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README.TXT

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README FOR HC
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Version 1.0.8 - 2018
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Version 1.0.15 - 2022
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Thorsten Becker - [email protected].edu
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Thorsten Becker - [email protected].edu
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HC is a global mantle circulation solver following Hager & O'Connell
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(1981) which can compute velocities, tractions, and geoid for simple
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density distributions and plate velocities.
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(1981) which can compute velocities, tractions, and the geoid for
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arbirtrary density distributions and radial viscosity variations.
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This particular implementation illustrates one possible way to combine
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the HC solver routines.
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Based on code by Brad Hager, Richard O'Connell, and Bernhard
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Steinberger, this version is by Thorsten Becker and Craig O'Neill.
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Note also that the Solid Earth Teaching and Research Environment
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(SEATREE, http://geosys.usc.edu/projects/seatree/), as preinstalled
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with software as a VirtualBox available from the Unified Geodynamics
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Earth Science Computing Environment (UGESCE,
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the HC solver routines. There is a forward tool example, as included
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in the graphical user interface SEATREE, and a parameter space
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exploration tool to scan viscosity distributions in terms of their
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predictions of the geoid.
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This code is based on Fortran routine by Brad Hager, Richard
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O'Connell, and most recently Bernhard Steinberger, who made several
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modifications. This version is by Thorsten Becker with contributions
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to the plate velocity inversion tool by Craig O'Neill (the latter
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remains incomplete).
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The Solid Earth Teaching and Research Environment (SEATREE,
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https://github.com/thwbecker/seatree/), as preinstalled with
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software as a VirtualBox available from the Unified Geodynamics Earth
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Science Computing Environment (UGESCE,
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http://www-udc.ig.utexas.edu/external/becker/ugesce.html) provides a
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convenient user interface for HC.
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convenient graphical user interface for HC to select seismic
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tomography models, edit viscosity structures, etc.
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INSTALLATION
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The code should compile on any basic UNIX/Linux system with the GMT
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tools (by default, version > 4.2.1, and only version 4.X.X is
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supported!) and libraries installed. See the Makefile for comments and
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tools (BY DEFAULT, VERSION > 4.2.1, AND ONLY VERSION 4.X.X IS
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SUPPORTED!) and libraries installed. See the Makefile for comments and
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what to modify.
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What is described below is the hc Hager & O'Connell (1981) forward
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flow and geoid computation. For plate velocity inversions following
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the Ricard & Vigny (1989) method, see the hcplates subdirectory and
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the README there. The plate inversion code, due to Craig O'Neill isn't
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quite working yet.
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the README there. The plate inversion code is not quite working yet.
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The Makefile assumes that the following environment variables are
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predefined:
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1) GMTHOME: needs to point to the base directory of the GMT installation,
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e.g.
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/usr/local/src/GMTdev/GMT4.5.6/
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/usr/local/src/GMTdev/GMT4.5.18/
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if you installed GMT yourself, or
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HC CODE usage
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Described in the help page that is displayed for "hc -h" as below.
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Also see SEATREE (http://geosys.usc.edu/projects/seatree/) for a
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Also see SEATREE (https://github.com/thwbecker/seatree/) for a
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graphical user interface, and example plotting scripts as provided
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below.
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(SEATREE) which provides a graphical user interface to flow
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computations and plotting.
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https://geosys.usc.edu/projects/seatree/wiki/
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https://github.com/thwbecker/seatree
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UGESCE
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Science data and software, all in one (big) package, ready to go.
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COPYRIGHT
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Versions of this software might include Numerical Recipes code (HC
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does not rely on it, only some related tools do) - copyright is with
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these authors, do not distribute without permission.
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For all of the HC code, copyright by Thorsten Becker,
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[email protected], under GPL of 1991.
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