Depostional mechanics and sequences of base surges, Songaksan tuff ring, Cheju Island, Korea. Sedimentology, 37: 1115-1135.

IAVCEI, 1973-80. Post-Miocene Volcanoes of the World. IAVCEI Data Sheets, Rome: Internatl Assoc Volc Chemistry Earth's Interior.

Lee M W, 1982. Petrology and geochemistry of Jeju volcanic island, Korea. Sci Rpt Tohoku Univ, Ser 3, 15: 177-256.

Sohn Y K, 1996. Hydrovolcanic processes forming basaltic tuff rings and cones on Cheju Island, Korea. Geol Soc Amer Bull, 108: 1199-1211.

Sohn Y K, Chough S K, 1989. Depositional processes of the Suwolbong tuff ring, Cheju Island (Korea). Sedimentology, 36: 837-855.

Sohn Y K, Park J B, Khim B K, Park K H, Koh G W , 2003. Stratigraphy, petrochemistry and Quaternary depositional record of the Songaksan tuff ring, Jeju Island, Korea. J. Volcanol. Geotherm. Res., 119: 1-20.

Sohn Y K, Park K H, 2005. Composite tuff ring/cone complexes in Jeju Island, Korea: possible consequences of substrate collapse and vent migration. J. Volcanol. Geotherm. Res., 141: 157-175.

Tomita T, 1969. Volcanic geology of the Cenozoic alkaline petrographic province of eastern Asia. In: Ogura T (ed) Geology and Mineral Resources of the Far East, Tokyo: Univ Tokyo Press, p 139-179.

Eruptive History

There is data available for 4 confirmed Holocene eruptive periods.

1007 Confirmed Eruption

Episode 1 | Eruption Episode

1007 - Unknown

Evidence from Observations: Reported

List of 2 Events for Episode 1

	Start Date	End Date	Event Type	Event Remarks
	- - - -	- - - -	Explosion
	- - - -	- - - -	Cinder Cone

1002 Confirmed Eruption

Episode 1 | Eruption Episode

1002 - Unknown

Evidence from Observations: Reported

List of 2 Events for Episode 1

	Start Date	End Date	Event Type	Event Remarks
	- - - -	- - - -	Explosion
	- - - -	- - - -	Cinder Cone

2050 BCE ± 200 years Confirmed Eruption

Episode 1 | Eruption Episode

SW flank (Songaksan tuff ring)

2050 BCE ± 200 years - Unknown

Evidence from Isotopic: 14C (uncalibrated)

List of 7 Events for Episode 1 at SW flank (Songaksan tuff ring)

Start Date	End Date	Event Type
- - - -	- - - -	Explosion
- - - -	- - - -	Pyroclastic flow
- - - -	- - - -	Lava flow
- - - -	- - - -	Ash
- - - -	- - - -	Lapilli
- - - -	- - - -	Blocks
- - - -	- - - -	Scoria

2830 BCE ± 50 years Confirmed Eruption

Episode 1 | Eruption Episode

NE flank (Ilchulbong tuff cone)

2830 BCE ± 50 years - Unknown

Evidence from Isotopic: 14C (uncalibrated)

List of 5 Events for Episode 1 at NE flank (Ilchulbong tuff cone)

Start Date	End Date	Event Type
- - - -	- - - -	Explosion
- - - -	- - - -	Pyroclastic flow
- - - -	- - - -	Ash
- - - -	- - - -	Lapilli
- - - -	- - - -	Blocks

Deformation History

There is no Deformation History data available for Halla.

Emission History

There is no Emissions History data available for Halla.

Photo Gallery

A cluster of scoria cones on the SW rift of Halla shield volcano is part of more than 360 flank cones that were erupted during the third and last stage of activity. Most of the cones were built along the SW-NE-trending rift zone that forms the axis of the island. The basaltic scoria cones are typically 150-200 m in height and are relatively uneroded.

Photo by Norm Banks, 1980 (U.S. Geological Survey).

A waterfall plunging over a trachytic lava flow is a popular tourist destination on Cheju Island. An extensive lava plateau underlies the Halla shield volcano and extends to the coast of the 40 x 80 km island. The volcano dominates the center of the island and has been active from the Pleistocene until historical time.

Photo by Norm Banks, 1980 (U.S. Geological Survey).

The massive Halla shield volcano, seen here from the south, forms much of the 40 x 80 km Cheju Island, which lies 90 km S of the Korean Peninsula. More than 360 late-Pleistocene and Holocene basaltic cones on the flanks of the low-angle volcano were erupted primarily along the long axis of the NE-SW-trending island. Most of these are scoria cones, but about 10 along the coast are Pleistocene tuff rings and tuff cones. Flank eruptions continued into historical time, with the final two taking place during the 11th century.

Photo by Norm Banks, 1980 (U.S. Geological Survey).

Prominent columnar jointing is visible on the steep sides of a trachytic lava dome on the southern coast of Cheju Island. A cluster of trachytic lava domes were erupted near the end of the second stage of activity of Halla, during which the shield volcano was formed in the center of the island.

Photo by Norm Banks, 1980 (U.S. Geological Survey).

Snow-capped Halla shield volcano is seen here from the north, near Cheju city, the largest on Cheju Island. Voluminous lava flows and an underlying lava plateau form the entire 40 x 80 km island. The volcano is capped by the 400-m-wide Backlockdam summit crater and its flanks contain hundreds of cones, some of which form small offshore islands.

Photo by Norm Banks, 1980 (U.S. Geological Survey).

GVP Map Holdings

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.

Smithsonian Sample Collections Database

There are no samples for Halla in the Smithsonian's NMNH Department of Mineral Sciences Rock and Ore collection.

External Sites

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.

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.

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.

Volcanic Hazard Maps

The IAVCEI Commission on Volcanic Hazards and Risk has a Volcanic Hazard Maps database designed to serve as a resource for hazard mappers (or other interested parties) to explore how common issues in hazard map development have been addressed at different volcanoes, in different countries, for different hazards, and for different intended audiences. In addition to the comprehensive, searchable Volcanic Hazard Maps Database, this website contains information about diversity of volcanic hazard maps, illustrated using examples from the database. This site is for educational purposes related to volcanic hazard maps. Hazard maps found on this website should not be used for emergency purposes. For the most recent, official hazard map for a particular volcano, please seek out the proper institutional authorities on the matter.

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 Halla. 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 Halla. 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.

Large Eruptions of Halla

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).