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Essay

Scenario Simulation of Glacier Collapse in the Amnye Machen Mountains, Qinghai–Tibetan Plateau

by
Jia Li
1,2,
Junhui Wu
1,2,*,
Xuyan Ma
3,
Dongwei Zhou
1,4,
Long Li
3,
Le Lv
1,
Lei Guo
1,2,
Lingshuai Kong
1,2 and
Jiahao Dian
1,2
1
School of Geoscience and Info-Physics, Central South University, Changsha 410083, China
2
Laboratory of GeoHazards Perception, Cognition and Predication, Central South University, Changsha 410083, China
3
Qinghai Remote Sensing Center for Natural Resources, Xining 810001, China
4
State Key Laboratory of Intelligent Geotechnics and Tunnelling (FSDI), Xi’an 710043, China
*
Author to whom correspondence should be addressed.
Geosciences 2025, 15(7), 254; https://doi.org/10.3390/geosciences15070254
Submission received: 12 May 2025 / Revised: 27 June 2025 / Accepted: 28 June 2025 / Published: 3 July 2025
(This article belongs to the Section Cryosphere)

Abstract

Simulating potential glacier collapses can provide crucial support for local disaster prevention and mitigation efforts. The Xiaomagou Glacier in the Amnye Machen Mountains, Qinghai–Tibetan Plateau, has experienced five collapses in the past two decades. Field investigation and remote sensing observations indicate that the topography and bedrock characteristics of the Qushi’an No. 22 Glacier, which is 3.5 km south of the Xiaomagou Glacier, are similar to those of the Xiaomagou Glacier. More importantly, the mass movement of the Qushi’an No. 22 Glacier since 2018 closely resembles that of the Xiaomagou Glacier exhibited before its previous collapses. Therefore, in the context of rising temperatures, it is possible that the Qushi’an No. 22 Glacier will collapse in the near future. Based on remote sensing imagery and the glacier’s surface elevation changes, we reconstructed the 2004 collapse process of the Xiaomagou Glacier via numerical simulation. The key parameters of the mass flow model were optimized based on the actual deposition area of the 2004 collapse. The model with optimized parameters was then used to simulate the potential Qushi’an No. 22 Glacier collapse. Two collapse scenarios were set for the Qushi’an No. 22 Glacier. In Scenario 1, the lower half of the tongue detaches; in Scenario 2, the whole tongue detaches. Simulation results show that, in Scenario 1, the maximum mass flow depth is 72 m, the maximum mass flow speed is 51.6 m/s, and the deposition area is 5.40 × 106 km2; in Scenario 2, the maximum mass flow depth is 75 m, the maximum mass flow speed is 59.7 m/s, and the deposition area is 6.32 × 106 km2. In both scenarios, the deposition area is much larger than that of the Xiaomagou Glacier 2004 collapse, which had a deposition area of 2.21 × 106 km2. The simulation results suggest that the Qushi’an No. 22 Glacier collapse could devastate the pastures and township roads lying in front of the glacier, seriously affecting local transportation and livestock farming; furthermore, it may deposit in the Qinglong River, forming a large, dammed lake. At present, the Qushi’an No. 22 Glacier remains in an unstable state. It is crucial to strengthen monitoring of its surface morphology, flow speed, and elevation.

