|
Volcanic Hazards Ash flows are dense masses of gas and tiny fragments of lava that flow down the sides of volcanoes at great speeds. Much less well known (and understood) than lava flows or explosive blasts, ash flows are a combination of a blast cloud and a lava flow. They form when gas-saturated lava comes near the surface of the Earth and the pressure in the lava becomes low enough to allow the dissolved gas to form bubbles. If the bubbles form fast enough, the lava breaks into tiny fragments of liquid rock (called ash) that are carried out of the surface vent with the gas. If the ratio of gas to fragments is large (lots of gas), the ash is carried by the gas into blast clouds that can reach the upper atmosphere. If the ratio of gas to ash is small (lots of fragments), the ash can drag the gas downward into red-hot flows. These red-hot flows are partially controlled by gravity, and since the gas makes the friction between the ash particles very small, they can flow very far (up to hundreds of miles), very fast (over 100 mph). The relatively small red-hot ash flows that have been seen by geologists are called glowing avalanches because of their similarities to snow avalanches. Photo: Courtesy of NGDC/NOAA Ash flows ultimately stop because the gas finally escapes from between the particles. Glowing avalanches usually leave thin deposits of loose fragments like sand mixed with gravel. The ash fragments are hot, however, and deposits of ash have been found that are so thick that the hot particles actually fused together to form solid masses of rock after they stopped flowing. Geologists have never actually watched the formation of such a deposit, but the amount of ash in these deposits is so large that it requires ash flows hundreds of times larger than the glowing avalanches that have been seen. The destructive power in ash flows is a result of both the high flow speed and the high temperatures of the gas and fragmented rock. Even relatively small ash flows can be incredibly destructive: A glowing avalanche destroyed the town of St. Pierre in less than 30 seconds. The force of the flow literally ripped buildings apart all over town; only the sturdiest of stone walls were left standing. All but two of the 30,000 inhabitants of St. Pierre were asphyxiated or burned to death by the dense, superhot cloud. Ash flows occur in explosive eruptions and have been a significant problem with eruptions in Japan and the American Cascades. Photo: Courtesy of NGDC/NOAA Ash falls are less devastating than ash flows but can be very disruptive to modern life. Ash falls are the blanketing deposits dropped downwind by the clouds of ash thrown into the atmosphere by explosive volcanoes. These deposits may be a thin dusting or a thick layer of grit. They appear grayish to whitish and look like fallen snow, but, unlike snow, ash deposits do not melt and must be physically removed. The ash is heavy and can collapse roofs, break branches, and coat the leaves of plants. Unless the plants are cleaned (manually or by rain), they can die. This is a significant problem for crops. The ash is particularly hard on machines. Some ash particles are so small that they can pass through the engine's air filters and ruin the engine. This image shows the ash layer on cars near Mount Pinatubo. Photo: USGS EROS Data Center Rock/Debris avalanches are masses of cold, dry rock that have broken free from the sides of a volcano. They are driven downslope by gravity, smashing everything in their path by the force of their motion and then burying what remains under a mass of rock and debris. A good example of a rock avalanche triggered by an eruption is the mass of rock that broke off the north face of Mount St. Helens and buried the valleys to the north. However, an eruption is not needed to trigger a rock avalanche. Simple undermining of a mass of rock or an earthquake unrelated to an eruption can start a rock avalanche. Of course, such rock avalanches can occur on any steep mountain slope, but volcanoes are particularly prone to rock avalanches because their sides consist of outward-sloping layers of solid and fragmental rock (it is easier to slide down a sloping tabletop than across the ends of a bunch of stacked tables), and volcanic rock is easily changed by water into slippery clay, which promotes failure and sliding.
[ Volcanoes & Climate ] [ Monitoring Volcanoes ] [ Home ] [ Teacher Pages ] [ Modules & Activities ] |
HTML code by Chris Kreger
Maintained by ETE Team
Last updated September 29, 2010
Discuss Exploring the Environment!
Some images © 2004 www.clipart.com.
Privacy Statement and Copyright © 1997-2004 by Wheeling Jesuit University/NASA-supported Classroom of the Future. All rights reserved.
Center for Educational Technologies, Circuit Board/Apple graphic logo, and COTF Classroom of the Future logo are registered trademarks of Wheeling Jesuit University.