USGS/CVO Logo, click to link to National USGS Website
USGS/Cascades Volcano Observatory, Vancouver, Washington

Volcanic Studies at the U.S. Geological Survey's
David A. Johnston Cascades Volcano Observatory,
Vancouver, Washington


-- Steven R. Brantley and Lyn Topinka, 1984,
Volcanic Studies at the U.S. Geological Survey's David A. Johnston Cascades Volcano Observatory, Vancouver, Washington: Earthquake Information Bulletin, March-April 1984, v.16, no.2
Mount St. Helens volcano in southwest Washington transformed one of the most scenic alpine landscapes of the Cascade Range into a gray, barren wasteland in only a few minutes. A catastrophic landslide and explosive eruption on May 18, 1980, devastated 550 square kilometers of forest, sent damaging mudflows down rivers draining the volcano, and produced ash fallout hundreds of kilometers to the east. Four years after the volcano's reawakening, Mount St. Helens remains active, and the devastated landscape wrought by the May 18 eruption continues to pose flood hazards to communities downstream from the volcano.


Image, click to enlarge
MSH82_st_helens_spirit_lake_reflection_05-19-82.jpg
Mount St. Helens and the devastated area is now within the 110,000-acre Mount St. Helens National Volcanic Monument, under jurisdiction of the United States Forest Service. Visitor centers, interpretive areas, and trails are being established as thousands of tourists, students, and scientists visit the monument daily. Mount St. Helens is once again considered to be one of the most beautiful and interesting of the Cascade volcanic peaks.
USGS Photograph taken on May 19, 1982, by Lyn Topinka.
[medium size] ... [large size]


Sixteen subsequent eruptions have taken place in the horseshoe-shaped crater formed by the May 18 eruption. No large explosive event has occurred since October 1980. The last 11 eruptions have built a lava dome to a height of 240 meters by the slow intrusion of magma into its interior and the extrusion of lava onto its surface; the most recent eruption of Marcy 29, 1984, added a new stubby lava flow to the top of the dome.

U.S. Geological Survey scientists at the David A. Johnston Cascades Volcano Observatory (CVO) in Vancouver, Washington, are studying the intermittent eruptive activity of Mount St. helens and hazards posed by the effects of the May 18 eruption. Many different monitoring techniques and instruments are used to record the "daily pulse" of the volcano to evaluate the change of future eruptive activity and to investigate fundamental volcanic processes. Studies also are made of the river basins and the new lakes around the volcano and of the massive debris avalanche that slid off the mountain on May 18, 1980. These studies provide data to asses water-related hazards to downstream communities from increased sedimentation, erosion, and flooding along the Toutle and Cowlitz Rivers. Such hydrologic hazards likely will persist long after the decline of eruptive activity at Mount St. Helens.


Map, Cascade Range Volcanoes, click to enlarge [Image,16K,GIF]
Cascade volcanoes in the Pacific Northwest


CVO is supported by the Geological Survey's Volcano Hazards Program, which is responsible for providing warnings of volcanic eruptions and related hazards in the United States. Information and advice are given to Federal, State, and local officials concerning specific volcanic hazards and the implementation of emergency-response plans. Activities designed to inform people of volcanic hazards include research on volcanic processes, monitoring active and potentially hazardous volcanoes, and mapping the types and the extent of volcanic deposits of past eruptions.

The goal of the monitoring and research activities of CVO is to give timely warnings of eruptive and related hydrologic hazards at Mount St. Helens. Three types of written public statements about volcanic activity are issued by CVO to provide hazard information to the public and to governmental agencies:

  • A factual statement describes current conditions of the volcano but does not anticipate future events; such statements are revised when warranted by new developments.

  • A forecast is a comparatively nonspecific statement about volcanic activity to occur weeks to decades in advance. A forecast is based on projections of past eruptive activity or is used when monitoring data are not well understood. This kind of statement is particularly useful for land use planning and development of emergency response plans.

  • A prediction is a comparatively specific statement giving place, time, nature, and, ideally, size of an impending eruption. Correct predictions were made of all 14 eruptions at Mount St. Helens from June 1980 to the end of 1982.

Water-related hazard information is provided to the National Weather Service and other Federal, State, and local agencies involved in flood mitigation planning.



Eruptive Activity of Mount St. Helens: March 1980 - March 1984

The present activity of Mount St. Helens began in March 1980. A magnitude 4.0 earthquake on March 20 was followed by 2 months of intense seismicity and phreatic "steam-blast" eruptions. These events accompanied the intrusion of viscous magma into the volcano, shoving the north flank outward more than 100 meters and creating the famous "bulge".

On May 18, a magnitude 5.1 earthquake shook loose the steepened north flank, resulting in the largest known landslide in historic time. Removal of 2.3 cubic kilometers of material released pressure on the hydrothermal and magmatic system within the volcano and triggered a devastating lateral blast to the north. Within minutes, an ash-laden eruptive column rose more than 20 kilometers above the volcano. Melting snow and ice formed mudflows and floods that raced down almost all the valleys draining the volcano. The largest and most destructive mudflow originated from water-saturated parts of the debris avalanche in the North Fork Toutle River Valley.


