Friction and Dynamics of Rock Avalanches Travelling on Glaciers

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Friction and Dynamics of Rock Avalanches Travelling on Glaciers

Rationale

The study of rock avalanches travelling on glaciers or glaciated areas has centred around interpreting data collected from case studies throughout history. Looking at this data can confirm that, in general, rock avalanches travelling on glaciers have a reduced coefficient of friction compared to rock on rock avalanches. The decreased resistance contributes to a higher velocity and further distance travelled. The precise reason for this behaviour is the subject of the research paper; it explains how and why the dynamics of rock avalanches on glaciers are different and creates a model that describes the specific contact between a rock landslide and a glacier.

Research into the friction and dynamics of rocks collapsing onto glaciers is particularly interesting at a point in time where rising global temperatures are melting glaciated areas and affecting the frequency of rock landslides. In addition, younger mountain ranges are more prone to earthquakes, as well as being bigger. (have a tendency to be higher, and subject to more seismic and tectonic activity, meaning that) research into the mechanics(dynamics) of rock landslides on glaciers is particularly apt. The aim of the research paper is to create a new model that effectively examines the mechanics and dynamics of rock avalanches on glacial surfaces. The difference between this research and previous work done in the same area, is that this model aims to account for the layer of melted ice between the two surfaces that is formed during landslides, and to identify a relationship between the coefficient of friction, the speed, and distance travelled.

Method

The initial part of the resea...

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... in multiple areas. Although not the main aim of the research, the findings could easily be used to estimate risk and severity of landslides in glaciated areas. A future direction for this research also points to extraterrestrial investigation, especially where satellite images can indicate certain characteristics of apparent landslides on Mars. The research could help to confirm or deny the possibility that ice may have once existed on Mars.

In terms of future work relating to friction specifically, it is mentioned there is the possibility of a fine layer of mud would result from the movement along the glacier. Mud would have a more viscous properties than the present ice/water combination, and might require further investigation. The present model also doesn’t consider the friction that occurs as a result of rocks hitting one another or breaking apart.

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