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Journal ojGlaciology, Vol. IS, No. 7B 19 77 WIND EROSION BY SNOW By R. V. DIETRICH ( Department of Geo logy, Centra l Michigan University , Mount Pl easa nt, Mi chigan 48859 , U.S.A. ) ABSTRACT. Calcite (Mohs hardn ess 3), Au oritc (hardn ess 4) and pcriclase (hardness si ) have been eroded by snow blown at moderate wind velo ci ti es, at temperatur es between - 10 and - 2S oC. Future interpretations involving ve ntifacts and apparently wind-bl asted rock exposures must take this inf orma ti on into account . R ESUM E. Erosion eolienne par la neige. De la calcite (ech ell e de durete 3), de la Auor it e (durete 4) et de la pericl ase (dur ete st ) ont subi un e erosion par de la neige souffi ee a d es vitesses de ven t mod erees, a des temperatur es a ll an t de - 10 a - 2SoC. Des interpr etations futur es comprena nt les ve nts reels et les exposi- ti ons appar ent es des rochers au souffle du ve nt devro nt t en ir com pte de ces r es ultats. ZUSAMMENFASSUNG. Wind-Erosion durch Schn ee. Calcite (H arte 3), Fluorite (Har te 4) und Periclase (Harte S,S ) wurden durch Schn ee erodiert, der bei Temp er at ur en zwi sc hen - ID und - 25 °C unt er massigen Geschwindigkeiten angeweht wurd e. Kiinftige U ntersuchungen iiber Windformen und offensichtli ch durch \Nind fr eigelegte Felsformationen miissen di ese Erken ntn is beriicksichtigen. ALONG with his summary of publish ed d at a about th e hardn ess of ice and descriptions of wind -eroded featur es spatially associated with g lac iation , Teiche rt ( 19 39, p. 1 47 ) co ncluded "There is thus no doubt that snow at low te mperatur es possesses the physi ca l prop erties required for corrasion effect s even on hard rocks". His "Iow temp era ture" r eq uir ement was based on the fact that the hardness of i ce in creas es with decreasing te mp e ratur e- for example, to 4 ( Mohs sca le) at - 44 °C and ::::::6 at - 78.5°C (for this latt er fi g ure see Blac kwelder (1939, p . 61 ». Calculations made durin g our study of ventifacts ( Whitn ey and Di e trich , 1973, p. 2577 ) indi ca te that th e relative hardness es of the missil e and th e targ et are not, as such, responsible for wh e ther there is or is not erosion. Rath er the kin e tic energy of th e missil e and the bond strength of the tar ge t mat erial dete rmin e th e res ult. This , of course, m eans th at hitting a relatively h ar d mat erial targe t with a rela- tively so ft mat er ial proj ect il e could res ult in brea ka ge of th e former as well as of the latt e r. The main contro ls would be the effective mass of th e missile ("e ffec tiv e" rather than actual because of diff ere nc es in shapes and sizes of collision surfaces), th e velocity of th e missile, angular relation ships at impact, and certain ph ys ical properti es of th e mat er ia ls in vo lve d. R ecently, I hav e completed expe rim ents that show th e reported calc ul at ions do obtain . Among the e xp e riments was one in whi ch snow was blown against cl eavage blocks of calcit e (Mohs hardn ess 3), fluorit e (hardness 4) and periclase ( hardn ess S! ). The snow had irreg ul a rl y shap ed silt-sized particles of naturall y agg lom e rated ice crystals. Th e temperatur e ran ged between - 10 and - 2SoC which indicat es that th e ice had a hardn ess ranging be tween approximately 2 and 3! . The wind ve lociti es were from 14 to 23 m .p .h . to 10.3 ms -I). Abrasion of th e mineral s used as tar gets was r ea dily apparent within a few minutes . Br ea kage of piec es from corn ers and edges of th e tar gets along with pittin g of th e fluorit e were th e obvious ma cro- scopic wind-b last fea tures. Th ese a nd microscopic featur es- all similar to those known to have been form ed by wind-blown dust and fin e silt- will be desc rib ed in a forth co ming pap er. Although th e ex perimental results support Teiche rt's conclusion th at rocks can be abraded by wind- blown snow, it do es not support his implication that such erosion occ urs only at temperatures below which the hardn ess of snow (ice) is equa l to or gr ea ter than th e ha rdn esses of th e abraded constituents of th e target rocks. Inst ead, it shows that wind-blown, relatively soft snow may be an effective tool for rock abrasion. In addition, th e experiment indi ca tes that such snow projectil es may be e ff ec tive tools even wh en imp elled by only mode rat e winds- that is, the mi ss il e fragme nts do not need to hav e velocities generally designat ed as of ga le or hurri cane strength. Brie fly stated, th e experime nt shows that p art icl es of snow blown at mode rat e wind sp ee ds may abrade rocks. This possibility of erosion by wind-blown snow shou ld be kept in mind by geomorpho- logists, glaciologists, pal eoclima tologist s and oth ers who study a nd int e rpr et occurrences of ventifacts and wind- eroded be dro c k. MS. recei ved 29 January 1976 and ill re vised form 29 March 1976 148

