Document Type

Article

Publication Date

12-2012

Keywords

lava flow simulation, modeling code, probabilistic hazard assessment, spatial density, Monte Carlo method, Armenia

Digital Object Identifier (DOI)

https://doi.org/10.1186/2191-5040-1-3

Abstract

Probabilistic modeling of lava flow hazard is a two-stage process. The first step is an estimation of the possible locations of future eruptive vents followed by an estimation of probable areas of inundation by lava flows issuing from these vents. We present a methodology using this two-stage approach to estimate lava flow hazard at a nuclear power plant site near Aragats, a Quaternary volcano in Armenia.

Comments

Supplementary material at https://doi.org/10.1186/2191-5040-1-3

Was this content written or created while at USF?

Yes

Citation / Publisher Attribution

Journal of Applied Volcanology, v. 1, art. 3

This article is published under license to BioMed Central Ltd. This is an Open Access article distributed under the terms of the Creative Commons Attribution License (http://creativecommons.org/licenses/by/2.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.

Additional file 1.PL (5 kB)
PERL script that estimates spatial density. This code depends on inputs generated by the SAMSE bandwidth estimation routine from the 'ks' library package as part of the 'R' programming package. This PERL script is an ASCII (text) file that can be viewed with any text editor. It is run from the command line: perl. (PL 6 KB)

Additional file 2.PL (13 kB)
PERL script that simulates volume-limited lava flows from vents on and around the Shamiram Plateau. This lava flow script depends on the output spatial density grid file generated by the above mentioned spatial density script (additional file 1). It is an ASCII file that can be viewed with any text editor. It is run from the command line: perl. (PL 13 KB)

Additional file 3.PL (13 kB)
Perl script that simulates effusion rate-limited lava flows from vents located on the flanks of Aragats. This lava flow script depends on the output spatial density grid file generated by the above mentioned spatial density script (additional file 1). It is an ASCII file that can be viewed with any text editor. It is run from the command line: perl. (PL 14 KB)

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