Image, click to enlarge
MSH80_st_helens_from_johnston_ridge_05-17-80.jpg
Mount St. Helens on May 17, 1980, one day before the devastating eruption. The view is from Johnston's Ridge, six miles (10 kilometers) northwest of the volcano.
USGS Photograph taken on May 17, 1980, by Harry Glicken.
[medium size] ... [large size]

Image, click to enlarge
MSH80_st_helens_from_johnston_ridge_09-10-80.jpg
Mount St. Helens soon after the May 18, 1980 eruption, as viewed from Johnston's Ridge.
USGS Photograph taken on September 10, 1980, by Harry Glicken.
[medium size] ... [large size]


Mount St. Helens erupted explosively five more times during 1980. None of these eruptions were as large as the events on May 18, but each eruption produced ash columns that rose 8 to 14 kilometers above sea level and hot, dry pyroclastic flows of pumice and ash that swept down the north flank as fast as 100 kilometers per hour. These pyroclastic flows deposited ash and pumice fragments in fanlike patterns of sheets, tongues, and lobes in an area extending up to 8 kilometers north of the vent. Individual pyroclastic flow units were generally less than 5 meters thick, and maximum temperatures recorded several hours after their deposition ranged from about 300 to 730 degrees C. The thickness of airfall deposits ranged from one-third to one-fortieth that of the May 18 airfall deposit at a given distance from the volcano.


Image, click to enlarge
MSH80_USGS_scientist_toe_pyroclastic_flow_10-17-80.jpg
U.S. Geological Survey scientist Pete Rowley examines pumice blocks at the toe of a pyroclastic flow.
USGS Photograph taken on October 17, 1980, by Terry Leighley, Scandia Labs.
[medium size] ... [large size]


Lava extruded from the vent and formed lava domes within a few days after the June 12, August 7, and mid-October explosive eruptions. The June and August domes were blown away by subsequent explosive eruptions, but the October dome survived to form the core of the still-growing dome. Domes are formed by thick, pasty masses of lava too sticky to flow very far from the vent. Lava of the Mount St. helens dome is dacite that contains a higher percentage of silica than the Hawaiian basalts and is about 1 million times more viscous.


Image, click to enlarge
MSH80_october_dome_10-24-80.jpg
A new dome started growing on October 18,1980. This October dome was 112 feet (34 meters) high and 985 feet (300 meters) wide, making it taller than a nine-story building and wider than the length of three football fields. This aerial view is from the north. This dome was not the first dome to grow in the crater. In June and August 1980, two domes formed, ony to be blasted away by the explosive events of July 22 and October 16.
USGS Photograph taken on October 24, 1980, by Terry Leighley, Scandia Labs.
[medium size] ... [large size]

Image, click to enlarge
MSH83_USGS_scientists_on_south_side_of_dome_05-26-83.jpg
Two U.S. Geological Survey geologists (one in orange, middle right, near base of dome) are dwarfed by the dome. The geologists stand on snow muddied from recent ashfall. By 1987, the dome had replaced only three percent of the volume removed by the May 18, 1980 eruption. If that rate of growth had continued it would have taken over 200 years to rebuild Mount St. Helens to its pre-1980 size. Instead, Mount St. Helens entered a quiet period which continued until 2004.
USGS Photograph taken on May 26, 1983, by Lyn Topinka.
[medium size] ... [large size]


The 11 eruptions since October 1980 have been dominantly nonexplosive events that have built a composite lava dome 750 x 675 x 240 meters high in the crater. Each eruption added a stubby lava flow to the dome. The lava flows commonly are extruded near the top of the dome, and over a period of several days, creep 1 to 5 meters per hour down one side; usually a few million cubic meters of new lava is added to the dome during one of these episodes. The dome-building eruptions in 1981 and 1982 were episodic and occurred every 1 to 5 months. Beginning in February 1982, the dome grew continuously by intrusion of magma into it and the extrusion of lava onto its surface; the most recent lava extrusion occurred in late March 1984. At the current rate of dome growth, about 1 million cubic meters per month, it would take 150 to 200 years to build Mount St. Helens to its former height, but it is unlikely that such a scenario will occur.


Graphic, click to enlarge [Graphic,22K,GIF]
The diagrams are profile views of dome growth at Mount St. Helens sketched from photographs taken at a photo station approximately 1.0 kilometers north of the dome. The small diagrams represent total increase in dome profile between 1980 and 1983. The large diagram represents the increase in the profile after each dome-building eruption. During 1983, the dome was in a "continuous growth" phase. The 1983 profile increase was sketched from an October photograph, although the dome did continue to grow.
-- Lyn Topinka, 1997, Modified from Swanson, et.al., 1987



Small explosions sometimes precede or accompany the dome-building eruptions at Mount St. Helens; if they occur when snow mantles the crater floor, then they can produce mudflows (lahars) and snow avalanches. The explosive onset of the March 19, 1982, eruption hurled hot pumice and dome rocks against the 640-meter-high south crater wall, dislodging snow and rock that avalanched through the crater and down the north flank of the volcano. Deep snow in the crater melted quickly from the volcanic heat, forming a small lake from which a destructive flood swept down the north flank and into the North Fork Toutle River. About a day later, new lava erupted on the southeast flank of the dome.


Image, click to enlarge
MSH82_lahar_from_march_82_eruption_03-21-82.jpg
Mount St. Helens erupted often between 1980 and 1986. An explosive eruption on March 19, 1982, sent pumice and ash 9 miles (14 kilometers) into the air, and resulted in a lahar (the dark deposit on the snow) flowing from the crater into the North Fork Toutle River valley. Part of the lahar entered Spirit Lake (lower left corner) but most of the flow went west down the Toutle River, eventually reaching the Cowlitz River, 50 miles (80 kilometers) downstream.
USGS Photograph taken on March 21, 1982, by Tom Casadevall.
[medium size] ... [large size]


In addition to the dome-building eruptions, vigorous emissions of gas and tephra have occurred from fractures and small craters on top of the dome since late 1980. These periodic outbursts usually last several minutes, occasionally sending ash plumes as high as 5 to 6 kilometers above the volcano. Most of the tephra consists of fragmented pieces of dome rock, not new liquid magma, in contrast to the more hazardous magmatic explosions of 1980.


