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Monitoring Images 1980 - 2004 |
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| Monitoring ... Before May 18, 1980 | ||
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MSH80_seismogram_RAN_harmonic_tremor_04-02-80.jpg
Seismogram from station RAN, harmonic tremor. USGS Photograph taken on April 2, 1980. [medium size] |
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MSH80_david_johnston_gas-detection_equipment_04-04-80.jpg
USGS geologist David A. Johnston, with gas-detection equipment. USGS Photograph taken on April 4, 1980. [medium size] |
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MSH80_USGS_geologist_DavidJohnston_with_gas-sampling_airplane_04-04-80.jpg
USGS geologist David Johnston stands by aircraft outfitted to carry the COSPEC, to sample gases from Mount St. Helens. USGS Photograph taken on April 4, 1980, by Tom Casadevall. [medium size] |
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MSH80_COSPEC_timberline_parking_lot_04-10-80_bw.jpg
Gas-sampling COSPEC setup at Timberline parking lot, April 10, 1980, with USGS geologist David Johnston (kneeling) and Larry Malinconico (standing). USGS Photograph taken on April 10, 1980, by Tom Casadevall. [medium size] |
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MSH80_aerial_coldwater_observation_post_04-11-80.jpg
Aerial view of the Coldwater observation post, later called "Coldwater I". This location is 8.4 miles northwest of Mount St. Helens. USGS Photograph taken on April 11, 1980, by C.Dan Miller. [medium size] |
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MSH80_establishing_target_on_sugarbowl_04-23-80.jpg
Establishing unmanned target on Sugar Bowl, northeast flank of Mount St. Helens. USGS Photograph taken on April 23, 1980, by Peter W. Lipman. [medium size] |
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MSH80_geodimeter_station_smith_creek_butte_04-25-80.jpg
Geodimeter station (EDM) set up at Smith Creek Butte, east side of Mount St. Helens. USGS Photograph taken on April 25, 1980, by Peter Lipman. [medium size] |
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MSH80_bulge_on_north_side_04-27-80.jpg
A "bulge" developed on the north side of Mount St. Helens as magma pushed up within the peak. Angle and slope-distance measurements to the bulge indicated it was growing at a rate of up to five feet (1.5 meters) per day. By May 17, part of the volcano's north side had been pushed upwards and outwards over 450 feet (135 meters). The view is from the northeast. USGS Photograph taken on April 27, 1980, by Peter Lipman. [medium size] ... [large size] |
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MSH80_USGS_geologist_DaveJohnston_enters_msh_crater_04-30-80.jpg
USGS geologist, David Johnston, enters crater of Mount St. Helens. USGS Photograph taken on April 30, 1980, by Rick Hoblitt. [medium size] |
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MSH80_USGS_geologist_DaveJohnston_samples_crater_lake_04-30-80.jpg
USGS geologist, David Johnston, samples the waters of Mount St. Helens crater lake. USGS Photograph taken on April 30, 1980, by Rick Hoblitt. [medium size] |
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MSH80_USGS_scientists_geodimeter_timberline_05-02-80.jpg
USGS geologists with geodimeter setup, Timberline parking lot, north side of Mount St. Helens. USGS Photograph taken on May 2, 1980, by Pete Lipman. [medium size] |
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MSH80_geodimeter_station_toutle_canyon_05-02-80.jpg
West side of Mount St. Helens, as seen from the geodimeter station Toutle Canyon. USGS Photograph taken on May 2, 1980. [medium size] |
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MSH80_geodimeter_measurements_to_north_flank_05-04-80.jpg
USGS scientists make geodimeter measurements to Mount St. Helens' north flank. USGS Photograph taken on May 4, 1980, by C.Dan Miller. [medium size] |
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MSH80_coldwater_II_observation_post_05-04-80.jpg
Coldwater II observation post. USGS Photograph taken on Map 4, 1980. Photographer unknown. [medium size] |
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MSH80_USGS_geologist_DavidJohnston_sampling_fumarole_05-17-80.jpg
USGS geologist David Johnston (red circle) sampling fumarole at the crest of the "bulge". Image taken from hovering helicopter. USGS Photograph taken on May 17, 1980, by unknown USGS photographer. [medium size] |
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MSH80_david_johnston_at_camp_05-17-80.jpg
