ENGLACIAL STRUCTURES OF THE VAUGHAN LEWIS ICEFALL, AND RELATED OBSERVATIONS ON THE JUNEJIU ICEFIELD, ALASKA. 1957 - 19.69 Thesis for the Degree of M. S. MICHIGAN STATE UNIVERSITY LOUIS RUTHARDT MILLER 1970 U) Michigan indie U ul‘V'JIJJ) East Lansing, Michiqrn .UBRARY IVIIchIgar: State University PLACE IN RETURN BOX to remove this checkout from your record. To AVOID FINES return on or before date due. MAY BE RECALLED with earlier due date if requested. DATE DUE DATE DUE DATE DUE 5/08 K2/Proj/Aoc8nPres/CIRC/DateDue.indd ABSTRACT ENGLACIAL STRUCTURES OF THE VAUGHAN LEWIS ICEFALL, AND RELATED OBSERVATIONS ON THE JUNEAU ICEFIELD, ALASKA, 1967-1969 BY Louis Ruthardt Miller Wave-ogives are defined as the three-dimensional surface wave forms found at the base of many glacial ice— falls. The morphogenesis of these wave forms is in dis- pute. Two main theories exist to explain their origin: (1) The ablation theory-~greater ablation during the sum- mer months forms a trough and the increased accumulation during winter months causes a wave-crest. (2) The com- pression theory-—wave-ogives result from a longitudinal compressive thickening at the base of an icefall, thus forming a wave during late summer presumably when com- pression is at its greatest. Measurements of englacial structures on the Vaughan Lewis Glacier, Alaska, including steeply dipping tectonic foliation and transecting thrust surfaces, plus supple— mental surface movement surveys obtained during the years 1967-1969 indicate that a longitudinal compressional stress does exist in the ice apron sector at the foot of the Louis Ruthardt Miller icefall, and indeed in the basal ice of the lower half of the icefall itself. This interpretation reinforces the argument for compression thickening. It does not, how- ever, rule out the possibility of at least some accentu— ation of surface bulges in the apron area by ablation, though this is considered to be a subordinate factor in basic genesis of these striking surface features. ENGLACIAL STRUCTURES OF THE VAUGHAN LEWIS ICEFALL, AND RELATED OBSERVATIONS ON THE JUNEAU ICEFIELD, ALASKA, 1967—1969 BY Louis Ruthardt Miller A THESIS Submitted to Michigan State University in partial fulfillment of the requirements for the degree of MASTER OF SCIENCE Department of Geology 1970 ACKNOWLEDGMENTS This study was made possible through financial and material support from the Foundation for Glacier and En— vironmental Research (FGER) via the Juneau Icefield Re- search Program (JIRP) in the years 1967, 1968, 1969, and research grants made through the Alaska Glacier Commemora- tive Project of the National Geographic Society, Washington, D.C. Assistance was also rendered by the Glaciological and Arctic Science Institute of Michigan State University and the U.S. Forest Service with the loan of surveying equip- ment. It is with sincere appreciation that thanks are extended to Professor Maynard M. Miller for his stimu- lation, encouragement, enthusiasm, and guidance both in the field and during preparation of this manuscript. Thanks are also extended to Drs. Hugh F. Bennett, Robert W. Little, and James W. Trow for helpful sug- gestions and critical review of the manuscript as the other members of the writer's thesis committee. Deep appreciation must also be extended to many of the members of JIRP, too numerous to mention, who have helped logistically. It is only through the assistance ii of these many selfless individuals that a topic of this magnitude could be approached and these results accom- plished in the main summer field seasons of 1968 and 1969. It is especially true in field research on glaciers that one's success depends on the close help and cooperation of one's colleagues. This is because not only must one work closely with them, but also one must live with and learn from them at times when one's life is wholly de— pendent on their concerns and their abilities. For this aspect as well, special thanks are extended to my field associates Dr. Alfred C. Pinchak, William Lokey, and John Schutt. Thanks are also extended by the writer to his brother, William M. Miller, and the writer's wife, Karin, for help in computer programming. iii .\.N N \w \. XI I ‘IVI TABLE OF CONTENTS Section LIST OF TABLES . . . . . . . LIST OF FIGURES. . . . . . INTRODUCTION AND PHYSICAL SETTING. . . METHOD AND AREAS OF RESEARCH . . . . INVESTIGATION OF THE VAUGHAN LEWIS GLACIER. Observations in the Crestal Névé . . Investigation of the Icefall Zone. . Morphogenetic and Structural Features in the Wave—Ogive Zone. . . . Crevasse Observations. . . . Surface Movement, 1967-1969. . . . Mass Transfer and Theoretical Considerations SUMMARY OF RESULTS AND CONCLUSIONS . . SUGGESTED ADDITIONAL INVESTIVATION . . REFERENCES . . . . . TABLES. . . . . . . . . APPENDICES Appendix A. on Cleaver West of Camp 18 . . Data 1, 23 July 1968 Part 1. Data 2, 29 July 1968 . iv Vaughan Lewis Glacier Computer Program Input Data, Taken from Survey Points FFGR #5 (Upper) and FFGR #4 (Lower) Page vi vii l7 l7 18 20 38 43 57 61 64 68 73 73 Section Page Part 2. Data 3, 8 August 1968 Data 4, 15 August 1968 Data 5, 25 August 1968 . . . . 74 Part 3. Data 6, 7 September 1968 Data 7, 27 July 1969 Data 8, 1 August 1969 . . . . 75 Part 4. Data 9, 23 August 1969 List of False Data, Substituting for Blanks for Computer Pro- gramming. . . . . . . . . 76 B. Laboratory Simulation of Vaughan Lewis Icefall Showing Mechanically Developed Wave—Bulges in a Visco—Plastic Material in a Scale Model . . . . . . . . . 77 GLOSSARY OF SELECTED GLACIOLOGICAL TERMS . . . . 81 LIST OF TABLES Fortran Computer Program, Vaughan Lewis Glacier Horizontal Movement . . Movement Computed for the Periods 23 July l968--29 July 1968 and 29 July 1968-- 8 August 1968. . . . . . . Movement Computed for the Periods 8 August 1968-~15 August 1968 and 15 August 1968—- 25 August 1968 O O O O O 0 Movement Computed for the Periods 25 August l968--7 September 1968 and 7 September 1968--27 July 1969 . vi Page 68 70 71 72 LIST OF FIGURES Figure Page 1. Map of Southeastern Alaska . . . . . . 2 2. Location Map of the Juneau Icefield . . . 3 3. Vaughan Lewis Icefall. . . . . . . . 4 4. Pyramid Pylon Marker Placed at Stake No. 15 on 6 August 1968. . . . . . . . 13 5. Stake No. 15 Area 26 July 1969. . . . . 13 6. Upper Herbert Glacier Mosaic . . . . . 16 7. Sketch Map of Wave-Ogive Crests on the Vaughan Lewis Glacier as Observed in August 1968 O O O O O O O O O O 21 8.3 Diagrammatic Reconstruction of Surface Detail on Longitudinal Traverse Across Wave-ogives K, L, and M o o o o o o 23 9. Tectonic Folia in Vertical Wall of Stream Channel. . . . . . . . . . . . 25 10. Tectonic Folia in Non—Vertical Crevasse wall. 0 O O O I O O O O O O O 25 11. Distribution of Tectonic Foliation Within Wave-Ogive J, B-Sector. . . . . . . 28 12. Distribution of Tectonic Foliation Within Wave-Ogive J, a-Sector. . . . . . . 28 13. Distribution of Tectonic Foliation Within Wave-ogive ‘K' B‘SGCtor. o o o o o o 29 14. Distribution of Tectonic Foliation Within Wave-Ogive K, a-Sector. . . . . . . 29 vii Figure page 15. Distribution of Tectonic Foliation Within Wave-Ogives L, M, N Combined, B—Sector . . 30 16. Distribution of Tectonic Foliation Within Wave-Ogives L, M, N Combined, a—Sector . . 30 17. Profile Diagram of Tectonic Folia of wave-Ogive J. a o o o o o o o o o 33 18. Ogive Section of the Vaughan Lewis Glacier . 4o 19. §§_Echelon Crevasses. . . . . . . . . 4o 20. Longitudinal Profile of Lower Icefall of the Vaughan Lewis Glacier . . . . . . 42 21. Plotted Results of Horizontal Surface Move- ment Below the Vaughan Lewis Icefall. . . 45 22. Kaolin Model of the Vaughan LeWis Icefall. . 52 23. Profile View of Wave—Ogive K . . . . . . 53 viii INTRODUCTION AND PHYSICAL SETTINGl "Ogives have puzzled generations of alpinists and their close study is long overdue, especially as their elucidation should advance considerably our knowledge of glacier movement." These are the words of William Vaughan Lewis (1956), of Cambridge University, England, whose name this glacier bears. The Vaughan Lewis Glacier on the Juneau Icefield (Figures 1 and 2) provides a classic example of the type of features Professor Lewis described. The Vaughan Lewis Glacier (Miller, 1963a), is considered to be a typical, climatologically-controlled normal discharge type of glacier (M. M. Miller, 1969, personal communication). It has been used since 1961 as a prototype on the Juneau Ice— field, Alaska for study of glacial behavior and movement within an icefall (Figure 3). The Vaughan Lewis Glacier is located in Southeast- ern Alaska at latitude 58° 49'N., longitude 134° 17'W. Its source area or névé lies immediately southeast of Mt. Ogilvie a boundary peak of the Northern Boundary Range lV. glossary on page 81 for definition of glacio- lOgical terms used in this presentation. 1 ... .. or .. )4 a a»: "’Y99% .Us 0 ‘)W/ O a. O 1 Q o .. «WV 2232 xx». \u < a as We. a“ .6 . utoésa .wb Q 9 I o . amuaa L Q. 325.23 29.3 .95 0\ b) o . \ . 50 4....» .\ av; 2.32 0 b . 0%) .238. ea 53:» 33:3: 4 (1).. 5.. .‘ awhttk ‘I’ ‘xtw 045+ JV‘J 9290 0Q 5’0 (.3 a a .. 3.80 32.2 .09. 43a ) 3. w < .— < no 6 9 , AV .2. 9 .. . w /. s .. 