Jökull


Jökull - 01.12.1953, Side 29

Jökull - 01.12.1953, Side 29
dirtlayered ice surface and one on a high mora- ine. Fig. 4 shows the comparative ablation dur- ing the second half of the summer. The moraine had such a protective layer of grit, pebbles and boulders that ablation was much less on the moraine than elsewhere until the end of the summer when, due to steepening sides of the moraine and long periods of rain, the moraine ablated at a much increased rate. The surround- ing glacier surface had by the end of the summer become more dirty and was losing its dirt cones by the slumping of dirt from the sides which had become too steep to retain their dirt cover. The three stakes at the different areas of detailed observation showed little difference in ablation recorded during the mid-summer, yet the ablation per hour plotted from the micro tests reveals a marked increase in ablation of clean ice and decrease in ablation of dirt cones during periods of bright sunshine. The near coincidence of the three ablation graphs is probably due to inevitable smoothing of marked differences in ablation by recording at the stakes only every few days. The stake at the dirt-cone site was not itself in a dirt cone and was thus little different from the clean ice. The stake in the dirty ice was at a surface which was a little steep and thus had melt water passing over it constantly. This caused a slight mudflow but was replenished by the dirt sludging down from ice farther up the slope of the extensive glacier snout. The clean ice surface melted 20 cms. more than the dirt-covered ice, 60 cms. more than the dirt-coned ice and 140 cms. more than the moraine-covered ice in eight weeks of late sum- mer. Rain following sunshine caused clean ice to melt most rapidly. See 27th July to lst Aug.: 21st August to 25th August; 6th September to lOth September. Sunshine following rain caused dirt covered ice to melt most rapidly. See 5th to 8th August; 9th to 14th August; 3rd to 6th September. Dirt-coned ice was rarely dominant in ablation. Those broad generalisations can- not be applied rigidly. Indeed the graph shows various anomalies but on the observations made the above conclusions were valid on this first analysis. A mathematical corroboration or con- tradiction should evolve from the calculations on heat transfer to be made in conjunction with the micro observations on ablation. Fig. 4. The comparative ablation of clean and dirt- or moraine covered ice. Samanburður á leysingu á hreinum og aurbornum is. ABLATION OF DEAD ICE. Three stakes were drilled into debris covered ice, one of which was very recently part of the glacier snout and had only a very thin dirt cover. The change in thickness of the dead ice was also measured at each point of observation on ablation. When the upper surface ablation was subtracted from the decrease in total thickness the amount of bottom melting was found. The surface ablation was 1, 13 and 7 cms. while the bottom melting was 1.5, 19 and 18 cms. re- spectively. In each case the bottom melting was greater than the top melting. The smallest difference being at the very thinly mantled ice mentioned above. In both the thickly mant- led areas the debris cover was nearly 50 cms. thick but at each site, if access could be made to permit measurement, then certainly the at- mosphere had sufficient access for some form of circulation. Much water was present under the dead ice and cauldron slumping on a small 27

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Jökull

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