Add analysis results: scripts 01-05 outputs

Benchmark, Homola replication, stress test, detrended analysis, and
geographic localisation results including figures. Pre-registration
and data availability already committed separately.

Co-Authored-By: Claude Sonnet 4.6 <noreply@anthropic.com>
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GPU vs CPU Surrogate Benchmark
==================================================
N timesteps: 16,000
N surrogates: 10,000
IAAFT iter: 100
CPU n_jobs: -1
GPU device: Tesla M40 (12.0 GB)
Method CPU (s) GPU (s) Speedup Equiv
------------------------------------------------
phase 61.7 20.9 2.9x PASS
iaaft 227.8 175.6 1.3x PASS

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USGS Earthquake Catalogue — Completeness Summary
==================================================
Total events loaded: 14,735
Date range: 2018-01-01 — 2019-12-30
Gutenberg-Richter b-value (M≥4.5): 1.410
Estimated catalogue completeness onset (CV < 15% over 5-year window):
M ≥ 4.0: no clear stabilisation
M ≥ 4.5: no clear stabilisation
M ≥ 5.0: no clear stabilisation
M ≥ 5.5: no clear stabilisation
M ≥ 6.0: no clear stabilisation
M ≥ 7.0: no clear stabilisation
NOTE: Use M≥4.5 from ~1976 onwards for global cross-correlation analysis.
Earlier data should be treated with caution — counts are systematically low.

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# Detrended CRSeismic Cross-Correlation Analysis
Generated: 2026-04-21T10:31:37Z
Study period: 1976-01-01 2019-12-31
Bin size: 5 days
Surrogates: 10000 IAAFT
Lag range: -1000…1000 days
## Significance table
| Method | N_eff | r(+15d) | σ_Breth(15d) | Peak r | Peak lag | p_global (IAAFT) | σ_IAAFT |
|---|---|---|---|---|---|---|---|
| Raw | 1169 | 0.3099 | 10.85 | 0.4691 | -525 d | 1.0000 | 0.0σ |
| HP filter | 3027 | 0.0411 | 2.26 | 0.3131 | -525 d | 0.0000 | 3.9σ |
| STL | 1880 | 0.1098 | 4.77 | 0.1554 | -125 d | 0.0000 | 3.9σ |
| Sunspot regression | 1850 | 0.1570 | 6.79 | 0.2657 | -525 d | 0.0000 | 3.9σ |
## Interpretation
**CAUTION**: The following variants retain p_global < 0.05 after detrending: HP filter, STL, Sunspot regression. Further investigation required.
## Methods
### HP filter (Hodrick-Prescott)
λ = 1.29e+05 calibrated for 5-day bins targeting removal of
variations longer than ~2000 days (Ravn & Uhlig 2002 scaling of the standard λ=1600).
### STL decomposition
Period = 803 bins ≈ 11.0 years
(11-year solar cycle). seasonal_jump=100, trend_jump=100 for computational efficiency.
The *residual* component (x trend seasonal) is used.
### Sunspot OLS regression
Contemporaneous + [0, 30, 90, 180]-day lagged sunspot numbers from SIDC WDC-SILSO.
The fitted solar-proxy component is subtracted from each series.
## Figure
`results/figs/detrended_xcorr.png`

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{
"generated": "2026-04-21T10:31:37Z",
"study_start": "1976-01-01",
"study_end": "2019-12-31",
"bin_days": 5,
"n_surrogates": 10000,
"results": [
{
"label": "Raw",
"n": 3215,
"n_eff": 1169.0,
"r_at_15d": 0.3099,
"sigma_15_naive": 18.01,
"sigma_15_breth": 10.85,
"peak_r": 0.4691,
"peak_lag_days": -525,
"sigma_pk_naive": 28.26,
"p_global_iaaft": 1.0,
"sigma_iaaft": 0.0
},
{
"label": "HP filter",
"n": 3215,
"n_eff": 3027.3,
"r_at_15d": 0.0411,
"sigma_15_naive": 2.33,
"sigma_15_breth": 2.26,
"peak_r": 0.3131,
"peak_lag_days": -525,
"sigma_pk_naive": 18.21,
"p_global_iaaft": 0.0,
"sigma_iaaft": 3.89
},
{
"label": "STL",
"n": 3215,
"n_eff": 1879.8,
"r_at_15d": 0.1098,
"sigma_15_naive": 6.24,
"sigma_15_breth": 4.77,
"peak_r": 0.1554,
"peak_lag_days": -125,
"sigma_pk_naive": 8.86,
"p_global_iaaft": 0.0,
"sigma_iaaft": 3.89
},
{
"label": "Sunspot regression",
"n": 3215,
"n_eff": 1849.6,
"r_at_15d": 0.157,
"sigma_15_naive": 8.96,
"sigma_15_breth": 6.79,
"peak_r": 0.2657,
"peak_lag_days": -525,
"sigma_pk_naive": 15.34,
"p_global_iaaft": 0.0,
"sigma_iaaft": 3.89
}
]
}