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The Vaughan Lewis Glacier (Figure 3) is of the glaciothermally (geophysically) temperate type with the main structures of concern in this study (surface wave bulges, wave—ogives and ogives) all lying downvalley from the mean névé-line of the 1960's. In the three years of this study the névé—line at end of summer attained an average elevation of 1277 m (4200 ft). It was as high as 1400 m (4600 ft) in the unusually warm and dry summer of 1968. In the unusually cool and stormy summer of 1969, however, it remained as low as 1160 m (3800 ft). This icefall and glacier is fed by a névé at a mean altitude of 1680 m (5600 ft) with a total accumulation 2 (8.6 miz). The icefall is area of approximately 26 km approximately 1 km (0.6 mi) wide, and drops 500 m (1500 ft) at an angle of descent varying between 24° and 40° (Figure 3). The ice depth at the base of the icefall has been measured at somewhere between 180 m (600 ft) and 210 m (700 ft) in depth (Kittredge, 1967; Prather, 1969, per- sonal communication based on 1968 seismic data). The wave-ogive area lies on the downvalley apron of the icefall where the lower Vaughan Lewis Glacier meets two other main valley glaciers. Adjacent to this icefall and on the south is an "unnamed" glacier. Immediately adjacent and to the north is the Gilkey Glacier. The framing position of these glaciers is shown in Figure 7, page 21. Each coelesces and flows as one continuum down- valley to a terminal position 15 km (9 mi) west southwest of the icefall. METHOD AND AREAS OF RESEARCH On the Juneau Icefield the Foundation for Glacier and Environmental Research has constructed a number of permanent research stations in connection with its long- term Juneau Icefield Research Program. These are aluminum- covered and usually well insulated frame structures which serve as main centers from which field parties obtain scientific data regularly each summer, including daily meteorological information at the main stations (Figure 2). The research done on the Vaughan Lewis Glacier, which is discussed in the present report, was carried out during the years 1968 and 1969. Some reconnaissance observations by the writer were also made in the summer of 1967. In all of this, Camp 18 and Camp 18B, and to a lesser extent, Camp 19 served as the main research centers. Camp 18B was a tent camp from which most of this research was con- ducted. Here two nylon mountain tents and related tem- porary field facilities, including a meteorological shelter, portable radio, etc. were used. Camp 18 is a more permanent installation, comprised of several build- ings. This was used as the radio relay station and permanent logistics base, and as such was revisited about once a week to replenish needed food and supplies at Camp 18B. Camp 19 was also employed. This camp has a single 2 (12 ftz) wood structure and metal-sheeted building 4 m situated on bedrock of a high berm at 1160 m (3800 ft) elevation. Its location faces the icefall on the south— west and lies 1.6 km (1 mi) distance from it. This camp was constructed in the spring of 1968 as a base for re- search not only on the Vaughan Lewis Glacier but also in the downvalley area of the lower Vaughan Lewis-Gilkey Glacier System. In the present study it was used as a station for working the lower glacier area, and especially in connection with movement data taken from the berm of Mt. Grosvenorl (Figure 2). Observations and measurements of the internal structures of the Vaughan Lewis Icefall were taken within natural Openings at the glacier's surface, especially in crevasses and stream channels (Figures 9 and 10). Measure- ments of strike and dip were made using a Brunton compass. Linear distance measurements were taken with a 100 ft lProvisional place name suggested in honor of Gilbert Hovey Grosvenor, National Geographic Society Presi- dent, 1920-1950. This is in recognition of the National Geographic Society which has provided prime support for regional glaciological studies of which this research is a part. (30.5 m) surveyor‘s chain (tape),1 and a 10 ft (3.05 m) carpenter's tape. Movement data were obtained with a Wild -T2 theodolite using triangulating methods from a base line the length of which was determined with an Invar Subtense Bar. Three meter (10 ft) sections of thin-wall electrical conduit were used as movement stakes. These proved to be easier to place in 3 cm (1 in) holes than the previously used 8 cm2 (2 in x 2 in) wooden stakes. Also by having a galvanized finish they did not ablate out as fast as wooden stakes with a lower albedo. The conduits were placed on the glacier at pre-selected points along each movement profile. They were drilled into the ice or firn pack to depths of 2 m (6.5 ft) either with a 2.5 cm (1 in) SIPRE drill or a 4 cm (1.5 in) Norwegian type hand drill. Later in the field season when bare ice was exposed the Norwegian "¢strem-type" drill was wholly used. Tape measurements were also taken along the SlOpe from movement stake to stake. After a few weeks, some of these stakes had to be reset to their initial vertical position. This was done by deepening the drill holes with an apprOpriate auger. This, of course, corrected for tipping due to ablation. Movement stakes aligned in strain-diamond patterns were 1Unfortunately these data were taken in feet and fractions thereof. In research of this kind the metric system is much preferred; however, the metric chain antici- pated was not at C-18 at the beginning of this study, and so for consistency the English tape continued to be used. Conversions are made in the following pages. 10 also implanted with measurements taken from carefully marked points on each stake. And similarly about every seven to fourteen days these movement stakes had to be redrilled because of ablation effects. Various types of smaller pegs in strain-diamond patterns were also installed in horizontal positions on vertical crevasse walls. The data obtained from these proved to be of little value. The reason for disappoint- ment here relates to a number of practical problems, mostly allied to ablation. For example, the installation of wooden dowels into horizontally drilled holes was tried first, then nails were driven into the ice. In each case methods to induce freezing around the markers failed. It was determined that any foreign material, wood or metal, would increase ablation around the marker and thus fall out before adequate records could be made. The best method was found simply to drill a hole and measure from its center. The error encountered, however, was of the same order of magnitude as the movement expected and so the results are so far inconclusive. With more time this method might prove to be of value if one applies a sta— tistical mean movement analysis. Toward the end of the 1968 field season, a new method was tried for the surface movement surveys. In this a pyramid pylon (Figure 4) was constructed to hold a movement stake more permanently in place, that is without necessitating redrilling the bore—hole. The ll pylon was also invoked to hold the stake perpendicular in spite of subsequent ablation. The technique was a modifi- cation of the movement tripod method used in many previous JIRP seasons. The pylon was constructed from 1.5 m (5 ft) sections of building material, put together in such a way as to form a pyramid with four triangular faces. The de- vice proved to be very effective. In July, 1969 the pylon which had been placed on survey point no. 3 in July, 1968 (wave—ogive K), was still holding its movement stake in a vertical position. Another pylon, however, placed at stake no. 15 in the upper apron area (Figures 4 and 5) could not be relocated during the 1969 field season. This one was assumed to have drOpped into a crevasse or to have been crushed by winter snow. It is probable that the existing pylon at survey point no. 3 was sturdy enough to withstand very high winds1 during the winter because the complete structure, except for the lower 15 cm (0.5 ft) was extremely abraded from the effects of wind-driven snow. Also, this would seem to indicate that little accumulation occurs on the crests of wave-ogives in the autumn, winter, and spring months, i.e., generally mid-September to late-June. Sequential movement records were taken on stake no. 3. Although not discussed lWind velocities of 128 km/hr (80 mi/hr) were re- corded at this site in September before the close of the field season. Velocities at various other icefield stations have been recorded in excess of 160 km/hr (100 mi/hr). 12 Figure 4.--Pyramid pylon marker placed at stake no. 15 in the summer of 1968. (Photo by L. R. Miller, 6 August 1968.) Figure 5.--Stake no. 15 area late i . n the summer of 1969. (Note absence of pyramid pylon to right of cloth phototheodolite marker.) . Glacier flow is f right. (Photo by L. R. Miller, 26 August 132? left to 14 in detail in this report, these data will be useful for comparison with future measurements. To better evaluate the nature of glacier movement and surface changes within an icefall, a unique and rather unorthodox program involving crevasse "seeding" was inaug- urated on 12 August 1968. In.this, sections of damaged triangular radio tower and a total of fifty-two rectangu- lar five-gallon gas cans (numbered with red paint) were dropped 30 m (100 ft) apart in two large crevasses at the tOp of the fall zone on the Vaughan Lewis névé--about 1620 m (5300 ft) elevation. For future reference a docu— mentation of locations of these markers is given in the 1968 Camp 18 log. The markers were positioned as a reference for obtaining velocity data at a later time. Everything de- pends, of course, on the cans subsequently becoming ex- posed by ablation further down glacier. With a knowledge of their initial position and depth--approximately 27 m (90 ft)—-it is hOped that we can then gain a better insight on the structure and ice flow within the icefall, as well as information on the effects of ablation.l 1That these markers will eventually become exhumed by ablation is indicated by a unique situation recently reported by M. M. Miller (personal communication) from the American Mount Everest Expedition of 1963. Certain items deposited in a crevasse of the Khumbu Glacier Icefall in March, 1963 were subsequently recovered on the surface of the ramp-slope (apron) of the icefall more than 1.6 m (1 mi) downvalley seven years later, i.e., in October, 1969. It will be highly significant, however, if this does not occur on the Vaughan Lewis Glacier a few years hence. 