Journal of Geophysical Research: Solid Earth

Did melting glaciers cause volcanic eruptions in eastern California? Probing the mechanics of dike formation



[1] A comparison of time series of basaltic and silicic eruptions in eastern California over the last 400 kyr with the contemporaneous global record of glaciation suggests that this volcanism is influenced by the growth and retreat of glaciers occurring over periods of about 40 kyr. Statistically significant cross correlations between changes in eruption frequency and the first derivative of the glacial time series imply that the temporal pattern of volcanism is influenced by the rate of change in ice volume. Moreover, calculated time lags for the effects of glacial unloading on silicic and basaltic volcanism are distinct and are 3.2 ± 4.2 kyr and 11.2 ± 2.3 kyr, respectively. A theoretical model is developed to investigate whether the increases in eruption frequency following periods of glacial unloading are a response ultimately controlled by the dynamics of dike formation. Applying results from the time series analysis leads, in turn, to estimates for the critical magma chamber overpressure required for eruption as well as constraints on the effective viscosity of the wall rocks governing dike propagation.

1. Introduction and Motivation

[2] Volcanic activity may be modulated by external physical processes acting over a wide range of timescales [Jupp et al., 2004]. At short timescales, volcanic eruptions may be triggered by Earth tides (see Johnston and Mauk [1972], Mauk and Johnston [1973], Hamilton [1973], and Sparks [1981], but see Mason et al. [2004] for evidence to the contrary), short-term climatic effects [Kennett and Thunell, 1975; Rampino et al., 1979; Dzurisin, 1980] and daily variations in atmospheric pressure and temperature [Neuberg, 2000]. Annual periodicity is also sometimes observed [McNutt and Beavan, 1987]. At long periods (i.e., greater than hundreds of years) it has been suggested that volcanism is influenced by changes in sea level [Walcott, 1972; Wallmann et al., 1988; McGuire et al., 1997] and by ice loading [Hall, 1982; Paterne et al., 1990; Sigvaldson et al., 1992; Nakada and Yokose, 1992; Paterne and Guichard, 1993; Jull and Mackenzie, 1996; Glazner et al., 1999]. In addition, at long periods both changes in hydrothermal circulation [e.g., Mastin, 1994] and melt productivity [Slater et al., 1998; Maclennan et al., 2002] have been invoked.

[3] In this study we reexamine the volcanic history of eastern California (Figure 1). For this region, Glazner et al. [1999] find an anticorrelation between volcanism and interglacial maxima over the past 800 kyr. One explanation presented by these authors is that an increase in the confining (lithostatic) pressure due to the presence of glaciers inhibits dike formation from magma chamber walls, resulting in a lower frequency of volcanic eruptions. Here, we show that although a correlation exists between glacial maxima and a lower eruption frequency, there is also a significant correlation between changes in eruption frequency and the rate of change in ice volume. We hypothesize that this volcanism is a response ultimately controlled by the dynamics of dike formation, which will be influenced by the rate of change of ice volume rather than the total ice volume. Moreover, we find the responses for basaltic and silicic systems to be distinct, allowing us to constrain the critical magma chamber overpressure required for volcanic eruptions as well as the mechanical properties of the wall rocks that govern silicic and basaltic dike formation, respectively. Our results are consistent with basaltic magmas being generated at greater depths than silicic magmas, in accord with geochemical observations.

Figure 1.

Map of the locations of basaltic (black dots) and silicic (grey dots) eruptions that have occurred in eastern California over the last 400 kyr.

2. Data and Methods

[4] Eruptions constituting the volcanic history of the Long Valley and Owens Valley volcanic fields over the last 400 kyr are shown in Figure 2. Eruption ages compiled from Glazner et al. [1999] and A. F. Glazner (unpublished data, 2003) are shown along with the SPECMAP time series, which serves as a proxy for global glaciation [cf. Shackleton, 1987; McIntyre et al., 1989]. We distinguish basaltic eruptions from “silicic” eruptions, which include all andesitic, dacitic and rhyolitic events. In accordance with the conventional view [e.g., Imbrie et al., 1984] the amplitudes of the δ18O variations in the SPECMAP time series are taken to be proportional to global ice volume. We assume that the average thickness of glacial ice in the Sierras, and thus the average surface loading, is governed mostly by global climatic conditions and is, thus, also indicated by variations in the SPECMAP data. This assumption is discussed in more detail below.

Figure 2.