Image, click to enlarge
MSH82_st_helens_plume_from_harrys_ridge_05-19-82.jpg
Plumes of steam, gas, and ash often occured at Mount St. Helens in the early 1980s. On clear days they could be seen from Portland, Oregon, 50 miles (81 kilometers) to the south. The plume photographed here rose nearly 3,000 feet (1,000 meters) above the volcano's rim. The view is from Harrys Ridge, five miles (8 kilometers) north of the mountain.
USGS Photograph taken on May 19, 1982, by Lyn Topinka.
[medium size] ... [large size]


The eruptive activity of Mount St. Helens presents unique opportunities for geologists to observe the formation of different types of volcanic deposits. Geologists typically study rocks and deposits that are thousands to millions of years old. By observing eruptive activity that occurs in the present, geologists are better able to recognize deposits preserved in the historic record. For example, a large hummocky deposit at the base of Mount Shasta Volcano in northern California has characteristics similar to those of the 1980 debris avalanche deposit at Mount St. Helens. Based on detailed studies of the Mount St. Helens debris avalanche, geologists now can infer with greater confidence that a large landslide also produced the deposit near Mount Shasta. Stratigraphic studies at Mount St. Helens include studies of the debris avalanche, the lateral blast, mudflows, pumiceous pyroclastic flows, airfall tephra, and lava domes.



Monitoring Activities at Mount St. Helens and Other Cascade Volcanoes

The continuing eruptions of Mount St. Helens provide an unusual opportunity for scientists to study volcanic activity and to devise and test methods for predicting eruptions. Many successful predictions have been issued for eruptions since June 1980. Eruption prediction and information about volcanic activity at Mount St. Helens provide the basis for hazard warnings of eruptive activity to the public and to local governments.

Volcano monitoring involves a variety of measurements and observations designed to detect changes at the surface of a volcano that reflect increasing pressure and stresses caused by the movement of magma, or molten rock, within or beneath it. An eruption occurs when magma rises from its source or from a storage reservoir and finally reaches the Earth's surface. As it rises, the magma fractures overlying rocks, which causes earthquakes, and parts of the volcano deform as magma approaching the surface makes room for itself.

Monitoring at Mount St. Helens chiefly involves the measurement of surface deformation, the investigation of earthquakes generated beneath the volcano, and the study of changes in gas emission rates accompanying the underground movement of magma. Additional geophysical and geochemical information is gathered through sampling of newly erupted lava and tephra, studies of thermal patterns on the dome, surveys of local electrical and magnetic fields, measurements of changes in the Earth's gravity field, examination of photographs, and measurements of temperature at fumaroles.

Many of the methods used to monitor Mount St. Helens were developed at the U.S. Geological Survey's Hawaiian Volcano Observatory where the activity of Kilauea and Mauna Loa shield volcanoes is monitored. Although the techniques are similar, their application and interpretation have been modified and adapted to Mount St. Helens and other stratovolcanoes of the Cascade Range.


Graphic, click to enlarge [Graphic,18K,GIF]
Monitoring sites at Mount St. Helens as of March 1982.
-- Modified from: E. Iwatsubo, 1996, and Brantley and Topinka, 1984



Seismic Studies

Seismic signals from 5 seismometers on the flanks of Mount St. Helens, one in the crater, and 10 others within 40 kilometers of the volcano are radioed to the Geophysics Laboratory at the University of Washington. Signals from several of these stations are also radioed to and recorded at the Cascades Volcano Observatory. This detailed seismic network enables seismologists to distinguish between different types of volcanic earthquakes and surface events. Although the seismic precursors to the May 18, 1980, eruption did not specify the time of its onset, seismologists have learned to recognize certain characteristic patterns of seismic activity that precede and accompany the subsequent eruptions. By plotting the cumulative seismic strain energy release of various types of seismic disturbances versus time, eruptions have been predicted from a few hours to several days in advance.


Image, click to enlarge
MSH81_installing_seismic_station_base_dome_08-04-81.jpg
Geologists install a seismic station near the dome. The U.S. Geological Survey, in conjunction with the University of Washington, maintained seismic stations at Mount St. Helens. An increase in seismicity (earthquakes) was often the first precursor to an approaching eruption.
USGS Photograph taken on August 4, 1981, by Gene Iwatsubo.
[medium size] ... [large size]


Earthquake data from the Mount St. Helens seismic network are stored on computer files at the University of Washington in Seattle. Seismologists review and classify the seismograms, or "seismic signatures," from several local stations each day; during periods of high earthquake activity, seismologists monitor the records 24 hours a day.

The following major types of seismograms have been recognized at Mount St. Helens: (1) deep earthquakes and those located away from the volcano, which produce high-frequency signatures and sharp arrivals similar to tectonic earthquakes, (2) shallow earthquakes, located under the dome at depths of less than 3 kilometers, which produce medium-to-low-frequency seismic arrivals, (3) surface events, such as gas and tephra events, rockfalls associated with dome growth, and snow and rock avalanches from the crater walls, which produce complicated signatures with no clear beginning or end, and (4) harmonic tremor, which is a long-lasting, very rhythmic signal whose origin is not well understood but which is often associated with active volcanoes.

The rate of activity of the various categories of seismic events is used to assist in predicting volcanic activity at Mount St. Helens. An increasing number of shallow volcanic earthquakes were observed several days to 2 weeks before each dome-building eruption from 1980 through 1982. As the number of earthquakes increase, total seismic energy release is calculated and plotted against time. The observation of a sudden upward turn in this smoothly accelerating curve a few hours before the eruption begins is the basis for relatively short-term predictions. Once the eruption is underway, shallow volcanic earthquakes cease, and surface events from rockfalls dominate the records.


Graphic, click to enlarge [Graphic,20K,GIF]
Four major types of seismograms, or "seismic signatures," are recognized from seismometers in the vicinity of Mount St. Helens. Seismologists review and classify the seismic records daily.