1. Introduction

Glacier collapse refers to the process by which a significant amount of ice suddenly detaches from the glacier tongue, triggering an ice–rock debris flow. Such instability typically occurs in glaciers with a relatively soft bed and abundant subglacial liquid water. The ice–rock debris flow caused by glacier collapse can travel several kilometers, resulting in devastating impacts on people, livestock, and infrastructure in its moving path [1]. In recent years, multiple glacier collapse events have occurred in western China. On 17 July 2016, the Aru-1 Glacier in the Aru Mountains, in the western Qinghai–Tibetan Plateau, collapsed, with numerous ice blocks breaking off and shattering. The ice–rock debris surged toward Arucuo Lake, located 6 km downstream from the glacier terminus, generating a deafening roar. As a result, nine herders and hundreds of livestock on the opposite shore of the lake lost their lives [2,3]. On 21 September of the same year, a similar collapse occurred at the Aru-2 Glacier, located 2.6 km south of the Aru-1 Glacier. On 16 October 2018, a glacier collapse occurred in the Sedongpu Gully, located on the west bank of the Yarlung Zangbo River in Tibet. A substantial volume of ice–rock debris blocked the Yarlung Zangbo River. The barrier lake formed by the deposited debris damaged a cross-river bridge, submerged riverside roads, and forced nearly 6000 residents to evacuate [4,5]. In the 21st century, the Xiaomagou Glacier in the Amnye Machen Mountains, Qinghai–Tibetan Plateau, has experienced five collapses. The first to the fourth collapses occurred in January–February 2004, October 2007, October 2016, and July 2019, respectively, causing serious damage to downstream roads and pastures [6,7,8,9]. During the authors’ investigation of the Xiaomagou Glacier on 7 August 2024, local herders told the authors that another collapse occurred on 3 August 2024. At that time, the collapsed ice melted, forming a flood that washed away a temporary road built over the previous collapse deposits, thereby interrupting the road connecting Guigou Town and Qiemada Town in Maqin County. Since glacier collapse can cause large-scale disasters, it is imperative to conduct disaster prevention and mitigation efforts against glacier collapse. Collapse scenario simulations intuitively present the collapse process and its consequences, facilitating the assessment of the possible range and severity of a glacier collapse’s impacts. Hence, it can provide essential guidance for formulating disaster prevention and mitigation strategies as well as emergency response measures.
With the help of advanced physical models, researchers can simulate the flow velocity, path, depth, impact force, and other factors of multiphase debris in a three-dimensional environment [10,11,12,13,14]. The main debris-flow simulation models include the Coulomb [15], Voellmy [16], Bingham [17], and Manning models [18]. These models describe the movement of debris based on different frictional and rheological properties. Based on the principle of static friction, the Coulomb model simulates the resistance of debris flows using cohesion and the base friction angle, making it suitable for modeling the resistance of landslide materials [15]. The Voellmy model was built upon the Coulomb model by adding turbulent friction. Within this model, the movement of debris is controlled by both the base friction angle and the fluid velocity, allowing for a better simulation of snow avalanches and rapid debris flow [16]. The Bingham model treats debris flow as a plastic flow with yield stress. It limits the movement of debris using ultimate shear stress and viscosity coefficients and can describe flow behavior under different shear rates, making it suitable for simulating high-viscosity mudflows [17]. The Manning model is widely used for calculating the resistance and flow velocity of water and debris flows. It takes into account the influence of multiple parameters on base resistance and focuses on mass flow in complex hydraulic environments and is especially suitable for hydraulic simulations in complex terrains [18]. The selection of a model impacts the results of scenario simulation. The ice–rock debris generated by glacier collapse consists of ice bodies, rock fragments, moraines, frozen soil, liquid water, and so on [19]. The Voellmy model considers the dual effects of Coulomb friction and turbulent friction. Coulomb friction effectively simulates the resistance among solid particles such as rock fragments and moraines, which is similar to the friction generated by the interaction of different solid particles in glacier collapse debris flow. Turbulent friction effectively captures the complex interactions between the debris and the surrounding air or other media when the debris flows at high speed. Moreover, this model is characterized by flexible and adjustable parameters. It adapts well to complex terrains and is capable of predicting debris-flow path and speed based on different slopes and geomorphological characteristics [16,20]. Therefore, compared to other models, the Voellmy model is more suitable for simulating glacier collapse.
Currently, there are very few studies on glacier collapse scenario simulations. The multiple large-scale collapses of the Xiaomagou Glacier have made the western piedmont zone of the Amnye Machen Mountains a key area for geological disaster prevention and control in Qinghai Province, China. After field investigation and remote sensing analysis, the authors found that the Qushi’an No. 22 Glacier (see its location in Figure 1) shares similar terrain and bedrock lithology with the Xiaomagou Glacier. The Xiaomagou Glacier and the Qushi’an No. 22 Glacier are both located on the steep western slope of the Amnye Machen Mountains, less than 4 km apart. They share similar geomorphological settings, with cirques formed on steep bedrock walls and long, narrow tongues stretching into valley floors. Both glaciers rest on soft lithologies, primarily arkose and slate, which are prone to failure under stress. And more importantly, the Qushi’an No. 22 Glacier is exhibiting the instability that the Xiaomagou Glacier ever exhibited before each of its collapses [21], including icefall from the cirque, surge-like behavior, and terminus advance. These factors indicate that the Qushi’an No. 22 Glacier may undergo a collapse process similar to that of the Xiaomagou Glacier.
However, if the Qushi’an No. 22 Glacier were to collapse, what would be the potential flow paths, runout distances, deposition patterns, and associated disaster impacts? In order to answer these scientific questions, we conducted collapse numerical simulation via the Voellmy model and analyzed the simulation results in detail. At first, numerical simulations were conducted for the Xiaomagou Glacier 2004 collapse. The key parameters of the Voellmy model were optimized based on the real deposition area of the 2004 collapse. Then, the Voellmy model with optimized parameters was used for the numerical simulation of the Qushi’an No. 22 Glacier collapse. The mass source area was defined based on the features of changes in glacier flow velocity, and the absolute thickness of the mass source was estimated based on changes in glacier boundary and thickness. Field ground-penetrating radar (GPR) measurement was also conducted on the Qushi’an No. 22 Glacier to evaluate the estimated mass source thickness. The simulation results were then used to analyze the possible runout paths, hazard extent, and potential impacts on roads, pastures, and downstream communities. This research contributes to both the scientific understanding of glacier collapse processes and the practical needs of disaster prevention in Qinghai’s mountainous regions.

2. Study Area

The Amnye Machen Mountains, located in the southeastern Qinghai Province, China (Figure 1), are part of the middle branch of the eastern Kunlun Mountains. They are the largest snowy mountains in the source area of the Yellow River. The highest peak has an elevation of 6282 m a.s.l. [22]. Records from the Dari National Meteorological Station (at an altitude of 4000 m, approximately 110 km from the Amnye Machen Mountains) show that the average annual temperature in this area from 2005 to 2022 was −4.0 °C, with an increase of 0.3 °C per decade. The rate of warming in this area is comparable to the average level for the Qinghai–Tibetan Plateau. The annual precipitation in this area is 514 mm, with relatively small fluctuations over the past 50 years [8]. Summer precipitation accounts for 56~62% of the annual precipitation. Precipitation on the west side of the mountain is less than that on the east side [23].
The Amnye Machen Mountains nurture many glaciers. Overall, the eastern slope of the mountains is relatively gentle, while the western slope is relatively steep (see Figure 1). Several large glaciers have developed on the eastern slope. Among them, the Halong Glacier is the largest glacier in the source area of the Yellow River, with an area of 2.05 × 107 m2 in 2024. The Yehelong Glacier and Dangxiong Glacier are the second- and third-largest glaciers in the Amnye Machen Mountains, with areas of 1.76 × 107 m2 and 1.25 × 107 m2 in 2024, respectively. On the western slope, multiple cirque glaciers and hanging glaciers are developed. Most of them have steep and fan-shaped accumulation zones. Long and slender glacier tongues are formed after the mass in the accumulation zones flows into narrow valleys. Among them, the Xiaomagou Glacier and the Qushi’an No. 22 Glacier are the main study objects of this study.
The area of the Xiaomagou Glacier (RGI6.0 number: RGI60-13.23943) is 2.26 × 106 m2 (in 2024). As mentioned in the introduction, the Xiaomagou Glacier has experienced five collapses since 2004. The collapse that occurred in 2004 was the largest in scale and had the widest impact. The collapse that occurred on 3 August 2024 was the smallest in scale, but it still disrupted local traffic. According to the authors’ previous research [21], icefall in the cirque and terminus advance were observed before each collapse of the Xiaomagou Glacier. The overview of Xiaomagou Glacier is shown in Figure 2.
The Qushi’an No. 22 Glacier (RGI6.0 number RGI60-13.23947) is located south of the Xiaomagou Glacier, with an area of 1.88 × 106 m2 (in 2024). The average slope of its tongue (18.1°) is slightly lower than that of the Xiaomagou Glacier (19.7°). During the field investigation on 5 August 2024, the authors found obvious ice–rock fall traces at the junction between the cirque and the glacier tongue. The exposed ice body in the upper part of the glacier tongue is highly fragmented and is suspected to be deposits of a recent icefall in the cirque. Further down, ice bodies with relatively flat and clean surfaces, ice bodies covered with thick moraine, and ice bodies covered with thin moraine are distributed in sequence. In addition, the terminus of the glacier is steep, which indicates that the glacier is advancing. These signs are consistent with the authors’ previous conclusion drawn from remote sensing observations, that the Qushi’an No. 22 Glacier has successively experienced cirque icefall, terminus advance, and tongue acceleration since 2018 [21]. At present, a large amount of debris generated by icefall has accumulated over the tongue, and a considerable part of the debris has moved to the zone within 1000 m of the terminus.

