VLF radio RMS envelope during 2024-04-08 total solar eclipse --- sensor ET0001 Cleveland OH (path of totality), 20 kHz sample rate, D-layer collapse creates higher predictability (Eclipse Research Group)
Standard analysis sees: high-complexity (noise-like); monofractal. The atlas finds no named structure, but the source is distinctively extreme on Bispectrum:off_diagonal_ratio (-2.8z) — beyond what the standard bank predicts for it.
Bispectrum:off_diagonal_ratio | -2.8z | bank-miss 1.5σ |
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_(centered)/signed_log_z/VLF_Radio_(Eclipse).png)
_(centered)/xy_path/VLF_Radio_(Eclipse).png)
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/barcode/VLF_Radio_(Eclipse).png)
/d_curve/VLF_Radio_(Eclipse).png)
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/phi_spectrum/VLF_Radio_(Eclipse).png)
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/default/VLF_Radio_(Eclipse).png)
/default/VLF_Radio_(Eclipse).png)
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| Nearest neighbor | Distance | |
|---|---|---|
| VLF Radio (Baseline) | 2.25 | |
| Voyager 1 X-band | 2.94 | cross-origin |
| Tohoku Aftershock Intervals | 3.24 |
2-adic › 2-adic:mean_distance | rank 2/307 | 0.6684 |
Attractor Reconstruction › Attractor Reconstruction:kaplan_yorke_dim | rank 4/307 | 5.5596 |