Increased seismic activity also preceded the post-May 18 explosive eruptions of 1980. Each of the seismic precursors were of a slightly different character, but two categories were recognized: shallow volcanic earthquake precursors and harmonic tremor precursors. Harmonic tremor is a nearly continuous train of vibrations lasting from a few minutes to several hours. An increase in shallow earthquakes preceded the July and October 1980 eruptions when a lava dome was present in the crater. Harmonic tremor preceded the May 25, June 12, and August 7, 1980 eruptions when the vent was open and no dome existed. Having learned from the seismic buildup preceding the May 25, explosive eruption, seismologists were able to issue warnings of the subsequent explosive events by at least 2 hours.

Although a characteristic pattern of seismic activity has accompanied most eruptions, there have been departures from the pattern. The explosive eruptions of 1980 were followed by swarms of deep earthquakes (deeper than 5 kilometers). In contrast, none of the subsequent dome-building eruptions were followed by deep earthquakes that could be related to the eruptions. The March 19, 1982, dome-building eruption began with an explosion and was preceded rather than followed by both deep and shallow earthquakes. The continuous dome-growth eruption that began in early February 1983 was preceded by an unusually small increase in shallow earthquake activity. Earthquakes and surface events occurred daily reflecting the continuous dome-growth activity in 1983.

Deformation Studies

Shortly after the May 18, 1980, eruption, geologists reestablished a surveying network on the volcano to measure changes that might signal additional eruptive activity. Glass prisms atop heavy steel towers on the volcano's upper flanks were surveyed with an electronic distance meter (EDM) and theodolite from instrument towers placed at the base of the volcano. Frequent measurements showed small movements during the summer of 1980, some of which may have indicated swelling before the explosive eruptions. No Systematic deformation of the outer flanks of the volcano has been detected since 1980.


Image, click to enlarge
MSH89_outerflanks_monitoring_station_05-15-89.jpg
In addition to monitoring stations within Mount St. Helens' crater, the U.S. Geological Survey also maintained a network of monitoring stations around the base of the volcano. Angle and distance measurements to the volcano's flanks were taken periodically to watch for any deformation similar to the 1980 bulge. Pictured here is an instrument station northeast of the volcano.
USGS Photograph taken in May 15, 1989, by Lyn Topinka.
[medium size] ... [large size]


The largest changes measured in 1980 were inside the new crater near the eruptive vent. As a consequence of these observations, monitoring has been focused inside the crater since fall 1980. Geologists visit the crater several times each week to measure deformation of the crater floor and the lava dome before eruptions. At the end of each field day, total measured displacements of ground cracks, thrust faults, and the dome are plotted against time. The observation of a gradual and then a rapid change in the curves a few days to several weeks before an eruption begins is the basis for relatively long-term predictions.

Ground-Crack Measurements

New ground cracks appeared on the crater floor from several days to 2 to 4 weeks before all the 1980 to 1982 eruptions. The cracks, commonly tens of meters long and tens of centimeters wide, extended outwards from the dome like spokes from the hub of a wheel. Incandescent rock was visible in some cracks, and temperatures of escaping gas were measured as high as 840 degrees C. Measured with a steel tape, the cracks commonly showed continual widening that accelerated before eruptions. Such accelerated movement was used to predict several eruptions in 1981 and 1982.


Image, click to enlarge
MSH81_USGS_scientists_measure_radial_crack_base_dome_05-12-81.jpg
The U.S. Geological Survey established both periodic and continuous 24-hour monitoring programs at Mount St. Helens to study and predict eruptions. In this slide, geologists used a steel tape to measure the distance across a crack on the crater floor. Widening of cracks was an indication that magma was rising and deforming the area, leading to an eruption. These cracks were generally radial to the dome, like spokes of a wheel.
USGS Photograph taken on May 12, 1981, by Lyn Topinka.
[medium size] ... [large size]


Thrust-Fault Measurements

From 1980 to 1982, parts of the crater floor became slightly wrinkled several weeks before eruptions. A few wrinkles developed into thrust faults, a low-angle fracture, along which rocks above the fracture are pushed over rocks below the fractures. By summer 1981, a complex system of thrust blocks had disrupted much of the southwestern part of the crater floor. The thrust faults formed as rising magma forcefully ruptured the crater floor, shoving parts of it upward and outward from the vent toward the rigid crater walls. Before the August 18, 1982, eruption, the leading edge of one thrust fault grew from less than 30 centimeters to roughly 5 meters high a few days before the eruption.

Movement along the faults was monitored by repeated measurements between benchmarks on either side of the fault by using a steel tape and by leveling between points on the upper and lower plates. The rate of movement accelerated before eruptions, and this provided the most consistent and reliable relatively long-term (1-3 weeks) predictive tool at Mount St. helens during 1981 and 1982. Rockfalls from the dome and crater walls have buried some major thrust faults under rock debris, others have been overridden by the dome itself; but new thrust faults occasionally appear, as in October 1983.

Tilt Measurements

In addition to cracking and faulting, the crater floor tilts before eruptions. Electronic tiltmeters, which are widely used in Hawaii, measure changes in slope or inclination of the ground surface. Tiltmeters specifically designed for use at Mount St. Helens have been installed on the crater floor tens to several hundred meters from the dome. Tilt data contributed to accurate predictions for eruptions during 1981 and 1982.

The tiltmeters, which employ two sensitive bubbles mounted at right angles on a 15-centimeter base plate, measure tilt of the crater floor in two directions. The direction of tilt is generally outward from the dome but is sometimes complicated by nearby cracks or faults. Amount of tilt is expressed in microradians, which is the angle turned by a 1-kilometer-long rod if one end is raised 1-millimeter. Although these tiltmeters are capable of measuring one-tenth of a microradian, precision is limited to 5 to 10 microradians in the crater because of surface thermal effects. Data from the crater tiltmeters are radioed directly to CVO in Vancouver and are stored in computer files. Tiltmeters provide the only realtime information about crater deformation and are, therefore, especially valuable when field work is impossible because of poor weather or hazardous volcanic activity.

