Pyroclastic flow

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Pyroclastic flows sweep down the flanks of Mayon Volcano, Philippines, in 1984
Rocks from the Bishop tuff, uncompressed with pumice (on left); compressed with fiamme (on right).

A pyroclastic flow (also known scientifically as a pyroclastic density current[1]) is a fast-moving current of hot gas and rock (collectively known as tephra), which reaches speeds moving away from a volcano of up to 700 km/h (450 mph).[2] The gas can reach temperatures of about 1,000 °C (1,830 °F). Pyroclastic flows normally hug the ground and travel downhill, or spread laterally under gravity. Their speed depends upon the density of the current, the volcanic output rate, and the gradient of the slope. They are a common and devastating result of certain explosive volcanic eruptions.

Origin of term[edit]

The word pyroclast is derived from the Greek πῦρ, meaning "fire", and κλαστός, meaning "broken in pieces". A name for some pyroclastic flows is nuée ardente (French for "burning cloud"); this was first used to describe the disastrous 1902 eruption of Mount Pelée on Martinique.[3] In the dark, these pyroclastic flows glowed red.

Pyroclastic flows that contain a much higher proportion of gas to rock are known as "fully dilute pyroclastic density currents" or pyroclastic surges. The lower density sometimes allows them to flow over higher topographic features such as ridges and hills. They may also contain steam, water and rock at less than 250 °C (482 °F); these are called "cold" compared with other flows, although the temperature is still lethally high. Cold pyroclastic surges can occur when the eruption is from a vent under a shallow lake or the sea. Fronts of some pyroclastic density currents are fully dilute; for example, during the eruption of Mount Pelée in 1902 a fully dilute current overwhelmed the city of Saint-Pierre and killed nearly 30,000 people.[4]

A pyroclastic flow is a type of gravity current; in scientific literature they are sometimes abbreviated to PDC (pyroclastic density current).

Causes[edit]

There are several factors which can produce a pyroclastic flow:

Size and effects[edit]

A scientist examines pumice blocks at the edge of a pyroclastic flow deposit from Mount St. Helens

The volumes range from a few hundred cubic meters to more than a thousand cubic kilometres. The larger ones can travel for hundreds of kilometres, although none on that scale have occurred for several hundred thousand years. Most pyroclastic flows are around one to ten cubic kilometres and travel for several kilometres. Flows usually consist of two parts: the basal flow hugs the ground and contains larger, coarse boulders and rock fragments, while an extremely hot ash plume lofts above it because of the turbulence between the flow and the overlying air, admixes and heats cold atmospheric air causing expansion and convection.[5]

The kinetic energy of the moving boulders will flatten trees and buildings in their path. The hot gases and high speed make them particularly lethal, as they will incinerate living organisms instantaneously:

Interaction with water[edit]

Testimonial evidence from the 1883 eruption of Krakatoa, supported by experimental evidence,[8] shows that pyroclastic flows can cross significant bodies of water. One flow reached the Sumatran coast as much as 48 km (30 mi) away.[9]

A 2006 documentary film, Ten Things You Didn't Know About Volcanoes,[10] demonstrated tests by a research team at Kiel University, Germany, of pyroclastic flows moving over water.[11] When the reconstructed pyroclastic flow (stream of mostly hot ash with varying densities) hit the water two things happened: The heavier material fell into the water, precipitating out from the pyroclastic flow and into the liquid; The temperature of the ash caused the water to evaporate, propelling the pyroclastic flow (now only consisting of the lighter material) along at an even faster pace than before on a bed of steam.

During some phases of the Soufriere Hills volcano on Montserrat, pyroclastic flows were filmed about 1 km offshore. These show the water boiling as the flow passed over it. The flows eventually built a delta which covered about 1 km2.

A pyroclastic flow can interact with a body of water to form a large amount of mud, which can then continue to flow downhill as a lahar. This is one of several mechanisms that can create a lahar.

On the Moon[edit]

In 1963, NASA astronomer Winifred Cameron proposed that sinuous rilles on the Moon may have been formed by the lunar equivalent of terrestrial pyroclastic flows. In a lunar volcanic eruption, a pyroclastic cloud would follow local relief resulting in an often sinuous track. The Moon's Schroter's Valley is one example.[12]

See also[edit]

References[edit]

  1. ^ Branney M.J. & Kokelaar, B.P. 2002, Pyroclastic Density Currents and the Sedimentation of Ignimbrites. Geological Society London Memoir 27, 143pp.
  2. ^ Pyroclastic flows USGS
  3. ^ Lacroix, A. (1904) La Montagne Pelée et ses Eruptions, Paris, Masson (in French)
  4. ^ Arthur N. Strahler (1972), Planet Earth: its physical systems through geological time
  5. ^ Myers, and Brantley (1995). Volcano Hazards Fact Sheet: Hazardous Phenomena at Volcanoes, USGS Open File Report 95-231
  6. ^ Weller, Roger. Mount Vesuvius, Italy. Cochise College Department of Geology, 2005. Web. 15 October 2010. <http://skywalker.cochise.edu/wellerr/students/mount-vesuvius2/vesuvius.htm>.
  7. ^ Sutherland, Lin. Reader’s Digest Pathfinders Earthquakes and Volcanoes. New York: Weldon Owen Publishing, 2000.
  8. ^ Freundt, Armin (2003). "Entrance of hot pyroclastic flows into the sea: experimental observations". Bulletin of Volcanology 65: 144–164. Bibcode:2002BVol...65..144F. doi:10.1007/s00445-002-0250-1. 
  9. ^ Camp, Vic. "KRAKATAU, INDONESIA (1883)." How Volcanoes Work. Department of Geological Sciences, San Diego State University, 31 Mar. 2006. Web. 15 Oct. 2010. [1].
  10. ^ Ten Things You Didn't Know About Volcanoes (2006) at the Internet Movie Database
  11. ^ Entrance of hot pyroclastic flows into the sea: experimental observations, INIST.
  12. ^ Cameron, W. S. (1964), An Interpretation of Schröter's Valley and Other Lunar Sinuous Rills, J. Geophys. Res., 69(12), 2423–2430, doi:10.1029/JZ069i012p02423.

External links[edit]