The Schumann Pulse chart lab

Read a Schumann chart.
Change one thing.

A taller peak, a different frequency and a brighter colour tell different stories. Explore four interactive lessons, then bring that understanding to a real station chart.

Original teaching models · no live readings · reviewed 22 October 2026

A closer lookAuthored teaching model

A taller peak. The same frequency.

Relative power
210
4812

Frequency (Hz)

Current exampleReference
Centre
8 Hz
Full width
2 Hz
Q
4

Reference: 8 Hz centre · 2 Hz full width · peak power 1.
Isolated power peak above a removed background; not a station recording.

What this tells you

Peak power is 1.6 times the reference. The centre remains 8 Hz and full half-power width remains 2 Hz. Q stays at 4.

Understand Schumann spikes

This example shows a power increase. The four lessons below explain what each chart feature means.

Four things worth telling apart.

01 / Strength

Higher does not mean faster.

A power peak can get taller while its centre frequency stays fixed. In this lesson only relative power changes. Amplitude and power are different quantities; always use the convention and units stated on a real chart.

What does a spike mean? ↗

02 / Frequency

Look at the peak’s position.

Moving the centre sideways changes frequency. Our example keeps power and full width fixed at 2 Hz. Q changes as a consequence, because it is the centre frequency divided by that width.

Understand the frequency bands ↗

03 / Width

A narrower peak has a higher Q.

At an 8 Hz centre, a full half-power width of 2 Hz gives Q = 4. Narrow the width to 1 Hz and Q becomes 8. Here the background is removed and the peak is isolated. Real spectra require fitting and a stated convention.

Explore quality factor ↗

04 / Colour

The display can change the story.

Both heatmaps use exactly the same invented samples. Lowering the colour ceiling makes more cells white. No values change and none disappear. This shows a display limit, not evidence of an overloaded instrument.

Read whiteouts and blackouts ↗

How these examples work.

This is a learning tool, not a simulation of today’s Earth–ionosphere cavity. A single smooth peak makes one relationship easier to see. The reference stays fixed so that each adjustment has a clear comparison.

The model, scales and limits

The isolated power curve is P(f) = H / [1 + 4((f − f₀) / Δf)²]. H is relative peak power, f₀ is the centre and Δf is the full width at half power. The spectrum axes remain 4–12 Hz and 0–2 relative power units.

The colour lesson uses a fixed 20 × 24 grid of invented values. Its frequency and hour labels provide teaching context only. White represents values at or above the chosen colour ceiling; the reference ceiling is 100. It does not model missing data or instrument saturation.

For the research behind the peak-width convention, see the sources in our Q guide. For real measurement limitations, read how stations record the signal.

Curious about the other charts? Explore Kp, Dst and Bz in the space-weather lab ↗

Put it into practice

Start with a real timestamp.

Explore available station readings with their source and measurement time. A station chart describes an observation; it does not explain why you feel a certain way.

See current readings

Your own perspective

Keep the context.
Build your own record.

Schumann Pulse brings environmental observations together with your journal. Record feelings, optional energy and sleep-quality ratings, then revisit suitable comparisons as your history grows.

See what you can track ↗

Coming soon for iPhone. History and personal comparisons live in the app.