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On the Secular Variation of Ice Flow Velocity at Lewis Glacier, Mount Kenya, Kenya

Published online by Cambridge University Press:  20 January 2017

Stefan Hastenrath
Affiliation:
Department of Meteorology, University of Wisconsin, Madison, Wisconsin 53706, U.S.A.
Phillip Kruss
Affiliation:
Department of Meteorology, University of Wisconsin, Madison, Wisconsin 53706, U.S.A.
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Abstract

Measurements at various epochs in the course of the twentieth century indicate a slowing down of surface ice flow velocity. This is consistent with the numerical modeling of the secular glacier recession, which furthermore shows a gradual upward shift of the regions of highest velocity and mass flux. Crevasse orientation is transverse above, and longitudinal below, the velocity maximum. The secular change in the longitudinal velocity profile seems to affect the crevasse pattern. Net balance in the next five years is a major factor in future changes of the glacier. With this reservation, model calculations for a possible extreme scenario indicate a drastic overall velocity decrease, and a moderate further displacement of the velocity and mass-flux maxima up-glacier, by the mid 1980’s.

Sur la variation seculaire de la vitesse de la glace au Lewis Glacier. Mount Kenya, Kenya. Des mesures à différentes époques au cours du vingtième siècle montrent un ralentissement de la vitesse superfieielle de la glace. Ceci est cohérent avec la modélisation numérique de la régression séculaire du glacier qui, de plus, montre une remontée progressive en altitude des régions de plus forte vitesse et de plus gros bilans. L’orientation des crevasses est transversale au-dessus et longitudinale au-dessous du point de vitesse maximum, Le changement séculaire du profil de vitesse longitudinal semble affecter la disposition des crevasses. Le bilan glaciaire des cinq prochaines années est le facteur majeur des changements futurs du glacier. Sauf cette réserve, les calculs sur modèle pour un scénario extrême montrent une forte diminution globale de la vitesse, suivie d’un déplacement modèré vers le haut de la vitesse et des flux maximum de glace, vers le milieu des années 1980.

Zusammenfassung

Zusammenfassung

Die säkularen Änderungen der Fliessgeschwindigkeil des Eises am Lewis Glacier, Mount Kenya, Kenia. Messungen zu verschiedenen Zeitpunkten im Laufe des zwanzigsten Jahrhunderts lassen eine Abnahme der Fliessgeschwindigkeit des Eises erkennen. Dies passt zur numerischen Modellrechnung des säkularen Gletscherrückgangs, die ausserdem auf eine allmähliche Verlagerung der Gebiete höchster Geschwindigkeit und Massenbewegung nach oben schliessen lassen. Die Orientierung der Spalten verläuft oberhalb des Geschwindigkeitsmaximums quer, unterhalb desselben jedoch parallel zur Fliessrichtung. Die säkulare Änderung im Geschwindigkeitslängsprofil scheint das Spaltenmuster zu beeinflussen. Die Nettobilanz der nächsten fünf Jahre wird ausschlaggebend für zukünftige Veränderungen des Gletschers sein. Mit dieser Einschränkung deuten Modellrechnungen unter extremen Annahmen auf eine drastische Abnahme der Gesamtgeschwindigkeit und eine weitere, mässige Verlagerung der Maxima von Geschwindigkeit und Massenfluss gletscheraufwärts um die Mitte der 80er-Jahre hin.

Information

Type
Research Article
Copyright
Copyright © International Glaciological Society 1982
Figure 0

Fig. 1.Surface velocities measured at various epochs during the twentieth century. Dots indicate the location of targets, and arrows the direction and magnitude of motion. Dotted, dash-dotted, broken, and solid arrows refer to measurements in 1934 (Troll and Wien, 1949), in 1957 (Charnley, 1959), in 1973–74, and during 1978–80, respectively. Solid arrows with small dot at right-hand side of tail denote measurements limited to January—February 1978. Open circle, dot, and arrow with short tick marks along right-hand side of shaft refer to 1958 and 1974 positions and 16 year average displacement rate of the remnants of a meteorological shelter. The dotted line represents the modeled central line, with tick marks at 50 m intervals indicating longitudinal distance. 1978 height contours in meters are entered as thin solid lines. Points Thomson, Lenana, Melhuish, L3, L2, S3 are control points outside the glacier. Scale 1:7500. Velocity scale in ma−1 is ten times the horizontal scale (i.e. 10 m a−1 would be represented as a 100 m arrow).

Figure 1

Fig. 2.Secular variation of surface velocity and mass flux along central line. Modeled longitudinal profiles are shown of (A) filtered velocity Vfilt and (B) mass flux Ø for various epochs as follows: 1899 double dot-dashed, 1934 dotted, 1957 dash-dotted, 1966 double dash-dotted, 1974 broken, 1978 solid line. In the graph of (A) of Vfilt, observed velocities are entered as asterisk for 1934, triangle for 1957, square for 1958 to 1974 mean displacement rate (labelled 1966), open circle for 1974, and large dot for 1978–80 (labelled 1978); vertical lines to the left indicate the estimated uncertainties of measurements. In the bottom part (C), bedrock topography is depicted as broken, and tarn and 1978 ice-surface topography by solid line. For the modeled maxima of surface velocity Vx and mass flux Øx and the observed terminus T, the positions since 1899 are entered in terms of down-glacier distance along the central line.