Time series showing the SPECMAP δ18O curve of oxygen isotope variations recorded in planktonic foraminifers [McIntyre et al., 1989], as well as the history of basaltic (black) and silicic (grey) eruptions in the Long Valley and Owens Valley volcanic fields. Discrete events composing each data set are binned as shown in order to form time series in terms of the number of events per kyr. Solid circles indicate individual basaltic (black) and silicic (grey) eruptions. Stairs show the binned volcanic data where the height of each stair indicates the number of eruptions over the indicated time interval. Depending on bin width, all three data sets are smoothed (bold curves) with a Gaussian kernel with a 22–25 kyr width (Table 1) such that they may be compared within equivalent frequency bands (see text for discussion). SPECMAP data are from J. Imbrie and A. Duffey (SPECMAP Archive 1,

[5] Figure 2 shows that the frequencies of silicic and basaltic eruptions vary in time. The apparent clustering of events at different times suggests also that temporal variations in eruptive behavior occur over a range of characteristic timescales. In addition to being related to the dynamics of the volcanic system itself, this temporal behavior may be due partly to erratic sampling associated with preservation bias as well as uncertainties on age determinations. In order to identify and minimize observational biases so that we can compare the time series for silicic and basaltic eruptions quantitatively with the oxygen isotopic data set within equivalent frequency bands, we perform two operations. First, discrete data points constituting each data set are grouped into 0.5, 1, 2, and 5 kyr bins to construct time series in terms of a number of events per thousand years. These bin widths are chosen such that the volcanic signal with the shortest period in the data sets is resolved. In particular, minimum recurrence intervals for silicic and basaltic volcanism over the last 150 kyr, observed during periods in which eruptive activity is concentrated, are in the range 0.7–2 kyr. In addition, assuming that the tectonic regime giving rise to volcanism evolves on a plate tectonic (i.e., 10–100 Myr) timescale it is reasonable to expect these eruptive periods to be present over the full 400 kyr data set. After binning the data we smooth all three data sets using a Gaussian kernel with a 22 to 25 kyr width (depending on the bin width, see Table 1) [e.g., Glazner et al., 1999]. A number of alternative kernel widths were employed, but the results are quantitatively insensitive to the choice. As an independent test of this filtering technique, we also perform moving polynomial interpolations of the time series [cf. Saar and Manga, 2003]. This latter approach has the advantage that the data is optimally matched in a least squares sense and that no artificial frequencies are introduced. Both approaches to the data analysis yield similar results. We choose to show the analysis based on the convolution with the Gaussian kernel because this smoothing method is similar to that presented by Glazner et al. [1999], and results may thus be compared easily.

Table 1. Parameters Used and Results Obtained During Time Series Analysesa
  • a

    Dotted, solid, dashed, and dash-dotted refer to lines in Figure 4. Some parameters, approximating time as number of bins (points), are rounded to the next appropriate integer value due to finite bin widths of 0.5, 1, 2, and 5 kyr. Upper and lower bounds of the 95% confidence intervals (CI) for random distributions of phases for each frequency are calculated for the first local maximum (correlation)and first local minimum (anticorrelation) cross correlation coefficients (Figure 5).

Bin width, kyr0.51250.512
Width of Gaussian kernel, kyr23232225232322
Width of Gaussian kernel, points4623115462311
Length of time series, kyr400400400400400400400
Length of time series, points80040020080800400200
Segment width, kyr300300300300300300300
Segment width, points60030015060600300150
Step size, kyr1125112
Step size, points2111211
Total number of segments100100502010010050
Time lag interval
  Lower CI, kyr[−2 30][−2 30][−2 30][−5 30][−2 8][−2 8][−2 8]
  Lower CI, points[−4 60][−2 30][−1 15][−1 6][−4 16][−2 8][−1 4]
  Upper CI, kyr[25 45][25 45][24 46][25 45][8 20][8 20][8 20]
  Upper CI, points[50 90][25 45][12 23][5 9][16 40][8 20][4 10]
Total number of correlations for CI calculated1000100050020010001000500
Mean time lag, kyr9.411.313.
2σ-SD, kyr0.
Combined mean time lag, kyr11.411.411.411.43.23.2N/A
Combined 2σ-SD, kyr6.
Combined mean time lag, kyrnot used12.012.012.0
Combined 2σ-SD, kyrnot used6.66.66.6
Combined mean time lag, kyr11.211.211.2not used
Combined 2σ-SD, kyr2.32.32.3not used