WIND EROSION BY SNOWWIND EROSION BY SNOW By R. V. DIETRICH (Department of Geology, Central Michigan University, Mount Pleasant, Michigan 48859, U.S.A.) ABSTRACT. Calcite (Mohs hardness

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Journal ojGlaciology, Vol. IS, No. 7B 1977

WIND EROSION BY SNOW

By R. V. DIETRICH

(Department of Geology, Central Michigan University, Mount Pleasant, Michigan 48859, U.S.A. )

ABSTRACT. Calcite (Mohs hardness 3), Auoritc (hardness 4) and pcriclase (hardness si) have been eroded by snow blown at moderate wind veloci ties, at temperatures between - 10 and - 2SoC. Future interpretations involving ventifacts and apparently wind-blasted rock exposures must take this information into account.

RESUME. Erosion eolienne par la neige. De la calcite (echelle de durete 3), de la Auorite (durete 4) et de la periclase (durete st) ont subi une erosion par de la neige souffiee a des vitesses de ven t moderees, a des temperatures a llan t de - 10 a - 2SoC. Des interpreta tions futures comprena nt les vents reels et les exposi­tions apparentes des rochers au souffle du vent devront tenir compte de ces resultats.

ZUSAMMENFASSUNG. Wind-Erosion durch Schnee. Calcite (H arte 3), Fluorite (H arte 4) und Periclase (Harte S,S) wurden durch Schnee erodiert, der bei T emperaturen zwischen - ID und - 25°C unter massigen Geschwindigkeiten angeweht wurde. Kiinftige U ntersuchungen iiber Windformen und offensichtlich durch \Nind freigelegte Felsformationen miissen diese Erkenntn is beriicksichtigen.

ALONG with his summary of published data about the hardness of ice and d escriptions of wind-eroded features spatially associated with glac iation, T eichert ( 1939, p. 147) concluded "There is thus no doubt that snow at low temperatures possesses the physical properties required for corrasion effects even on hard rocks". His "Iow temperature" r equirement was based on the fact that the hardness of ice increases with decreasing temperature- for example, to 4 (Mohs scale) at - 44°C and ::::::6 a t - 78. 5°C (for this latter figure see Blackwelder (1939, p . 61 » .

Calculations made during our study of ventifacts (Whitney and Die trich, 1973, p. 2577 ) indicate that the relative hardnesses of the missile and the target are not , as such, responsible for whether there is or is not erosion. Rather the kinetic energy of the missile and the bond strength of the target material d etermine the result. This, of course, m eans that hitting a relatively hard material target with a rela­tively soft material proj ectile could result in breakage of the former as well as of the latter. The main controls would be the effective mass of the missile ("effective" rather than actual because of differences in shapes and sizes of collision surfaces) , the velocity of the missile, angular relationships at impact, and certain physical properties of the materia ls involved.

R ecently, I have completed exp e riments that show the reported calculat ions do obtain . Among the experiments was one in which snow was blown against cleavage blocks of calcite (Mohs hardness 3), fluorite (hardness 4 ) and periclase (hardness S! ). The snow had irregula rly shaped silt-sized particles of naturally agglomerated ice crystals . The temperature ranged between - 10 and - 2SoC which indica tes that the ice had a hardness ranging b etween approximately 2 and 3!. The wind velocities were from 14 to 23 m.p.h . (~6.2 to 10.3 ms- I).

Abrasion of the minerals used as targets was readily apparent within a few minutes. Breakage of pieces from corners and edges of the targets along with pitting of the fluorite were the obvious macro­scopic wind-blast features. These a nd microscopic features- all similar to those known to have been formed by wind-blown dust and fin e silt- will be d escribed in a forthcoming paper.

Although the experimental results support T eich ert's conclusion tha t rocks can be abraded by wind­blown snow, it does not support his implication that such erosion occurs only at temperatures below which the hardness of snow (ice) is equal to or greater than the hardnesses of the abraded constituents of the target rocks. Instead , it shows that wind-blown, relatively soft snow may be an effective tool for rock abrasion. In addition, the experiment indicates that such snow projectiles may be effective tools even when impelled by only moderate winds- that is, the missile fragm ents do not need to have velocities generally designated as of gale or hurricane strength.

Briefly stated, the experiment shows that part icl es of snow blown at moderate wind speeds may abrade rocks. This possibility of erosion by wind-blown snow should b e kept in mind by geomorpho­logists, glaciologists, paleoclima tologists and others who study and interpret occurrences of ventifacts and wind-eroded bedrock.

MS. received 29 January 1976 and ill revised form 29 March 1976

148

SHORT NOTES 149

REFERENCES

Blackwelder, E. 1939. The hardness of ice. American J ournal oj Science, Vo!. 238, No. I , p. 61- 62. T e ichert, C. 1939. Corras ion by wind-blown snow in polar regions. American J ournal oJ Sciellce, Vo!. 237, No. 2,

p. 146- 48. Whitney, M. 1. , and Die trich, R. V. 1973. Ventifact sculpture by windblown dust. Geological Society oJ America.

BuLLetin , Vo!. 84, No. 8, p. 2561 - 82.