VLF radio RMS envelope from normal day (2024-04-10) --- same sensor ET0001 Cleveland OH, 20 kHz, no eclipse, standard D-layer daytime absorption conditions (Eclipse Research Group)
Standard analysis sees: high-complexity (noise-like). The atlas finds no named structure, but the source is distinctively extreme on Bispectrum:off_diagonal_ratio (-3.0z) — beyond what the standard bank predicts for it.
Bispectrum:off_diagonal_ratio | -3.0z | bank-miss 1.8σ |
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_(centered)/signed_log_z/VLF_Radio_(Baseline).png)
_(centered)/xy_path/VLF_Radio_(Baseline).png)
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/barcode/VLF_Radio_(Baseline).png)
/d_curve/VLF_Radio_(Baseline).png)
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/phi_spectrum/VLF_Radio_(Baseline).png)
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/default/VLF_Radio_(Baseline).png)
/default/VLF_Radio_(Baseline).png)
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| Nearest neighbor | Distance | |
|---|---|---|
| VLF Radio (Eclipse) | 2.16 | |
| Voyager 1 X-band | 2.94 | cross-domain |
| Pink Noise | 3.42 | cross-domain |
Bispectrum › Bispectrum:off_diagonal_ratio | rank 294/298 | 0.2023 |