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 (-2.9z) — beyond what the standard bank predicts for it.
Bispectrum:off_diagonal_ratio | -2.9z | bank-miss 1.6σ |
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_(centered)/signed_log_z/VLF_Radio_(Eclipse).png)
_(centered)/xy_path/VLF_Radio_(Eclipse).png)
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/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)
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| Nearest neighbor | Distance | |
|---|---|---|
| VLF Radio (Baseline) | 2.16 | |
| Voyager 1 X-band | 2.75 | cross-domain |
| Pink Noise | 3.30 | cross-domain |
2-adic › 2-adic:mean_distance | rank 3/298 | 0.6681 |
Attractor Reconstruction › Attractor Reconstruction:kaplan_yorke_dim | rank 5/298 | 5.4896 |