3. Data and Methods

3.1. Data

Landsat-7, Planet, and Sentinel-2 images were used to interpret the changes in glacier morphology. The primary mission of the Landsat satellite series is Earth observation and surface change monitoring. The first satellite was launched in 1972. At present, Landsat-7, 8, and 9 are still operational. The revisit cycles of these satellites are 16 days, and all images are accessible through the USGS Earth Explorer. Planet satellite imagery is operated by Planet Labs. It includes two major series: PlanetScope and SkySat. PlanetScope consists of more than 150 CubeSats, allowing for 100–300 times of revisit per day with a spatial imaging resolution of 3–5 m. SkySat consists of 21 satellites, allowing for 40–60 revisit times per day with a spatial imaging resolution of 0.5 m. The Sentinel-2 satellite series is mainly designed for Earth observation and has been in operation since 2015. The series includes two satellites, Sentinel-2A and Sentinel-2B, capable of achieving a 5-day revisit. All images can be accessed through the Copernicus Open Access Hub.
ASTER stereo images were used to extract the historic digital elevation model (DEM) of the glaciers. ASTER is a multispectral sensor jointly developed by the Japan Aerospace Exploration Agency (JAXA) and the National Aeronautics and Space Administration (NASA). It was launched on the Terra satellite in 1999. The ASTER stereo pair includes both nadir and backward viewing images with a resolution of 15 m. The backward viewing angle is 27.6°, and the base-to-height ratio is 0.6. ASTER stereo imagery is widely used in topographic mapping. In addition, to capture the latest surface elevation changes, this study also used a UAV-derived DEM of the Qushi’an No. 22 Glacier (with a resolution of 8 × 8 cm). The specific data are listed in Table 1.

3.2. Estimation of Changes in Glacier Surface Elevation

Changes in glacier surface elevation were estimated through DEM differencing. Firstly, historical DEMs were generated from the ASTER stereo images. The ASTER DEM generation process includes the following main steps: (1) geometric and radiometric rectifications were applied to the ASTER stereo images to eliminate geometric distortions and radiometric discrepancies caused by terrain and sensor; (2) the stereo images were matched with each other to automatically generate tie-points, and an initial DEM was created from the parallax in the overlapping areas of the stereo images; (3) the initial DEM underwent filtering and interpolation to improve its accuracy and coverage; and (4) the generated DEM was calibrated using elevation control points to remove systematic errors. Subsequently, DEMs acquired at different times were matched with each other to eliminate the shifts among them. The matched DEMs were then differenced to generate an elevation change map. For the Xiaomagou Glacier, the two DEMs used for differencing were generated from ASTER images acquired before and after the 2004 collapse (4 October 2000 and 13 September 2004). In our previous study, the Qushi’an No. 22 Glacier was found to accelerate abnormally in 2018 [21]. Hence, for the Qushi’an No. 22 Glacier, the DEMs used for differencing were those generated from the ASTER image on 31 October 2018 and the one derived by UAV on 5 November 2023. To minimize the impacts of seasonal glacier mass changes, the two DEMs used for differencing were acquired in the same season.

3.3. Measuring Glacier Ice Thickness Through Ground Penetrating Radar

The thickness of the mass source is crucial for collapse scenario simulation. To verify the accuracy of the estimated thickness of the mass source, ground penetrating radar (GPR) measurements were conducted on the tongue of the Qushi’an No. 22 Glacier on 5 August 2024 (see the location in Figure 3a). The GPR system used was the SIR4000 produced by Geophysical Survey Systems, Inc., (GSSI) in Nashua, New Hampshire, United States, equipped with a 100 MHz shielded antenna (see Figure 3e). Data were collected using the profile observation method. The main data processing procedures included zero-point calibration, finite impulse response (FIR) filtering, adaptive attenuation compensation, amplitude spectrum fitting, and distance normalization. The propagation speed of electromagnetic waves in glaciers generally ranges from 0.167 m/ns to 0.171 m/ns [24,25]. The relative permittivity of the glacier, inferred from the propagation speed formula, ranges from 3.08 to 3.23. In this study, a relative permittivity of 3.1 was used for GPR data processing, which is within the aforementioned range. A total of seven measurement points were observed. The observation locations are shown in Figure 3a.