Tilting of the crater floor began several weeks before each eruption in 1981 and 1982, accelerated a few days before, and, on several occasions, abruptly reversed direction minutes or hours before the eruption began; for example, tilt before the March 19, 1982, eruption at one station increased from about 14 microradians per day 3 weeks before the event to 360 microradians per day on March 19. The tilt reversed direction about 30 minutes before the eruption began.


Image, click to enlarge
MSH82_leveling_slope_changes_crater_floor_05-82.jpg
Geologists did precise leveling to measure changes in the slope of the crater floor, due to moving magma. Changes in slope was also measured electronically by tiltmeters. Tiltmeters allowed 24-hour monitoring as the information was telemetered back to CVO. Other instruments such as displacement meters for measuring cracks, seismometers for measuring earthquakes, gas sensors for measuring gas concentrations, and magnetometers for measuring the magnetic field, were also used for 24-hour monitoring. Spirit Lake is visible in the background in this image.
USGS Photograph taken in May 1982, by Holly Martinson.
[medium size] ... [large size]


Lava-Dome Measurements

Measurements show that the dome expands as magma moves up into it before eruptions. Repeated surveys using an electronic distance meter (EDM) and theodolite between points on the crater floor and targets placed on the dome reveal movements that speed up as the eruption nears. A target on the west side of the dome was moving roughly 2 centimeters per day 2 weeks before the May 14, 1982, eruption; these movements increased to about 200 centimeters per day by May 13. Such accelerations were frequently used to predict eruptions in 1982.

Generally, all sides of the dome were monitored in 1981 and 1982 from four to five stations on the crater floor. Experience has shown that the dome deforms differently at each of the stations, thus making it necessary to monitor more than one side for reliable predictions. During the winter months, one and sometimes two sides of the dome can be monitored; it is no longer possible to monitor the east sector of the dome because of hazardous rockfalls from the dome and the east crater wall. This technique has become essential fro predicting the most recent eruptions because most of the ground cracks and thrust faults have been buried by the dome and associated rockfall debris. This type of measurement also documents movements of the dome during prolonged eruptions, such as that of 1983, and is used to foretell significant changes in such continuous activity.


Image, click to enlarge
MSH84_USGS_scientists_survey_the_dome_05-26-84.jpg
U.S. Geological Survey geologists use a theodolite and EDM (Electronic Distance Meter) to measure angles and slope-distances to the lava dome. Changes in these angles and distances are used to calculate "deformation rates". An increase in deformation rates is an indication that magma is slowly entering the dome. In the early 1980s deformation rates often reached 30 feet per hour (10 meters/hour) as magma rose and the dome expanded before extrusion started. During the winter months, the instrument stations often had to be dug out of the snow before measurements could be made.
USGS Photograph taken on May 26, 1984, by Lyn Topinka.
[medium size] ... [large size]


Gas Emission Studies

Gas emissions are measured regularly in conjunction with seismicity and ground deformation to monitor eruptive activity. Mount St. Helens continuously emits volcanic gas from fumaroles on and around the dome. Most of the gas emitted by the volcano is water vapor, but emissions also include sulfur dioxide, carbon dioxide, hydrogen, and lesser amounts of helium, carbon monoxide, hydrogen sulfide, and hydrogen chloride.

Gas studies include (1) frequent airborne measurements of sulfur dioxide and, in 1980 and 1981, carbon dioxide in the plume and (2) less frequent sampling of gases from crater fumaroles. The emissions of sulfur dioxide are measured in the plume by a correlation spectrometer (COSPEC) designed originally for pollution studies. The instrument measures the amount of solar ultraviolet light absorbed by sulfur dioxide in the plume and compares it with an internal standard. Three to six traverses are made beneath the plume at right angles to the plume trajectory several times each week to calculate daily emission rates.


Image, click to enlarge
MSH81_collecting_gas_samples_base_dome_09-24-81.jpg
USGS geologists collect gas samples around the dome. Samples were gathered from vents on the dome and crater floor, and were used to monitor changes in chemical composition. Additionally, sulfur dioxide gas was measured from a specially-equipped airplane before, during, and after eruptions to determine "emission rates" for the volcano. During eruptions, emission rates typically increased to 5 to 10 times their pre-eruptive value.
USGS Photograph taken on September 24, 1981, by Thomas J. Casadevall.
[medium size] ... [large size]

Image, click to enlarge
MSH83_USGS_scientists_COSPEC_on_SugarBowl_10-21-83.jpg
USGS scientists use a COSPEC (correlation spectrometer), to measure sulfur-dioxide gases being emitted from the dome. Setup on Sugar Bowl, located on the northwest flank of Mount St. Helens.
USGS Photograph taken on October 21, 1983, by Lyn Topinka.
[medium size] ... [large size]


The emission rates of sulfur dioxide peaked during summer 1980 at about 1,500 tons per day, decreased rapidly in late 1980, and remained low at about 100 tons per day through 1983. Emission rates of carbon dioxide decreased rapidly in late 1980 until they were below the detection limit of 1,000 tons per day. These patterns correspond generally to a change in eruptive style from the explosive activity of 1980 to the now predominantly nonexplosive activity. The patterns suggest steady outgassing of a single batch of magma under the volcano to which no significant new magma has been added since mid-1980.

Increased rates of sulfur dioxide emissions measured before several nonexplosive eruptions are interpreted as the result of accelerated degassing of a small volume of magma as it moved toward the surface. During the nonexplosive eruptions, gas emissions remained elevated during the active extrusion of lava and generally dropped to preeruption levels once extrusion stopped. The occasional outbursts of gas and tephra are accompanied by brief, sudden increases in the emission rate of sulfur dioxide, water vapor, and probably other gases as well. It is not known whether this increase in gas is derived directly from magma within the dome or released during periodic, geyserlike flashing of a shallow hydrothermal system.

