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Night Sky Platform

Space Weather

Space weather — solar flares and geomagnetic storms — explained with the standard NOAA scales, alongside the current conditions measured by NOAA SWPC. Nothing is fabricated: a provider that cannot be reached shows no value at all.

Night SkyReference data

Space weather right now

Current conditions →
  • Solar wind

    Live

    351 km/s

    Moderate

    2026-10-07 17:22 UTC

  • Planetary Kp

    Recent

    1.00

    Quiet

    2026-10-07 12:00 UTC

  • Geomagnetic scale

    Live

    None

    no storm in the last 24 h

    2026-10-07 17:27 UTC

  • X-ray flux

    Live

    B9.2

    current GOES class

    2026-10-07 17:25 UTC

Source: NOAA Space Weather Prediction Center. Times are UTC, as published by the provider.

Solar flare classes

Flares are ranked A–B–C–M–X by X-ray brightness, each class ten times stronger than the last. Solar flares in detail →

Class A
Background level; negligible effects.
Class B
Minor; no noticeable effects.
Class C
Small flares with few noticeable consequences.
Class M
Medium flares; can cause brief radio blackouts and minor radiation storms.
Class X
The most intense flares; can trigger planet-wide radio blackouts and strong radiation storms.

Geomagnetic storm scale

NOAA ranks geomagnetic storms G1–G5. Geomagnetic storms in detail →

G1
Minor: weak power-grid fluctuations; aurora at high latitudes.
G2
Moderate: aurora reaches mid-high latitudes.
G3
Strong: aurora at mid-latitudes; possible satellite and navigation effects.
G4
Severe: widespread aurora and grid/navigation impacts.
G5
Extreme: aurora far from the poles; major infrastructure risk.

Related in the Knowledge Graph

Sources & references

The primary and reference sources this topic draws on.

  • NOAA SWPCNOAA Space Weather Prediction Center

    Space-weather forecasts and alerts: aurora (OVATION), the Kp index, and the G1–G5 geomagnetic storm scale.

  • NASA DONKINASA Community Coordinated Modeling Center

    The Space Weather Database Of Notifications, Knowledge, Information: solar flares, CMEs, and geomagnetic storms.