3.4. Numerical Simulation Method for Glacier Collapse

The r.avaflow 2.3 software is specifically designed to simulate geological disasters in mountainous regions, such as snow avalanches, debris flows, and landslides. This software employs a two-phase model, capable of simultaneously considering the dynamic behaviors of both solid and fluid components [26]. The Voellmy model was integrated into the mixed-phase simulation module of the r.avaflow software. Compared to other simulation tools, r.avaflow has better scalability. Through the built-in functions of validation and sensitivity analysis, users can optimize model parameters to enhance the accuracy of simulation results [10,11,27]. The Voellmy model was utilized to calculate the frictional and turbulent resistances during the mass movement.
In order to optimize the model parameters, the numerical simulation of the 2004 collapse of the Xiaomagou Glacier was first conducted. The mass source area of the collapse was determined by interpreting optical remote sensing images, and the thickness changes in the mass source area were obtained by differencing the DEMs generated from the ASTER stereo images. The turbulence coefficient, basal friction angle, and internal friction angle are key model parameters. Using the real deposition area of the 2004 collapse as external constraints and assuming independence among these parameters, adjustments were gradually made to the parameters during experiments [19]. The accuracy of the simulation was assessed by calculating the synthetic performance index (SPI). The SPI, as defined by Mergili et al. [26], was used to assess the simulation accuracy by integrating three indicators: the critical success index (CSI), the distance to perfect classification (D2PC), and the factor of conservativeness (FoC). The SPI ranges from 0 (poor performance) to 1 (perfect agreement), reflecting the empirical adequacy of the model. The Voellmy model with optimized parameters was then used for the scenario simulations of the Qushi’an No. 22 Glacier collapse. The output of the collapse scenario simulation includes the depth and velocity of the debris flow.

4. Scenario Simulation of the Collapse of the Xiaomagou Glacier

The mass source area (i.e., detached area) and the deposition area of the Xiaomagou Glacier 2004 collapse can be discerned in the optical images (Figure 4). The mass source area covers approximately 2.14 × 105 m2, and the deposition area spans approximately 2.21 × 106 m2. Within the mass source area, the change in surface elevation derived by differencing the ASTER DEMs before and after the collapse (4 October 2000 and 13 September 2004) was regarded as the glacier thickness change caused by the collapse (Figure 4). Due to cloud cover and snow/ice coverage, the elevation changes in some areas (particularly in the glacier accumulation zone) were significantly biased and were masked out. The results indicate that the thickness of the mass source area has decreased by more than 30 m. The volume of the mass released by the collapse is approximately 5.71 × 106 m3. The thickness of the fan-shaped deposition area’s edge exceeds 20 m.
According to reported glacier collapse data [13,19,28], the simulation duration was set to 150 s. After multiple experiments, various combinations of the basal friction angle, turbulence coefficient, and internal friction angle were tested. The simulation results were compared with the actual deposition area. The parameter set that produced the highest synthetic performance index (SPI), while remaining physically consistent with the known geological conditions of the bedrock, was selected as the optimal configuration. The final determined values were a basal friction angle of 5°, a turbulence coefficient of 3.3, and an internal friction angle of 10°. Figure 5 illustrates the simulated flow mass depth at different times (T = 0 s, 30 s, 60 s, 90 s, 120 s, and 150 s). The simulation results show that 90 s after the initiation of collapse, all released material exits the mouth of the Xiaomagou gully. A significant amount of debris eventually deposits between the gully mouth and the Qinglong River. Some areas exhibit a deposition height of up to 20 m, consistent with the real dam height of the barrier lake [7]. Both the mass flow depth and flow velocity peak at the gully mouth. This is reasonable because the slope suddenly reduced at the gully mouth, facilitating the conversion of substantial gravitational potential energy into kinetic energy. The maximum mass flow depth and the maximum mass flow velocity reach 33 m and 48 m/s, respectively.

5. Scenario Simulation of the Collapse of the Qushi’an No. 22 Glacier

The surface elevation change map (Figure 6a) shows that the tongue of Qushi’an No. 22 Glacier significantly thickened between October 2018 and November 2023. The thickening is particularly pronounced near the terminus, and the average thickening was up to 13.2 m. This result further confirms that the icefall in the cirque since 2018 has resulted in considerable mass loading on the tongue. According to our previous study, the Qushi’an No. 22 Glacier experienced terminus advancing between October 2018 and November 2023 (as shown in Section 5.1). Within the area that increased between October 2018 and November 2023, the increased thickness can be considered the absolute thickness in November 2023, because the original thickness in these areas was zero before October 2018. We assumed that the absolute thickness of a point in the glacier tongue in November 2023 was the sum of the maximum thickness within the advanced portion and the thickness increase at that point between October 2018 and November 2023. For a glacier tongue that is melting and retreating, its thickness generally decreases with altitude, and the corresponding flow velocity also decreases with elevation [29]. However, between October 2018 and November 2023, the tongue of the Qushi’an No. 22 Glacier kept advancing, and in 2022 and 2023, the flow velocity at the lower part of the glacier tongue had already exceeded that of the upper part (see Figure 6b). Therefore, the thickness of the glacier tongue is not likely to significantly decrease with altitude. The absolute glacier thickness at a given point ( x , y ) in November 2023 is estimated by the following equation:
H 2023 ( x , y ) = H m a x , a d v + Δ h ( x , y )
where H 2023 ( x , y ) is the glacier thickness at point ( x , y ) , H m a x , a d v is the maximum surface elevation increase within the advanced area, and Δ h ( x , y ) is the local surface elevation change between 2018 and 2023, obtained from DEM differencing.
Based on this assumption, the thickness of the glacier tongue was estimated to be between 20 and 75 m. To validate the assumption, the estimated thickness was compared with the thickness measured by GPR. The measured values at GPR points (P1–P7, shown in Figure 3a and Figure 6a) used to validate the estimated glacier thickness are listed in Table 2 for comparison. The estimated glacier thickness was found to be close to the GPR-measured thickness, with an error of approximately 7.2%.
The flow velocity of the Qushi’an No. 22 Glacier between March 2016 and December 2024 was obtained through phase correlation of optical images (Figure 6b) [21]. The results indicate that the tongue of the Qushi’an No. 22 Glacier began to accelerate in September 2018 (see Figure 6b). From September 2018 to the end of 2021, the flow velocity in the middle reach (approximately 1000 m to 2000 m from the starting point) increased from 10 cm/day to 50 cm/day. After the end of 2021, the high-speed zone gradually shifted downstream. By January 2022, the high-speed zone had completely moved to the lower reach (approximately 2000 m to 3050 m from the starting point), and the maximum velocity remained as high as 40 cm/day. From September 2023 to February 2024, a new round of acceleration occurred in both the middle reach and the lower reach. The boundary between these two high-speed zones was clear. Between February and December 2024, the flow velocity in the middle reach returned to the levels observed before June 2018; the flow velocity in the lower reach decreased notably but remained relatively high (about 25 cm/day).
Considering the distribution characteristics of surface flow velocity, two collapse scenarios were set for the Qushi’an No. 22 Glacier (see Figure 6a). In Scenario 1, the mass source area extends from the middle of the tongue to the terminus, i.e., the glacier’s lower reach that has maintained high flow velocities since 2022. The detached glacier body covers an area of 2.73 × 105 m2, with a mass volume of 1.49 × 107 m3. In Scenario 2, the mass source area extends from the entrance of the tongue to the terminus, i.e., the glacier’s middle and lower reaches that have experienced significant acceleration since 2018. The detached glacier body covers an area of 5.37 × 105 m2, with a mass volume of 2.97 × 107 m3.