[6] Smoothed time series are compared with binned and raw volcanic and SPECMAP data in Figure 2 for different bin widths. Corresponding power spectra for each of the time series are calculated using a standard adaptive multitaper algorithm and shown in Figure 3. Two observations are apparent from a comparison of Figures 2 and 3. First, the choice of bin width not surprisingly governs the temporal scale of structure that can ultimately be resolved. For example, whereas well-established (Milankovitch) periods at 23, 40, and 100 kyr (not shown) are evident in the SPECMAP data if this time series is binned at 0.5 and 1 kyr, only the 100 kyr period is retained for a 5 kyr bin. Second, the 40 kyr glacial period is apparent in both the basaltic and silicic data sets produced using 0.5, 1, and 2 kyr bin widths. This result supports a hypothesis that the cyclical growth and retreat of Sierran glaciers influences regional volcanism.

Figure 3.

Power spectra for the silicic (thin line) and basaltic (dash-doted line) volcanic time series as well as the SPECMAP (thick line) data set shown as a function of bin width. For bin widths in which the well-established 40 kyr glacial period in the SPECMAP data set is resolved, this period is also expressed in both the silicic and the basaltic eruption time series.

[7] The application of the SPECMAP data set as a proxy for glacial ice thickness in the Sierras requires some justification because the correlation of alpine to continental glaciation is contentious [Gillespie and Molnar, 1995]. In particular, analyses of time series of local δ18O variations in vein calcite from Devils Hole, Nevada [e.g., Winograd et al., 1992, 1996; Herbert et al., 2001], as well as temporally similar variations in temperature-calibrated alkenone unsaturation indices gathered along the northern California margin, indicate that rises in groundwater, precipitation, and Pacific sea surface temperature (PSST) in this region over the last 500 kyr generally precede global sea level rises following glacial maxima by 10–15 kyr [Herbert et al., 2001], suggesting that continental and alpine glaciation in the Sierras are asynchronous [Winograd et al., 1992; Gillespie and Molnar, 1995]. However, Herbert et al. [2001] find a tight correspondence between changes in PSST and the global ice volume in interglacial and early glacial phases. Furthermore, in accord with biogeochemical indicators of oceanic upwelling and productivity along the California margin [Dean et al., 1997; Herbert et al., 1995; Sancetta et al., 1992], as well as modeling studies of the influence of Laurentide glaciation on atmospheric circulation over North America [e.g., Kutzbach and Wright, 1985; Manabe and Broccoli, 1985], Herbert et al. [2001] show that increases in PSST preceding glacial terminations correspond to collapses of the cold California current, and probably indicate subsequent intrusions of warm water from the central Pacific. Thus the nearly synchronous California PSST and Devils hole temperature records [Winograd et al., 1996; Herbert et al., 2001] apparently reflect the influence of global glaciation on local climate and are not inconsistent with Sierran glaciation being similar to the global glacial record indicated by SPECMAP [Imbrie et al., 1993].

[8] In section 3 we argue that the rate of change of glacial unloading influences the dynamics of dike formation governing the frequency of volcanic eruptions. Accordingly, in Figure 4 we take the first derivative of the SPECMAP time series, δ18O′, and the first derivatives of the basaltic, B′, and silicic data sets, S′. An important additional result of this procedure is that the time derivatives of the eruption time series vary about a well-defined mean and may be characterized in terms of average statistical properties in a straightforward way. Consequently, Figure 5 shows the cross correlations between δ18O′ and B′ and S′, respectively. Calculated absolute time lags indicate the interval of time between a maximum in the rate of glacial unloading and a peak in associated volcanic response. In more detail, we determine moving normalized unbiased cross-correlation coefficients on overlapping segments within each of the time series. The segment width for all bin widths is 300 kyr, and the step size is 1–5 kyr, depending on bin width. Table 1 summarizes input parameters for, and results from, the time series analysis as a function of bin width. Finally, the segment width of 300 kyr is sufficiently large that multiple periods contribute to the calculation of each cross-correlation coefficient and sufficiently small so that locally highly correlated segments of the time series cannot dominate average cross-correlation coefficients, which ensures that the analysis is statistically valid.

Figure 4.

Plots of the first derivatives of the SPECMAP data set, δ18O′, and the basaltic, B′, and silicic, S′, eruption time series as a function of bin width. Time derivatives for each time series have a zero mean. Each plot shows values for the SPECMAP and the eruption time series at the left and the right y axis, respectively.