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# Geographic Localisation of CRSeismic Cross-Correlation
Generated: 2026-04-21T23:59:51Z
Study period: 1976-01-01 2019-12-31
Bin size: 5 days
Lag range: -200…200 days (step 5 d)
Surrogates: 1000 × phase-randomisation (GPU: Tesla M40 (12.0 GB))
Min events per cell: 100
Grid: 10°×10° (648 cells total)
Stations loaded: 44
Total (station, cell) tests: 7,037
BH q: 0.05
## Main finding
**455 significant pairs** (BH q=0.05), barely exceeding the expected false-discovery count (351.9). This marginal excess does not constitute reliable evidence for geographic localisation.
## Distancelag analysis (all 7,037 pairs)
The OLS regression of τ* on d is not significant (β = -0.45 d/1000 km, p = 0.2114). No distance dependence in optimal lag is detected — consistent with H_CR (CR isotropy).
| Regression | slope (per 1000 km) | R² | p-value |
|---|---|---|---|
| τ*(s,g) ~ d | -0.450 d | 0.0002 | 0.2114 |
| |r*|(s,g) ~ d | 0.00073 | 0.0025 | 0.0000 |
## Significant pairs (BH q=0.05)
- Total significant pairs: **455** / 7,037
- Expected false discoveries: **351.9**
- Significant cells: 177
- Stations contributing significant pairs: 32
## Scientific context
Homola et al. (2023) report the global CRseismic correlation disappears in
location-specific analyses, which would be puzzling for any mechanistic
hypothesis. This analysis tests that claim quantitatively by controlling
the false-discovery rate across all 7,037 geographic pairs.
Under **H_CR** (cosmic rays are the causal agent, and they are near-isotropic):
- No geographic localisation expected.
- τ*(s,g) should be independent of d(s,g).
- |r*(s,g)| should be independent of d(s,g).
Under **H_local** (ionospheric, radon, or EM propagation mechanism):
- Nearby (s, g) pairs should show stronger or differently-lagged correlations.
- τ*(s,g) or |r*(s,g)| should vary systematically with d(s,g).
## Figures
- `results/figs/geo_heatmap.png`log₁₀(min p) per cell + BH-significant stations
- `results/figs/geo_distance_lag.png` — distance vs peak lag and distance vs |r|

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{
"script": "scripts/02_homola_replication.py",
"git_sha": "unknown",
"seed": 42,
"timestamp_utc": "2026-04-21T09:02:19.401598+00:00",
"study_window": [
"1976-01-01",
"2019-12-31"
],
"bin_days": 5,
"lag_range_days": [
-1000,
1000
],
"min_magnitude": 4.0,
"nmdb_coverage_threshold": 0.6,
"min_stations_requested": 3,
"min_stations_effective": 3,
"n_stations_used": 44,
"n_cr_bins_total": 3215,
"n_cr_bins_valid": 3215,
"cr_data_coverage_pct": 100.03,
"peak_lag_days": -525,
"peak_lag_bins": -105,
"peak_r": 0.469101,
"naive_p_value": 5.631233e-170,
"naive_sigma": 27.791,
"n_pairs_at_peak": 3110,
"r_at_tau_15d": 0.309878,
"p_at_tau_15d": 1.93927e-72,
"sigma_at_tau_15d": 18.0,
"n_lags_scanned": 401,
"note_significance": "Naive p from Pearson t-test treating 5-day bins as i.i.d. Not corrected for: (1) temporal autocorrelation, (2) shared solar-cycle trend, (3) scan over multiple lags. Expected to be grossly over-significant \u2014 corrected tests in phase 2."
}

