In the study on ablation hollows on snow (Reference Jahn and KłapaJahn and Kłapa, 1968) published in this journal, we called attention to the characteristic, concentric arrangements of material on snow. We wrote then: “It is worth noting that in the course of dirt concentration due to ablation elongated dirt particles, e.g. grass blades or conifer needles, are arranged in such a way that their long axes follow the ridge line", and further on: “Dirt particles are accordingly arranged along these lines to form a system of concentric rings” (Reference Jahn and KłapaJahn and Kłapa, 1968, p. 306 and 307).
At that time I did not have a clear view of the problem. In subsequent years, however, I have performed a series of field experiments on the Juneau Icefield in Alaska (lat. 58° 30' N.) as well as in the Kebnekaise mountains in Swedish Lappland (lat. 68° N.). The research conducted at both of these glacio-nival field stations lasted several months. This note covers a fragment of these investigations, which will receive a full description in a later article.
The first place of observations was in the vicinity of Camp 10 of the Summer Institute of Glaciological and Arctic Sciences on Juneau Icefield. The site of the station is marked on the map published in Reference MillerMiller (1969), and the climatic conditions have been given in the paper by Reference MarcusMarcus (1964). This is on an extensive nunatak in the large ice field, the peak of which reaches 1200 m. The rocks are covered with a thick layer of firn and snow. In such a snow-field, 0.5 km from the camp, observations were carried out in August 1970. At the time the weather was fine and sunny, and the snow underwent rapid ablation at a sunny, and the snow underwent rapid ablation at a daily mean rate of 5–10 cm.
The place of the other experiments was a snow-field near the glaciological station of Stockholm University at Tarfala in the Kebnekaise mountains at a height of 1140 m (Reference SchyttSchytt, 1979). At the time of the observations, July 1982, the sky was cloudless and the air temperature reached 18° C. The daily ablation rate reached 10 cm. It is worth mentioning that it was in this region of Sweden that Reference Ashwell and HannellAshwell and Hannell (1966) carried out their studies on snow ablation processes.
Thus for both experiments the meteorological conditions were very similar. Similar too was the structure of the crystallized snow, its density being 0.4 – 0.5 Mg m−3. The experiments were very simple and consisted in placing light, oblong elements on the snow, that is objects such as blades of grass, small wooden sticks, or, most often, matches. These were arranged in different ways, e.g. in squares, circles or star-like shapes. Every few hours any changes, i.e. deformations in the arrangement were recorded. The result was unmistakable in all the cases. The objects placed on the snow had sunk into its surface and simultaneously turned in the direction corresponding or opposite to the movement of the Sun. Three hours were Sufficient for a turn to be noticed (Fig. 1), and within a 24 h period a form had developed on the snow, which has here been called a “sun spiral”.
The result was most easily noticeable where the original shape had been that of a star, e.g. matches arranged radially (Fig. 2). While the particular stages of the turn were being traced, it was found that the process took place either in one direction only or in two directions. This fact is illustrated in Figures 3 and 4.
An element placed on the snow gradually warmed and, emitting its heat, sank into the snow. If the element did not warm up evenly, if one of its ends got warm earlier, then the element sank into the snow slantwise (Fig. 5) and with a simultaneous change of direction. With the Sun turning from east to west, there exist conditions for the element to turn in accordance with the Sun's movement or against it. Different conditions appear before and after Sun culmination (Figs 3, 4). When the sky was clear all day, the prevailing turn was against the Sun’s movement. Morning sunshine caused a turn in two directions. When, however, the sky was partly clouded, the elements started to sink into the snow at different times of the day, a fact that had a decisive effect on the direction the turn was to take.
Simultaneously with the turn, a longitudinal shift of the elements may take place (Fig. 1). Below the element which had sunk into the snow there developed a trough-like depression inclined towards the warmer end. In this trough the element shifted horizontally in accordance with the direction of its axis.
At Tarfala station many of the experiments included strewing the snow surface with mineral dust. This type of thermal accelerator increased the melting rate of the snow. In the resulting hollows the elongated wooden elements (matches) were subjected to horizontal turns which, however, did not occur earlier than did the turns on clean, unsprinkled snow surfaces (Fig. 6).
The problem of ablation forms on snow has always aroused great interest. These are ablation hollows (sun cups) or ablation hillocks (dirt cones). Apart from the form of the snow surface itself, there exists the problem of regular forms developed from material deposited on the snow by wind action. This material is mostly of organic origin such as grass, leaves, twigs (Fig. 7), which often form in regular shapes. This phenomenon has most often been linked with turbulent, whirling air movement over the snow surface.
The experimental results presented here prove that independently of the turbulence factor many of these forms are derived from the direct action of the Sun's rays, which with their varying angle of incidence and their changes of direction corresponding to the Sun’s movement may by themselves suffice to initiate the development of forms that have here been termed “sun spirals” of ablation.
Acknowledgements
I wish to express my gratitude to Professor Maynard M. Miller, Head of the Summer Institute of Glaciological and Arctic Sciences, who made it possible for me to do nival research on Juneau Ice-field in 1970. I am also indebted to Professor Valter Schytt, Head of the Glaciological Station of Stockholm University at Tarfala, Kebnekaise, Swedish Lappland, whose generous permission enabled me to carry out investigations at this station in 1979 and 1980.