Figure 5.

Cross correlations as a function of bin width of the first derivative of the SPECMAP data with the first derivatives of the (top) silicic and (bottom) basaltic eruption time series along with the 95% confidence limits (corresponding fine horizontal lines). Average time lags for the effects of glacial unloading on silicic and basaltic volcanism are distinct and are 3.2 ± 4.2 kyr and 11.2 ± 2.3 kyr, respectively.

[9] Uncertainties on the correlation coefficients are obtained using a Monte Carlo method with the goal of identifying all statistically significant correlations over the full time lag interval of interest (Table 1). In general terms, for each time lag interval uncertainties are calculated by randomly assigning different phases (between 0 and 2π) to each frequency in the frequency domain and then picking one minimum and one maximum cross-correlation coefficient for the complete time lag interval. This method is modified from Saar and Manga [2003] and allows for simultaneous inferences over all time lags within the time lag interval of interest. This procedure is repeated sufficiently many times that a 95% confidence interval can be established within which 95% of all minimum and maximum cross correlation coefficients fall (Table 1) representing anticorrelations and correlations, respectively. In addition, moving cross correlations are chosen in all calculations to reduce the dominating effects of (locally) highly (anti)correlated segments of the time series. This approach allows us to determine formal uncertainties for the time lags as a function of bin width, shown by bars indicating 2σ standard deviations. This approach allows us to determine formal uncertainties for the time lags as a function of bin width. Comparison of the results for different bin widths provides an additional measure of observational bias. For basaltic events calculated time lags are similar or overlapping for each bin choice (Table 1). Neglecting results for the 5 kyr bin width, which are under-resolved (compare Figure 3), we obtain an average time lag of 11.2 ± 2.3 kyr, where the uncertainty reflects two standard deviations. For silicic eruptions time lags and their 2σ standard deviations are similar when the bin width is 0.5–1 kyr and unresolved at a 95% confidence level for larger bins. Thus the average time lag for silicic eruptions is 3.2 ± 4.2 kyr.

3. A Theoretical Model

[10] In a model developed by Jellinek and DePaolo [2003] the evolution of overpressure, ΔPch = (Pch − σr), within a spherical magma chamber contained in Maxwell viscoelastic wall rocks is given by

equation image

where Pch is the pressure in the chamber, which is taken to be hydrostatic, σr is the remote lithostatic stress, and E and μwr are the elastic modulus and effective viscosity of the wall rocks, respectively. Here, ΔPmax = 2μwrQ/3Vch is the maximum sustainable magma chamber overpressure and corresponds to the condition dΔPch/dt = 0. For a given long-term average magma supply, Q, effective wall rock viscosity, μwr, and magma chamber volume, Vch, ΔPmax is approximately constant. Dike formation is expected to lead to volcanic eruptions if ΔPmax > ΔPcrit, where ΔPcrit is the critical overpressure required to propagate a dike from the bounding chamber wall rocks to the surface, resulting in an eruption [Jellinek and DePaolo, 2003]. In this study we are interested in how the rate of change of glacial unloading affects the evolution of chamber overpressure and thus the timing of dike formation and volcanism (Figure 6). In principal, glacial unloading can influence the frequency of dike formation, by both reducing the confining lithostatic stress, which retards the stretching and radial expansion of chamber walls due to an overpressure [Sammis and Julian, 1987; McLeod and Tait, 1999; Jellinek and DePaolo, 2003], as well as the rate of decompression melting in the mantle, which governs the long-term magma supply [e.g., Jull and Mackenzie, 1996]. The time lags identified in Figure 5, however, show that glacial unloading affects silicic and basaltic volcanism differently. This observation is inconsistent with volcanism being due to a uniform increase in the magma supply rate resulting from enhanced decompression melting. Moreover, mantle-derived basalts are likely to form at depths greater than about 50 km [e.g., Kushiro, 1996; DePaolo and Daley, 2000]. Stresses resulting from a narrow Sierra ice sheet will fall off with depth as 1/r3, where r is the radial distance from the center of mass of the ice load [e.g., Jaeger and Cook, 1979]. Thus we expect the effect of Sierra glacial loading on underlying mantle melting to be small.

Figure 6.

