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Today, above you.

These are the measurements space-weather forecasters watch. Each card shows where the number comes from and when it was taken, so you can see how fresh it is.

Right now: the live cards below show the current values.

1 · On the sun

What the sun is doing

Flares and active regions start here. Light from a flare reaches Earth in about eight minutes.

The sun today

Latest NASA SDO image of the sun at 171 angstroms
The sun today · NASA SDO, extreme ultraviolet 171 Å

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Bright loops mark active regions, where flares start. Dark patches are coronal holes, the source of fast solar wind.

Solar flares

Loading

Waiting for a published sample.

NOAA SWPC ↗ ·
Values and source
What it tells you

How bright the sun is in X-rays right now. Flares are classed A, B, C, M and X, each step ten times stronger.

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2 · Between the sun and Earth

What is on its way

Measured by spacecraft about 1.5 million kilometres sunward, roughly an hour before it reaches us.

Solar wind speed

Loading

Waiting for a published sample.

NOAA SWPC ↗ ·
Values and source
What it tells you

The speed of the stream of charged particles leaving the sun. Around 400 km/s is typical; above 600 km/s is a fast stream.

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Magnetic field direction

Loading

Waiting for a published sample.

NOAA SWPC ↗ ·
Values and source
What it tells you

When Bz points south (negative) for hours, solar wind energy couples into Earth’s field much more easily. A strong, lasting negative Bz is what turns a fast stream into a storm.

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3 · At Earth

How Earth’s magnetic field responds

The Kp index, the three-day outlook, the aurora oval and Earth’s electromagnetic background.

Geomagnetic activity

Loading

Waiting for a published sample.

NOAA SWPC ↗ ·
Values and source
Kp, last 24 hours · NOAA SWPC, provisional · UTC
Values and source
NOAA JSON
What it tells you

How disturbed Earth’s magnetic field was over the last three hours, on a scale from 0 to 9. From 5 upwards it counts as a geomagnetic storm.

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Next 3 days

Loading forecast

Waiting for NOAA’s published forecast.

Forecasts can shift by several hours.

Values and source
NOAA SWPC JSON ↗

Flare, CME or storm? →

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Northern lights tonight

Latest NOAA OVATION aurora model for the northern hemisphere
NOAA SWPC · OVATION northern hemisphere · model time is printed in the image.

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Where aurora is likely right now. In central Europe it usually takes Kp 7 or more to see it low on the northern horizon.

Space Weather: How Solar Activity Reaches Earth

Live data: NOAA Space Weather Prediction Center, GFZ Potsdam (Kp), NASA Solar Dynamics Observatory. Values are shown as published; gaps stay visible.
Retrieved . Kp values here use NOAA’s provisional feed; GFZ is the definitive-index reference.

Try it

How long until it reaches us?

Light from a flare arrives in about eight minutes. The solar wind takes days from the sun and about an hour from the L1 monitor. Enter a speed or use today’s live value.

Solar wind travel time

Enter a speed or use today’s live value.

Constant-speed estimate. L1–Earth: 1.5 million km; Sun–Earth: 150 million km. Real CME transit is more complex.

JSON values may be cached for five minutes. Source timestamps remain unchanged.

Noticed something today?

Write it down together with the time. Over a few weeks, your notes and these numbers start to tell a story, or show that there isn’t one. Both are worth knowing.

The SolarHealth app is being built for exactly this →