15 With respect to englacial structures in the ramp area where these movement data were obtained, apparent dips in the tectonic foliation were measured in the first five wave-ogives found in the ice-apron area below the icefall. These measurements were made in existing openings and fissures in the ice surface, including longitudinal crevasses, splaying crevasses, and meltwater runoff chan— nels. Such features permitted observations to depths of 20 m (64 ft). The mean lower limit of actual measurement was at about 10 m (32 ft). From the tectonic foliation, inferences can be drawn about the structural stress and strain distribution within the ice, as will be discussed later. The upper Herbert Glacier (Camp 16 arm) on the west side of the Juneau Icefield (v. map in Figure 2 and photo in Figure 6) was also studied in 1969 in a similar manner, although more in a reconnaissance fashion as this was the first field season in which that glacier was ex- plored by members of JIRP. This activity was carried out from Camp 16, at 1590 m (5200 ft) elevation at the upper Mendenhall-Herbert Glacier névé. Aspects of this study too will be discussed in the following pages. 16 A.moma umsmsa v .umaanz .m .q an ouozmo .umm mo mpflm cnmfiuuo: co cowumum mw>usm xooupmn HmHflawm mm>Hm0Iw>ms mcw30£m «Sum ma QEMOV Hmfio mauDOm on» Unm3ou mcHxOOH .Hmwomam Scum cmxou 3mH> .mfl3wq Gwsmsm> Op mam pnmnnmm Hmmmbll.m szmwm INVESTIGATION OF THE VAUGHAN LEWIS GLACIER The Vaughan Lewis Glacier has been divided into five glaciomorphic sectors-—the crestal névé or prime accumulation zone, the icefall zone, the wave-ogive zone (wave-band zone), the ogive zone, and the terminal sector (Freers, 1966). Observations in the Crestal Névé The source névé or prime accumulation zone of the glacier lying between 1700-1800 m (5600—5900 ft) is not of major concern in the present study. Information concern- ing firn stratigraphy and glaciothermal conditions has been reported by other researchers for this and the adjoining zone of the Taku Glacier (Miller, 1952, 1963b; Freers, 1966). In addition, surface movement data have been ob- tained in this zone but are not discussed here as they do not bear directly on current studies of structural fea- tures below the icefall (Miller, g£_al., 1968). In 1968, however, a detailed study in the lower névé which adjoins the upper icefall zone was made empha- sizing the sector just above the change of gradient in the fall zone. The purpose here was to determine the type and 17 18 proportion of firn and glacier ice and to gain some in— sight into the nature of primary structures in the glacier. Crevasses were examined down to a depth of 27 m (90 ft), as near to the fall zone as practical and safe. This was done to determine if the structures observed below the icefall and especially within the wave-ogives are of subsequent or secondary deformational origin or of primary stratigraphic origin. The material observed varied from new to old surface snow to dense firn. It is of signifi- cance that no glacial ice or foliation structures were observed, even on exposed crevasse walls. The only pri- mary structures found were dust layers (annual ablation surfaces) and various diagenetic structures such as ice strata (bands), ice glands, and ice lenses formed gener- ally parallel to initial bedding in the firn by the re- freezing of percolated surface water. It is emphasized again that nearly all of these features were planar in form, having horizontal orientations and distinguished quite easily from the tectonic folia found in wave-Ogives well below the icefall. Investigation of the Icefall Zone The icefall zone is defined by Freers (1966) as that area below a point where crevasses are seen with their downglacier walls lower than their upglacier walls, i.e., essentially the serac and bergshrund zone. This zone has been noted to lie within the 1675 m (5500 ft) to 19 1225 m (4000 ft) range, and as such has been the object of intensive study by Pinchak (1968) with respect to the periodicity and cause of diurnal avalanches. Between 1964 and 1968, photogrammetric surveys have been made of the Vaughan Lewis Icefall including, of course, the acquisition of comparative photographs. These photos also cover the wave-ogives and ogives from selected base-lines and glacier-surface stations (Chrzanowski, 1968). They have been obtained with a Wild P-30 phototheodolite and are currently the base for a large-scale map of the icefall and apron area being plotted by Dr. Adam Chrzanow- ski and Professor Gerhard Gloss at the University of New Brunswick. The glass plates have also been helpful in the writer's study of annual changes in the nature of the morphogenic features below the icefall. At the t0p of the Vaughan Lewis Icefall there are large curvilinear tension crevasses which degenerate down— ward into a pronounced zone of seracs and ice pinnacles. Within this area much avalanching occurs. During 1968 and 1969 as many as seventy-five avalanches were recorded in a single twenty—four hour period. Although the crevasses at the head of the icefall are wide and deep and so could be investigated directly, because of avalanch- ing none could be investigated within the icefall (Figure 3). A similar role for avalanches was found to character- ize the upper Herbert Glacier (Camp 16 arm) icefall near Camp 16 (Figure 6), proving that both of these glaciers 20 are vigorously discharging through their icefall outlets from their source névés. King and Lewis (1961), in reference to the Odins- breen of the Norwegian glacier Austerdalsbreen, have sug— gested that in such instances crevasses may extend down— ward to the bottom layers of ice and into less disordered ice masses which survive ablation in the icefall and thence are moved downslope to the ice apron area below. This has not been observed by the writer or others on the Vaughan Lewis or the Herbert Glaciers (Freers, 1966; Kittredge, 1967). Actually what this entails is that only shallow crevasses survive in the icefall zone and that these become largely filled with slump material, and hence in general obscured. Freers (1966) has cited evidence that a few do survive into the apron and wave-ogive zone. This sub- stantiates the writer's view that such crevasses do not extend into ice at the bed of the glacier. Morphogenetic and Structural Features in the Wave—Ogive Zone The three-dimensional wave-ogive forms in the apron below the icefall (Figure 3) are the main focus of attention in this study. Downglacier these surface waves or bulges attenuate to form two—dimensional ogives (Figure 18). For reference purposes the wave-ogives are lettered in a downglacier sequence (Figure 7), starting 21 MO'OII ES bedrock modlol naming E "on o! wove-o3“. E5: survey "all. [3 Nov-no lino: VAUGHAN LEWIS GLACIER Angus! '96. Figure 7.--Sketch map of wave-ogive crests on the Vaughan Lewis Icefall as observed in August 1968. 22 with J, which designates the uppermost wave-ogive studied in 1968-69. By starting at a midpoint in the alphabet it will be possible in the next few years of this long-term study to extend the series by adding I, H, etc., as new wave—ogives develOp at the base of the icefall and without changing a numbering system each year. In Figure 7 the present sequence downglacier is labeled as J, K, L, M, N, O, and P. Wave-ogive P refers to the end of the dominant surface bulges designated as wave-ogives observed in August 1968. The amplitude of the wave—ogives on the Vaughan Lewis varied from 25 m (82 ft) at the base of the icefall to 0 at a point about 2 km (1.2 mi) downglacier (Figures 8, 20, and 23). The wave length of the wave-ogives varied from 90 to 150 m (288-480 ft). Maximum amplitude could at no time be accurately measured without drilling a test hole because winter snow in the intervening troughs had not totally melted, even by the mid-September end of the ablation season in 1968 (v. Figure 23). In 1969, the situation was worse because new snow arrived and remained at this level by mid-August--1969 being the year of heavi- est summer accumulation in the whole of the past twenty- five years of record on the Juneau Icefield. As originally suggested by Miller (1952) and sup- ported by Kamb (1964), the key to understanding wave-ogives and ogives will come from studies of their internal 23 .mzmsouu new mummno m>m3 mo cowuwmom on w>aumamu mnmuma ca mo aummp ou coauwHHOM cacoyomu mo map mcfl3onm an musmflm .>V 2 was .A .m mm>amOIm>63 mmouom mmum>muu HmcflcsuwmsoH so meump mommusm mo cofluosuumgoomu owumEEMHmMHntl.m whamfim locates: Jufltucum. z .032»: .— .0933. 24 structure, particularly at depth. Thus in this present study, primary attention is given to the nature and origin of the tectonic folia. Tectonic foliation is a term first suggested by Miller (Glacier bands, conference on terminology, 1953; also v. Miller, 1952, 1955; and Taylor, 1963). As defined in this study these are planar or foliation structures produced by shear or compression and consisting of alter- nate zones or seeming layers of fine and coarse-grained ice. In some cases, grains of ice and trapped air bubbles are elongated in the plane of the layer (Figures 9 and 10). Rigsby (1958) and Kamb (1959b) have indicated that both polar ice and temperate ice show a single maximum crystal orientation (rather than the two areas of concen- tration from the possibility known in biaxial ice crystals). In other analyses, Gow (1964) has shown two, three, and four maxima, but for the present analysis the probability of a single maximum is emphasized because of the strong unidirectional stress suggested by the geometry of the present case. In this analysis (v. Kamb, 1959a) the c-axis orien- tation would be centered about the pole. Thus a single area of concentration of the c-axis perpendicular to the basal plane or plane of foliation is determined and plotted. The point where the perpendicular to this plane intersects the projection sphere is called the pole of that plane. 