5.1. Scenario 1

The simulation results of the collapse in Scenario 1 are presented in Figure 7. At T = 120 s (i.e., 120 s after the initiation of collapse), the mass source completely detaches from the glacier tongue. The ice–rock debris spreads symmetrically after rushing out of the gully mouth, ultimately forming a fan-shaped deposition area in the piedmont zone. Some debris is deposited in the Qinglong River, potentially forming a dam with a height of 8 m. About 2.9 km of the township road is destroyed by the debris flow, and the thickness of the deposit over it reaches 15 m (Figure 7g). During the collapse process, the maximum mass flow depth and the maximum mass flow velocity reach 72 m and 51.6 m/s, respectively. The impact area of the collapse in Scenario 1 is 7.19 × 106 m2, and the deposition area covers 5.40 × 106 m2.

5.2. Scenario 2

The simulation results of the collapse in Scenario 2 are shown in Figure 8. At the end of the collapse process, the mass source has not completely rushed out of the glacier tongue. A small amount of ice–rock debris (with a thickness of 5 m) remains in the glacier bed. Compared to Scenario 1, Scenario 2 has more ice–rock debris deposited in the Qinglong River. A dam with a height of 12 m may form in the river channel. The length of the township road destroyed by the debris flow (3.2 km) is close to that in Scenario 1. However, the deposit over the road is much thicker, reaching 23 m (Figure 8g). During the collapse process, the maximum mass flow depth and the maximum mass flow velocity reach 75 m and 59.7 m/s, respectively. The impact area of the collapse in Scenario 2 is 8.36 × 106 m2, and the deposition area covers 6.32 × 106 m2.

6. Discussion

6.1. Possible Triggers of the Qushi’an No. 22 Glacier Collapse

Previous studies have summarized that the collapse of the Xiaomagou Glacier in the Amnye Machen Mountains is subject to multiple factors, including the steep terrain in the glacier’s accumulation zone, rising temperatures, and soft glacier bedrock [1,6,7,9,19,30]. As mentioned above, for the Xiaomagou Glacier, icefall in the accumulation zone and terminus advance were observed before each collapse. The terminus advance indicates that the front of the glacier tongue is not frozen to the underlying bed [3]. The glacial condition of the Xiaomagou Glacier resembles that of the Kolka Glacier (Russian Caucasus Mountains), which is also temperate and experienced a series of ice–rock falls before its catastrophic collapse on 20 September 2002 [3,31,32]. The accumulation of debris from heavy ice–rock falls increased the driving stresses and caused the glacier geometry to reach the critical state [3].
Field investigation and remote sensing monitoring demonstrated that the Qushi’an No. 22 Glacier shares similar collapse-nurturing conditions with the Xiaomagou Glacier. The Qushi’an No. 22 Glacier also has an accumulation zone located on a steep slope, with the glacier bed rock primarily composed of soft lithic materials such as arkose and slate. Multiple icefalls have occurred in the accumulation zone and descended over the tongue since 2018, resulting in rapid accumulation of ice–rock debris on the tongue. The anomalous mass loading has altered the stress regime of the glacier tongue, leading to the onset of surge-like instability that further intensifies local mass accumulation [21]. Like the Xiaomagou Glacier, the Qushi’an No. 22 Glacier has been found to be advancing since July 2022, about 4 years after the first icefall event. From July 2022 to December 2024, its terminus advanced by 264 m (see Table 3 and Figure 9a). Moreover, mudflow-like fans of basal fines were found over the glacier tongue in August 2024 (see Figure 9b), which indicates high subglacial water pressure. Given the continued temperature rising, more meltwater will enter the glacier’s base. As a result, the basal water pressure will rise, and the shear strength of the subglacial sediments will reduce [32].
The Qushi’an No. 22 Glacier remains unstable. In particular, icefall in the upper reach is still ongoing, with more bedrock exposed in the higher elevations. The terminus is still advancing (Figure 9a), and the flow velocity in the lower reach remains much higher than it was before 2018 (Figure 6b). Theoretically, the temperate front is good, allowing the glacier geometry to adapt to the reduction in basal friction or the increase in driving stress. However, if the additional mass accumulation continues to be enhanced by the ice–rock fall and surge-like instability, or the subglacial water pressure soars after rainfall or strong melting, the present fragile balance of stress regime will be broken. The subglacial till will fail, and the surge-like behavior of the tongue will turn into collapse [1,32].

