Software Open Access

Tesseroids v1.2.1: Forward modeling of gravitational fields in spherical coordinates

Uieda, Leonardo


Dublin Core Export

<?xml version='1.0' encoding='utf-8'?>
<oai_dc:dc xmlns:dc="http://purl.org/dc/elements/1.1/" xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/ http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
  <dc:creator>Uieda, Leonardo</dc:creator>
  <dc:date>2017-05-23</dc:date>
  <dc:description>A collection of command-line programs for modeling the gravitational potential, acceleration, and gradient tensor. Tesseroids supports models and computation grids in Cartesian and spherical coordinates.

Official website and documentation: http://tesseroids.leouieda.com/

Changes to version 1.2.1:


	Binaries for Windows 64bit are now available for download as well.
	Validate order of boundaries for input tesseroids. Errors if boundaries are switched (e.g, W &gt; E).
	Ignore tesseroids with zero volume from the input file (i.e., W == E, S == N, or top == bottom). These elements can cause crashes because of infinite loops during adaptive discretization.
</dc:description>
  <dc:identifier>https://zenodo.org/record/582366</dc:identifier>
  <dc:identifier>10.5281/zenodo.582366</dc:identifier>
  <dc:identifier>oai:zenodo.org:582366</dc:identifier>
  <dc:rights>info:eu-repo/semantics/openAccess</dc:rights>
  <dc:rights>https://www.eclipse.org/org/documents/edl-v10.php</dc:rights>
  <dc:subject>geophysics</dc:subject>
  <dc:subject>gravity</dc:subject>
  <dc:subject>tesseroids</dc:subject>
  <dc:subject>C</dc:subject>
  <dc:title>Tesseroids v1.2.1: Forward modeling of gravitational fields in spherical coordinates</dc:title>
  <dc:type>info:eu-repo/semantics/other</dc:type>
  <dc:type>software</dc:type>
</oai_dc:dc>
591
116
views
downloads
All versions This version
Views 591591
Downloads 116113
Data volume 585.6 MB572.5 MB
Unique views 545545
Unique downloads 7170

Share

Cite as