25 A.mmma um nose v .umaaflz .m .q mn ouonmv .mflaom mo QHU pamOAMHcmflm mamm>wu mcflnum no mswmcmn mmmmfiou Scum mafia m>wm01w>w3 Houomm :0 ommomxm mm ma Hmoauum> umnu muoz .M In HHM3 mmmm>wuo mcfluuSUImmouo How oacouomall.oa wusmflm fli x.mmma umsms4 hm . whom one .umaawz .m .4 an ouonmv 3 . Eonm hHHmoflprb mcwmsmn mxm 00H muoz .2 m>HUOIm>m3 mo Houummlm mawuuso Immono Hmcgmno Emmnum mo Hana HMOfiuHm> CH mwaom oacouomall.m mnsmflm 26 Kamb further states that the recrystallization of glacier ice in situ during glacier flow will give a preferred orientation of the c-axis normal to the foliation planes. On this basis the basal planes of the individual hexagonal crystals would be parallel to the folia. Such orientation minimizes the chemical potential which is required for equilibrium across the plane normal to the greatest princi— pal axis of stress. Such a comparative relationship has been studied previously in this region, in fact on the adjoining Taku Glacier where deep drill core samples were analyzed by Bader in 1950 (Miller, 1963b). From this three-dimensional field study of crystal fabric it was determined that from the surface of the Taku Glacier to 42.5 m (140 ft) the c-axes of the natural ice crystals were preferably at low angles to the horizontal, but without any azimuth. Below 42.5 m (140 ft), the c-axes were still preferably hori- zontal but in successively deeper samples to the base of the bore, a progressive crowding of azimuth values was observed towards a line of unknown orientation (presumably, according to the above noted discussion, this would be normal to the direction of "flow"). From this morphogenic relationship given by pre— vious investigators of basal plane foliation (tectonic folia) and related planar structures (Bader, 1951; Risgby, 1958; Kamb, 1959b; Miller, 1963), it was concluded that fabric data from thin sections of Vaughan Lewis ice are 27 not mandatory for purposes of the present study. Also it was realized that the effort required in obtaining such information in the field time available would have limited the areal extent of the ice structure investi- gation. Thus, by using this seemingly relevant c-axis to foliation relationship, an attempt is made to plot the orientation of measured tectonic foliation. In turn some apparent conclusions are discussed. In Figures 11 through 16 strike and dip orien— tations of measured folia are plotted using the lower hemisphere of an azimuthal equal-area (Schmidt) projection (Billings, 1954). Such a technique has been successfully employed by Untersteiner (1955) on the Pasterze Glacier of the Grossglocker in the Eastern Alps. Wave-ogive J on the Vaughan Lewis Glacier (Figure 7) is referred to as a "pre-ogive" because it did not have a well-developed trough on the upglacier side. Here the orientation of folia varied in true dip from 34° down- glacier to 17° upglacier; however, it must be stated that most were very steep dips, i.e., within 20° of perpendicu— lar. Below this, each wave—ogive was arbitrarily divided into two sectors using the crest of the wave as the divid— ing point. With this point of separation, structural relations on each half of a wave could be more accurately determined with respect to changes in the surface con- figuration of each limb of the wave. 28 .3ouum an omumowpcw cofluomufip 30am .uowomamms E H.o~nlm>mz mo ummuo .NH wusmwm .uwwomaquop E H.mmltw>m3 mo smouu .HH musmam h m>am01m>m3 ca mwaom mo meowumusmwuo map was mxflnum mo cowusnflupmwo .mmnmaa qcapmaaoh you umnsopnoo mmHom vqaom no mnoapmnanoonoo pomonmm :26. so.-. 3.... x.-. X?“ .25. 'eesmalflu PF mnsmym mp mnswam 29 .zounm an omumofiocfl cofluowufip 30Hm .HmwomHmms E m.m¢|lm>m3 mo ummnu .wa wusmflm .Hmaomamc3oo E v.avllm>m3 mo ummnu .MH wusmwm .M m>am0um>m3 :H MAHOM mo mcoflumucmwuo map was mxfluum mo coflusnflnumflo .mosmao :cavmaatm you cohsopnoo mwaoa «mace no mnoapmupuoonoo unmouom a?! so... x.-. x.-. so." an... m— onsmam 30 .30num an topmofipsfl cofluomnflp 30am .Hmfiomamms E a.mm|so>m3 mo ummHO .ma mnsmfim .umeomHmcsop E N.Mh:tm>m3 mo ummuo .mH musmflm .2 tom .2 .q mm>metm>m3 ea mflaom mo mcoflumusmfluo map was mxflnum mo cofiusnflnpmflp pmcanfiou .mmsmao ecaumaaou you nmuzopsoo peace peace Ho mooaumhmeonoo unmohom :2... so... x... x.-. a?" an... I see W a a mu m. ohswam m_ ohsmam 31 As noted above, the folia distributions were plotted on a Schmidt net, a projection which is true to area. For clarity each limb of the wave-ogive was con- sidered separately. The data from the wall exposures of several crevasses radiating across the wave-ogives make up the total for a single projection. Thus the strike and dip of either exactly 100 or 150 measurements consti- tute the point poles used to construct each Schmidt pro- jection (again refer to the following Figures 11-16). In many cases the bands or tectonic folia were found to be distorted, faulted, fractured, and sometimes bifurcated. In each instance, the most linear and distinct section was used for measurement. Each dip reading was taken with a possible error factor of 12°. This figure includes both systematic error and random error, viz., the result of instrumentation and human limitations--and as such, are subject to the laws of probability. By using a percentage distribution, as shown by area on a pro— jection, each single reading represents only 1 per cent or less of the total information, and therefore any ex- tremes, either unique or by personal error, do not affect the general trend. As can be seen in Figures 11 through 16, the direction of folia seem to be in no way irregular or random. There is a misleading aspect here when one looks at the distributions in Figures 11 through 16. This is 32 because each figure is a representation of one or the other limb of a wave; viz., those folia which are near the centerline of a wave-ogive crest are either on one side or the other of this centerline and thus are divided between each half. This division lessens the total number in each half having a dip near the perpendicular and hence gives a misleading overall percentage near the edge of the Schmidt projection (especially note Figure 11). For purposes of this analysis the true dip angles are extended artificially to depth as is done in Figure 17. Note in this figure that below the limiting depth of observation the extension lines are dashed. The purpose of extending these lines is to better compare the relation- ship of adjacent dips and to see whether there is any possible point of focus. This figure combines the foli- ation dips as a generalized composite of data geometrically representing information from separate but sequential traverse lines. In this, we see that (v. Figure 12) the tendency is for most of the folia to dip downglacier in the trailing or upglacier sector of a wave (hereafter referred to as the d-sector). Conversely in Figure 11 we see the dip to be generally upglacier in the leading or downglacier sector of a wave (hereafter referred to as the B-sector). Again it is stressed that the exten— sion of the folia lines in Figure 17 does not imply that these structures in nature extend in this manner at depth. In fact, it is further noted that indeed this 33 .uxmu on» CA pmmmsomflo m H. mgmmv A 0:.H U mmmm>OHO 3OH® E o uHEHH map . was .HMMUHMfluHm mamnsm we pcmeHsmmmoOWSmomE mmmfla MAHOM Hamz . musm soamcmuxm HHSM mono: .mcoN mommnsm . m usmEm>QE um h m>HmOIm>m3|t ha coauMHHOM mo map mawBOSm .e .oc wxmu . - / I /’v.\. y —1 u 1 . 111 1.1\ 1 1.\ \ 1.11 11:.1w611/flz/ C13. 1 1.11 . “1 1 11 ~.\\1 . \1 \\ 1 1 1. 1 11! \/ // .1. fl .. 1 2 .1 1 1 .. .... _ 1.1x 1 1.1. .1 ....m. 1119‘ :1. 1:1. an... . 11 1 .1\ 1 1\g\ 1 11 . . wr11 1.; ,, ,2 .1. . -... 111.1 1.1.1.11». 1\1.\1.1 1 11 1.1. 1:? 111 / zl/x/xaz1m1 1 ... .v; 1 \ —\\ \~\ 1 11 \1 11\\ 1.1.1 y N N ‘— fl ’1! II I 1/r‘ff— -. ._ \ - \V \ 1.1111111. 011... 1.1.. 17.112131: 7.2/61... 1 ”\\\‘\\1 1\ 1 \ \1—..\. 11111-1... 1 _ ////§~a“z 1. 1~1\111 \ 1 .1 1~\.1\ 1 Z»: 11 1 \vAa/z 3,. . 5‘ 11 1‘ _ 11 1‘ § 11. .u 1 \\ ' l4 3' ../,/\ 3‘11 1\ 1 1 \.»\1.1‘ ~ 1 .1 1. \ *\ z I. '61. I. I“ 13.1\\ 1 11 \x 1.1... 1 11 F 1‘1. k W 1 raw/‘11”; .1 1/ 5.1.2.3.: 1¥x 1 1 x111.\\ 1.... .111 1x. 1 1: 1 firs... . ...x . ‘1 \ I case: 1!.\ 1 \+1 %n\1$.. 1311“ " .144Wfir/x \ . \\ 1 1 x 1. 11 .1 1. 1. 1 1. a 1 1. n. .../#1142; 1. ,. l . 1 \ 1 _.1 _ _ 1 "...... AVIS/VII I .. ...-0 30.3w .:*05L E05 00 83: .1: II I I \- 1 ///. 