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PreprintCC BY 4.0arXiv

The istr-graph: Interactive Visualisation of any Classic-Graph in DDLab

  • Andrew Wuensche
Open at sourcePDFDOICite

Abstract

Any type of attractor basin (classic-graph) created in DDLab can now be visualised, manipulated, and deconstructed as a drag/drop ``interactive state transition graph'' (istr-graph). The new istr-graph applies to subtrees, single basins, the basin of attraction field, compression, and all other classic-graph parameters. This is an important update on the pre-existing ``interactive basin of attraction field graph'' (ibaf-graph) specific to just the complete uncompressed field, but the ibaf-graph is nevertheless retained for some of its unique attributes. These issues are discussed with a focus on the scope and implementation of the new istr-graph.

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Cite

BibTeXRIS
BibTeX
@misc{wuensche2026istrgraph,
  title = {{The istr-graph: Interactive Visualisation of any Classic-Graph in DDLab}},
  author = {Andrew Wuensche},
  howpublished = {arXiv},
  year = {2026},
  month = aug,
  doi = {10.48550/arxiv.2608.29962},
  eprint = {2608.29962},
  archivePrefix = {arXiv},
  url = {https://arxiv.org/abs/2608.29962},
  note = {CC BY 4.0},
}
RIS
TY  - UNPB
TI  - The istr-graph: Interactive Visualisation of any Classic-Graph in DDLab
AU  - Andrew Wuensche
PY  - 2026
DA  - 2026/08/30
PB  - arXiv
DO  - 10.48550/arxiv.2608.29962
UR  - https://arxiv.org/abs/2608.29962
AB  - Any type of attractor basin (classic-graph) created in DDLab can now be visualised, manipulated, and deconstructed as a drag/drop ``interactive state transition graph'' (istr-graph). The new istr-graph applies to subtrees, single basins, the basin of attraction field, compression, and all other classic-graph parameters. This is an important update on the pre-existing ``interactive basin of attraction field graph'' (ibaf-graph) specific to just the complete uncompressed field, but the ibaf-graph is nevertheless retained for some of its unique attributes. These issues are discussed with a focus on the scope and implementation of the new istr-graph.
ER  -