MOUNT ST. HELENS
 |
| Plate V-8 |
These next four pages are dedicated to a more comprehensive
review of perhaps the best-documented volcanic eruption in
history and of the role that satellite remote sensing has played in
this study. On May 18, 1980, in southwest Washington State, on
the western slopes of the Cascade Mountains some 75 km northeast
of Portland, Oregon, in less than 1 minute, Mount St. Helens
(MSH)--the youngest of the active andesitic volcanoes in the
Cascade chain-blew its top in a dramatic and awesome sequence of
events that took 60 lives, destroyed more than 200 homes, and
exacted damage to the Pacific Northwest that exceeded $1 billion.
In addition to camera-wielding ground witnesses (several of
whom perished), observers in light aircraft recorded on film the
instant of eruption and most of the subsequent activity during the
entire eruption phase. Scientists had been monitoring changing
conditions at MSH for several months before the fateful day and
had carried out numerous measurements during a continuing watch
for several previous years. Because the day itself was crystal clear
over much of the western United States, a NOAA Weather Satellite
successfully tracked the initial and subsequent ash clouds as they
progressed hundreds of kilometers to the east. Later that summer,
both Landsat and the Heat Capacity Mapping Mission (HCMM)
satellites obtained striking visible and thermal images of the scene.
The earliest dated eruptions at MSH began some 40,000 years
ago. Much of its growth to a composite stratocone reaching a pre-1980
altitude of 2975 m was accomplished in the last 4000 years.
It experienced a strong eruption (4 km3 of airborne ejecta) around
1900 B.C. Its last previous pulse of intermittent activity fell between
1831 and 1857, in which a new summit crater and an exogenous
dome were formed. Because its record indicated that MSH commonly
experiences major activity every 100 to 200 years, an eruption before
the close of this century seemed likely to the several geologists studying
this volcano. This threatened to disfigure one of the most symmetrical
of the Cascade stratocones. (See
Figure V-5.2, and
Figure V-8.1.)
The first sign of reawakening was a notable Earth
tremor on March 20, 1980, followed by a steam and ash
eruption on the 27th that produced a small crater by steam
"reaming." Several phreatic eruptions,
originating from the influx of snow meltwater into ascending
magma, pulverized parts of the summit. That magma accounts
for the gradual swelling (at 1 to 2 m per day) of the northern
upper slopes as a magma pocket (or cryptodome) neared the
surface. By mid-May, the bulge had risen about 150 m
just above the 1857 Goat Rocks Dome, and reference points
along it had shifted 100 m or more to the north.
The catastrophic eruption of May 18 began at 8:32:20
PDT with a 5.l-magnitude earthquake that apparently
triggered the next reaction some 15 seconds later -a massive
landslide or avalanche that tore open the summit as weakened
rock slid as a debris flow along a detachment plane. First to fail
was ground around Goat Rock Dome, then a second mass that
included the pre-eruption crater broke loose, and finally the
remaining section of the summit dome itself slid away. At
8:32:41, the first of several expulsions of fragmented
rock (some blocks of house size), ash, and steam emerged from
the old crater vent and the new gash along the flank
(Figure V-8.2).
Part of the rising cloud and the lateral blast combined into a surge
that proceeded downslope at speeds up to ~1000 km/hr,
being directed mainly to the North Fork of the Toutle River, which
flows west, and Spirit Lake to the north. The surge raced
indiscriminately over rough terrain for the next 30 seconds
(Figure V-8.3 and
Figure V-8.4). Out to
distances of about 12 km, the Direct Blast Zone is characterized
by almost total tree upheaval from the dense coniferous forests along
the slopes. Farther out to 19 km, the Channelized Blast Zone is marked
by flattened tall trees, many of which fell like "matchsticks"
in an array of parallel-aligned trunks
(Figure V-8.5). For a few kilometers beyond, the lateral blast
and surge singed trees in the Seared Zone.
Within 10 minutes of the beginning of the eruption, a
mushroom-capped ash plume had risen to 18 km, well
into the stratosphere
(Figure V-8.6). The dispersing first cloud and a later
ejection of ash are evident in the NOAA Weather Satellite image
(Figure V-8.7) taken
shortly after noon PDT. Parts of central and eastern Washington
and neighboring Idaho were quickly blanketed by 3 to 7 cm of fine
powdery gray tephra. Measurable traces of ashfall were deposited
as far away as Minnesota, New Mexico, and an isolated pocket in
Oklahoma. All told, 540,000,000 tons of ash came to rest over
about 55 000 km2. Fine tephra remained suspended in the upper
atmosphere for several years.