1 - . --Ii)- .00 ‘1 ‘l‘ “‘ I“ 0" V): —--r-‘- o— cozuom 301U o mmomnsm was H ma nummp on m am ('w) H1630 34 manner of plotting revealed no apparent relationship in nature allied to such hypothetical focal points as the intersections of these lines might imply. In Figure 17 a wide range of dips is represented. The highest percentages, however, center around 70° dip on each limb of a wave—ogive. The strike of these folia is essentially parallel to the arcuate centerline of the wave-bulge--i.e., roughly parallel to the trend of the wave-ogive crest. The values recorded do not vary more than :10° from this centerline, with a mean variance of :3°. The amount of error in strike is considered to reflect human error in the method of measurement rather than inherent differences in value. Here the mean variance is greater because of the irregular surface upon which measurements were taken. One factor is the direct exposure of these surfaces to atmospheric pro- cesses, producing much greater ablation on horizontal sur- faces than on crevasse walls. A further consequence is that glacier ice on these top surfaces is more bubbly, making the strike of specific foliation zones more diffi- cult to distinguish and trace. In the distal or B-sectors the folia in longi— tudinal cross-section have a tendency to be either concave or convex downglacier; i.e., the deeper folia at the same distance from the centerline of a crest are found to have either larger or smaller angles to the horizontal in com- parison with their surface dips. With all folia at a 35 rather high dip to the surface and with lesser dips on distal B—sectors, an asymmetrical appearance is created by the B-sector of each wave-ogive. This asymmetry is greatest in wave-ogive J (which we see in Figure 20, with wave-ogive J and K, left and center, reSpectively), sug- gesting overthrusting or underthrusting effects. Indeed on several crevasse wall profiles truncating overthrust surfaces have been observed (Miller, 1958). According to Billings (1954) this would be similar to the layers in metamorphic rock1 which have yielded the most under a given stress as in the forward B-sector of a wave—ogive, and therefore show greater deformation. In various places there are non-continuous lines of folia cut by more strongly developed lines of foliation at slightly different angles. Such foliation has been observed by Chamberlin (1928) and also Perutz and Selig- man (1939) along the margins of glaciers, and has been related to differential movement and shearing. It also suggests deep ice translation into new stress fields as the glacier flows downvalley. From the predominance of cross folia in the B-sector of most wave—Ogives studied, one might conclude that in some cases high angle over- thrusts or underthrusts have indeed developed. There is usually well—marked foliation throughout the entire wave-Ogive. In some areas it appears rather lGlacial ice is technically a metamorphic rock. 36 jumbled, possibly because of the presence of avalanche material which has not yet become consolidated. This dis- orientation becomes less as one proceeds downglacier from wave-ogive J to wave-ogive N. As stated previously, the folia dip angle in wave- Ogive J surface ice ranges from 34° downglacier in a- sector to 17° upglacier in the B-sector. The total range of similar dips in a— and B-sectors, respectively, of wave- ogive K; are 51° and 28°, 62° and 42° in L, 70° and 38° in M, and 67° and 71° in N. These are the extreme dip values (i.e., angles from the horizontal) recorded in a total of nineteen traverse cross-sections of the five largest wave— ogives (v. Figure 7). It is noted again that all folia in the a-sector do not necessarily dip downglacier, nor do all folia in a B-sector always dip upglacier. This can be seen from the distribution of folia in Figures 11 through 16 and in part of the profile of wave-ogive J in Figure 17 (v. anomalus distribution of 2—8% concentrations of point poles on east side of Figure 11 and west side of Figure 12). This again may be the result of local deformation effects. Also note is made of the trend toward greater angles in the a-sectors with increasing distance down— glacier, which in turn corresponds to changes in surface lepe and attenuation of the wave-bulges downvalley. In these lower valley sectors, however, the englacial folia remain somewhat normal to the surface. A similar 37 situation, of course, is noted with respect to the mean dip of the tectonic folia described in Figures 11 through 16. In individual wave-ogives there are notable changes along the crest of the wave as well. In wave— ogive J, for example, the amplitude increases on the order of 5-10 m (16-32 ft) as one walks from the north end to south. This increase in amplitude is also associ— ated with an increase of slope on the downvalley wave surface--i.e., from 30° on the north end to 67° on the south end of the B—sector of this wave—ogive. Freers (1966) described nine whiter ice folds found in the summer of 1964 above, or upglacier from, the full-formed wave-ogives in the apron sector of the Vaughan Lewis icefall. Most of these were extended continuously across glacier, though some were segmented (Figure 3). These folds have the appearance of symmetrical, double plunging anticlines. Kittredge (1967) and the writer have noted that these small folds seem to appear most commonly on the surface of the larger waves. These smaller super- imposed cleaner-ice folds diminish in frequency and size downglacier from wave-ogive J. That is, they appear to have their maximum expression in the upglacier sector of the apron. Far downglacier in the main ogive zone they disappear completely. 38 Crevasse Observations Crevasses and fracture patterns on a glacier are principally a reflection of the compressional, tensional, and shear stresses within the upper part of the glacier. The crevasses at the head of the Vaughan Lewis icefall are, as have been shown, entirely of the tension type. We have also seen that significant or deep cre— vasses do not occur in the main icefall, but reappear in the sector just above or at the beginning of the wave— ogive develOpment. There are some depressions parallel- ing the wave-ogive crests which, of course, may be cre- vasses at depth. But essentially, as can be seen in plan view, the most dominant crevasses are radial. This means they are normal to the arcuate crest axes of the wave- ogives (Figure 18). In some cases these radial fissures are efi echelon. In others, firn in the largest radial crevasses contain smaller fissures with efi echelon pattern (Figure 19). It is not clear whether this smaller pattern of fissures relates to tensional spreading of the large crevasse walls, or to some other stress couple not yet measured. This may even be a result of firn-pack slump within the crevasse, combining effects of ice stress and ablation. Such warrants further examination in a subse~ quent field season. Such ice at the base of icefalls is subjected to longitudinal compressional stress (Nye, 1951, 1952, 1959; Glen, 1956). This is because of the abrupt decrease in 39 Figure 18.--Lower Vaughan Lewis Glacier showing wave- ogives and ogives in compression zone below the icefall. Note position of stream channel and ponded water between wave-ogives. (Photo by L. R. Miller, August 1967.) Figure l9.--§fi echelon fissure pattern within radial crevasse on southern edge of Herbert Glacier. View looking southerly Wlth main section of glacier on right and flow direction is away from viewer. Phot ' 4 August 1969.) ( o by L. R. Miller, 40 L Figure 19 41 bedrock slope (Figures 18 and 20) and the consequent damming effect and slowing of forward velocity. (See effect of longitudinal stress trajectories as controlled by even small changes in bedrock $10pe in Miller, 1958, as measured on the adjoining Taku Glacier.) This com- pression tends to bring pre-existing planar features or inhomOgeneities of any kind (e.g., basal tectonic folia) within the ice into a more vertical transverse attitude (Allen, et_al., 1960). This mechanism has been emphasized for the Vaughan Lewis in a new theory of wave-ogive for- mation elucidated by Miller (1968); also Miller, et_gl. (1968). In this regard, Untersteiner (1955) points out further possible complexities by showing that: "corres— ponding to the two main normal stresses we would have altogether six directions of maximum shear stress in which gliding could theoretically be expected." This would imply also characters of c-axis maximum. Here again reference can be made to the two to four maxima observed in studies by Gow (1964), as noted earlier. Thus, the writer is quite aware that much detailed work on this subject is yet to be done. But again the geometry of the Vaughan Lewis icefall suggests a single maxima. Regardless of the foregoing, it is clear that wave-ogives M and N have transverse crevasse patterns. According to Nye's initial plastic flow analysis for ice (1951), a transverse pattern can be associated with ex— tended flow and can be further correlated from data 42 .1nmmav mmomuuuflxaomwnwwwmww ea nmflomao mHBmA wn omummmmsm mm nummo xoonomm .mmm n mm>fl00Im>m3 was gonna .Hamwmofi HmBOH mo maamo Illll. mamm o xHOB UHE . .Hm um .nmnumum mcmnm5m> .m was s 61H Hm Hmcflosuflmsoqin om mu: .m § \ \ I o — s \ \ \. 1. I I I I I I I s I . a I I 1 \/\/\\...I||.H..Ih.l/nu\. 1 ...... ..7 xUOaOIwn11l.\\ .IW1 \ llllllEII-IIIUIHPIVI I’llnllral ’ \\.\. $050.30 510‘ \ 0.8:: 9.2.1... :29: 1 9‘0“. >0>unu V 12:21.21 13:1.) mu. 220:1 an .o mw>.OO o m><3 :39: 01.30 a»; 1.... coin :1 1191.03: 2.. .1 1.11.1... 1311-11105“. 