6.2. Potential Impact of the Glacier Collapse

Multiple collapses of the Xiaomagou Glacier in the 21st century have caused severe damage to the ecological environment and infrastructure in the western piedmont zone of the Amnye Machen Mountains. The debris flows generated by the collapse devoured pastures and destroyed the only road across the western piedmont zone of the Amnye Machen Mountains. With the local transportation blocked, animal husbandry products and necessities of herdsmen cannot be delivered in a timely manner, which directly impacts the livelihoods of local herders. Moreover, the collapse deposits blocked the Qinglong River for one and a half years, forming a large, dammed lake. A subsequent breach of this lake triggered floods [8], diffusing the impact to downstream areas.
Compared to the Xiaomagou Glacier, the Qushi’an No. 22 Glacier has a longer and gentler tongue that provides stronger buffering capability against ice–rock falls originating from the accumulation zone. However, its larger volume means a greater impact force in the event of potential collapse. The numerical simulation results indicate that the collapses in both scenarios may have significant impacts on the piedmont zone. The debris flow generated by the collapse could damage pastures and the road in front of the glacier. The deposition area may significantly exceed that of the Xiaomagou Glacier 2004 collapse (2.21 × 106 m2). The deposition in the Qinglong River could form a large, dammed lake. If the dam subsequently breaches, the lake outburst flood, mixing with the loose deposits in the river (including those from the Xiaomagou Glacier collapse), could transform into a mudflow, thereby expanding the affected area. Hence, it is necessary to maintain a high level of vigilance with regard to the changes in morphology, flow velocity, and surface elevation of the Qushi’an No. 22 Glacier.

6.3. Uncertainties in Glacier Collapse Scenario Simulation

In glacier collapse simulations, the setting of simulation parameters impacts the results. This study conducted 48 simulation experiments to test the influence of three key parameters: the turbulence coefficient, the basal friction angle, and the internal friction angle. Among them, the turbulence coefficient and basal friction angle exert a more significant influence on the simulation outcomes. The turbulence coefficient represents the turbulent resistance encountered by the ice–rock debris flow. Variations in this coefficient can alter the speed and diffusion range of the debris flow. When the turbulence coefficient increases, the resistance to the debris flow also increases, leading to a reduction in debris speed, an extension of time to exit the gully, and a change in the location and shape of the deposits. The basal friction angle determines the magnitude of friction between the debris flow and the base. A lower basal friction angle facilitates the slide of the debris on the base, thus altering its flow path and diffusion range. The internal friction angle reflects the friction between the particles within the debris flow, influencing the overall stability and movement characteristics.
The parameter value ranges tested in sensitivity experiments and the final adopted values used in the scenario simulations are shown in Table 4.
The final set of parameters was determined by minimizing the difference between the simulated and observed deposition range of the 2004 Xiaomagou Glacier collapse. The optimized parameters yielded the highest SPI, and the same settings were applied to the simulation of the Qushi’an No. 22 Glacier collapse under Scenario 1 and Scenario 2 to ensure consistency.
In addition to parameter variability, the simulation results are subject to several other sources of uncertainty; for instance, when using the r.avaflow software for simulations, the model assumes the ice–rock debris flow to be a homogeneous two-phase mixture, but the debris flow’s composition and physical properties exhibit spatial heterogeneity. Differences in the distribution of ice and rock debris, frictional forces, and flow characteristics may affect the accuracy of the simulation results. Simulating glacier collapse is more complex than simulating other types of mass flows, such as snow avalanches, landslides, and mudflows. The strength of this study lies in its ability to optimize model parameters using data from the Xiaomagou Glacier, which shares similar geological and topographical conditions with the targeted glacier. Hence, the simulated mass flow speed, impact range, and deposition thickness are relatively reliable. One key parameter in disaster risk assessment is the potential impact range [33]. Glacier collapse simulations offer valuable insights for delineating danger zones and assessing the volume of a dammed lake. However, research on glacier collapse scenario simulations remains in its early stages. Simulation methods require further development. Future studies should improve the models based on more field observations.

7. Conclusions

This study used the Voellmy model that has been incorporated into the r.avaflow software to simulate the collapse scenario of the Qushi’an No. 22 Glacier. Two potential collapse scenarios were established. The mass source area was delineated according to the spatio-temporal characteristics of the flow velocity, and the thickness of the mass source area was estimated from the combination of glacier surface elevation change and boundary change. Since the model parameters were constrained by the 2004 collapse data of the Xiaomagou Glacier, which shares a similar glacial condition with the Qushi’an No. 22 Glacier, the simulation results are relatively reliable. In both scenarios, the debris flow generated by the glacier collapse can destroy the township road and pasture in front of the glacier, and the deposits can block the Qinglong River. Due to the larger volume of the mass source, the potential Qushi’an No. 22 Glacier collapse will have a broader deposition area and greater impact force than the Xiaomagou Glacier 2004 collapse. At present, the terminus of Qushi’an No. 22 Glacier is still advancing, and the lower part of the glacier tongue remains highly mobile. With ongoing climate warming, additional mass accumulation caused by successive ice–rock fall and surge-like behavior or subglacial water pressure rise, potentially caused by heavy melting or rainfall, are possible triggers of glacier collapse. The Amnye Machen Mountains are a grand and sacred mountain range. People often pass by the Piedmont region because of religious faith and livelihood. Avoiding human casualties is the first priority of local disaster prevention and mitigation. Therefore, it is necessary to strengthen the monitoring of the surface morphology, flow speed, and elevation of the Qushi’an No. 22 Glacier via advanced field and spaceborne techniques; in the meantime, it is better to set up a disaster alert area according to the simulation results during the warm season.

