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Osceola Mudflow

The Osceola Mudflow was a massive volcanic debris flow, or lahar, that erupted from Mount Rainier in Washington state approximately 5,600 years ago, triggered by the catastrophic sector collapse of the volcano's summit during phreatomagmatic eruptions that mobilized hydrothermally altered rock and ice.^[1]^[2] This event released about 3.8 cubic kilometers of water-saturated debris, which initially traveled as a high-velocity avalanche exceeding 19 meters per second and reached a peak discharge of roughly 2.5 million cubic meters per second, filling the White River canyon to depths over 100 meters.^[1]^[3] The mudflow surged more than 120 kilometers downstream, inundating over 200 square kilometers of the Puget Sound Lowland and extending into Puget Sound itself, where subsurface deposits alone accounted for about 1.26 cubic kilometers across 157 square kilometers.^[1] It deposited thick layers of poorly sorted, clay-rich sediment in three main facies: thick, normally graded axial flows up to 25 meters deep; thinner, ungraded valley-side veneers; and hummocky accumulations from the initial avalanche phase.^[1] The collapse reduced Mount Rainier's elevation by around 300 meters and carved a prominent east-side amphitheater, still visible today and exposing yellowish, concrete-like outcrops along trails like Glacier Basin.^[2] As the largest lahar known from Mount Rainier and one of the world's most voluminous volcanic mudflows, the Osceola event underscores the volcano's ongoing hazard potential, particularly for downstream communities along the White and Puyallup Rivers, where similar future flows could affect modern infrastructure.^[4]^[3] Geologic mapping and radiocarbon dating, with a calibrated age of approximately 5,600 years before present, have refined its timing and characteristics, informing hazard assessments by agencies like the U.S. Geological Survey.^[1]^[5]

Geological Context

Mount Rainier Overview

Mount Rainier is a prominent stratovolcano in the Cascade Range of Washington state, United States, rising to an elevation of 4,392 meters (14,411 feet) above sea level and dominating the skyline of the Puget Sound region.^[6] As one of the highest peaks in the Cascade volcanic arc, it exemplifies the region's active tectonics and glacial landscape, with its massive edifice built from layered volcanic materials that contribute to its steep, symmetrical profile.^[7] The volcano formed primarily during the Pleistocene epoch, approximately over the last 500,000 years, through repeated eruptions of andesitic and dacitic lava flows, along with pyroclastic deposits such as pumice and ash.^[6] These materials accumulated around older volcanic cores, creating a composite cone that has undergone significant erosion by ice and water, shaping its current form while preserving evidence of its eruptive history in the surrounding terrain.^[8] At its summit, Mount Rainier features a permanent ice cap that nurtures one of the most extensive glacial systems in the contiguous United States, including 26 major glaciers covering about 36 square miles.^[6] Notable among these are the Emmons Glacier, the largest by surface area at over 4 square miles on the northeastern flank, and the Nisqually Glacier, a well-studied valley glacier descending the southern slope.^[9] Additionally, active hydrothermal systems manifest as fumaroles, steam vents, and hot springs, particularly along fault zones and within the summit crater, indicating ongoing subsurface heat from magmatic activity.^[6] Mount Rainier's geological setting is defined by its position within the Cascade subduction zone, where the oceanic Juan de Fuca Plate is subducting beneath the continental North American Plate at a rate of about 4 centimeters per year, fueling magma generation and volcanism across the arc.^[6] This tectonic regime not only sustains the volcano's growth but also heightens risks from interactions between eruptions and its voluminous ice cover, such as the generation of lahars.^[6]

