Abstract

Atmospheric Lagrangian particle dispersion models, LPDM, simulate the dispersion of passive tracers in the atmosphere. At the most basic level, model output consists of the position of computational particles and the amount of mass they represent. In order to obtain concentration values, this information is then converted to a mass distribution via density estimation. To date, density estimation is performed with a nonparametric method so that output consists of gridded concentration data. Here we introduce the use of Gaussian mixture models, GMM, for density estimation. We compare to the histogram or bin counting method for a tracer experiment and simulation of a large volcanic ash cloud. We also demonstrate the use of the mixture model for automatic identification of features in a complex plume such as is produced by a large volcanic eruption. We conclude that use of a mixture model for density estimation and feature identification has potential to be very useful.

Highlights

  • Atmospheric Lagrangian particle dispersion models, LPDM, model the path of computational particles which represent passive tracers in the atmosphere

  • This task is usually integrated into the modeling code itself, so that the main model output consists of gridded concentrations

  • We provide examples of its use for modeling distal volcanic ash clouds

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Summary

Introduction

Atmospheric Lagrangian particle dispersion models, LPDM, model the path of computational particles which represent passive tracers in the atmosphere. In order to obtain concentration values, this information is converted to a mass distribution via density estimation This task is usually integrated into the modeling code itself, so that the main model output consists of gridded concentrations. A three dimensional grid, the concentration grid, is defined and gridded concentrations are calculated by summing the mass of the particles within each grid box and dividing by the volume. This method works quite well for regions in which the number of computational particles in the bin, N, is large but shot noise dominates at lower values of N. In some cases it is desirable to define a high resolution concentration grid for close to the source and a coarser concentration grid for computing concentrations far from the source [1]

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