Chapter 2 Avalanches
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An avalanche is a mass of snow that slides down a mountainside. In the United States, approximately 100,000 avalanches occur annually, of which about 100 cause injuries, death, or the destruction of property. According to a database of reported incidents from 1999-2000 to 2008-2009, about 350 people per year are caught or otherwise involved in avalanches.3 Of these, approximately 90 individuals are partly or wholly buried, 40 sustain injury, and 28 are killed. Average annual property damage varies tremendously, depending on the severity of the winter. From 1999 to 2009, damages as a result of avalanches ranged from a low of $30,000 to a high of $16.5 million (median = $265,000).4 This chapter describes the properties of the mountain snowpack that contribute to avalanche formation; avalanche safety techniques; rescue; and victim physiology and treatment.
Properties of Snow
Snow Climates
In between the maritime and continental regions is a transitional snow climate that, in North America, is often referred to as the “intermountain” snow climate. Many mountain regions in this class tend to exhibit intermediate features that reflect both of the other types of climates (Table 2-1). Examples of these mountain ranges include the Wasatch Range in Utah, Teton Range in Wyoming, and Columbia Mountains of British Columbia.
Physical Properties
The density of new snow can have a wide range of values. This depends on how closely the new snow crystals pack together, which is controlled by the shapes of the crystals. The initial crystals that fall from the atmosphere have a variety of shapes, and some pack more closely together than do others (Figure 2-1). For example, needles pack more closely than stellars; thus the density of snow made of compressed needles may be three to four times greater than that of snow composed of stellars.
FIGURE 2-1 International classification of solid precipitation.
(From the International Association of Scientific Hydrology, with permission.)
At the same time, the complex and intricate shapes that characterize the new snow crystals begin to change. They become more rounded and suitable for closer packing. Intricate crystals (e.g., stellars) possess a shape that is naturally unstable and that changes quickly. New snow crystals have a large surface area–to–volume ratio and are composed of a crystalline solid that is close to its melting point. In this regard, snow crystals are unique among the materials that are found in nature. Surface energy physics dictate that this unstable condition will lead to a change in the crystalline shape toward an energy equilibrium; in other words, the warmer the temperature, the faster the change. Under very cold conditions, the original shapes of the snow crystals are sometimes still recognizable after they have been in the snow cover for several days or even after a week or two. However, as temperatures warm and approach the melting point, such shapes disappear within a few hours to a day. Changes in the shape or texture of snow crystals are examples of metamorphism, which in geologic terms defines changes that result from the effects of temperature and pressure. As the crystal shapes simplify, they can pack more closely together, thereby enhancing further settlement and strength (Figure 2-2, online).
Averaged diurnally, snow temperatures are generally coldest near the surface and warmest near the ground at the base of the snow cover, which creates a temperature gradient across a snow layer that is sandwiched between cold winter air and the relatively warm ground (Figure 2-3, online). The effect of temperature gradients is an ongoing dynamic process that can cross ice, large empty spaces filled with air, and dense snow.
Figure 2-4 shows how the texture of the snow layer changes during this temperature-gradient process. Water molecules sublimate from the upper surfaces of a grain. The vapor moves upward along the temperature (and vapor) gradient and is deposited as a solid ice molecule on the underside of a colder grain above. This process will continue as long as a strong temperature gradient exists. If the gradient continues long enough, all grains in the snow layer are transformed from solid to vapor and back to solid again; in other words, they recrystallize. The new crystals are completely different in texture and shape from their initial form. They become loose, coarse crystals with faceting, straight sides, and sharp angles (also known as faceted crystals or sugar snow), and they may eventually evolve into a large, striated, hollow-cup form. Examples of these crystals are shown in Figure 2-5. This process is called temperature-gradient metamorphism or kinetic metamorphism. Well-developed crystals that typically form at the basal layer of the snow cover are commonly known as depth hoar. Depth hoar and faceted crystals are of particular importance to avalanche formation, because these crystals are very weak, with little or no cohesion (bonding) at the grain contacts. They can form the weak layer that fails under a slab and causes an avalanche.