Author Contributions

Conceptualization, J.L. and J.W.; Methodology, J.W. and L.G.; Software, J.W., L.G., and X.M.; Validation, J.W., J.L., and D.Z.; Formal analysis, J.W. and L.G.; Investigation, J.L., J.W., L.K., L.L. (Long Li), and L.L. (Le Lv); Resources, J.L., J.W., L.L. (Long Li), L.L. (Le Lv), L.K., and J.D.; Data curation, X.M., J.W., L.L. (Long Li), L.L. (Le Lv), D.Z., L.K., and J.D.; Writing—original draft preparation, J.W. and J.L.; Writing—review and editing, J.L.; Visualization, J.W. and J.L.; Supervision, J.L.; Project administration, J.L.; Funding acquisition, J.L. All authors have read and agreed to the published version of the manuscript.

Funding

This work was supported by the National Key Research and Development Program of China (2022YFB3903602), the National Natural Science Foundation of China (42374053), and the Natural Science Foundation of Hunan Province (2023JJ30656).

Data Availability Statement

The Landsat-7/ETM+ image is available at https://earthexplorer.usgs.gov/ (accessed on 16 August 2024). The Planet image is available at https://www.planet.com/ (accessed on 16 August 2024). Sentinel-2 images are available at https://dataspace.copernicus.eu/ (accessed on 16 January 2025). ASTER Stereo Imageries are available at https://search.earthdata.nasa.gov/ (accessed on 16 August 2024).

Acknowledgments

The authors thank the following institutions for providing materials for this study: USGS for Landsat series images, ESA for Sentinel-2 images, Planet Labs for Planet images, JAXA and NASA for ASTER images, and Qinghai Natural Resources Remote Sensing Center for high-precision UAV DEM.

Conflicts of Interest

The authors declare no conflicts of interest.