3 43 obtained. Attempts have been made, however, to measure the strain rate on the Vaughan Lewis by having four stakes at the corners of a square and measuring the inter- vals between successive stakes (Nye, 1959), as suggested by Nye (1967, personal communication) and have yet to yield much information. A similar technique for measur- ing surface strain-rates has been applied by Wu and Christensen (1964) on the Taku Glacier, with not entirely satisfactory results. Many of the problems have resulted from an inability in even solid firn to measure small values of deformation accurately over short periods of time. In other words, it is most difficult to avoid error encountered by settling and ablation of surface markers. ReCOgnizing this, in 1969 R. Little (personal communi- cation) installed a set of 2.5 cm (1 in) pipes, 4.8 m (16 ft) long, in squares on the Lemon Glacier at the southwest edge of this icefield near Juneau, and attached piano wires to a set of sensitive strain gauges placed at the corner of each square. This technique is also cur— rently being organized for use in a similar proqram on the Vaughan Lewis Glacier planned for 1971. Surface Movement, 1967-1969 Movement stakes were positioned on wave-ogive J through M as indicated in Figures 7 and 20. In Figure 20 particularly we can see the upper movement stakes in relation to the apron cross—section. Seven movement 44 stakes were also positioned on the apron below the icefall zone. Theodolite resection of these stakes has provided positions from which horizontal components of the move— ment have been calculated. Longitudinal horizontal com— ponents of daily movement have been calculated from a Fortran computer program (Table l) which reconstructs the triangulation surveys. The resection data were obtained under conditions yielding a :15 seconds of arc reproduci- bility, thus giving a maximum movement error of only 10.05 m (0.16 ft). The results are given in daily move- ment in Tables 2, 3, and 4; with the plotted rendition of these data shown in Figure 21. As we look at this figure we can see that the rates of daily horizontal movement do not agree with what Freers (1966) found nearly a decade ago for movement on similar stake placements on the wave—ogive zone (wave—band) in the late summer of 1961. For the interval 8-10 August, 1961, Freers calculated a movement for stake F-4 (compares to the position of 1968 stake 15) of 5.20 m/day (17.1 ft/day). For stake 15 the 1968-69 data actually give 1.06 m/day (3.5 ft/day) as a corrected mean velocity between 8 August and 7 September 1968. On Freers' stake F—7 a 1.68 m/day (5.5 ft/day) movement in 1961 is shown for the stake 10 area of this 1968 study. Again one can see that these values differ from Freers' by a factor of nearly 5. Some of Freers' movement values have been labeled by him as "questionable," due to the small triangulation angles 45 MH .coauamom HouGONHHOQ OMMWMMM may BOHOQ . . asmq : ucme>oz .sofium>nmmno mo m60flnmm pmpomamm um>o Hammmonmonmtl.Hm muumflm powmcmuu HmcHUsuHmGOH co ucoEm>oE oommusm amuGONHHon o Illllltitllllillllltitxfi I us...‘ f 2: o 6' I. I. I I 1 o 1 4 a e n e c 1 ... x o . o .............. 3o. :31. a - .2: .1...“ 1 B o lllll l :2 .1113 k .. .25 2 a. 3 (I'll 32...; 3 I 6.5 .... o .... 31a; :2 ...i a a ...... on 1 '2 0 Lap / s totem 46 from his base line. On this basis, the writer is willing to assume that the 1968-1969 surveys are more representa- tive, though of course there could be a slowing down of the glacier's flow over this ten—year period. This latter conclusion is deemed improbable, though, in View of the consistency of the 1968-1969 trends as revealed in Figure 21. More detailed future movement surveys will help to clarify the correct interpretation. From Havas' 1964 data as presented by Freers (1966, Havas, 1965) surface movement of 0.35-0.42 m/day (1.15-1.38 ft/day) is noted, although the position relation- ship is not precisely known with respect to the stake locations for the 1968 data. Havas' strain diamonds, however, were in the upper wave-ogive zone--i.e., just below the apron area--thus giving good correlation with the computed velocities determined for 1968-1969. Kittredge (1967) with respect to surveys made in August, 1965 states, "The velocity of the ice in the ice— fall itself was found to be 18 ft/day versus 2.7 ft/day at the apron" (5.49 m/day vs. 0.82 m/day). These positions are not located precisely either with respect to the 1968 positions, but Kittredge's values are partially corrobor— ative. Freers' (1966) calculated movement was determined from two readings two days apart; Havas' (1965) calcu— lated movement was from two readings forty-eight days apart; Kittredge's (1967) two readings were a month apart. 47 In comparison to these somewhat sparse earlier data, the current investigation comprised readings taken at nine different times extending over thirteen months. The first was on 23 July 1968; the last on 23 August 1969. Thus again, the writer has more confidence in these compu- tations. At least they are a more detailed contribution to the long-term records obtained through the years by JIRP personnel. The 1968-69 field data are listed in complete form for future reference in Appendix A. All of these calculated movements are not shown in Tables 2 through 4 and three readings taken in 1969 do not appear in the total. The reason for this is that in 1969, some stakes were missing, by being buried under the winter snow-pack and by sliding into crevasses. Thus the computer program used in the analysis has to take this into account by substituting false data as fill-ins in the program cycle. The initial setting of these stakes was on 25 June 1968. Due to subsequent ablation effects they were reset between the 8th and 15th of August in that year. At this time, because of distorted holes resulting from ablation, it was necessary to make slight changes in position of some stakes. For example, stakes l and 2 were re- positioned, with stake 2 being moved £0.15 m (0.5 ft) north. (The exact change in stake 1 is not known because the original reference hole became ablated out.) Stake 4 was moved 0.45 m (1.5 ft) NNE and stake 15 was moved 4.4 m 48 (14.6 ft) east of its original position. A field check of the 23 July-29 July movement of stake 15 showed that a point a short distance upglacier might be useful as an indicator of the position of the first wave-ogive to be developed for the summer of 1969 (wave-ogive I). The position change of stake 15 was, therefore, to check this possibility. (It is noted that the stake 15 position in Figure 7 represents this later location. Also at this time the marker was changed from a flag and pole arrange- ment to a pyramid pylon as discussed early in this report, and as shown in Figure 4.) Thus by adding 4.4 m (14.6 ft) to the total movement of 3.26 m (10.33 ft) for stake 15 (v. Table 2), and calculating for a mean daily movement, one derives a horizontal movement of 1.09 m/day (3.49 ft/day), thus putting it back within the expected range of values obtained for stake 15 during other time inter- vals. This, again, is shown in Tables 2 through 4. The subsequent field check of stake 15 showed movement to be about 1.6 m/day (5.8 ft/day). By early September it became apparent, even from empirical obser— vations, that this stake had been repositioned inappro- priately and would end up after a year of movement some- what upglacier from the crest of the develOping 1969 wave-ogive I. More accurate movement information deter- mined by computer indicated that ice movement in the apron area is not as great as was originally assumed. Thus the adjustment made in stake 15 was actually in the 49 wrong direction. It should have been moved downglacier to reposition it on the developing crest of wave-ogive I. From data in Tables 2 through 4, it is clear that there is a change in velocity in the vicinity of the form— ing wave-ogive I. In corroboration, when stake 10 on the upper apron was resurveyed in 1969, a smaller velocity was calculated than for 1968. Whether this is a significant difference cannot be determined. As seen in Table 4, the velocities in the bottom set of data include movement for the whole preceding year and hence give an approximation of annual surface mass transfer. Whether in fact movement in the colder months is in agreement with those found for the warmer months of July and August cannot from these records be inferred with certainty. This is because the period of comparison averages ten months (1968—1969) against two months (summer of 1968) and hence may be subject to critical question. It nevertheless tends to agree with an assumption by Nye (1967, personal communication at time of his visit to this glacier) that the velocity in such outflow glaciers may be constant within the icefall during any given year. This poses some question about ideas concerning seasonal changes in velocity as discussed by Kittredge (1967). It also enhances the current idea concerning local position changes in velocity; i.e., a consequent damming or abrupt change at the base of the icefall, thus giving further credence to the concept of longitudinal stress. 50 The writer does not note a significant increase in velocity downglacier as is stated by Kittredge (1967) con- cerning a wave-ogive leaving the compression zone and pro- ceeding downvalley. The foregoing interpretation can, of course, be checked by more frequent periodic measurements of longitudinal flow and surface deviation changes through- out a whole year and especially surveys in the autumn, winter, and spring. In this context it is of interest that year around measurements on the flat intermediate elevation névé of the Taku Glacier (Miller, 1958, 1963b) have re- vealed a 10 per cent increase in surface velocity during the winter months. This indication of greatest movement in the winter months is in contraSt to what may be sug- gested by the all too scanty data in Table 4. It may be significant, however, that the data on the Taku Glacier are from the broad upland zone of perennial accumulation at about 1075 m (3500 ft) elevation in the vicinity of Camp 10, a region of entirely different stress distri- bution than to be expected on the Vaughan Lewis apron area. The possibility is, however, that such seasonal variation in "flow" in the Vaughan Lewis névé, may, still be re- flected in and below the icefall zone, though perhaps in an attenuated fashion. Therefore, the validity of any interpretation suggesting uniform flow should, of course, be checked by subsequent winter surveys. Nevertheless, at this juncture we are reminded of the consistency in the thirteen-month record covered by Tables 2, 3, and 4. 