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Chaotic dynamics of a glaciohydraulic model

Published online by Cambridge University Press:  10 July 2017

J. Kingslake*
Affiliation:
British Antarctic Survey, Natural Environment Research Council, Cambridge, UK Department of Geography, University of Sheffield, Sheffield, UK
*
J. Kingslake <jonngs@bas.ac.uk>
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Abstract

A model subglacial drainage system, coupled to an ice-dammed reservoir that receives a time-varying meltwater input, is described and analysed. In numerical experiments an ice-marginal lake drains through a subglacial channel, producing periodic floods, and fills with meltwater at a rate dependent on air temperature, which varies seasonally with a peak value of T m. The analysis reveals regions of T m parameter space corresponding to ‘mode locking’, where flood repeat time is independent of T m; resonance, where decreasing T m counter-intuitively increases flood size; and chaotic dynamics, where flood cycles are sensitive to initial conditions, never repeat and exhibit phase-space mixing. Bifurcations associated with abrupt changes in flood size and timing within the year separate these regions. This is the first time these complex dynamics have been displayed by a glaciohydraulic model and these findings have implications for our understanding of ice-marginal lakes, moulins and subglacial lakes.

Information

Type
Research Article
Copyright
Copyright © International Glaciological Society 2015
Figure 0

Fig. 1. Our model ice-dammed reservoir system. (a) A subglacial channel is hydraulically coupled to an ice-dammed lake that receives meltwater at a rate Qi. The channel receives a constant and uniform supply of water along its length M. (b) The prescribed basic hydraulic gradient ψ (blue curve) is negative near the lake – a topographic seal. Also displayed is an example pair of ice surface and bed profiles (zs and zb; black and brown curves) that would produce this hydraulic gradient. In this example the bed slope φb = 0.01.

Figure 1

Table 1. Summary of model variables

Figure 2

Table 2. Model parameters and physical constants

Figure 3

Fig. 2. Synthetic air temperature and lake input time series defined by Eqns (6) and (7).

Figure 4

Fig. 3. Simulated flood cycles. Results from three simulations using seasonally varying air temperatures to drive lake input, with (a, b) Tm = 10°C, (c, d) Tm = 12.7°C and (e, f) Tm = 15°C. (a, c, e) Time series of discharge at the lake outlet Q(0,t) (blue curves) and lake input Qi(t) (green curves) for 20 model years after transients have ended. (b, d, f) Solution orbits in Q(0,t)−hL(t) phase space from the complete 120-year-long simulations.

Figure 5

Fig. 4. Tm parameter space. (a) Peak discharge of floods recorded during 120 year simulations plotted against the value of the midsummer air temperature Tm used in each simulation. The first ten flood peaks of each simulation are omitted to remove transients. The black box indicates the region shown in more detail in (b). Horizontal quantization visible in (a) (Tm > 16°C) is the result of a coarse search through this region. The vertical lines in (b) correspond to orbits plotted in Figure 9. Lines that are one point in vertical extent (e.g. 6 ≤ Tm ≤ 11°C and Tm > 19°C) correspond to limit cycles, where all the recorded floods have the same peak discharge; slightly thicker lines (e.g. 14 ≤ Tm ≤ 17°C) correspond to simulations during which transients lasted longer than ten flood cycles; and large blocks of points indicate dense, chaotic orbits. The colour of each point indicates the day of the year on which the flood peak occurs. In (a) the green arrows indicate two regions where floods occur progressively later in the year as Tm decreases.

Figure 6

Fig. 5. Sensitivity to initial conditions. (a) Time series of lake depth from two simulations which used Tm = 12.7°C. Simulations are identical except for a slight difference in their initial lake depth hL(0). The blue curve corresponds to hL(0) = 40.00 m, and the red curve corresponds to hL(0) = 40.01 m. (b, c) Corresponding orbits in Q(0,t)−hL(0)–S(0,t) phase space, with the initial and final conditions shown in green and red respectively. (d) Time series of the normalized separation between the orbits in (b, c). Normalized separation is calculated by differencing each component of the orbits’ positions normalized with the maximum value of the corresponding variable. The Pythagorean sum of the normalized separation is plotted. Note the different time axes in (a) and (d).

Figure 7

Fig. 6. The Nye attractor and topological mixing of phase space. (a) A solution orbit in Q(0,t)−hL(t)−t phase space of a simulation that used Tm = 12.7°C and hL(t = 0) = 40 m. The blue curve’s distance from the vertical green line denotes the lake depth hL(t), its position along the vertical axis denotes the discharge at the lake Q(0,t) and its rotation around the green line denotes the fractional part of time t multiplied by 2π (one rotation corresponds to 1 year). (b) Poincaré sections taken perpendicular to the t-dimension at nine different stages of the year, denoted by the day of the year d. The points locate the intersection of the orbit with each section. Each section’s location in Q(0,t)−hL(t)−t space is indicated by the boxes in (a). The colour of the points indicates simulation time t.

Figure 8

Fig. 7. Orbits in Q(0,t)−hL(t) phase space of solutions with (a) Tm = 13.888000°C and (b) Tm = 13.888002°C, which lie on each side of an abrupt bifurcation in Tm parameter space (Fig. 4) for 20 ≤ t ≤ 90 years. Points are colored to indicate simulation time t and are separated by ∼4.5 model days.

Figure 9

Fig. 8. Time series of lake input Qi and discharge through the lake outlet Q(0,t) from two simulations that lie close to the abrupt bifurcation at Tm ≈ 13.88°C. (a) Initial Qi(t) and Q(0,t) time series from two simulations that used Tm = 13.888000°C and Tm = 13.888002°C. (b, c) Long-time time series of the same variables from simulations that used Tm = 13.888000°C and Tm = 13.888002°C respectively.

Figure 10

Fig. 9. Period-doubling bifurcations. Long-time solution orbits (transients have been removed) in Q(0,t)−hL(t) phase space of four simulations that used (a) Tm = 13.701°C, (b) Tm = 13.401°C, (c) Tm = 13.201°C and (d) Tm = 13.151°C. (a–d) correspond respectively to the positions in Tm-parameter space indicated in Figure 4b by the vertical lines A–D.