Pre-Event Volcanic Activity

During the Holocene epoch, Mount Rainier exhibited a series of volcanic episodes that shaped its edifice and set the stage for later instability, with activity intensifying between approximately 10,000 and 5,600 years ago. Eruptive records from this period include multiple instances of lava flows, ballistic bombs, ash falls, and pyroclastic deposits, primarily composed of augite-hypersthene andesite, which contributed to the growth of the volcano's summit cone.^[10] Notable events encompass the Sunrise eruptive period around 11,000 years ago, marked by ash layer R and associated landslides, and the Cowlitz Park period from 7,400 to 6,700 years ago, which produced at least seven tephra layers alongside pyroclastic flows that melted snow and ice, triggering lahars extending up to 70 km to Puget Sound.^[11] Additionally, dome-building activities during the Holocene added layers of andesitic material to the Columbia Crest summit, elevating the cone to 2,100–2,400 meters above its surroundings by around 10,000 years ago.^[12] Explosive events were prevalent, evidenced by numerous tephra layers that record both phreatic (steam-driven) and magmatic eruptions. At least 11 tephra layers have been identified from this timeframe, with volumes ranging from 0.001 to 0.3 km³, including layers F, N, S, and W dated between 5,700 and 6,600 years ago, which contain fresh andesite fragments indicative of magmatic input alongside altered materials suggesting phreatomagmatic interactions.^[10]^[12] Layer S, for instance, represents a significant steam explosion depositing sand, silt, and rock fragments up to 1.5 feet in size, while layers A, L, D, and S are linked to pumice-producing eruptions around 5,800–6,600 years ago.^[10] Although direct ice core data from Mount Rainier for this period is limited, tephra stratigraphy serves as a primary proxy, correlating with regional ash falls and confirming recurrent explosive activity without reliance on modern monitoring.^[10] These eruptions often preceded non-eruptive lahars, such as the Greenwater lahar around 6,600 years ago and the Paradise lahar from 5,800–6,600 years ago, highlighting the interplay between volcanism and slope failure.^[11]^[10] Repeated eruptions facilitated the buildup of unstable summit ice and rock, as accumulating andesitic breccias and lava were subjected to hydrothermal alteration, forming clay-rich zones that weakened the edifice.^[12] This process created friable, clayey rock masses prone to sliding, with geological proxies like altered debris in pre-Osceola lahar assemblages (5,700–6,600 years ago) indicating progressive destabilization of the upper slopes.^[10] Specific precursors to heightened activity are inferred from these proxies, including steam explosions like layer S that likely signaled increased fumarolic output and phreatic unrest, as well as evidence of rock avalanches triggered by hydrothermal weakening in the summit region.^[10] Such indicators, drawn from stratigraphic and lithologic analysis, underscore a pattern of intermittent unrest that amplified the volcano's vulnerability without direct seismic records from the era.^[12]

The Mudflow Event

Triggering Eruptions

The Osceola Mudflow was triggered by phreatomagmatic eruptions at the summit crater of Mount Rainier approximately 5,600 years ago, involving violent interactions between ascending magma and groundwater or glacier meltwater. These eruptions produced explosive steam-driven blasts that destabilized the volcanic edifice, initiating the sector collapse.^[13] The eruptions involved the explosive ejection of hot rock fragments, pumice, and ash, with laterally directed explosions depositing tephra layers across the landscape. This activity rapidly melted summit ice and snow, generating substantial steam and adding water to the system, which further saturated and lubricated the unstable rock mass. Deposit analysis indicates an eruption intensity comparable to Volcanic Explosivity Index (VEI) 4 or higher events, characterized by high explosivity and widespread tephra dispersal. Prior hydrothermal alteration had critically weakened the edifice by converting rocks into clay-rich, low-strength materials through acid-sulfate and argillic processes, reducing shear strength and increasing water retention. These altered zones, concentrated near radial dikes and fractures, made the summit particularly susceptible to failure during the eruptive stress, transforming the initial debris into a highly mobile, cohesive flow.^[14]