Dome Composition

Since October 1980, each eruption has added a new flow of viscous dacitic lava to the dome. Chemical and mineralogic analyses of dome samples show that lava composition throughout successive eruptions has remained nearly constant. This suggests that the magma feeding the eruptions has not undergone any significant changes and is consistent with the model of a single, shallow magma reservoir supplying the eruptions. Whether the chemical composition of future extrusions remain the same or show systematic changes, new analyses must be interpreted in the light of all other observations to help anticipate the character of future behavior.

Thermal Observations

Nighttime aerial observations of the lava dome also have been useful in monitoring volcanic activity. An image intensifier attached to a 35-millimeter or video camera can detect hot spots on the dome that are not visible to the naked eye. The intensifier magnifies the glowing spots 20,000 to 40,000 times. Increased visible glow is sometimes observed a few days before and eruption. This technique, currently under development, shows promise for monitoring the dome should work in the crater be curtailed for any reason.

Other Volcanoes

Survey networks and tilt stations have been established on other volcanoes of the Cascade Range: Mount Baker and Mount Rainier in Washington, Mount Hood and Crater Lake in Oregon, and Mount Shasta and Lassen Peak in northern California. Current plans are to remeasure these networks every 3 years, unless conditions, such as increased seismicity, warrant more frequent monitoring. Earthquake activity is continuously monitored at these volcanoes. Monitoring earthquakes and ground movement on these volcanoes will probably record changes before future eruptive activity, but it is unlikely that the monitoring will define the exact time or type of an eruption as precisely as is currently possible at Mount St. Helens.

The drama of the May 18, 1980, eruption of Mount St. Helens captured the attention of people throughout the world to a degree matched by few natural events in recent decades. However, the energy and volume of this eruption were exceeded considerably by several eruptions elsewhere in the world during the past century. Even so, the fact that a great natural disaster occurred in one of the highly developed countries has brought volcanoes in general and Mount St. Helens in particular a degree of recognition and visibility not previously achieved. Systematic observations and monitoring of the activity since its beginning in 1980 probably have exceeded those associated with any major eruption elsewhere, thus providing both an opportunity for education on a worldwide scale and a responsibility for disseminating the lessons learned.

Scientists and public officials from at least 25 countries have visited CVO and Mount St. Helens and have gained improved insights into volcanic processes and into how society interacts with natural disasters. In turn, scientists of the U.S. Geological Survey's Volcano Hazards Program have participated in monitoring active volcanoes in other countries, including Indonesia, Papua New Guinea, and New Zealand, and have visited areas of active volcanism in several other countries and have consulted with their scientists. This kind of interaction is of immeasurable value in helping the international community of volcanologists to deal with the vital goals of improving the ability to predict volcanic eruptions and to mitigate volcanic risks.



The Changing Hydrology at Mount St. Helens

The effects of the May 18, 1980, eruption of Mount St. Helens significantly increased the threat of flooding along rivers draining the volcano, especially the Toutle and lower Cowlitz Rivers. The erosion of unconsolidated volcanic debris around the volcano and the possible failure of debris dams impounding Spirit, Coldwater, and Castle Lakes pose hazards to communities downstream from the volcano. Steps have been taken by the U.S. Army Corps of Engineers to reduce the threat of flooding, and discussion is currently underway to implement long-term solutions. Data collected by U.S.Geological Survey hydrologists from the Cascades Volcano Observatory and from Tacoma, Washington, are given to Federal, State, and local officials who are responsible for flood-mitigation and emergency-response plans.

Hydrologic Monitoring

The May 18, 1980, eruption significantly increased the rate of surface runoff during storms and the availability of readily erodible sediment by destroying vegetation and by depositing loose debris over a wide area north of the volcano. The directed lateral blast stripped trees from most hillslopes within 11 kilometers north of the volcano and leveled nearly all vegetation as far as 20 kilometers in a 180-degree arc north of the mountain. The blast deposited blocks, smaller rock fragments, and organic debris over the 550-square-kilometer area in layers to more than 1 meter in thickness. Surrounding this zone of toppled vegetation is a narrow 100-square-kilometer band of scorched, but standing, timber in which sandy deposits are as thick as 8 centimeters.


Image, click to enlarge [Image,21K,GIF]
The effects of the May 18, 1980 eruption.


Image, click to enlarge
MSH80_blowdown_smith_creek_09-24-80.jpg
The slopes of Smith Creek valley, east of Mount St. Helens, show trees blown down by the May 18, 1980 lateral blast. Two U.S. Geological Survey scientists (lower right) give scale. The direction of the blast, shown here from left to right, is apparent in the alignment of the downed trees. Over four billion board feet of usable timber, enough to build 150,000 homes, was damaged or destroyed.
USGS Photograph taken on September 24, 1980, by Lyn Topinka.
[medium size] ... [large size]

Image, click to enlarge
MSH80_mudline_muddy_river_with_USGS_scientist_10-23-80.jpg
Nearly 135 miles (220 kilometers) of river channels surrounding the volcano were affected by the lahars of May 18, 1980. A mudline left behind on trees shows depths reached by the mud. A scientist (middle right) gives scale. This view is along the Muddy River, southeast of Mount St. Helens.
USGS Photograph taken on October 23, 1980, by Lyn Topinka.
[medium size] ... [large size]


Rivers with headwaters in the blast area have a rapid streamflow response to rainfall, owing to reduced infiltration rates on hillslopes and low roughness along channels. Streams now respond more quickly to a given amount of rainfall and produce higher peak flows as rainfall is quickly flushed through the drainage system. Greater streamflow increases the erosion and transportation of sediment from hillslopes and river channels; deposition of this debris in the lower reaches of the Toutle and Cowlitz Rivers reduces channel depths, thereby increasing the possibility of flooding. Flood levees, channel dredging, and debris-retention structures built by the U.S. Army Corps of Engineers have thus far prevented serious flooding to communities along the Toutle and Cowlitz Rivers.

