Strong G3 geomagnetic storm

Sunday, 26 August 2018 10:03 UTC

The plasma cloud was slow which is something that actually was to be expected and the solar wind speed had a constant speed of around 400 to 450km/s during the past 36 hours or so. There was no classic shock impact which we often see with faster coronal mass ejections so what gave away that this indeed was a coronal mass ejection?

These unexpectedly strong geomagnetic storm conditions are caused by an enhanced magnetic field with a persistent southward orientation (Bz) which is a common occurrence when the core of a coronal mass ejection (magnetic cloud) passes our planet. Indeed, this was not just a glancing blow! Negative (southward) Bz values have been observed since around 15 UTC yesterday and these values gradually increased to a minimum of -17nT. Not bad for a wimpy coronal mass ejection! The persistent southward orientation of the IMF constantly fueled the auroral displays above our planet resulting in unexpectedly strong geomagnetic storm conditions.

Geomagnetic storming gradually increased in strength until 05:59 UTC today when the NOAA SWPC reported that the strong G3 geomagnetic storm threshold was reached. Even the Disturbance Storm Time index dropped deep to a lowest value of -186nT.

Strong G3 geomagnetic storm (Kp7)
Threshold Reached: 05:59 UTC
Follow live on https://t.co/Zkq26B89Y7 pic.twitter.com/8JeudpHZ7z

— SpaceWeatherLive (@_SpaceWeather_) August 26, 2018

At the time of writing, the solar wind speed has now increased slightly to 450km/s and the Bz once again drops well below the -10nT so geomagnetic storm conditions are likely to persist in the hours ahead which should be great news for sky watchers in the northern USA, southern New Zealand, and Tasmania/Melbourne area.

Header image: Aurora above Kiruna, Sweden by Marcel de Bont.