Sector Collapse and Initial Flow

The Osceola Mudflow was initiated by a catastrophic sector collapse on the northeast flank of Mount Rainier approximately 5600 years ago, triggered by phreatomagmatic eruptions at the summit. This failure involved the gravitational instability of hydrothermally altered volcanic edifice, weakened by extensive clay-rich alteration that reduced rock cohesion and facilitated slip along low-friction surfaces.^[15] The collapse removed an estimated 2 to 2.5 km³ of material, primarily consisting of altered bedrock and overlying glacier ice, excavating a prominent amphitheater-shaped scar visible today as a large embayment partially filled by later summit crater development.^[15] The initial debris avalanche descended rapidly from the upper slopes, achieving velocities of approximately 60 m/s (over 200 km/h) near the source due to the steep terrain and high momentum of the collapsing mass. The avalanche incorporated loose glacial and alluvial sediments from the upper White River canyon, significantly increasing its volume through bulking. This phase transitioned quickly—within about 2 km of the summit—into a water-saturated, cohesive debris flow, or lahar, as pore water from the altered rocks combined with meltwater from disrupted glaciers and eruptive steam to achieve high fluidity. The resulting initial lahar exhibited distinct facies: a clay-rich axial zone of high-velocity flow with contrasting hummocky, block-rich lateral margins derived from the avalanche's fragmented core. Overall, this early mobilization phase expanded the total event volume to about 3.8 km³ through dilation and entrainment, setting the stage for the flow's prolonged downstream travel while maintaining its destructive, fluid-like behavior.

Path and Deposits

Descent into White River Valley

Following the initial sector collapse on Mount Rainier's northeast flank, the Osceola Mudflow rapidly descended the White River canyon, channeling its massive volume through the confined valley walls. The flow, originating at elevations near the summit (approximately 4,392 m), traveled about 20-30 km down the steep gradient to the canyon mouth at roughly 500 m elevation, where it transitioned toward the broader Puget Lowland. Throughout this phase, the mudflow maintained high velocities, estimated at around 19 m/s, driven by the steep terrain and incorporation of water from glacial melt and hydrothermal sources. As it progressed through the narrower sections of the White River canyon, the flow exerted immense erosional power, scouring up to 100 m of valley walls and incorporating significant volumes of alluvium, colluvium, and glacial drift. This entrainment bulked the debris, transforming the initial avalanche-like mass into a hyperconcentrated stream with enhanced sediment load, while retaining characteristics of a cohesive, clay-rich lahar. The process not only deepened the channel but also mixed in coarser sands and gravels, altering the flow's rheology and increasing its downstream sorting efficiency. Boulder-rich fronts characterized surges in these confined reaches, where high-energy pulses carried megaclasts—some exceeding 10 m in diameter—derived from the volcano's andesite and exotic bedrock. Depositional evidence of these high-energy dynamics is preserved in the valley's hummocky terrain and giant boulder concentrations, particularly in axial and valley-side facies. Hummocks, reaching heights of up to 20 m and widths of 60 m, formed from irregular settling of coarse debris during flow deceleration, while basal deposits of boulders and cobbles mark the inundation limits along the canyon floor. These features, observed up to 100 m thick in places, underscore the mudflow's capacity for repeated surging and erosion-deposition cycles within the White River system.

Spread to Puyallup River and Puget Lowland

After descending through the White River valley, the Osceola Mudflow breached a ridge near the modern site of Mud Mountain Dam, diverting a significant portion of its mass westward into the Puyallup River valley.^[16] This diversion transformed the flow from a primarily confined canyon descent into a broad sheet flood across the Puget Lowland, enabling rapid inundation of low-relief terrain.^[16] The event, occurring approximately 5,600 years ago, marked one of the most extensive Holocene lahars from Mount Rainier, reshaping the regional hydrology.^[17] The mudflow ultimately covered an area of approximately 550 km² in the Puget Lowland, including subsurface deposits extending into river deltas and embayments.^[16]^[18] In the narrower segments of the Puyallup valley, flow depths reached 30–50 meters, creating profound scour and deposition that buried preexisting landscapes.^[16] As the flow expanded onto the flatter lowlands, depths progressively thinned to 1–2 meters near the margins approaching Puget Sound, where it entered the marine environment at locations including Commencement Bay and the Puyallup delta.^[16]^[10] This widespread coverage disrupted ancestral drainage networks, with the lahar's volume overwhelming valley capacities and extending marine influence inland temporarily.^[19] Traveling a total distance of more than 120 km from the volcano's flank to the Puget Lowland extremities, the mudflow propagated at high velocities initially but slowed considerably in the low-gradient terrain.^[16]^[20] The entire transit to the lowlands occurred within several hours, reflecting the lahar's high mobility despite its immense bulk.^[16] Distally, flow speeds diminished to walking paces (roughly 1–5 km/h), allowing for more uniform sediment distribution across the broad plain.^[16] During this phase, the mudflow interacted extensively with ancestral river channels of the Puyallup and Duwamish systems, eroding and incorporating floodplain sediments while creating temporary dams through rapid deposition.^[19] These impoundments backed up water and finer materials, fostering localized ponding and further altering post-event river courses for centuries.^[16]

