G2 geomagnetic storm, M2.9 solar flare

Thursday, 27 August 2015 09:03 UTC

G2 geomagnetic storm, M2.9 solar flare

Geomagnetic conditions have been at the moderate G2 geomagnetic storming level in response to an extended period where the direction of the IMF (Bz) stayed southward. Source of this activity is unknown but we think this might be one of the faint and slow M-class coronal mass ejections that passed our planet, which would explain the lack of any solar wind speed or density increase.

Fantastic aurora displays have been reported from many locations around the world. Below you will find a quick selection of fantastic images made by photographers around the world during the past 24 hours:

Header image: Isaac Diener (Painesdale, Michigan, USA)

Image: Stewart Watt‎ (Thurso, Scotland)

Image: Pauli Purtilo (Espoo, Finland)

Image: Yvonne Johannesström‎ (Ljungaverk, Sweden)

Image: Edwina Aitken (Oban, Scotland)

Image: Roy J Hopwood (Howden Boat Ramp, Tasmania, Australia)

Image: Jeremy Rowe (Calumet, Michigan, USA)

Image: Randy Martin (Murillo, Ontario, Canada)

Image: Kevin Lewis (Cemlyn bay, United Kingdom)

M2.9 solar flare

Sunspot region 2403 remaines in a state of decay but it did found the strength this morning to produce an M2.9 (R1-minor) solar flare that peaked at 05:44 UTC. There was no coronal mass ejection associated with this event. More M-class events are becoming more unlikely as the magnetic complexity of sunspot region 2403 diminishes.

Any mentioned solar flare in this article has a scaling factor applied by the Space Weather Prediction Center (SWPC), the reported solar flares are 42% smaller than for the science quality data. The scaling factor has been removed from our archived solar flare data to reflect the true physical units.

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