Station Detail

Cumiana, Piedmont, Italy (44.97°N, 7.39°E)

IK1QFK Home Observatory, Renato Romero

35
Current Score
Calm Updated 11 min ago

Right now

Cumiana: 35 · global avg: 58

Quieter than: Tomsk (45), Etna (55), Eskdalemuir (65), California (65), Alberta (85)

Latest Spectrogram

Cumiana Schumann Resonance spectrogram
Updated 11 min ago

2nd harmonic frequency tracker only

This week at

Hey there! This past week at our Cumiana station has been quite lively, with a peak score of 85, which is pretty high! We had a few moments where things really picked up, with five readings soaring above 80, but there were also plenty of quieter periods in between. Overall, it's been an interesting week of Schumann Resonance activity!

Week of 2026-06-29 · peak: 85 · avg: 43

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30-day hourly activity

Each cell is one UTC hour. Click any active cell to explore that day.

Notable events (last 30 days)

  1. 85
    2026-07-01

    At the rightmost edge, the ULF noise (purple) has surged significantly toward the -20 dB level, while the ELF noise (…

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  2. 85
    2026-06-30

    At the rightmost edge, the purple ULF noise line has surged sharply toward -20 dB, while the pink ELF noise line has …

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  3. 85
    2026-06-30

    At the rightmost edge, the ULF (purple) and ELF (pink) noise lines exhibit a sudden, sharp vertical ascent toward the…

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  4. 85
    2026-06-28

    At the rightmost edge, the ULF (purple) and ELF (magenta) noise levels have risen sharply to approximately -20 dB and…

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  5. 85
    2026-06-28

    At the rightmost edge, the purple ULF noise line has risen sharply to approximately -20 dB, while the pink ELF noise …

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  6. 85
    2026-06-24

    At the rightmost edge, the purple (ULF 10Hz) line has risen to approximately -20 dB, indicating high noise levels. Th…

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  7. 85
    2026-06-24

    At the rightmost edge, both the ULF (purple) and ELF (pink) noise lines show a sharp, sustained upward trajectory, wi…

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  8. 85
    2026-06-23

    At the rightmost edge of the chart, the ULF noise (purple) shows a dramatic vertical surge peaking near -20 dB. The E…

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  9. 85
    2026-06-08

    At the rightmost edge, the ULF noise (purple) shows a dramatic vertical surge toward -25 dB, while the ELF noise (pin…

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  10. 85
    2026-06-08

    At the rightmost edge of the chart, the purple ULF noise line exhibits a dramatic vertical surge toward the -25 dB le…

    View day →

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Cumiana — the Piedmont observer

Cumiana captures Schumann resonance from northern Italy's Piedmont region, a quiet alpine valley shielded by the Cottian Alps.

Run by vlf.it (Renato Romero's IK1QFK home observatory), it produces a distinctive rainbow multistrip spectrogram that shows the full 0–43 Hz band — wider than most stations in our network.

The multistrip format captures not just Schumann harmonics but also sferics (distant lightning signals), giving it a unique profile during Mediterranean thunderstorm season. Visit vlf.it

Trust & authority

IK1QFK Home Observatory, Renato Romero

Operating since 2008 · 18 years of continuous monitoring

Research & publications

Frequently asked questions

How does Cumiana measure Schumann resonance?

Cumiana uses a VLF coil (Marconi multistrip) that captures 0.2–43 Hz. The output is a daily stripchart with multiple 4-hour strips stacked vertically, published at vlf.it.

Why is Cumiana important to our network?

Cumiana shows the widest frequency range in our live network (0.2–43 Hz vs the usual 3–40 Hz) and catches sferics from distant lightning, giving us a richer view of Mediterranean electromagnetic weather.

When was its last major event?

Check the Notable events section above — it lists the top 10 highest-score events at Cumiana from the last 30 days, each linked to its full daily report.

How reliable is the data?

Cumiana is run by Renato Romero (IK1QFK), a veteran VLF researcher whose work is referenced in academic literature. The station has been operating since 2008. We cross-validate readings against other network stations.

Where does the raw data come from?

Raw spectrogram images come from vlf.it (last-marconi-multistrip-slow.jpg). We download, analyze and cache them as they update. Visit vlf.it for the full feed and background on the instrumentation.

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