Volume and Sediment Characteristics

The Osceola Mudflow had an estimated total volume of approximately 3.8 km³, making it one of the largest known Holocene lahars worldwide.^[20]^[21] This substantial volume reflects the event's origin as a massive sector collapse and subsequent debris avalanche that incorporated significant material during its transit through adjacent valleys.^[10] The sediment composition of the Osceola Mudflow deposits features a clay-rich matrix derived primarily from hydrothermally altered volcanic rock, with clay content averaging around 9% of the total fraction and ranging from 6% to 12%.^[10] This matrix, comprising 60-80% clay minerals such as montmorillonite and kaolinite, supported the flow's cohesive nature and enabled long-distance transport with minimal transformation.^[10] The deposits also include boulders and megaclasts up to 10 m or more in diameter, often forming prominent mounds and incorporating megaclasts of unconsolidated gravel, sand, and silt from eroded valley fills.^[10]^[15] Grain size distribution in the deposits spans from fine silt to coarse gravel, with mean sizes ranging from 1.2 mm to 51 mm and a notable presence of sand (28-41%), silt (11-16%), and clay (6-12%).^[10]^[15] The sediments exhibit poor sorting, characterized by sorting coefficients of 9 to 16.34 (averaging 11.53), which indicates rapid deposition from a high-energy, ungraded flow.^[10] The age of the Osceola Mudflow has been established at approximately 5,600 years before present through radiocarbon dating of incorporated wood fragments, with calibrated ages ranging from 5,550 to 5,800 years.^[10]^[15] This dating method confirms the event's Holocene timing and distinguishes it from younger lahars at Mount Rainier.^[10]

Impacts and Legacy

Immediate Environmental Effects

The Osceola Mudflow devastated extensive forested areas across its path, plowing through dense stands of mature conifer trees up to 2 meters in diameter and burying soils beneath meters-thick layers of clay-rich debris. This destruction affected riparian habitats along the White and Puyallup River valleys, inundating over 210 square kilometers of lowland terrain and eliminating vegetation that stabilized riverbanks and supported aquatic-terrestrial ecosystems.^[20]^[15] The mudflow temporarily blocked river drainages by aggrading channels with sediment mounds up to 15 meters high, causing upstream flooding in backwater areas and generating downstream pulses of fine-grained material that disrupted normal hydrological flows for years following the event. For instance, the flow dammed Kapowsin Creek, forming a temporary lake up to 9 meters deep and altering local drainage patterns in the Puyallup River system.^[15]^[20]

Geomorphic Changes to Landscape

The Osceola Mudflow profoundly reshaped the topography of the White and Puyallup River valleys through extensive erosion and sediment deposition, leading to the widening and straightening of these channels. In the White River valley, lateral erosion during and after the event widened the active channel, while similar processes extended to the Puyallup River, where the mudflow's high-energy flow scoured valley walls and floors.^[22] These erosional effects were compounded by the mudflow's immediate burial of pre-existing landscapes, setting the stage for long-term reconfiguration.^[10] The event facilitated the formation of expansive new floodplains across both river systems, as massive sediment loads—estimated at 3.8 km³—were deposited, elevating valley floors by an average of 10–20 meters in many reaches. In the White River valley, this aggradation created broad, flat surfaces that now serve as modern floodplains, with deposits reaching thicknesses of up to 60 meters in proximal areas.^[22] Comparable raises occurred in the Puyallup River valley, where the infilling of pre-existing depressions with clay-rich debris smoothed topographic lows and stabilized the valley bottom against further incision.^[10] Marginal deposition from the mudflow generated hummocky terrain and natural levees, particularly along the edges of the flow path in the White River valley, where irregular mounds up to 10 meters high formed from uneven sediment settling. These features disrupted local drainage patterns by impounding water and redirecting surface flows into new channels, creating a patchwork of poorly drained basins.^[22] In the Puyallup River reaches, levee-like ridges similarly confined post-event streams, promoting lateral migration over downcutting.^[10] The mudflow's legacy persists in the modern river courses, most notably through the avulsion of the White River, which shifted from its pre-event path—now traced by South Prairie Creek—to a more northwesterly alignment toward the Puget Lowland. This rerouting reduced the sediment transport efficiency in the lower Puyallup River floodplain corridor, leading to ongoing aggradation and narrower, more sinuous channels compared to pre-mudflow conditions.^[22] Such alterations have influenced contemporary hydrology, with the raised valley floors limiting flood conveyance in both systems.^[10]