Cartoon illustrating the model problem and our analytical approach. The rate of change in surface loading due to melting glaciers influences the mechanics of dike formation and thus the frequency of volcanic eruptions. The response of the magmatic system to this external forcing is an intrinsic property that is characterized by the transfer function H(iω). Our theoretical model is linear and thus the output response (eruption frequency), Y(iω), to the input forcing (rate of change of glacial loading), X(iω), is the product X(iω)H(iω).

[11] In contrast to the large depth of melt generation, silicic volcanism in this region is thought to occur from shallow (5–8 km depth) chambers, where the influence of glacial loading and unloading on the lithostatic stress may be significant. In particular, the tensile deviatoric stress parallel to the chamber walls, which occurs in response to the chamber overpressure and acts to dilate fractures such that dikes may form, is governed by the lithostatic stress [McLeod and Tait, 1999; Jellinek and DePaolo, 2003]. Thus, assuming that ΔPmax ≥ ΔPcrit, harmonic glacial unloading may govern the dynamics of dike formation as well as the eruption frequency in this region. To investigate this possibility, we assume ΔPmax ≥ ΔPcrit and replace the constant source term (EwrPmax with the rate of change of glacial unloading, −dΔPf/dt, and obtain a new equation for the evolution of magma chamber overpressure:

equation image

Here, the quantity τm = μwr/E is the Maxwell relaxation timescale. Of particular importance to this discussion is that whether unloading occurs over a timescale that is long or short in comparison to this timescale ultimately governs the response of the system. Thus the rate of change of surface loading will have a larger influence on dike formation than the absolute ice load. In the asymptotic situation of effectively infinite μwr the second term can be neglected. In this case, glacial unloading occurs over a timescale that is small in comparison to the Maxwell time. Wall rock rheology is approximately elastic and the response of the evolution of chamber overpressure to deglaciation will be instantaneous and of the same mathematical form as the external forcing. In contrast, for finite μwr the second term cannot be neglected. In this situation, glacial unloading occurs on a timescale that is comparable to, or long compared with, the Maxwell time. The viscous part of the wall rock rheology is important and this additional damping causes the response of the magmatic system to lag behind glacial unloading.

[12] In order to reduce the number of parameters and simplify the discussion it is useful to nondimensionalize equation (2). Making the substitutions Pch = ΔPchPcrit, Pf = ΔPfPcrit and τ = tm gives

equation image

To further compare the model with data, it is useful to look at the solution to equation (3) in the frequency domain. The frequency response of the system is given by the transfer function H(iω) = Y(iω)/X(iω), where X(iω) and Y(iω) are the Fourier transforms of the input (rate of change of surface stress due to temporal changes in ice thickness) and output (critical overpressure for dike formation and eruption), respectively. Thus for equation (3),

equation image

Multiplying equation (4) by (iω − 1)/(iω − 1) and rearranging yields

equation image

where −ω2/(ω2 + 1) and −ω/(ω2 + 1) are the real, equation image, and imaginary, equation image, parts of H(iω), respectively. Trigonometry in the complex plane gives the magnitude, ∣H(iω)∣ = equation image, and phase, θ(ω) = tan−1 (equation image) = tan−1(1/ω). The magnitude of the transfer function describes the amplitude filtering characteristics of the dike formation model and is a distinctive property that can be obtained from the data analysis:

equation image

where the forcing timescale τf is normalized by the Maxwell time, τm. The phase of equation (3) gives the lag between the glacial forcing and the response of the model system and (for positive frequencies) is related to the time lag, Γ, determined from the analysis in Figure 5:

equation image

Physically, the phase or “time lag” provides information about the temporal response of the magmatic system to forcing at different frequencies.

4. Discussion

[13] Figure 7 shows θ(ω) and ∣H(iω)∣ as functions of the normalized forcing frequency τmf. Also included are the time lags for basaltic and silicic eruptions determined from the data analysis. Each of these time lags, along with their uncertainties, may be projected onto the theoretical curve for θ(ω), which, in turn, identifies a range of values for the ratios τmf and ∣H(iω)∣. Consequently, the time lags determined from the data analysis constrain ∣H(iω)∣ to be about 0.8 for silicic volcanism and <2 × 10−2 for basaltic volcanism. In principle, with additional constraints on ΔPcrit or ΔPf, values for either parameter may be obtained. However, Glazner et al. [1999] suggest that a plausible estimate for the mean ice thickness and lake depth in this region is around 300 m which corresponds to ΔPf ≈ 3 MPa. Thus from Figure 5, for silicic and basaltic volcanism, this loading constrains ΔPcrit to be 3 MPa and ≪1 MPa, respectively. For comparison, using a theoretical model Jellinek and DePaolo [2003] argue that ΔPcrit is in the range 10–30 MPa for silicic magmas and is likely ≪1 MPa for basaltic magmas. We note that Glazner et al. [1999] indicate that the maximum ice thickness was about 1.5 km; if this estimate for ice thickness is more accurate then 15 MPa and ≪1 MPa may be more appropriate estimates for silicic and basaltic volcanism, respectively. The present analysis, based on data, thus provides an additional independent constraint on ΔPcrit.