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Figure 1. Overview of the Amnye Machen Mountains. The background is the shaded DEM of the Amnye Machen Mountains. The red rectangle in the inset panel denotes the location of the Amnye Machen Mountains.
Figure 1. Overview of the Amnye Machen Mountains. The background is the shaded DEM of the Amnye Machen Mountains. The red rectangle in the inset panel denotes the location of the Amnye Machen Mountains.
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Figure 2. Overview of the Xiaomagou Glacier: (a) Sentinel-2 image of the Xiaomagou Glacier acquired on 12 August 2024. (b) Full view of the Xiaomagou Glacier. (c) Scene of the deposits of the Xiaomagou Glacier collapse that occurred on 3 August 2024. (d) Scene of the temporary road in front of the Xiaomagou Glacier being destroyed by a flood formed by the meltwater of the deposited ice blocks. (e) Waterway formed by the meltwater of the deposited ice blocks, and ice blocks washed down can be seen on both sides of the waterway (shown in the red rectangles). (f) Extent of the deposit of five glacier collapse events delineated from the optical images. (be) Pictures taken by the authors on 7 August 2024.
Figure 2. Overview of the Xiaomagou Glacier: (a) Sentinel-2 image of the Xiaomagou Glacier acquired on 12 August 2024. (b) Full view of the Xiaomagou Glacier. (c) Scene of the deposits of the Xiaomagou Glacier collapse that occurred on 3 August 2024. (d) Scene of the temporary road in front of the Xiaomagou Glacier being destroyed by a flood formed by the meltwater of the deposited ice blocks. (e) Waterway formed by the meltwater of the deposited ice blocks, and ice blocks washed down can be seen on both sides of the waterway (shown in the red rectangles). (f) Extent of the deposit of five glacier collapse events delineated from the optical images. (be) Pictures taken by the authors on 7 August 2024.
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Figure 3. Overview of the Qushi’an No. 22 Glacier: (a) planet image of the Qushi’an No. 22 Glacier acquired on 21 August 2023, (b) a photo taken in front of the Qushi’an No. 22 Glacier, (c) a photo taken in the middle of the tongue of the Qushi’an No. 22 Glacier, (d) a photo taken at the junction of the exposed ice body and the thick debris-covered ice body of the tongue of the Qushi’an No. 22 Glacier, (e) a photo of the authors measuring ice thickness with ground penetrating radar over the tongue of the Qushi’an No. 22 Glacier, and (f) a photo of the lower part of the tongue of the Qushi’an No. 22 Glacier.
Figure 3. Overview of the Qushi’an No. 22 Glacier: (a) planet image of the Qushi’an No. 22 Glacier acquired on 21 August 2023, (b) a photo taken in front of the Qushi’an No. 22 Glacier, (c) a photo taken in the middle of the tongue of the Qushi’an No. 22 Glacier, (d) a photo taken at the junction of the exposed ice body and the thick debris-covered ice body of the tongue of the Qushi’an No. 22 Glacier, (e) a photo of the authors measuring ice thickness with ground penetrating radar over the tongue of the Qushi’an No. 22 Glacier, and (f) a photo of the lower part of the tongue of the Qushi’an No. 22 Glacier.
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Figure 4. The mass source area and the deposition area of the Xiaomagou Glacier 2004 collapse. (a) Landsat-7 image of the Xiaomagou Glacier acquired on 5 August 2004. (b) The difference between the ASTER DEMs on 4 October 2000 and 13 September 2004 in the Amnye Machen mountain region. (c) An enlarged view of the area in the red rectangle in (b).
Figure 4. The mass source area and the deposition area of the Xiaomagou Glacier 2004 collapse. (a) Landsat-7 image of the Xiaomagou Glacier acquired on 5 August 2004. (b) The difference between the ASTER DEMs on 4 October 2000 and 13 September 2004 in the Amnye Machen mountain region. (c) An enlarged view of the area in the red rectangle in (b).
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Figure 5. The simulation results of the Xiaomagou Glacier 2004 collapse: (af) the simulated mass flow depth at different times, and (g,h) the simulated maximum mass flow depth and mass flow velocity. The background is a shaded DEM.
Figure 5. The simulation results of the Xiaomagou Glacier 2004 collapse: (af) the simulated mass flow depth at different times, and (g,h) the simulated maximum mass flow depth and mass flow velocity. The background is a shaded DEM.
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Figure 6. Scenario division of the Qushian No. 22 Glacier: (a) The surface elevation changes of the Qushi’an No. 22 Glacier during October 2018 to November 2023. Mass source areas under two scenarios are outlined. The background is a Planet image taken on 21 August 2023. The front position of the mass source area is the glacier terminus in November 2023. (b) The flow velocity along the central profile of the Qushi’an No. 22 Glacier from 7 March 2016 to 15 December 2024.
Figure 6. Scenario division of the Qushian No. 22 Glacier: (a) The surface elevation changes of the Qushi’an No. 22 Glacier during October 2018 to November 2023. Mass source areas under two scenarios are outlined. The background is a Planet image taken on 21 August 2023. The front position of the mass source area is the glacier terminus in November 2023. (b) The flow velocity along the central profile of the Qushi’an No. 22 Glacier from 7 March 2016 to 15 December 2024.
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Figure 7. The simulation results of the Qushi’an No. 22 Glacier collapse in Scenario 1. (af) Mass flow depth at different times. (g,h) The maximum mass flow depth and the maximum mass flow velocity. The background is a shaded DEM.
Figure 7. The simulation results of the Qushi’an No. 22 Glacier collapse in Scenario 1. (af) Mass flow depth at different times. (g,h) The maximum mass flow depth and the maximum mass flow velocity. The background is a shaded DEM.
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Figure 8. The simulation results of the Qushi’an No. 22 Glacier collapse in Scenario 2. (af) Mass flow depth at different times. (g,h) The maximum mass flow depth and the maximum mass flow velocity. The background is a shaded DEM.
Figure 8. The simulation results of the Qushi’an No. 22 Glacier collapse in Scenario 2. (af) Mass flow depth at different times. (g,h) The maximum mass flow depth and the maximum mass flow velocity. The background is a shaded DEM.
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Figure 9. (a) Changes in the terminus position of the Qushi’an No. 22 Glacier from 29 July 2022 to 15 December 2024. The background is a Sentinel-2 image acquired on 15 December 2024. (b) A photo of the authors measuring ice thickness with ground penetrating radar over the tongue of the Qushi’an No. 22 Glacier on 5 August 2024. Mudflow-like fans of basal fines can be seen within the oval.
Figure 9. (a) Changes in the terminus position of the Qushi’an No. 22 Glacier from 29 July 2022 to 15 December 2024. The background is a Sentinel-2 image acquired on 15 December 2024. (b) A photo of the authors measuring ice thickness with ground penetrating radar over the tongue of the Qushi’an No. 22 Glacier on 5 August 2024. Mudflow-like fans of basal fines can be seen within the oval.
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Table 1. Data list.
Table 1. Data list.
Data TypeAcquisition DateUsage
Landsat-7/ETM+5 August 2004Interpretation of changes in glacier morphology
Planet21 August 2023
Sentinel-21 November 2023
30 January 2024
12 August 2024
15 December 2024
ASTER Stereo Imagery4 October 2000
13 September 2004
31 October 2018
Estimation of changes in glacier surface elevation
UAV-derived DEM5 November 2023
Table 2. Comparison between estimated and measured glacier ice thickness.
Table 2. Comparison between estimated and measured glacier ice thickness.
Point NumberP1P2P3P4P5P6P7
Estimated thickness (m)65.9769.1670.4071.8273.2373.4073.93
Measured thickness (m)74.1375.0674.0074.8977.1979.3379.86
Table 3. Advancing distance of the Qushi’an No. 22 Glacier from 29 July 2022 to 15 December 2024.
Table 3. Advancing distance of the Qushi’an No. 22 Glacier from 29 July 2022 to 15 December 2024.
Time PeriodTime Interval (Day)Advance Distance (m)
29 July 2022–30 January 2023 18563
30 January 2023–21 August 202320349
21 August 2023–1 November 20237249
1 November 2023–30 January 20249036
30 January 2024–12 August 202419545
12 August 2024–15 December 202412522
Table 4. Tested and adopted model parameters in r.avaflow simulation.
Table 4. Tested and adopted model parameters in r.avaflow simulation.
ParameterTested RangeFinal Optimized Value
Turbulence coefficient (ξ)0.5–5.03.3
Basal friction angle (μ)1–10°
Internal friction angle (φ)5–45°10°
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Li, J.; Wu, J.; Ma, X.; Zhou, D.; Li, L.; Lv, L.; Guo, L.; Kong, L.; Dian, J. Scenario Simulation of Glacier Collapse in the Amnye Machen Mountains, Qinghai–Tibetan Plateau. Geosciences 2025, 15, 254. https://doi.org/10.3390/geosciences15070254

AMA Style

Li J, Wu J, Ma X, Zhou D, Li L, Lv L, Guo L, Kong L, Dian J. Scenario Simulation of Glacier Collapse in the Amnye Machen Mountains, Qinghai–Tibetan Plateau. Geosciences. 2025; 15(7):254. https://doi.org/10.3390/geosciences15070254

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Li, Jia, Junhui Wu, Xuyan Ma, Dongwei Zhou, Long Li, Le Lv, Lei Guo, Lingshuai Kong, and Jiahao Dian. 2025. "Scenario Simulation of Glacier Collapse in the Amnye Machen Mountains, Qinghai–Tibetan Plateau" Geosciences 15, no. 7: 254. https://doi.org/10.3390/geosciences15070254

APA Style

Li, J., Wu, J., Ma, X., Zhou, D., Li, L., Lv, L., Guo, L., Kong, L., & Dian, J. (2025). Scenario Simulation of Glacier Collapse in the Amnye Machen Mountains, Qinghai–Tibetan Plateau. Geosciences, 15(7), 254. https://doi.org/10.3390/geosciences15070254

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