Modern Implications

Hazard Potential for Lahars

The Osceola Mudflow serves as a benchmark for assessing the hazard potential of large lahars at Mount Rainier, with USGS models estimating a recurrence interval of approximately 500 to 1,000 years for events of comparable scale.^[15] These models classify such cohesive debris flows as low-frequency but high-impact occurrences, often triggered by sector collapses or heavy rainfall mobilizing volcanic sediments, and capable of traveling tens of kilometers into populated lowlands. Approximately 80,000 people live in Mount Rainier's lahar-hazard zones.^[15] Downstream communities face significant vulnerability, as areas inundated by past lahars like the Osceola are now densely populated. In Orting, located in the Puyallup River valley, nearly 100% of its approximately 9,000 residents (as of 2025 estimates) live within lahar inundation zones, exposing homes, schools, and infrastructure to rapid flooding.^[23]^[24] Similarly, Enumclaw in the White River valley has substantial exposure, with a substantial portion of its approximately 13,000 residents (as of 2025 estimates) in hazard zones, implying over 1,500 based on prior mapping proportions, amplifying risks to agriculture and transportation routes.^[23]^[25] Population growth since early assessments has further increased the potential for loss of life and property in these areas.^[23] Ongoing monitoring efforts mitigate these risks through integrated systems operated by the USGS Cascades Volcano Observatory. Seismic networks, including over a dozen stations within 20 km of the volcano, detect precursory earthquakes that could signal instability leading to lahars.^[26] Lahar detection systems, deployed along drainages like the Puyallup and White Rivers since 1998 and upgraded in 2024 with enhanced capabilities, use seismic, infrasound, and tripwire sensors to provide real-time alerts of debris flows, offering 30 to 60 minutes of warning downstream; new sensors were installed on the east side in 2025.^[27]^[28]^[29] Glacier mass balance studies, tracking annual changes in ice volume via satellite imagery and field measurements, assess water availability for potential lahar generation, as retreating glaciers alter sediment mobilization patterns.^[30] Mitigation strategies emphasize rapid response and community preparedness. Early warning sirens, part of the All Hazard Alert Broadcast system, are installed in at-risk towns from Orting to Tacoma, automatically activating upon lahar detection to prompt evacuations.^[27] Designated evacuation routes, such as pedestrian bridges and uphill paths in the Puyallup valley, facilitate movement to higher ground, supported by annual drills involving schools and residents to test response times; in March 2024, over 45,000 students participated in the world's largest lahar evacuation drill.^[31]^[32] These measures, coordinated with local emergency management, aim to reduce casualties despite the short travel times of large lahars.^[31]