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# Homola et al. 2023 — Stress Test Report
Generated: 2026-04-21 | git SHA: `unknown` | seed: 42
---
## Study parameters
| Parameter | Value |
|-----------|-------|
| Data | NMDB (44 stations) + USGS M≥4.0 |
| Study window | 1976-01-01 2019-12-31 |
| Bin size | 5 days |
| Valid bins (CR) | 3,215 |
| Seismic events | 409,763 |
| Lag range | ±1000 days |
| Surrogates | 10,000 |
---
## Effective sample size
The Bretherton et al. 1999 formula corrects for serial autocorrelation:
N_eff ≈ N × (1 ρ₁_CR × ρ₁_seismic) / (1 + ρ₁_CR × ρ₁_seismic)
| Series | Lag-1 autocorrelation ρ₁ |
|--------|--------------------------|
| Global CR index | +0.6701 |
| Seismic Σ Mw | +0.6969 |
| **N_eff (Bretherton)** | **1169** of 3,215 bins (36.4%) |
---
## τ = +15 days (Homola claimed signal)
Observed r(τ = +15 d) = **+0.30988**
| Method | r(+15 d) | p-value | σ equivalent | Notes |
|--------|----------|---------|--------------|-------|
| Naive Pearson (N bins i.i.d.) | +0.30988 | 1.666e-72 | 18.01σ | Homola 2023 baseline |
| Bretherton N_eff (1169) | +0.30988 | 1.954e-27 | 10.85σ | Autocorr. corrected |
| Phase-randomised surrogate | +0.30988 | 6.300e-02 | 1.86σ | Spectrum preserved |
| IAAFT surrogate | +0.30988 | 1.000e+00 | 0.00σ | Spectrum + amplitude |
---
## Global test — best lag (τ ∈ [1000, +1000] days)
Observed peak: r = **+0.46910** at τ = **-525 days**
| Method | Peak r | Peak lag | p-value | σ equivalent | Notes |
|--------|--------|----------|---------|--------------|-------|
| Naive Pearson | +0.46910 | -525 d | 1.193e-175 | 28.26σ | Best-lag scan not corrected |
| Bretherton N_eff | +0.46910 | -525 d | 5.178e-65 | 17.03σ | Autocorr. corrected |
| Phase-randomised (global) | +0.46910 | -525 d | <1.0e-04 | 3.89σ | Max-|r| over all lags |
| IAAFT (global) | +0.46910 | -525 d | 1.000e+00 | 0.00σ | Max-|r| over all lags |
---
## Interpretation
### Solar-cycle artefact
The dominant correlation peak (τ = -525 days, r = +0.469) is
**not** at the Homola-claimed +15 days. Its lag is close to a half-period of
the ~11-year solar cycle (~4,015 days / 2 ≈ 2,008 days at its harmonics).
Both NMDB cosmic-ray flux and global seismic activity are modulated by the
solar cycle via distinct physical mechanisms (cosmic-ray shielding by the
heliospheric magnetic field; possible solartectonic coupling debates aside).
This shared low-frequency variation inflates naive correlations at many lags.
### Naive vs corrected significance
The naive 18σ significance at τ = +15 d collapses dramatically once
autocorrelation is accounted for:
- Bretherton correction alone reduces N from 3,215 to 1169 effective
observations (a 3× reduction).
- Surrogate tests account for the full autocorrelation structure, including
the solar cycle common to both series.
### Conclusion
The observed peak correlation is **not significant** under the surrogate null model once the shared autocorrelation structure is accounted for. The naive 18σ Pearson significance collapses entirely. The Homola claim of a 6σ CRseismic cross-correlation is not reproduced once the solar-cycle confound is removed.
---
## Caveats
- Surrogates randomise the **CR index** phases, testing whether the CR
autocorrelation alone could produce the observed correlation with the real
seismic series. A complementary test (randomising the seismic series) or
a bivariate surrogate test would provide additional evidence.
- IAAFT converges to an approximate solution; 100 iterations suffice for
smooth spectra but may not fully converge for very spiky distributions.
- The Bretherton formula is a first-order approximation valid for AR(1)
processes. The CR index has a more complex spectrum (solar cycle,
Forbush decreases) that may require higher-order corrections.
- This analysis does not test the solar-cycle detrended residuals, which is
the correct test for the Homola claim. See Phase 3 of this study.

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{
"script": "scripts/03_stress_test.py",
"git_sha": "unknown",
"seed": 42,
"timestamp_utc": "2026-04-21T10:03:23.369813+00:00",
"study_window": [
"1976-01-01",
"2019-12-31"
],
"bin_days": 5,
"lag_range_days": [
-1000,
1000
],
"min_magnitude": 4.0,
"n_bins": 3215,
"n_stations": 44,
"n_events": 409763,
"r1_cr_index": 0.6701,
"r1_seismic": 0.69687,
"n_eff_bretherton": 1169.0,
"tau_15d": {
"r": 0.309878,
"naive_p": 1.6659911463430199e-72,
"naive_sigma": 18.00866469588119,
"bretherton_p": 1.9536877842478326e-27,
"bretherton_sigma": 10.851878248025837,
"phase_surr_p": 0.06300000101327896,
"phase_surr_sigma": 1.8591914873206736,
"iaaft_surr_p": 1.0,
"iaaft_surr_sigma": 0.0
},
"peak_lag": {
"r": 0.469101,
"lag_days": -525,
"naive_p": 1.1932567507933964e-175,
"naive_sigma": 28.256232973744382,
"bretherton_p": 5.178335317026674e-65,
"bretherton_sigma": 17.027010022743948,
"phase_surr_p_global": 0.0,
"phase_surr_sigma_global": 3.890591886413094,
"iaaft_surr_p_global": 1.0,
"iaaft_surr_sigma_global": 0.0
},
"n_surrogates": 10000,
"method": "both"
}