Figure 7.

Plots of the (top) theoretical time lag and (bottom) magnitude of the transfer function as a function the ratio of the Maxwell time to the characteristic period for glacial forcing (i.e., this is a dimensionless frequency). Also shown are the time lags determined from the data analysis for basaltic and silicic volcanism (Figure 5). Constraints on these time lags lead to estimates for the critical magma chamber overpressure required for volcanic eruptions and for the effective viscosity of the wall rocks governing dike formation (shaded regions). See text for discussion.

[14] Figure 7 also shows that our estimate for τf ≈ 40 kyr constrains a lower bound for the Maxwell time, τm, governing silicic dike formation and volcanism to be approximately 30–80 kyr. Our results constrain an upper bound for τm for basaltic volcanism of around 2 kyr. Taking E = 1010 Pa to be typical for all rocks, these Maxwell times imply that the average effective wall rock viscosities governing silicic and basaltic volcanism are around ≥1022 Pa s and ≤6 × 1020 Pa s, respectively. If the forcing time was chosen instead to be τf ≈ 100 kyr, the dominant period in the glacial record, then the inferred viscosities are 2 × 1022 to 3 × 1023 Pa s and <1.5 × 1021 Pa s, respectively. The 100 kyr period is not dominant in the volcanic eruption record that we have analyzed. We expect that the 100 kyr period will be suppressed because older eruptions are less well sampled. The additional well-known glacial period of τf ≈ 23 kyr that is evident in the SPECMAP data and the silicic time series (Figure 3) is not significantly expressed in the volcanic time series. It is noteworthy, however, that Paterne et al. [1990] and Paterne and Guichard [1993] identify this period (and not the 40 kyr period found in this study) in a time series of volcanic eruptions from the Campanian area of southern Italy. They suggest on further geochemical grounds that harmonic glacial forcing may govern the influx of new magma to magma chambers from which the observed eruptions originate.

[15] Assuming that the effective viscosity of crustal rocks declines with increasing temperature [e.g., Kirby, 1985], and that temperature increases monotonically with depth in the crust, these results are consistent with basaltic magmas coming from a greater depth than silicic magmas. Geochemical and petrological observations suggest that whereas the rhyolite magmas may erupt from depths of 5–8 km in eastern California [e.g., Anderson et al., 1989; Wallace et al., 1995], basaltic magmas may erupt from the base of the lithosphere [e.g., DePaolo and Daley, 2000]. Finally, these wall rock viscosities are consistent with the conclusion of Jellinek and DePaolo [2003] that under most plausible conditions for silicic magma chambers in intracontinental settings, the dynamics governing dike formation are likely to lead to volcanism if μwr > 1020 Pa s.

5. Concluding Remarks

[16] Magmatic and volcanic systems involve processes that operate over a wide range of timescales and length scales. In our particular example, an analysis of the response of a magmatic system to glacial forcing at the kiloyear timescale provides new insight into crustal dynamics (e.g., the Maxwell timescale and wall rock viscosity) and magma transport (e.g., dike propagation).

[17] The values obtained here for crustal and magma chamber properties rely on the accuracy of the two time series: eruption frequency and glacial loading. We can expect improved estimates to follow from further refinements in the ages of eruptions, more dated eruptions, and a continuous and complete record of local ice and lake volume.


[18] We thank Alan Glazner for critical comments on an earlier version of this manuscript and for supplying the raw eruption data used to compile Figures 1 and 2. This manuscript has benefited from thoughtful reviews by D. M. Pyle and an anonymous reviewer as well as from comments by Bernd Milkreit, Catherine Johnson, Cathy Constable, Giorgio Spada, and Francis Albarede. This study was supported by NSF EAR 019296, the Canadian Institute for Advanced Research (CIAR), and NSERC.