| _version_ | 1866901762526412800 |
|---|---|
| author | Luis Pablo Araya Salazar |
| author_facet | Luis Pablo Araya Salazar |
| contents | <h2>EUREKA III - ARAYA2 V1.3</h2> <p><strong>Eureka III Araya2 V1.3</strong> presents a non-enabling blind forecast protocol designed to validate selected outputs of the proprietary <strong>Araya2 Multiscale Metric</strong>, developed by <strong>Luis Pablo Araya Salazar</strong>.</p> <p><strong>Eureka III Araya2 V1.3 </strong>builds on the public non-enabling Araya2 record established through AraY2 v1.0, the 96-hour post-event verification, Eureka Araya2 v1.1 and Eureka II Araya2 v1.2. It extends that trajectory into a sealed HVS blind forecast protocol astronomical state verification.</p> <p>This publication establishes a timestamped verification framework before the observational confirmation window of <strong>May 13–14, 2026</strong>. The document records a sealed validation structure based on <strong>HVS milestones</strong>: four critical physical-state checkpoints per astronomical block. This structure allows later comparison against NASA/JPL Horizons-derived ephemeris data while avoiding disclosure of the continuous vector time series, internal constants, and generative derivation of the Araya2 operator.</p> <p>The forecast framework covers three validation blocks:</p> <ul> <li>Europa–Jupiter vector-state validation</li> <li>NEO 2026 JD1 geocentric trajectory validation</li> <li>Moon–Saturn angular separation validation</li> </ul> <p>Each block is expressed through UTC/TDB timestamps, reference frames, selected physical-state variables, Horizons/JPL-derived inputs, sealed Araya2 outputs, and residual validation criteria.</p> <p>The sealed residual benchmark reported for the Araya2 residual-correction operator is:</p> <p><strong>EDMS_rel = 0.0345506917%</strong></p> <p>This value is below the internal Eureka III critical validation threshold:</p> <p><strong>EDMS_rel < 0.0598%</strong></p> <p>This record is <strong>not presented as a final post-event validation</strong>. It is a pre-registered forecast artifact intended for later comparison after the May 13–14, 2026 verification window.</p> <p>To protect the proprietary structure of Araya2, this publication discloses only four verification points per astronomical block:</p> <ol> <li>Window start</li> <li>Central event / closest-state condition</li> <li>Window exit</li> <li>Validation closure</li> </ol> <p>The full generative method, internal constants, continuous vector series, and proprietary derivation remain undisclosed. This publication functions as a priority record, validation framework, and non-enabling forecast artifact for subsequent independent comparison.</p> <p> </p> |
| format | Recurso digital |
| id | zenodo_https___doi_org_10_5281_zenodo_20129946 |
| institution | Zenodo |
| language | |
| publishDate | 2026 |
| publisher | Zenodo |
| record_format | zenodo |
| spellingShingle | Eureka III —Araya2 V1.3 Blind Forecast Protocol for Orbital-State Validation Using HVS Milestones Luis Pablo Araya Salazar Araya2; Multiscale Metric; Blind Forecast; Orbital Validation; Ephemeris; JPL Horizons; Europa; Jupiter; 2026 JD1; Moon-Saturn; Residual Correction; HVS Milestones; Non-Enabling Publication; Astronomical State Verification; Luis Pablo Araya Salazar <h2>EUREKA III - ARAYA2 V1.3</h2> <p><strong>Eureka III Araya2 V1.3</strong> presents a non-enabling blind forecast protocol designed to validate selected outputs of the proprietary <strong>Araya2 Multiscale Metric</strong>, developed by <strong>Luis Pablo Araya Salazar</strong>.</p> <p><strong>Eureka III Araya2 V1.3 </strong>builds on the public non-enabling Araya2 record established through AraY2 v1.0, the 96-hour post-event verification, Eureka Araya2 v1.1 and Eureka II Araya2 v1.2. It extends that trajectory into a sealed HVS blind forecast protocol astronomical state verification.</p> <p>This publication establishes a timestamped verification framework before the observational confirmation window of <strong>May 13–14, 2026</strong>. The document records a sealed validation structure based on <strong>HVS milestones</strong>: four critical physical-state checkpoints per astronomical block. This structure allows later comparison against NASA/JPL Horizons-derived ephemeris data while avoiding disclosure of the continuous vector time series, internal constants, and generative derivation of the Araya2 operator.</p> <p>The forecast framework covers three validation blocks:</p> <ul> <li>Europa–Jupiter vector-state validation</li> <li>NEO 2026 JD1 geocentric trajectory validation</li> <li>Moon–Saturn angular separation validation</li> </ul> <p>Each block is expressed through UTC/TDB timestamps, reference frames, selected physical-state variables, Horizons/JPL-derived inputs, sealed Araya2 outputs, and residual validation criteria.</p> <p>The sealed residual benchmark reported for the Araya2 residual-correction operator is:</p> <p><strong>EDMS_rel = 0.0345506917%</strong></p> <p>This value is below the internal Eureka III critical validation threshold:</p> <p><strong>EDMS_rel < 0.0598%</strong></p> <p>This record is <strong>not presented as a final post-event validation</strong>. It is a pre-registered forecast artifact intended for later comparison after the May 13–14, 2026 verification window.</p> <p>To protect the proprietary structure of Araya2, this publication discloses only four verification points per astronomical block:</p> <ol> <li>Window start</li> <li>Central event / closest-state condition</li> <li>Window exit</li> <li>Validation closure</li> </ol> <p>The full generative method, internal constants, continuous vector series, and proprietary derivation remain undisclosed. This publication functions as a priority record, validation framework, and non-enabling forecast artifact for subsequent independent comparison.</p> <p> </p> |
| title | Eureka III —Araya2 V1.3 Blind Forecast Protocol for Orbital-State Validation Using HVS Milestones |
| topic | Araya2; Multiscale Metric; Blind Forecast; Orbital Validation; Ephemeris; JPL Horizons; Europa; Jupiter; 2026 JD1; Moon-Saturn; Residual Correction; HVS Milestones; Non-Enabling Publication; Astronomical State Verification; Luis Pablo Araya Salazar |
| url | https://doi.org/10.5281/zenodo.20129946 |