Equilibrium Metamorphism
In the absence of a strong temperature gradient, a totally different type of snow texture develops. When the gradient is less than about 1° C (1.8° F) per 10 cm (3.9 inches), there are still vapor pressure differences, but upward movement of vapor through the snow layers occurs at a much slower rate. As a result, water vapor that is deposited on a colder grain tends to cover the total grain in a more homogeneous manner rather than showing the preferential deposition that is characteristic of faceted crystals. This process produces a grain with a smooth surface of a more rounded or oblong shape. Over time, vapor is deposited at the grain contacts (concavities) as well as over the remaining surface of the grain (convexities). Connecting bonds that are formed at the grain contacts give the snow layer strength over time (Figure 2-6, online). Bond growth, which is called sintering, yields a cohesive texture, which is in contrast to the cohesionless texture of depth hoar and other forms of faceted crystals. This type of grain has been referred to by various terms: equilibrium snow, equitemperature snow, equilibrium metamorphism, or simply rounds. These grains can generally be described as fine and well-sintered (bonded) snow. Such bonded and interconnected grains are shown in Figure 2-7. Weak temperature gradients and high-density new snow force water vapor molecules to form bonds and thus drives equilibrium metamorphism.
Avalanche Types
There are two basic types of avalanche release. The first is a point-release avalanche or a loose snow avalanche (Figure 2-8). A loose snow avalanche involves cohesionless snow; it is initiated at a point, and it spreads out laterally as it moves down the slope to form a characteristic inverted “V” shape. A single grain or a clump of grains slips out of place and dislodges those below on the slope, which in turn dislodge others. The avalanche continues as long as the snow is cohesionless and the slope is steep enough. In dry snow, this type of avalanche usually involves only small amounts of near-surface snow. However, in wet snow, which is caused by warm air temperatures or rain, these avalanches can be very large and destructive.
FIGURE 2-8 Loose snow or point-release avalanche.
(Courtesy U.S. Department of Agriculture Forest Service.)
The second type of avalanche, the slab avalanche, requires a cohesive layer of stronger snow over a layer of weaker snow. The cohesive blanket of snow breaks away simultaneously over a broad area (Figure 2-9). A slab release can involve a range of snow thicknesses, from the near-surface layers to the entire snow cover down to the ground. Slab avalanches can occur in dry or wet snow. In contrast with a loose snow avalanche, a slab avalanche has the potential to involve very large amounts of snow.
FIGURE 2-9 Slab avalanche.
(From the U.S. Department of Agriculture Forest Service; Williams K, Armstrong B: The snowy torrents, Jackson, Wyo, 1984, Teton Bookshop, with permission. Top courtesy Alexis Kelner.)
Because dry slab avalanches are responsible for 95% of U.S. fatal accidents, these avalanches receive the interest of researchers.4 The majority of the information in this chapter deals with dry slab avalanches or dry loose snow avalanches. Because wet snow avalanches have received little research, relatively little is known about the processes that cause these avalanches. Recent research reaffirms the challenges to “observe, measure, and quantify the characteristics leading to wet snow avalanches.”32
Slab Avalanche Formation
To understand the conditions of snow cover that contribute to dry slab avalanche formation, it is essential to reemphasize that snow cover develops layer by layer. The layered structure is directly tied to the two ingredients that are essential to the formation of slab avalanches: the cohesive layer of snow and the weak layer beneath. If the snow cover is homogeneous from the ground to the surface, slab avalanche danger is low, regardless of the snow type. If the entire snow cover is sintered, dense, and strong, stability is very high. Even if the entire snow cover is composed of depth hoar, there is still no hazard from slab avalanches, because the cohesionless character precludes formation of a slab, which is one of the essential ingredients. Loose snow avalanches may still occur in this situation on steep slopes. The combination of a basal layer of depth hoar with a cohesive layer above provides the ingredients for slab avalanche danger. For successful evaluation of slab avalanche potential, information is needed about the entire snowpack and not just its surface. A hard wind slab at the surface may intuitively appear strong and safe. However, when it rests on a weaker layer that may be well below the surface, it may fail under the weight of a skier and be released as a slab avalanche. Many snow structure combinations can contribute to slab avalanche formation, but the prerequisite conditions are a cohesive layer over a weak layer sitting on a bed surface. Figure 2-10 describes other combinations that result in brittle or cohesive layers of snow on a weak layer.
Mechanical Properties: How Snow Deforms On a Slope
With regard to avalanche formation, it is important to know when snow acts primarily as an elastic material and when it responds more like a viscous substance. These conditions are shown in Figure 2-11. Laboratory experiments have shown that conditions of warm temperatures and the slow application of force favor viscous deformation. One sees examples of this as snow slowly deforms and bends over the edge of a roof or sags from a tree branch. In such cases, the snow deforms but does not crack or break. By contrast, when temperatures are very cold or when force is applied rapidly, snow reacts like an elastic material. If enough force is applied, it fractures. We think of such a substance as brittle; release of stored elastic energy causes fractures to move through the material. In the case of snow cover on a steep slope, forces associated with accumulating snow or the weight of a skier may increase until the snow fails. At that point, stored elastic energy is released and is made available to drive brittle fractures over great distances through the snow slab.
