Testing the accuracy of a 1-D volcanic plume model in estimating mass eruption rate by Larry G. Mastin, U.S. Geological Survey, Cascases Volcano Observatory ([email protected]) v=~0.34 2 10 4/4a 0.04 1 0 0 Fuego 15 10 g vº N g =increase in wind speed per m altitude N=Brunt-Vaisala frequency Hekla 1974 v=0.11 0 10 10 5 5 1980 1970 v=0.06 0 0 v=0.12 St. Helens 20 15 10 0.10 0.09 6/12 5/25 5/18 5 7/22 40 Pinatubo v=0.05 30 20 10 Hudson 15 0.06 0.03 When v<~0.35, Hmax=Hnowind , indicating weak winds (Fig. 1b). 21 of these 25 eruptions are in this category. 10 Ruiz 10 5 5 0 0 Redoubt 15 Reventador 25 10 v=0.38 g 10 20 10 0 20 40 8/18 Figure 2 9/17 6/27 0 0 20 40 0 0 20 40 0 0 20 40 wind speed, m/s Eruptions examined ù æ ö dE d é u2 a dM = M + gZ + h = gZ + h () ê ú ç ÷ ds ds ë 2 ds è ø û The model considers ambient wind, temperature variations in the atmosphere, and enthalpy of phase changes of water & ice. Input conditions: (1) Mass eruption rate based on assumed magma temperature (900 C), magma gas content (3 wt%), ejection velocity (~150 m/s), and vent diameter adjusted to give a specified eruption rate. (2) Atmospheric inputs, including temperature, humidity and wind vector as a function of elevation. Solution method: The conservation equations are integrated upward using a Cash-Karp Runge-Kutta method with automatic step-size adjustment. Information sources: 1[Hill et al., 1998],2[Carey and Sigurdsson, 1986],3[Scollo et al., 2007],4[Bonis and Salazar, 1973],5 [Rose et al., 1973],6 [Rose et al., 2008],7[Thorarinsson and Sigvaldason, 1971],8[Gronvold et al., 1983],9[Naranjo S. et al., 1993],10[Scasso et al., 1994],11[Tupper et al., 2004],12[Nakada et al., 2005],13[Geshi et al., 2002],14[Sarna-Wojcicki et al., 1981],15[PaladioMelosantos et al., 1996],16[Hoblitt et al., 1996],17 [Pallister et al., 1992],18[Koyaguchi, 1996],19[Koyaguchi and Ohno, 2001],20[Holasek et al., 1996],21[Miller and Chouet, 1994],22[Scott and McGimsey, 1994],23[Smithsonian Institution, 2002],24[Prata and Grant, 2001],25[Bonadonna and Houghton, 2005],26[Naranjo et al., 1986],27[Neal et al. [1995],28[Eichelberger et al., 1995],29 [McGimsey et al., 2001] real plumes eq obs max Model representation max min max min max nowind max max max nowind min max max min Figure 1 max i 2 4 6 8 10 Mmax Mmin s =0.53 m =0.07 0 -2 bent-plume model 0 10 20 30 40 0 -2 plume model ignoring wind 0 10 20 30 40 ? Low s indicates better predictive s =0.50 m =-0.07 2 s =0.62 m =-0.25 2 accuracy ? Positive (negative) m suggests tendency to over- (under-) predict 0 empirical curve -2 10 20 30 40 For eruptions overall: ? Neither the empirical curve (Mempir) nor 1-D model (Mavg) systematically over- or underpredict eruption rate relative to Mobs. ? Standard error for the 1-D model (0.53) is not better (more accurate) than for the empirical curve (0.50). ? But the data are few, observations are poor, and most plumes occurred during low-wind conditions. Modeling plume height in real winds obs 2 Figure 5 Observed plume height, km 40 Calculated plume height, km obs Mavg 2 0 Model limitations: Each step in the model is assumed to represent the center of a control volume whose mass, momentum, and energy flux is being tracked. ? In the absence of wind (Fig. 1d), this results in a vertical stack of control volumes that don’t overlap. The maximum height (Hnowind) is the point where ascent velocity-->0. Strong wind ? In high-winds (Fig. 1f), the No wind Weak wind model produces a bending a b c stack of control volumes H H whose maximum height is H between the maximum H z r height of the plume axis (zmax) and that elevation plus the plume radius (zmax+rmax). ? In low winds (Fig. 1e), control volumes overlap, and sometimes zmax+rmax>Hnowind, H =H f producing an unrealistically H =z +r H straight high plume. H =z d cylinders e Thus, for specified input conditions, the model gives a range of possible H =H plume heights, Hmin to Hmax . H bent H =z +r If zmax+rmax>Hnowind, Hmax=Hnowind. cylinders H g Otherwise, Hmax=zmax+rmax. h 4 Below are residuals between calculated eruption rates and the observed (Mobs), with standard error s and mean m . v=0.21 5 10 6 Modeled vs. empirical: which is more accurate? Spurr 0.13 Mnowind plume model w/o wind M max plume model Mmin with wind 8 vent elevation 5 0 empirical curve top of