Lahars, or mudflows, and floods accompanying the May 18 eruption rushed down nearly all the streams draining the volcano and spread over valley floors, raised channel beds, and destroyed roads, bridges, and homes. Lahars formed during the initial blast, and pyroclastic flows occurred in the Smith, Pine, and Muddy River drainages on the east flank of the cone and in the South Fork Toutle River on the west flank. The most voluminous and destructive lahar originated by the slumping and flowing of water-saturated parts of the debris-avalanche deposit. This lahar peaked near the mouth of the Toutle River at midnight and left deposits 1 meter thick on parts of the flood plain and 5 meters thick in the channel. These deposits immediately reduced channel depths and increased the possibility of flooding along the Toutle and lower Cowlitz Rivers. Smaller lahars were formed by the melting of debris-laden ice and snow during the afternoon of May 18.

The debris avalanche that triggered the eruption slid north into Spirit Lake and west 25 kilometers down the North Fork Toutle River valley, covering the valley floor with unconsolidated debris to an average depth of 45 meters and as much as 180 meters in some places. Rapid erosion resulting from the breaching of numerous ponds and lakes on the deposit and surface runoff have produced a new drainage system on the avalanche. Streams following the initial drainage pattern quickly eroded narrow channels because of the generally steep slopes and the readily erodible character of the avalanche deposit. Channels more than 300 meters wide and 45 meters deep have been carved by the new North Fork Toutle River. Nearly 4 years after the devastating eruption, erosion rates remain high, and the channels display complex, alternating scour-and-fill sequences.


Image, click to enlarge
MSH83_debris_avalanche_north_fork_toutle_11-30-83.jpg
Downstream view of the North Fork Toutle River valley, north and west of St. Helens, shows part of the nearly 2/3 cubic miles (2.3 cubic kilometers) of debris avalanche that slid from the volcano on May 18, 1980. This is enough material to cover Washington, D.C. to a depth of 14 feet (4 meters). The avalanche traveled approximately 15 miles (24 kilometers) downstream at a velocity exceeding 150 miles per hour (240 km/hr). It left behind a hummocky deposit with an average thickness of 150 feet (45 meters) and a maximum thicknes of 600 feet (180 meters).
USGS Photograph taken on November 30, 1983, by Lyn Topinka.
[medium size] ... [large size]


The debris avalanche raised the level of Spirit Lake 64 meters and dammed its natural outlet even higher. Many small ponds filled closed depressions on top of the avalanche deposit, and several lakes formed in tributaries dammed by the avalanche; the largest lakes formed in the tributaries of Coldwater and Castle Creeks. In late 1980, some of the ponds overtopped and swiftly eroded their new outlets. The rapid release of water generated highly erosive flows on the avalanche and transported large volumes of sediment down the lower reaches of the Toutle and Cowlitz Rivers.

Failure of the debris dams holding Spirit, Coldwater, and Castle Lakes would result in catastrophic mudflows comparable to or larger than those of May 18, 1980. Controlled outflow channels have been constructed to stabilize the water levels of Coldwater and Castle Lakes, and water from Spirit Lake is currently being pumped into the Toutle River by the Corps of Engineers as a temporary measure to control its level. Permanent solutions are being considered to alleviate the flood threat from Spirit Lake.


Image, click to enlarge
MSH80_blast_area_spirit_lake_with_rainier_10-04-80.jpg
Spirit Lake, once surrounded by lush forest, is within the area devastated by blast. Remnants of the forest float on the surface of the lake. Another Cascade volcano, Mount Rainier (14,410 feet [4,392 meters]), is in the distance. The view is from the south.
USGS Photograph taken on October 4, 1980, by Lyn Topinka.
[medium size] ... [large size]

Image, click to enlarge
MSH84_castle_lake_debris_avalanche_march_1984.jpg
The May 18, 1980 debris avalanche from Mount St. Helens covered over 24 square miles (62 square kilometers) of the upper Toutle River valley and blocked tributaries of the North Fork Toutle River. New lakes such as Castle Lake (pictured here) and Coldwater Lake were created.
USGS Photograph taken in March 1984 by Robert L. Schuster.
[medium size] ... [large size]


The Geological Survey gathers information on hydrologic hazards at Mount St. Helens in the following ways: (1) by measuring the annual rates of erosion, transportation, and deposition of sediment along streams draining the volcano, (2) by monitoring the water elevations and the stability of the debris dams impounding Spirit, Coldwater, and Castle Lakes, and (3) through research on the flow characteristics of lahars and streams with high sediment loads.

Erosion, Transportation, and Deposition of Sediment

Thirteen gaging stations were constructed after the May 18 eruption to measure water and sediment discharge of the rivers draining Mount St. Helens; these stations supplement those already in place on reservoirs and rivers around the volcano. Gaging stations continuously record the water-surface elevation or stage of a river. Stream discharge is calculated from the relationship between this recorded stage and periodic manual discharge measurements. Hydrologists also collect water samples at the gage sites and analyze them to determine total suspended sediment transported by the streams.

The network of river gages provide information for flood forecasting and for long-term sediment-transport trends. These data are used by the National Weather Service to warn of severe flooding conditions and by the Corps of Engineers to develop sediment-control solutions.