51 An explanation may be in the possibility that this repre- sents an example of a dynamic self-regulating steady state in a classical open system--a concept now well recognized in hydrological systems (Chorley, 1962). Though the theoretical implications of the fore- going are tantalizing, with the insufficient data we have available on this glacier to date one cannot really say much more. Because of interest in this question, however, the writer has attempted to develOp a laboratory model (Figure 22a, b, and c) to simulate these flow patterns using a mixture of kaolin and water along the lines first demonstrated by Vaughan Lewis and M. M. Miller (1955). This laboratory test was carried out in a scale-model valley of the Vaughan Lewis Glacier itself. In this experiment wave—bulges not unlike those on the Vaughan Lewis apron (Figure 23) were indeed reproduced, though on a strictly qualitative basis. Details of this effort are given in Appendix B, and brief comments on the rele- vance of its results are made in the final section of this paper. The periodicity of individual surface bulges below the icefall on this glacier has been considered in detail by Kittredge (1967) and others, and demonstrated via repeated plane-table surveys to be annual in nature. What this means is that the wave-crests of successive wave-ogives in the apron zone move downglacier at a rate approximately one full wave length per year. Thus, 52 .un nose + s 1A1 m3“ fin...” mmmHDQIQ>M3 101 1.mmmH noun: .umaanz .m .q an mononm1 .nn coma + a 101 .HS 0000 + OHON QEHB «av msfi3oam HammmOH mwzmq 1n1 .usmfimoam>mp mo mommum msoanm> ca no . . Doom :0 gmsmsm> man no HmUOE :HHOMMII.NN musmam new 53 GOHNQ OHOZ .m .0: mxmum 11mmma nmsmsm..umaflns .m .q an ouonm1 .M w>HmOIw>m3 mo 1£usom msHMOOHv 30H> maflmonmit. pummno um nmxnmE .mm mnsmflm ...-‘1‘“ 54 presumably this is an annual rather than a seasonal phenomenon, though it may attain its maximum deve10pment at the end of the period of maximum accumulation load, i.e., late spring. Therefore, although direct seasonal variation may not be apparent, we may conclude that there isia strong develOpment of at least one notable new wave- bulge each year, and hence also a new wave-ogive annually. Mass Transfer and Theoretical Considerations Using measurements from Kittredge (1967) and also the current United States Geological Survey map at a scale of l:63,360, a rough volumetric analysis was made of the mass transfer in the Vaughan Lewis Glacier for the year 1968. The icefall is about 671 m (2200 ft) wide, the apron 854 m (2800 ft) wide and the wave-ogive area about 732 m (2400 ft) wide. By using a conservative depth value of 198 m (650 ft) for the wave-ogive area and a velocity of 0.5 m/day (1.5 ft/day) one would find a volumetric movement of 7.15 x 105 m3/day (2.34 x 106 ft3/day) through a given wave-ogive cross-section. If one were to pass a mass of ice through the apron cross-section of 854 m, at the measured apron velocity of 1 m/day, one would need a depth of 76 m (250 ft) to accommodate this same volume. Such a theoretical depth is indicated by dotted line in the middle left part of Figure 20. If the depth of ice in the apron area is greater than this theoretical depth of 76 m (250 ft), and it 55 presumably is for reasons given below, an effective sur- face change would be necessary to accommodate such a volume. As there is significant summer ablation in the apron and wave-ogive zones, of course the theoretical depth of the icefall has to be greater. Thus the note— worthy change in velocity-~e.g., from 1.0 m/day at stake 15 to 0.5 m/day at stake 4 in a downglacier distance of 300 m--could coincide with a strong compressional force lifting the surface upward into a wave-bulge. Such a deformation is possibly produced by a vertical stress release both by flow recrystallization and even discrete movement along foliation planes, i.e., a form of intra- foliation deformation. The accentuated pattern of foli— ation itself may even be a result of this phase of the deformation sequence. The upbulging represents about a 10 per cent increase in total ice thickness compared to that beneath the adjoining wave troughs (Figure 23). The wave-bulge would then be similar to the effects of tangential—compression or bench-vise squeezing described by Badgley (1965) in considering the role of oroqenic stress in crustal tectonics. A further consideration here is the possibility that the up-bulging (wave-ogive surface) is not as directly related to the presence of a bedrock threshold (v. Figure 20) as some other observers have suggested. A qualitative basis for this suggestion is given in 56 discussion of the writer's kaolin model experiment noted in Appendix B. In View of the foregoing discussion of the close association and possible develOpment of tectonic folia contemporaneously with the upbulging of ice where there is an abrupt change of slope at the base of the icefall, it should be mentioned that the development of tectonic foliation has been considered by others to be prior to this stage. Miller (1968a and 1968b) considers the tectonic folia to be initiated by shear stresses at depth some distance upglacier-—i.e., in the area of ex- tending flow, within the icefall itself. These are pro- duced first parallel to the bedrock surface, and then in a complicated flow history becoming folded and deformed and eventually to be exposed in the wave-ogives by later ablation. The mechanism he describes relates to the com- bined factors of rapid downvalley movement, the squeezing of ice in the defile outlet, and to the damming effects of compressive flow at the base of the icefall. SUMMARY OF RESULTS AND CONCLUSIONS Movement data corroborate the hypothesis of a compression mechanism existing within ice of the apron and upper wave-ogive zones. To recapitulate the results of this study, a significant change in velocity has been demonstrated to exist along the longitudinal transect between the upper apron zone at the base of the icefall and the main zone of wave-ogives. A marked change in bedrock slope (6) translating extending (tensile) flow into compressive (compression) flow, is well illustrated by the shear formulae basic to the description of verti- cal velocity profiles in glacier mechanics (i.e., ? or rate of flow = KTn in which T = Dogsine).l Thus the marked change in bedrock slope (0) presumed to be the prime factor resulting in increased longitudinal com- pression coincident with the foregoing velocity change. This compression effect is considered to be manifest by the described up-bulging at the surface of the glacier lWhere T = shear stress in bars; D = depth of ice in cm; p = density; g = acceleration of gravity; and 6 = surface slope angle. 57 58 in the apron sector just below the icefall. This up- bulging is further supported by the writer's laboratory model tests (Figure 22) and by the cited surface con- figuration shown in plotted cross-sections in the apron and wave-ogive zones. As for the periodic nature of surface bulges in this wave-ogive system, it has been demonstrated by previous investigators on the Juneau Icefield Research Program (v. Kittredge, 1967) that the wave crests in the apron zone move downglacier approximately a full wave-length per year. Thus, although direct seasonal variations in stress may not be significant, or at least not apparent, there is presumably one new wave-bulge developed each year which eventually results in a wave— Ogive downvalley (v. left hand edge of Figure 23). These compression effects are also consistent with the strong develOpment and orientation of the tectonic foliation described in earlier pages, further detailed as follows. The dominant shear stress which Kamb (1959a) theoretically has placed parallel to the folia and which Miller (1968) has allied as parallel to the tectonic folia on the margins and bed of this glacier, still may pertain in the icefall zone. But the conclusion of this study suggests that the dominant effect in the lobate apron zone is not shear, but compression, the direction of which lies normal to the folia surface (as shown in Figures 11-16). Thus with the related c-axis of 59 individual ice crystals in this polycrystalline aggregate explained in this way, the c-axis would lie parallel to the longitudinal compression axes which extend radially outward from the center of the icefall where the apron begins and the wave-ogives originate. Thus further, the folia develop normal to this dominant radial stress field in this critical sector of the glacier. The existence of this significant zone of compression is also corroborated by the radial development and systematic distribution of crevasses, dominated by lobate radial fissures in the ice apron and upper wave-ogive zones. With respect to other factors, including the always controversial role of ablation, the results of reconnaissance meteorological observations by the writer and others reveal that substantial ablation does occur. Though detailed discussion of this, however, is beyond the quantitative SCOpe of this present report, it re- veals that there is upwards of 20 m (64 ft) or more of downwasting per average ablation season. Because of the dimensional characteristics of the wave-ogives, and further because of the results of the writer's kaolin model experiment described in Appendix B, ablation is considered as no more than a subordinate co-factor in the morphogenesis of wave—ogives. In concert the various data here discussed seem to indicate that longitudinal compression plays the dominant role. If one is willing to assume that the measured changes in surface velocity 60 are accompanied also by gradationally related deformation of ice at depth in turn related to a total stress field, then one could conceive of positive overall downvalley compression resulting in a combined but not necessarily contemporaneous continuous and discontinuous compressive deformation along either pre-develOped shear foliation or (and) currently produced radial compressive foliation, with a strong upward component. To such a mechanism is attributed the striking development of folia which are suggested further to be genetically associated with the