Comparison to Other Mount Rainier Events

The Osceola Mudflow, occurring approximately 5,600 years ago with a volume of about 3.8 km³, stands as the largest Holocene lahar at Mount Rainier, dwarfing other significant events like the Electron Mudflow (~500 years ago, ~0.3 km³) and the Paradise lahar (~5,600 years ago, 0.05–0.1 km³).^[10]^[17] While the Electron Mudflow traveled roughly 60 km down the Puyallup River valley, and the Paradise lahar extended about 50 km into the Nisqually River drainage, the Osceola event reached over 120 km to the Puget Lowland and Puget Sound, burying an area of more than 200 km² under up to 30 m of deposits.^[10]^[1] All three events share similarities in their triggers, originating from sector collapses of hydrothermally altered volcanic rock, often linked to volcanic activity such as phreatomagmatic eruptions that destabilize the edifice.^[10]^[18] The Osceola and Paradise lahars were contemporaneous, suggesting a shared eruptive episode that produced multiple flows from different flanks of the volcano, whereas the Electron Mudflow may have been initiated by an avalanche or seismic activity without direct eruptive ties.^[21] However, differences in scale highlight Osceola's exceptional magnitude: its volume exceeded the Electron by more than an order of magnitude and the Paradise by nearly two orders, enabling broader downstream inundation that reshaped river valleys and lowlands far beyond the volcano's immediate vicinity.^[1] A key distinction lies in sediment characteristics, particularly the Osceola Mudflow's higher clay content (6–12%, dominated by montmorillonite and kaolinite from hydrothermal alteration), which transformed the initial debris avalanche into a highly cohesive lahar within 2 km of the source, enhancing its mobility and allowing sustained long-distance flow.^[17]^[10] In contrast, the Electron Mudflow had 3–11% clay but was less cohesive overall, limiting its depositional spread, while the Paradise lahar contained only 1–5% clay, resulting in a more debris-dominated flow with restricted reach.^[10] These multi-event timelines from Mount Rainier's Holocene record illustrate recurring patterns of eruption-triggered sector collapses leading to lahars, with clay-rich compositions amplifying hazard extent in larger events like Osceola.^[21]^[13]