David Johnston at Coldwater II, at 1900 hours. Dave did not survive the next day's eruption. Coldwater II would eventually be re-named "Johnston Ridge" in honor of Dave. USGS Photograph taken on May 17, 1980, by Harry Glicken. [medium size] ... [large size] ... [TIF Format, 18 M] |
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MSH80_seismogram_CPW_05-18-80.jpg
Seismogram, May 18, 1980 eruption of Mount St. Helens. USGS Photograph taken on May 18, 1980. [medium size] |
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| Monitoring ... Remote TV-Video, 1980 | ||
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MSH80_video_camera_installation_harrys_ridge_10-08-80.jpg
Video-camera installation on Harry's Ridge, 5-miles north of Mount St. Helens. Camera is mounted on top of the shelter that contains microwave telemetry equipment. USGS Photograph taken on October 20, 1980, by C.Dan Miller. [medium size] ... [large size] |
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MSH80_remote_tv_hut_on_harrys_ridge_08-06-80.jpg
Video-camera installation on Harry's Ridge, 5-miles north of Mount St. Helens. Camera is mounted on top of the shelter that contains microwave telemetry equipment. USGS Photograph taken on August 6, 1980, by M. Lukk. [medium size] ... [large size] |
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MSH80_video-monitor_in_vancouver_Summer1980.jpg
Video-monitor and control console in the Emergency Coordination Center in Vancouver, Washington. USGS Photograph taken Summer 1980, by Rick Hoblitt. [medium size] ... [large size] |
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| Monitoring ... Deformation, 1980 to 2004 | ||
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MSH80_scientists_installing_temperature_probe_05-22-80.jpg
USGS scientists installing steep pipe and temperature probe in pumice, southeast side of Mount St. Helens. USGS Photograph taken on May 22, 1980. [medium size] ... [large size] ... [TIF image, 24 M] |
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MSH80_NewCastle_monitoring_target_05-24-80.jpg
New Castle monitoring target, established around the base of Mount St. Helens. USGS Photograph taken on May 24, 1980, by Pete Lipman. [medium size] ... [large size] ... [TIF image, 24 M] |
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MSH80_geologist_setting_up_rampart_target_06-29-80
Geologist setting up deformation target on the rampart inside Mount St. Helens crater, north of the lava dome. USGS Photograph taken on June 29, 1980, by Pete Lipman. [medium size] ... [large size] ... [TIF Format, 24 M] |
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MSH80_geologist_at_Road100_06-29-80
Geologist at Road 100 station, northeast of Mount St. Helens, measuring distances to stations installed on the volcano's flanks. USGS Photograph taken on June 29, 1980, by Pete Lipman. [medium size] ... [large size] ... [TIF Format, 24 M] |
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MSH80_harrys_ridge_with_helicopter_06-29-80
On June 19, 1980, a new instrument station was established on the high point of a ridge about 5 miles north of the crater and to the west of Spirit Lake. This ridgetop provided a good view directly into the crater and distinctive features of the dome can be tracked from there. The station is informally known as Harry's Ridge because it overlooked the now-buried site of the Mount St. Helens Lodge, where proprietor Harry Truman presumably was killed during the May 18 eruption. USGS Photograph taken on June 29, 1980, by Pete Lipman. [medium size] ... [large size] ... [TIF Format, 24 M] |
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MSH80_deformation_monitoring_from_harrys_ridge_08-06-80.jpg
Geodimeter setup on Harry's Ridge, 5-miles north of Mount St. Helens. USGS Photograph taken on August 6, 1980, by M. Lukk. [medium size] ... [large size] |
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MSH80_vertical_thermal_image_msh_08-13-80.jpg
Vertical thermal image of Mount St. Helens taken shortly after the August 7, 1980 eruption, using a RS-14A scanner from 15,000 feet, with color calibrated by computer. Blue is coldest and Red is hottest. Image from USGS Professional Paper 1250, Figure 173. USGS Photograph taken on August 13, 1980. [medium size] ... [large size] ... [TIF Format, 24 M] |
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MSH80_mount_st_helens_harrys_ridge_09-30-80.jpg
Aerial view of Mount St. Helens volcano, with Harrys Ridge in the foreground. USGS Photograph taken September 30, 1980, by Lyn Topinka. [medium size] ... [large size] ... [TIF Format, 25 M] |