pronounced development of wave-bulges. Together these internal and surface phenomena constitute what has been described as wave-ogives. SUGGESTED ADDITIONAL INVESTIGATIONS Evidence indicates a strong causal relation be— tween stresses that cause faulting and crevassing near the surface and those causing recrystallization and foli— ation well below the ruptured zone. Thus the ice fabric measured near the surface is indicative of fabric below this point or certainly at depth sOme distance upglacier from it. However, one should have some evidence that this does exist at depth and to what extent. Consider— ation should be given to exploration at depths greater than 18-20 m (57—64 ft). A bore-hole with core samples retrieved from depth and a pipe placed in such a bore- hole, with its deformation to be subsequently measured below the crest of a wave-ogive to a depth of 30—60 m (96-192 ft), could yield needed information. Ideally such information should be obtained in the glacier above the icefall zone as well as in the apron sector below it. Surface strain-mechanics measurements in greater detail are also needed using the surveyed square or strain—diamond method. Such short term data will hope— fully be obtained on this glacier in the future from 61 62 instrumentation and measurement method currently being developed by R. W. Little, G. Cloud, and others in re- finement of the technique invoked by T. Wu and R. Christensen in earlier JIRP work. The further use of depth measuring seismic units would also yield much further data concerning details of bedrock configuration, eSpecially in the icefall and apron zones. The program concerning "seeded" markers should be pursued with the resurveying of markers as they are found and the evaluation of their three-dimensional movement and the role of ablation. Very detailed micro-ablation measurements are needed using large arrays of stakes across much of the ice apron and ogive zones. Such records should extend over the melting season from April through September. One should continue detailed periodic theodolite surface movement stake surveys, throughout the year to determine whether or not there are significant differences in surface movement from summer to winter. Also time— lapse photography would yield helpful information con— cerning significant seasonal changes in the icefall and possibly even direct evidence of "up—bulging" of the wave-ogives. This kind of information can be obtained without great expenditures of money. An expanded pro— gram of P—30 mapping for volume comparisons also should be invoked. 63 Added to the above, is the excellent potential for significant results via either laser range finder, or (and) micro-wave surveying equipment using continuous 24-hour-a-day monitoring of surface glacier flow. Allied to this could be continuous recording, portable seismo- grams in the ice, as well as in adjoining bedrock, to delineate discontinuous or spasmodic flow for comparison with the aforementioned continuous micro-wave survey data. Such would well lead to a break-through in understanding the true nature of continuous versus discontinuous pro- cesses in glacier mass transfer. Basic to the success of any such research projects, is a small yet dedicated team of field men deeply interested in this fascinating phase of glaciology. This team must, however, be willing to spend a consecutive six-month span from spring to autumn while conducting the kind of systematic observations and measurements sug— gested here, and of course in much more detail than the present study has permitted. REFERENCES REFERENCES Allen, C. R., W. B. Kamb, M. F. Meier and R. P. Sharp. (1960). Structure of the Lower Blue Glacier, Wash- ington. Jour. Geology, v. 68, no. 6, pp. 601-625. Bader, H. (1951). Introduction to Ice Petrofabrics. Jour. Geology, v. 59, no. 6, pp. 519-536. Badgley, C. P. (1965). Structural and Tectonic Principles. Harper and Row, Pub., New York. 521 p. Billings, M. P. (1954). Structural Geology. 2nd ed. Prentice-Hall, Inc., New Jersey. 514 p. Chamberlin, R. T. (1928). Instrumental work on the nature of glacier motion. Jour. Geology, V0 36' pp. 1-300 Chorley, R. J. (1962). Geomorphology and general systems theory. Geological Survey Professional Paper, no. 500—B, pp. 1-10. Chrzanowski, A. (1968). Glacier mapping on the Juneau Icefield, Alaska—B.C. (abs.). Alaska Sci. Conf., 19th, Whitehorse, Y. T. Freers, T. F. (1966). A structural and morphogenetic investigation of the Vaughan Lewis Glacier and adjacent sectors of the Juneau Icefield, Alaska, 1961-1964. Michigan State Univ. (unpublished Master's thesis). Glacier bands, conference on terminology. (1953). Jour. Glaciology, v. 2, no. 13, pp. 229-232. Glen, J. W. (1956). Measurement of the deformation of ice in a tunnel at the foot of an ice fall. Jour. Glaciology, v. 2, no. 20, pp. 735-745. 64 65 Gow, A. J. (1964). The inner structure of the Ross Ice Shelf at Little America V, Antarctica, as revealed by deep core drilling. I.A.S.H. Commission of Snow and Ice, Pub. No. 61, pp. 272—284. Havis, T. W. (1965). Surface velocity and strain-rate measurements on several Alaskan glaciers; 1964. Michigan State Univ. (unpublished Master's thesis). Kamb, W. B. (1959a). Theory of preferred cyrstal orien— tation developed by crystallization under stress. Jour. Geology, v. 67, pp. 153—170. Kamb, W. B. (1959b). Ice petrofabric observations from Blue Glacier, Washington in relation to theory and experiment. Jour. Geophysical Research, v. 64, no. 11, pp. 1891—1909. Kamb, B. (1964). Glacier geophysics. Science, v. 146, no. 3642, pp. 353-365. King, C. A. M., and W. V. Lewis. (1961). A tentative theory of Ogive formation. Jour. Glaciology, V0 3’ no. 29' pp. 913-9390 Kittredge, T. F. (1967). Formation of wave-ogives below the icefall on the Vaughan Lewis Glaciers, Alaska. University of Colorado (unpublished Master's thesis). Lewis, W. V. (1956). The future lines of progress in glaciology, a symposium. Jour. Glaciology, v. 3, no. 20, pp. 695-697. Lewis, W. V., and M. M. Miller. (1955). Kaolin model glaciers. Jour. Glaciology, v. 2, no. 18, pp. 533-538. Miller, L. R., A. C. Pinchak, D. Traband and D. Trent. (1968). Some 1967 and 1968 measurements on surface bulges and englacial structures of the Vaughan Lewis Glacier, Alaska. (abs.) Alaska Sci. Conf., 19th, Whitehorse, Y. T. Miller, M. M. (1952). Preliminary notes concerning certain glacier structures and glacial lakes on the Juneau Ice Field. Juneau Icefield Research Project. JIRP, Report No. 6, pp. 49—86. Miller, M. M. (1955). A nomenclature for certain . . englacial structures. Acta Geographica, Helsinki, v. 14, no. 17, pp. 291—299. Miller, Miller, Miller, Miller, Miller, Nye, J. Nye, J. Nye, J. Perutz, 66 M. M. (1958). Phenomena associated with the deformation of a glacier borehole. Internat. Geod. Geophys. Union, Assoc. Sci. Hydro., Ge . Assembly, Toronto, 1957, v. 4, pp. 437-452. M. M. (1963a). The Vaughan Lewis Glacier, Juneau Icefield, Alaska. Jour. Glaciology, v. 4, no. 36, pp. 666-667. M. M. (1963b). Taku Glacier evaluation study. State of Alaska, Dept. of Highways, rept., 200 p. M. M. (1968). Theory of wave-ogive formation on the Vaughan Lewis Glacier, Northern Boundary Range, Alaska—B.C. Symposium on Surging Glaciers and Their Geologic Effects, National Research Council of Canada, Banff, Alberta. M. M., T. F. Freers, T. F. Kittredge, and T. Havas. (1968). Wave-ogive formation and associated phenomena on the Vaughan Lewis and Gilkey Glaciers, Juneau Icefield, Alaska-B.C. (abs.) Alaska Sci. Conf., 19th, Whitehorse, Y. T. F. (1951). The flow of glaciers and ice-sheets as a problem in plasticity. Proc. Roy. Soc., ser. A, v. 207, no. 1091, pp. 554-572. F. (1952). The mechanics of glacier flow. Jour. Glaciology, v. 2, no. 12, pp. 82-93. F. (1959). The deformation of a glacier below an icefall. Jour. Glaciology, v. 3, no. 25, pp. 387-408. M. F., and G. Seligman. (1939). A crystallo— graphic investigation of glacier structures and the mechanism of glacier flow. Proc. Roy. Soc., 581'. A, V. 172' pp. 335-3600 Pinchak, A. C. (1968). Avalanche activity on the Vaughan Lewis Icefall, Alaska. Jour. Glaciology, v. 7, no. 51, pp. 441-448. Prather, B. W., L. Schoen, D. Classen, and H. Miller. (1968). 1968 seismic depth measurements on the Taku, Vaughan Lewis, and Lemon GlaCiers, Alaska. (abs.) Alaska Sci. Conf. 19th, White- horse, Y. T. 67 Rigsby, G. P. (1958). Fabrics of glacier and laboratory deformed ice. Internat. Assoc. Sci. Hydrology, pub. 47, Symposium of Chamonix, pp. 351-358. Rigsby, G. P. (1960). Crystal orientation in glacier and in experimentally deformed ice. Jour. Glaciology, v. 3, no. 27, pp. 589—606. Taylor, L. D. (1963). Structure and fabric on the Burroughs Glacier, South—East Alaska. Jour. Glaciology, v. 4, no. 36, pp. 731—752. Untersteiner, N. (1955). Some observations on the banding of glacier ice. Jour. Glaciology, v. 2, no. 17, pp. 502—506. Wu, T. H., and R. W. Christensen. (1964). Measurement of surface strain-rate on Taku Glacier, Alaska. Jour. Glaciology, v. 5, no. 39, pp. 305-313. TABLE S 68 Doommno «\now~umm+_mvu¢me AO©\Anoc\Nmmv+N£muv+NQmuNm noo\nn00\—wmv+_zmvv+—Omn~m nN\Aow~IN¢+1¢vvuow_uHQZM~qmv qum Nmmqwznqmomq1mmq~£mq10m~1m¢O\Z >¢D\P& 2 HL :qquZuml we? u H 0% GO — u 7 .. 00.. u Amv Mlzh : mm: H Amy MJHk .. PO: u nfiv wJHk : 00: u new wdmu .. mQ: H nmu widmu : VD: u “WV HANK .. MD: M AMV MAM.”— : mm: H ANV MI—HF— .. ~Q: H n—v Mlzu \qufismmms—~qO~q>q01~©\>Qo GREGG Cw» >1QQ zwowhzm may MJHE Zunzmzfio IMHME 41mm 0— owm 01.0 com 0mm ovm own 0mm 01m 000 com owm ohm com Cow GQN OMN com 00— Om— or— C0— 0m. 01»— om." Cm— m: N: O: OO— .o>lomla .Emumoum ucmEm>oz HMDGONHHom Hmwomaw mw3mq cmnmsm>ll .H Bmdfi 69 sz wDZHHZQO Amy mmmado AJQU n1u EMWQAU JJ¢U 0— SH 86 Amoommvv quxum xwhmxoqNquwhmquaow HZHmd n~v>qo\mwhwz u mwhwza AHV>