Mudflows (lahars), formed as volcanic debris mixed
with steam and water, moved out from the slopes within the
first 20 minutes into nearby drainage channels such as the
North and South Forks of the Toutle River to the west
(Figure V-8.8)
and Pine Creek to the southeast. Even the navigation channel
of the Columbia River downstream from the Toutle River/
Cowlitz River network was temporarily reduced from 13 to 4 m
in depth by the choking mud debris. En route, mudflows may
locally have surged up valley walls as much as 100 m, but their
final deposits were much thinner. Phreatic craters
(Figure V-8.9)
formed where pyroclastic flows and lahars encountered pockets
of trapped fluids.
After the dust cleared, the devastation wreaked by the
May 18 eruption could be fully appreciated. The highest
remaining section of the upper peak is now 400 m lower
than the original summit; the rock at that summit point was
dropped about 1000 m to the crater floor. The avalanche and
subsequent blast left a crater 680 m deep and 2 by 3 km wide,
readily visible from space
(Figure V-8.10). Dispersed deposits from the debris
avalanche have an equivalent volume of ~2.8 km;
another 1 km was entrained in the plume expulsions. The initial
eruption devastated an area of about 20 by 30 km (east-west).
The full extent of this damage, roughly coincident with the area of
tephra deposits of 2 to 5 cm and thicker, is evident in the Landsat-3
image shown in the main plate. Multispectral Scanner (MSS) data
from this July 31, 1980, scene were used to construct a supervised
classification of several classes of deposits (Figure
V-8.11); class colors are: blue = clear
water; gray = silty (ash-laden) water; dark
green = conifers; light green = other vegetation;
aqua = ash-covered terrain, with trees down (also bare
soil); purple = ash plus standing trees (deneedled);
yellow = avalanche deposits; orange = mudflows;
red = pyroclastic flows plus mudflows; and black =
pumice flow. Earlier, the HCMM satellite obtained a thermal Night IR
image of the MSH area on June 19, 1980. Using an internal calibration
lamp within the sensor to estimate ground temperature, C. Bohn of
NASA's Goddard Space Flight Center used a computer program to
calculate a surface temperature distribution
(Figure V-8.12). Highest temperatures (white-coded) occur at
the crater and along a lobe (red) extending to Spirit Lake; lowest
temperatures (black) are associated with snow still covering part of the
peak. A thermal IR image
(Figure V-8.13) made with an airborne sensor on July 22, 1980,
shows surface temperature variations along a pyroclastic flow lobe.
A remarkable airborne SLAR (X-band radar) image
(Figure V-8.14) of MSH
was obtained from a flight near the volcano just over 2 hours after it
had erupted on May 18.
Mount St. Helens has continued to erupt through 1985.
Another Plinean eruption took place on May 25, 1980, carrying
ash toward Seattle, followed by still more smaller eruptions in
June, July, August, and October. By the end of 1980, tephra in
the devastation area had built to thicknesses of a half meter or
more close in. By mid-June of 1980, a lava dome began to
push up at the surface within the crater and has grown periodically
to a height of 600 m since then
(Figure V-8.15). The surface heat state of this dome in 1984
is depicted in a Thematic Mapper band 6 thermal image
(Figure V-8.16).
More than 800 m across, the dome is warmer than its surroundings.
By some standards, MSH was not a large explosive event.
It compares with the 1586 eruption of Kelutin in Indonesia and
Mt. Pelée (1902) on the Caribbean island of Martinique
and was somewhat smaller than the famous 79 A.D. eruption of
Vesuvius. It was much smaller (1 km3 of airborne tephra) than
Crater Lake's Mt. Mazama (42 km3) or the great 1815 eruption
of Tambora in Indonesia (80 km3) and was inconsequential
compared to the welded tuff-forming eruptions in the
Yellowstone region and at the Vanes Caldera in prehistoric times.
Nevertheless, it remains in one sense the most spectacular of all
famous eruptions in the thoroughness with which it has been
recorded and studied. It is likewise a cogent example of how a
dominantly constructional landform can convert almost instantly
to one that has a look of total destruction around it. After only 5
years, however, the ecology around it has begun to revert to its
past state. Caption modified from comments by N. H. MacLeod,
USGS. Additional References: Foxworthy and Hill (1982),
Tilling (1984), U.S. Geological Survey General Information Bulletin.
Landsat Subscene, July 31, 1980.
Continue to Plate V-9 |
Chapter 3 Table ofContents |
Complete Table of Contents |
Geomorphology Home Page
|
 |