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X-ray Flux — live and explained

The raw GOES satellite measurement behind every solar flare classification — the number that turns into letters like C, M, and X.

Current X-ray Flux

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Updated every minute from live GOES data.

Data Layer: GOES Satellites

Why it matters

X-rays from a flare reach Earth in about 8 minutes (at the speed of light) and can ionize the upper atmosphere on the sunlit side, disrupting high-frequency radio communication — this is why strong flares cause immediate radio blackouts, unlike CMEs or geomagnetic storms which take hours to days to arrive.

Normal range

Background (quiet-sun) flux sits below 10⁻⁷ W/m² (A-class). C-class flares (10⁻⁶-10⁻⁵ W/m²) are common and mostly unnoticed on Earth. M-class (10⁻⁵-10⁻⁴) can cause brief blackouts near the poles. X-class (≥10⁻⁴) are the rare, major events capable of wide-area radio blackouts.

What today's value means

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What is X-ray flux?

GOES weather satellites carry X-ray sensors (XRS) that continuously measure how much X-ray radiation is reaching Earth from the Sun. This page shows the "long" channel (0.1-0.8 nanometers), the standard measurement used to classify solar flares. Flux rises sharply — sometimes a hundredfold within minutes — during a flare, then decays back toward background levels over the following hour or so.

Flare classification scale

ClassX-ray flux thresholdTypical effect
A< 10⁻⁷ W/m²Background level, no flare.
B10⁻⁷ – 10⁻⁶ W/m²Minor, no noticeable effects on Earth.
C10⁻⁶ – 10⁻⁵ W/m²Small flares, minimal Earth effects.
M10⁻⁵ – 10⁻⁴ W/m²Moderate — can cause brief radio blackouts near the poles.
X≥ 10⁻⁴ W/m²Major — can cause wide-area radio blackouts and radiation storms.

FAQ

How is flare class calculated from X-ray flux?

Each letter represents a tenfold jump in flux. The number after the letter is a linear multiplier — an M5.0 flare has 5 times the flux of M1.0, and an X2.0 flare has twice the flux of X1.0.

Why do X-ray flares affect radio communication?

X-rays from a flare reach Earth in about 8 minutes and ionize the upper atmosphere on the sunlit side, which can absorb or disrupt high-frequency radio signals — this is why strong flares cause radio blackouts.

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