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On the Formation of Snow Penitentes

Published online by Cambridge University Press:  02 May 2017

G. C. Amstutz*
Affiliation:
Missouri School of Mines and Metallurgy, Rolla, Missouri
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Abstract

An attempt is made to throw some light on the physical processes in the development of penitentes as a result of new observations in Peru and a study of the literature. This paper offers a variety of approaches to the problem rather than any final view or theory, and is therefore mostly suggestive and intended to be a program for further, more detailed research.

Zusammenfassung

Zusammenfassung

Anhand von neuen Beobachtungen von den Hochanden in Peru und auf Grund von Literaturstudien wird versucht neues Licht auf die physikalischen Einzelheiten der Bildung von Büisserschnee zu werfen. Es werden verschiedene Wege vorgezeichnet und neue Lösungsmethoden vorgeschlagen.

Information

Type
Research Article
Copyright
Copyright © International Glaciological Society 1958
Figure 0

Fig. 1Snow penitentes striking approximately east-west, on top of Volcán Tutupaca, Southern Peru. Lee side of mountain (south-east side). Elevation 5820 m. Photograph taken on 1 October 1953.

Figure 1

Fig. 2Field of snow penitentes on the shoulder just below the top of Volcán Tutupaca, Southern Peru, at an elevation of about 5800 m. Looking south, toward the smoking southern peak of Tutupaca

Figure 2

Fig. 3Snow penitentes on the east slope of Volcán Tutupaca, Southern Peru, at an elevation of about 5700 m. As in Figs. 1 and 2, the strike of’ the penitentes is about east-west. The layering is clearly visible and is parallel to the slope. A recent snowfall has partly filled the spaces between the individual penitentes. The two types of thermal absorption effects are clearly visible from the geometry of the penitentes. All penitentes are seasonal or periodic and not perennial (see Troll4, p. 27 and p. 70). The fact that the volcano Tutupaca is usually covered with heavy snow throughout the rainy season allows us to assume that the term seasonal is most appropriate

Figure 3

Fig. 4Cross section through two snow penitentes showing the reflection and capture of light in space element A and B. The size of the penitentes may vary anywhere from 1 mm. (in which case space A is only a few times the site of space B) to 3 m.

Figure 4

Fig. 1 (top)Lines of dirt cones on the upper Whakapapa Glacier. In the background melt borders of volcanic ash

Figure 5

Fig. 3 (center Left)Dirt cones along a crevasse. The ash cover is 5-7 cm, thick. Pinnacle ridge in background

Figure 6

Fig. 4 (center right)Hummocky surface on the upper Whakapapa Glacier. The hummocks developed later into isolated dirt cones

Figure 7

Fig. 6 (bottom left)Lines of submerged dirt cones, Whakapapa Glacier. In the foreground center and right the top of some dirt cones are still visible. Melt borders of volcanic ash are visible in the background

Figure 8

Fig. 7 (bottom right)Large ice cone on the saddle of the North Crater, Ruapehu. The cone has been tilted towards the interior of the crater. The thin black lines indicate annual dirt strata. The thick lines represent ash layers of volcanic eruptions Ruapehu or Ngauruhoe