References

[1]
[PDF] The Osceola Mudflow from Mount Rainier - morageology.com
The 3.8 km3 Osceola Mudflow began as a water-saturated ava- lanche during phreatomagmatic eruptions at the summit of Mount. Rainier about 5600 years ago.
[2]
[PDF] Geology of Mount Rainier - National Park Service
A small eruption caused the upper portion of the mountain to collapse into a fast-moving flow of mud and debris known today as the Osceola Mudflow.
[3]
Geology and History - USGS.gov
Osceola Mudflow, 50 km (31 mi) downstream, 8 m (26 ft. Lahars are common at Mount Rainier, because its mantle of snow and ice provides water when melted, and ...<|control11|><|separator|>
[4]
surficial deposits shown on the geologic map - NPS History
The Osceola Mudflow is the largest mudflow that has originated at Mount Rainier and is one of the largest volcanic mudflows in the world. It originally covered ...
[5]
Osceola Mudflow from Mount Rainier inundates the White River ...
Jan 23, 2003 · Approximately 5,600 years ago, a massive landslide removes .7 cubic miles of earth from the summit of Mount Rainier. The ensuing mudflow ...
[6]
Geology and History Summary for Mount Rainier - USGS.gov
Volcanism occurs at Mount Rainier and other Cascades arc volcanoes because of the subduction of the Juan de Fuca Plate off the western coast of North America.
[7]
Mount Rainier | U.S. Geological Survey - USGS.gov
Mount Rainier, the highest peak in the Cascade Range at 4,392m (14,410 ft), forms a dramatic backdrop to the Puget Sound region.Monitoring Lahars at Mount... · National Volcano Early... · News · Data
[8]
Geology of Mount Rainier National Park, Washington
Mount Rainier National Park includes 378 square miles of rugged terrain on the west slope of the Cascade Mountains in central Washington.Missing: stratovolcano Range
[9]
Glaciers on Mount Rainier - Washington Water Science Center
Nisqually Glacier is one of the most accessible glaciers on Mount Rainier. ... Emmons Glacier, on the east slope of Mount Rainier, has a surface area of 43 ...
[10]
[PDF] Postglacial Lahars From Mount Rainier Volcano, Washington
Aug 30, 2025 · before the Osceola Mudflow occurred. The base of the lahar assemblage is ·below the White River at nearly every outcrop; at many of these ...
[11]
None
### Summary of Holocene Volcanic Activity at Mount Rainier (10,000 to 5,600 Years Ago)
[12]
3 Development and History of Mount Rainier | Mount Rainier: Active Cascade Volcano | The National Academies Press
### Summary of Holocene Volcanic Activity of Mount Rainier (10,000–5,600 years ago)
[13]
Holocene, or Post-Glacial, Eruptions of Mount Rainier - USGS.gov
We know more about the recent volcanism at Mount Rainier because deposits postdate extensive glaciation and therefore are well preserved.<|control11|><|separator|>
[14]
Implications for debris-flow hazards and mineral deposits
Hydrothermal alteration at Mount Rainier waxed and waned over the 500,000-year episodic growth of the edifice. Hydrothermal minerals and their ...
[15]
[PDF] Sedimentology, Behavior, and Hazards of Debris Flows at Mount ...
Note large embayment, now partly filled by the snow-clad summit crater, which yielded the sector collapse that formed the Osceola Mudflow. The flow diverged ...
[16]
[PDF] Sedimentology, behavior, and hazards of debris flows at Mount ...
The Osceola Mudflow contains weak megaclasts of unconsolidated, stratified gravel, sand, and silt that represent flood plain deposits. Some such ...
[17]
The Osceola Mudflow from Mount Rainier - USGS.gov
The 3.8 km3 Osceola Mudflow began as a water-saturated avalanche during phreatomagmatic eruptions at the summit of Mount Rainier about 5600 years ago.
[18]
[PDF] SIR 2017-5022-A: Geologic Field-Trip Guide to Volcanism and its ...
Mount Rainier prior to the Osceola Mudflow. The Reflection. Lakes lahar swept through a notch in Mazama Ridge to the northwest of us and into Reflection ...<|control11|><|separator|>
[19]
[PDF] Catastrophic debris flows transformed from landslides in volcanic ...
Jun 6, 1994 · The Osceola Mudflow at Mount Rainier is an example of a "maximum" cohesive debris flow (Vallance and Scott, 1997), and is so treated in the ...<|control11|><|separator|>
[20]
[PDF] Modeling the Dynamics of Lahars that Originate as Landslides on ...
For our simulations, we chose two volumes: a large volume similar to that of the prehistoric Electron. Mudflow at Mount Rainier (~260 Mm3) and a smaller volume.
[21]
the early history of archaeology in mount rainier national park
Oct 18, 2004 · Rice suggested that the bone fragments were deer. The bone remains, however, may not have been deer at all. Fauna from Fryingpan Rockshelter ...
[22]
[PDF] Geomorphic Analysis of the River Response to Sedimentation ...
Heavy rainfall and concomitant large floods transport sediment to lowland reaches where the coarser material deposits in aggrading reaches and the finer ...
[23]
[PDF] Community Exposure to Lahar Hazards from Mount Rainier ...
Orting is one of many communities that are in lahar-prone areas below the flanks of Mount Rainier. (USGS photograph taken on September 8, 2009, by Nathan Wood.) ...
[24]
Earthquake Monitoring at Mount Rainier - USGS.gov
Mount Rainier seismicity has been monitored by the Pacific Northwest Seismic Network (PNSN) and CVO via a network of seismic stations located within 20 km (12 ...
[25]
Monitoring Lahars at Mount Rainier | U.S. Geological Survey
Lahar detection systems, such as this monitoring site at Mount Rainier, Washington, will become activated when a lahar is moving down a nearby drainage.
[26]
[PDF] Changes in glacier extents and estimated changes in glacial volume ...
The mass of glaciers on Mount Rainier highlights one of its largest geological hazards – lahars (Scott et al., 1995). Lahars (volcanic debris flows) have ...
[27]
Community preparedness for volcanic hazards at Mount Rainier, USA
Dec 9, 2021 · Lahars pose a significant risk to communities, particularly those living near snow-capped volcanoes. Flows of mud and debris, typically but ...
[28]
Significant Lahars at Mount Rainier - USGS.gov
This edifice collapse removed a bite-shaped section from the Osceola Mudflow crater, so that subsequent eruptive products could spill west as well as northeast.