observed plume 15 5 Mempir Log(M ), kg s-1 Main Findings: obs 6 ? For small eruptions (Mobs< ~10 kg/s), the empirical relationship (Mempir) consistently underestimates eruption rate; however the 1-D plume model (Mmin to Mmax) mostly overestimates it. (but there are only four eruptions in this category!) ? For larger eruptions there is no clear tendency for any method of calculation to underor overestimate. v=0.07 0.12 v=0.03 5 Miyakejima 20 15 30 v=0.69 1 wind soundings every 12 hrs 10 0 Ruapehu v=~1.03 20 0.31 0 2 15 v=0.22 6/12 6/15 3 0 20 15 15 0.06 5 0 20 20 1971 0.03 Log calculated eruption rate, kg s-1 4/4b 10 log(Mnowind/Mobs) n n 1/ n dM a é ù when r = 2p r r r a uvs1 ) + b v^ ( ( ) >=r a ë û ds d M x dM = vx s=distance along the curving plume path ds ds u=plume ascent (axial) velocity a r =plume bulk density, r =ambient air density d M y dM M = vy vx, vy are x & y components of wind vector ds ds a and b are radial & crossflow entrainment coeffificients vP =wind velocity component parallel to plume axis dMz 2 a = p r () r r g v^ =wind velocity component perpendicular to plume axis ds 3 Eruption rate estimates are compared to those obtained by mapping. 4 v=0.03 20 Etna 2001 5 3/29 4 km asl v=~0.14 El Chichon log(Mavg/Mobs) n n 1/ n dM a é ùwhen r = 2p r r a uvs1 ) + b v^ ( ( ) <r a ë û ds total energy E 5 Cerro Negro 1995 5 30 Hnowind Each plume is modeled using the observed eruption rate Mobs to obtain Hnowind, Hmin, and Hmax. Results are compared with the observed height Hobs Hmax 30 Hmin in order to improve estimates of eruption rate through 1-D plume models, we need more accurate observations of plume height. plume model w/o wind plume model with wind 20 10 References: Figure 3 0 0 10 20 Hobs, km 30 40 Estimating eruption rate Mass eruption rate is estimated by running 5 model simulations (Fig. 4) and finding the range of eruption rates (Mmin to Mmax) for which Hmin<Hobs<Hmax. Simulations were also repeatedly run ignoring wind, to find the eruption rate (Mnowind) at which the calculated height agreed with Hobs. Plume height, km momentum wind soundings every 12 hrs 0 In this study I modify the 1-D plume model Plumeria (Mastin, 2007) to account for crosswinds, using the following conservation equations: mass M 10 Cerro Negro 1992 Residuals Model formulation I examine atmospheric wind, temperature, and humidity during the 25 historical eruptions below. Conditions are obtained from the NCEP/NCAR Reanalysis 1 2.5 degree model. For each eruption I calculate a dimensionless wind: Elevation, km asl During volcanic eruptions, empirical relationships are used to estimate mass eruption rate from plume height. Although simple, such relationships can be inaccurate and can underestimate rates for eruptions in windy conditions. 1-D plume models can incorporate atmospheric conditions and are hypothesized to give potentially more accurate estimates. Here, I present a 1-D model for plumes in cross wind and use it to simulate 25 historical eruptions where plume height Hobs was well observed, and where mass eruption rate Mobs could be calculated from mapped deposit mass and observed duration. The simulations considered wind, temperature, and phase changes of water. Atmospheric conditions were obtained from the NCEP/NCAR Reanalysis 2.5 degree model. Simulations calculate the minimum, maximum, and average values (Mmin, Mmax , and Mavg) that fit the plume height. Eruption rates were also estimated from the empirical formula Mempir=140Hobs4.14 (Mempir is in kg s-1, Hobs is in km). For these eruptions, the standard error of the residual is about 0.53 for Mavg and 0.50 for Mempir. Thus for this dataset, the model is slightly less accurate at predicting Mobs than the empirical curve. The empirical curve however tends to underestimate eruption rate for low plumes during small eruptions. Improved eruption-rate estimates using this (or other) 1-D plume model(s) may require more accurate plume-height observations and improvements in model formulation. Modeled vs. observed eruption rates Wind during real eruptions log(Mempir/Mobs) Abstract Run 1 2 Hmax 3 4 5 Hobs Hmin Figure 4 Mmin Mmax Log mass eruption rate Finally, mass eruption rate is calculated using an empirical formula rearranged from Mastin et al. 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