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MSH81_USGS_geologists_hydrogen_site_south_ridge_03-06-81.jpg
USGS geologists working at hydrogen sampling site, South Ridge, on the south flank of Mount St. Helens. Snow-covered Mount Adams is in the background. USGS Photograph taken on March 6, 1981, by Tom Casadevall. [medium size] ... [large size] ... [TIF Format, 24 M] |
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MSH81_USGS_scientists_put_targets_on_dome_05-12-81.jpg
Two USGS scientists (left middle) install targets and prism reflectors on Mount St. Helens dome. USGS Photograph taken on May 12, 1981, by Lyn Topinka. [medium size] ... [large size] ... [TIF Format, 24 M] |
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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] ... [TIF Format, 18 M] |
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MSH81_USGS_scientists_measure_thrust_fault_05-12-81.jpg
Two USGS scientists measure thrust fault at base of Mount St. Helens' dome. USGS Photograph taken on May 12, 1981, by Lyn Topinka. [medium size] ... [large size] ... [TIF Format, 24 M] |
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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] |
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MSH81_monitoring_dome_crater_floor_08-22-81.jpg
Monitoring the dome from the crater floor, north of the dome -- summer. USGS Photograph taken on August 22, 1981, by Lyn Topinka. [medium size] ... [large size] |
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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] |
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MSH81_USGS_scientists_on_harrys_ridge_10-31-81.jpg
USGS Scientists take deformation measurements from Harry's Ridge, located 5 miles (8 kilometers) north of Mount St. Helens. USGS Photograph taken on October 31, 1981, by Lyn Topinka. [medium size] ... [large size] ... [TIF Format, 24 M] |
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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] |
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MSH82_camera_barrel_base_dome_08-17-82.jpg
Fifty-five gallon barrel drum used as a time-lapse camera mount, set up on the crater floor at the south side of the dome. Drum was easy to transport to the site, filled with dome rock for ballast, and camera installed and turned on. At the end of the day the camera and top case were retrieved. Barrel was covered by dome rock shortly after. USGS Photograph taken August 17, 1982, by Lyn Topinka. [medium size] ... [large size] ... [TIF Format, 24 M] |
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MSH82_USGS_scientists_EDM_to_dome_08-17-82.jpg
USGS scientists take EDM measurements to Mount St. Helens' growing lava dome. USGS Photograph taken on September 17, 1982, by Lyn Topinka. [medium size] ... [large size] ... [TIF Format, 23 M] ... |
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MSH83_monitoring_dome_crater_floor_03-22-83.jpg
Monitoring the dome from the crater floor, north of the dome -- winter. USGS Photograph taken on March 22, 1983, by Lyn Topinka. [medium size] ... [large size] |
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MSH83_harrys_ridge_09-15-83.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 the station Harry's Ridge, 5 miles north of Mount St. Helens' crater, with a USGS scientist setting up a theodolite. USGS Photograph taken in September 15, 1983, by Lyn Topinka. [medium size] ... [large size] |
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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] ... [TIF Format, 18 M] |
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MSH84_harrys_ridge_and_st_helens_03-22-84.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 the station Harry's Ridge, 5 miles north of Mount St. Helens' crater, with the EDM set up within the building. USGS Photograph taken in March 22, 1984, by Lyn Topinka. [medium size] ... [large size] ... [TIF Format, 25 M] |
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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] |
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MSH84_measuring_magnetic_field_in_crater_06-18-84.jpg
Geologists measured the strength of the magnetic field surrounding the dome. The strength of the field increased as the dome cooled and magnetic minerals formed. During the eruptions the strength usually changed rapidly as magma heated and deformed the dome. USGS Photograph taken on June 18, 1984, by Lyn Topinka. [medium size] ... [large size] |
