Strong G3 geomagnetic storm

woensdag 7 oktober 2015 23:29 UTC

Strong G3 geomagnetic storm

The anticipated coronal hole high speed solar wind stream sure delivered and sparked a strong G3 geomagnetic storm. Aurora displays were reported from northern Poland, northern Germany and even the Netherlands had some photographic aurora!

The direction of the IMF (Bz) went as low as -20nT during the afternoon and quickly sparked a moderate G2 geomagnetic storm. The strong G3 geomagnetic storming threshold was reached during the European evening hours.

Header image: Aurora Borealis captured just a few hours ago by Carl Bergstand (Gotland, Sweden)

Image: Kristian Potsepp (Estonia)

Image: Bart Broekhuijsen (The Netherlands)

Image: Ronan Mc Monagle (Donegal, Ireland)

What to expect in the coming hours

We expect these enhanced geomagnetic conditions to persist in the coming hours. The total strength of the IMF (Bt) decreased significantly to 7nT but the solar wind speed increase to 750km/s which is high. Minor G1 geomagnetic storming conditions remain likely in the coming hours. The upper United States and of course Canada should be alert for aurora in the coming hours. Sky watchers in Quebec already report visual aurora.

False G5 geomagnetic storm alert

On our website and Twitter you might have noticed that the observed Kp-index showed 9 for a while. We believe this is an error as all the magnetometer data, auroral observations as well as NOAA itself reported at most strong G3 geomagnetic storming conditions.

Our data comes from NOAA's Wing-Kp index which uses magnetometer data from the USAF and it is normally a very reliable source. We are glad that we can use this data but this issue is unfortunately beyond our control. We apologize for any inconvience.

Bij elke genoemde zonnevlam in dit artikel werd een schaalfactor toegepast door het Space Weather Prediction Center (SWPC). Vanwege de SWPC-schaalfactor worden zonnevlammen 42% kleiner gerapporteerd dan voor de wetenschappelijke data. De schaalfactor werd verwijderd uit onze gearchiveerde zonnevlamdata om de werkelijke fysieke eenheden weer te geven.

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