New script 09_raw_pairwise_correlations.py downloads OOS NMDB/USGS data and computes Pearson r and Spearman ρ (with Bonferroni correction) for all three variable pairs across in-sample, OOS, and combined windows. CR flux is represented by its per-bin station distribution (p5–p95 band with min–max overlay); seismic energy uses the physically correct E ∝ 10^(1.5·Mw) sum; sunspots shown with 365-day smoothed + raw spread. Key findings: CR vs sunspot r=-0.82 to -0.94 (Forbush decrease); CR vs seismicity r=0.057 raw (OOS: r=0.046, not significant); confounding triangle motivates HP-filter detrending analysis. Paper gains a new Section 4.1 "Raw Pairwise Correlations" with three scatter figures and a 9-test Bonferroni summary table; 24 pages total. Co-Authored-By: Claude Sonnet 4.6 <noreply@anthropic.com> |
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| .. | ||
| 01_download_data.py | ||
| 02_homola_replication.py | ||
| 03_stress_test.py | ||
| 04_detrended_analysis.py | ||
| 05_geographic_localisation.py | ||
| 06_check_data_availability.py | ||
| 07_out_of_sample.py | ||
| 08_combined_timeseries.py | ||
| 09_raw_pairwise_correlations.py | ||
| benchmark_gpu.py | ||
| catalog_completeness_check.py | ||