Sistemas planetarios · PLA 002
Uso responsable y licencias del repositorio ISHEA
Los archivos, datos y scripts del repositorio son de acceso público para investigación y replicación; cualquier uso comercial o adaptación de la metodología Δ±1 requiere permiso escrito del ISHEA Institute.
Pieza original en inglés.
ISHEA Repository Responsible Use & Licensing Guidelines
- Introduction
Welcome to the ISHEA Institute repository system. All projects, datasets, scripts, and preprints published under ISHEA are made publicly accessible for research, replication, and academic purposes.
The Δ±1 framework and related methodologies represent sensitive intellectual property developed by ISHEA. While public availability promotes transparency and scientific reproducibility, any adaptation, modification, or commercial use requires prior written consent from the ISHEA Institute.
- Scope
This Wiki applies to all ISHEA projects including but not limited to:
Datasets (CSV, JSON, experimental raw data)
Scripts, code, and computational notebooks
Preprints, manuscripts, and posters
Supplementary materials and figures
Public sharing does not imply permission for commercial exploitation or unregulated application.
- Responsible Use
Researchers and users may:
- Download and use data or scripts for:
Academic research
Reproduction of results
Teaching and training purposes
- Cite the original source using DOI or OSF project links.
Users may NOT:
Apply the Δ±1 methodology in commercial or product development without explicit written consent
Redistribute datasets or scripts as “own work” or under another license
Modify core algorithms or weighting systems for external applications without ISHEA approval
- Citation
When using any ISHEA materials, please cite:
Pérez Pulido, C.J. · ISHEA Institute · [Project Title] · [Year] · DOI: [DOI Link]
Example for PEFI / Planetary Energy Flow data:
Pérez Pulido, C.J. · ISHEA Institute · Integrating Planetary Energy Flows, Solar Cycles, and Biosystem Dynamics · 2026 · DOI: 10.17605/OSF.IO/GY83R
- Contact for Commercial or Applied Use
All inquiries for commercial or applied use of Δ±1 methodology, proprietary weighting, or datasets should be addressed to:
ISHEA Institute
isheainstitute.org@gmail.com
Include:
Your intended use case
Project or organization details
Requested data/methodology
- Opt-Out / SHARE Indexing
By default, OSF public projects are indexed into SHARE for discoverability. While your profile and projects are included, all public projects, files, and preprints remain discoverable.
To reduce indexing of your personal profile, follow OSF settings:
Go to Profile > Account Settings > “Exclude me from SHARE indexing”
Note: public content will still appear in searches.
- Headers for Files
For every dataset or document, include the following header (first line):
© 2026 ISHEA Institute. Public access for academic research only. Commercial application requires prior written consent.
- Updates
This Wiki will be updated periodically to reflect:
New datasets
Methodological revisions
Additional legal guidance
Always check the latest version before citing or using ISHEA materials.
✅ Summary
Public access = academic/research use only
Commercial use = prior written consent required
Cite all ISHEA materials
Centralized project Wiki ensures consistent legal guidance
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En la misma sala — Sistemas planetarios
PLA 001 · Sistemas planetarios
Zona HALO
Línea de investigación planetaria del ISHEA Institute: HALO nombra la franja en la que un sistema puede sostener complejidad organizada, una lectura de la habitabilidad más allá de la distancia orbital.
PLA 003 · Sistemas planetarios
Detección híbrida del vórtice polar y del calentamiento súbito estratosférico
Un índice físico Δ±1 combinado con XGBoost capta las interacciones no lineales entre clima espacial y dinámica estratosférica; los datos sintéticos avalan la viabilidad antes de validarlo con observaciones.
PLA 004 · Sistemas planetarios
Evidencia empírica de la formación de péptidos impulsada por energía
La energía dirigida induce la formación de péptidos a partir de glicina en condiciones interplanetarias, un apoyo empírico al acoplamiento energético universal y la autoorganización molecular del marco ECU.