The slab avalanche provides the best example of elastic deformation in snow cover. Although the deformation cannot actually be seen, evidence of the resultant brittle failure is clearly present in the form of the sharp, linear fracture line and crown face of the slab release (Figure 2-12). The crown face is almost always perpendicular to the bed surface, which is evidence that snow has failed in a brittle manner.
To fully understand the slab avalanche condition or the stability of the snow cover, its mechanical state must be considered. Snow is always deforming in a down-slope fashion, but, throughout most of the winter, the strength of the snow is sufficient to prevent an avalanche. The snow cover is layered, and some layers are weaker than others. During periods of snowfall, blowing snow, or both, an additional load or weight is being applied to the snow in the starting zone, the snow is creeping faster, and these new stresses are beginning to approach the strength of the weakest layers. The weakest layer has a weakest point somewhere within its continuous structure. If the stresses caused by the load of the new snow or the weight of a skier reach the level at which they equal the strength of the weakest point, the snow fails completely at that point (Figure 2-13); this means that the strength at that point immediately goes to zero. This is analogous to what would happen if someone on a tug-of-war team were to let go of the rope. If the remainder of the team was strong enough to make up for the lost member, not much would change immediately. The same situation exists with snow cover. If the surrounding snow has sufficient strength to make up for the fact that the strength at the weakest point has now gone to zero, nothing happens beyond perhaps a localized movement or collapse in the snow, which is often heard as a “whumpf” sound. If the surrounding snow is not capable of compensating, the area of snow next to the initial weak point fails, then at the next, and so forth, until a propagating chain reaction begins.
Avalanche Dynamics
The topic of avalanche dynamics includes how avalanches move, how fast they move, and how far and with how much destructive power they travel. The science of avalanche dynamics is not well advanced, although much has been learned during the past few decades. Measured data for avalanche velocity and impact pressure are still lacking. Although any environmental measurement presents its own set of problems, it is clear that opportunities for making measurements inside a moving avalanche are extremely limited. Although avalanche paths exist in a variety of sizes and shapes, they all have three distinct parts with respect to dynamics (Figure 2-14). In the starting zone, which is usually the steepest part of the path, the avalanche breaks away, accelerates down the slope, and picks up additional snow. From the starting zone, the avalanche proceeds to the track, where it remains essentially constant and picks up little or no additional snow as it moves; the average slope angle becomes less steep, and frequently the snow cover is more stable than in the starting zone; however a significant amount of snow can be entrained into the avalanche from the track.40 Small avalanches often stop in the track. Larger avalanches travel down the track and into the runout zone, where the avalanche motion ends. Most avalanches stop quickly, within seconds, although very large avalanches tend to slowly decelerate across a gradual slope, such as an alluvial fan. As a general rule, the slope angle of starting zones is 30 to 45 degrees, the track is 20 to 30 degrees, and the runout zone is less than 20 degrees.
FIGURE 2-14 The three parts of an avalanche path: the starting zone, the track, and the runout zone.
(Courtesy B. Armstrong.)
In most cases, the avalanche simply follows a path down the steepest route on the slope while being guided or channeled by terrain features. However the higher-speed avalanche may deviate from this path. Terrain features (e.g., the sidewalls of a gully) that would normally direct the flow of the avalanche around a bend may be overridden by a high-velocity powder avalanche (Figure 2-15). The slower-moving avalanches, which travel near the ground, tend to follow terrain features, thereby giving them somewhat predictable courses.
FIGURE 2-15 The large powder cloud associated with a fast-moving dry snow avalanche.
(Courtesy R. Armstrong.)
Factors That Contribute to Avalanche Formation
Weak Layers
The most troubling layers are called persistent weak layers, which are usually made of snow crystals and include larger faceted snow, depth hoar, and surface hoar. These crystals are slow to change shape and gain strength, so they may persist for days, weeks, months, or even all season. One common weak layer is an old snow surface that offers a poor bond for new snow. Another weak layer that forms on the snow surface is hoar frost or surface hoar (see Physical Properties, earlier). On clear and calm nights, this hoar forms a layer of feathery, sparkling flakes that grow on the snow surface. The layer can be a major contributor to avalanche formation when it is buried by snowfall as a result of its frequent persistence in the snowpack. Many avalanches have been known to release from a buried layer of surface hoar, and sometimes this layer is more than 1 month old and 180 cm (6 feet) or more below the surface.