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MSH85_USGS_scientists_deformation_top_of_dome_05-17-85.jpg
USGS scientists make deformation measurements from top of the dome. USGS Photograph taken on May 17, 1985, by David Wieprecht. [medium size] ... [large size] |
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MSH88_deformation_monitoring_top_dome_04-18-88.jpg
In 1983, the U.S. Geological Survey extended both its periodic and its 24-hour monitoring programs to the top of Mount St. Helens' dome. In this aerial view, three geologists (middle bottom) were busy taking measurements to determine deformation rates USGS Photograph taken in April 18, 1988, by Lyn Topinka. [medium size] ... [large size] |
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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] |
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| Monitoring ... Hydrology, 1980 to 2004 | ||
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MSH80_muddy_bridge_devastation_09-23-80.jpg
Remains of the bridge crossing the Muddy River. USGS scientist in yellow on far bank, right, is measuring erosion along the reach. USGS Photograph taken on September 23, 1980, by Lyn Topinka. [medium size] ... [large size] ... [TIF Format, 25 M] |
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MSH80_cross_section_survey_upper_pine_creek_10-09-80.jpg
USGS hydrologists measure the cross section at Upper Pine Creek. Mount St. Helens steams in the background. USGS Photograph taken on October 9, 1980, by Lyn Topinka. [medium size] ... [large size] |
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MSH80_pine_creek_cross_section_10-09-80.jpg
USGS hydrologist on rod at cross section along Pine Creek. USGS Photograph taken on October 9, 1980, by Lyn Topinka. [medium size] ... [large size] ... [TIF Format, 24 M] |
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MSH80_pine_creek_bridge_remnant_10-24-80.jpg
Remains of the bridge crossing the Pine Creek. Note USGS Hydrologist holding rod for cross section survey. USGS Photograph taken on October 24, 1980, by Lyn Topinka. [medium size] ... [large size] ... [TIF Format, 25 M] |
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MSH81_pine_creek_bridge_remnant_after_storm_03-16-81.jpg
Remains of the bridge crossing the Pine Creek. The original bridge was taken out during the mudflows of May 18, 1980. The banks were further eroded during the first major floods of 1981. Compare with image above. Note USGS Hydrologist holding rod for cross section survey. USGS Photograph taken on March 16, 1981, by Lyn Topinka. [medium size] ... [large size] ... [TIF Format, 25 M] |
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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 (circled, lower left) and instrument persons (circled, upper right) give scale. USGS Photograph taken on June 26, 1981, by Lyn Topinka. [medium size] ... [large size] ... [TIF Format, 24 M] |
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MSH81_spirit_lake_USGS_water_quality_boat_09-16-81.jpg
USGS hydrologists (in boat, yellow circle) sample Spirit Lake for water quality, one year after the May 18, 1980 eruption of Mount St. Helens. USGS Photograph taken on September 16, 1981, by Lyn Topinka. [medium size] ... [large size] ... [TIF Format, 24 M] |
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MSH81_sediment_sampling_hwy-99_12-06-81.jpg
Sediment sampling, Highway 99 Bridge. USGS Photograph taken on December 6, 1981, by Lyn Topinka. [medium size] ... [large size] |
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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] |
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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] |
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MSH85_USGS_hydrologists_sample_sediment_04-27-85.jpg
Hydrologists measured stream discharge and took water samples to determine how much sediment is suspended in the stream and how much sediment is moving along the streambed. USGS Photograph taken on April 27, 1985, by Lyn Topinka. [medium size] ... [large size] |
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MSH86_USGS_scientist_stability_experiment_08-86.jpg
USGS Researcher, Dr. Richard Iverson, conducting debris flow stability experiment. USGS Photograph taken in August 1986, by Lyn Topinka. [medium size] ... [large size] |
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