Image, click to enlarge
MSH82_sediment_sampling_toutle_at_tower_road_12-12-82.jpg
USGS hydrologists sample sediment moving down the Toutle River. View at Tower Road.
USGS Photograph taken on December 12, 1982, by Lyn Topinka.
[medium size] ... [large size]


Since May 18, 1980, sediment transport rates for the rivers flanking Mount St. Helens, especially the Toutle River, have been among the highest in the world. More than 20 million tons of suspended sediment was transported from the Toutle River basin in the first 7 months after the May 18, eruption, or 15 million tons in only 13 days. About 39 million tons of suspended sediment was transported from October 1981 to September 1982, enough to cover an average city block to a depth of 8 kilometers. Since 1980, storms have been of only low to moderate intensity; consequently, less than 5 percent of the total volume of the avalanche deposit has been removed by erosion, so it will persist as a sediment-management problem for many years.

More than 150 cross-sections of river channels are surveyed regularly to determine areas of erosion and deposition along rivers draining Mount St. Helens. These repetitive surveys measure bank and channel erosion and channel deposition at specific locations. Repeated aerial photographs also are used to identify sediment sources and sinks.

In many places since the 1980 eruptions, channel modifications have been equal to or greater than those resulting directly from the damaging lahars on May 18. Generally, erosion and sediment transport by channel widening and downcutting dominate the upper reaches of the drainage basins, and aggradation and sediment transport dominate the lower reaches.


Image, click to enlarge
MSH81_USGS_hydrologists_measure_erosion_06-26-81.jpg
U.S. Geological Survey hydrologists measured changes in erosion along the stream channels affected by the May 18, 1980 eruption. These measurements were used to study the erosion processes and to estimate the severity of the sedimentation problem. The view here is along the Muddy River drainage, approximately one mile (1.5 kilometers) southeast of the volcano's base. Rod person (lower left) and instrument persons (upper right) give scale.
USGS Photograph taken on June 26, 1981, by Lyn Topinka.
[medium size] ... [large size]


Lake Monitoring

Six lake gages, maintained by the Geological Survey in cooperation with the National Weather Service and the Federal Emergency Management Agency, monitor the water levels of Spirit, Coldwater, and Castle Lakes. The gages serve as an emergency warning system if one of the debris dams fails. Each gage has at least two recording instruments that transmit several lake elevations each hour by way of a satellite to a ground receiving station in Tacoma, Washington. If a lake level drops faster than the specified rate, alert transmissions send lake elevations every 5 minutes.


Image, click to enlarge
MSH82_coldwater_lake_early_warning_gage_10-01-82.jpg
One major concern to people living downstream of Mount St. Helens was a breakout of any of the impounded lakes, such as Coldwater or Castle Lakes, due to the instability of the debris dams blocking them. Flood waters from a breakout could be more catastrophic than the lahars of May 18, 1980. Gages, such as this Early Warning Gage on Coldwater Lake, were installed at lakes and streams surrounding the volcano. These gages continuously monitored changes in water levels. Major increases or decreases in levels trigger warnings which are telemetered to the U.S. Geological Survey's Cascades Volcano Observatory in Vancouver.
USGS Photograph taken on October 1, 1982, by Lyn Topinka.
[medium size] ... [large size]


Overtopping of the debris dams due to filling from normal precipitation was considered to be the most likely cause of lake breakouts and resulting floods; controlled outlet channels and the Spirit Lake pumping operation have eliminated this possibility. However, a sudden influx of a large volume of volcanic debris from an eruption of Mount St. Helens could raise rapidly the level of Spirit Lake. An eruption producing pyroclastic flows more voluminous than those of May 18, 1980, would be necessary to cause overtopping.

Several geologic and geophysical studies evaluate and monitor the potential instability of unconsolidated material that blocks the lakes. Failure of these debris dams could result from slumping of the dams, liquefaction from shaking during earthquakes, or headward erosion of gullies and channels. The studies suggest, however, that these possibilities are unlikely in the near future.

A seismic zone about 1,000 kilometers long trends north-northwest through Mount St. Helens and beneath the debris-avalanche deposit. During recent decades, several significant earthquakes have occurred along this zone, the largest of which was magnitude 5.5 and occurred in February 1981. Ground-water wells and seismometers on the surface of the avalanche deposit and in holes 6 to 30 meters deep are used to monitor the response of the unconsolidated debris to earthquake activity.

The relatively narrow debris blockage at Castle Lake is most subject to slumping or gravitational failure. Instruments in drill holes as deep as 30 meters monitor slope movements of the Castle and Spirit Lake dams, and ground-water tables are recorded at all three lake blockages. Erosion is monitored by repeated photographs and channel geometry surveys.

Research

The Hydrologic Monitoring Program provides hazard information and improves understanding of the hydrologic processes involved in the devastation and recovery of areas affected by the May 18, 1980 eruption and lahars. Information collected by the monitoring techniques are used to investigate factors affecting the stability of stream channels and the fluid dynamics of flows that transport high sediment loads.

The May 18 lahar deposits and small debris flows that continue to occur on the volcano also help hydrologists to interpret deposits in the historic record at Mount St. Helens and other Cascade volcanoes. Newly recognized pre-1980 lahar deposits in the Toutle River valley are interpreted to have been emplaced from previous breakouts of Spirit Lake. Lahar-hazards studies on Mount Hood Volcano in northern Oregon also have been aided greatly by the study of recent deposits at Mount St. Helens.

Mount St. Helens offers an unusual opportunity to study the flow characteristics of lahars and debris flows and to develop models for predicting their behavior and effects downstream. Information from these studies and the development of better scientific techniques will continue to improve understanding and the expertise needed to manage water resource problems caused by future volcanic eruptions.

Return to:
[Report Menu] ...
[Mount St. Helens Monitoring Menu] ...



ButtonBar

URL for CVO HomePage is: <http://vulcan.wr.usgs.gov/home.html>
URL for this page is: <http://vulcan.wr.usgs.gov/Volcanoes/MSH/Publications/EIB84/EIB84.html>
If you have questions or comments please contact: <GS-CVO-WEB@usgs.gov>
02/07/05, Lyn Topinka