Second strongest storm, M6.6 CME analysis

Tuesday, 23 June 2015 10:39 UTC

The direction of the IMF remains south at the time of this post and more geomagnetic storming is likely in the hours ahead. We have seen reports of vivid aurora displays from many places around the world. If you also witnessed an auroral display and made images or videos that you would like to share with us feel free to send them in to photos[at]spaceweatherlive.com. Thanks!

Image: Aurora Borealis as seen from Viewmont, NY (USA) by Pete Mauney.

Image: Aurora Borealis as seen from Sparta, WI (USA) by Jacob Jones. 

M6.6 coronal mass ejection analysis

Yesterday evening at the same time as the coronal mass ejection arrival, sunspot region 2371 erupted once more. This time it found the strength for an M6.6 (R2-moderate) solar flare that peaked at 18:23 UTC.

Strong M6.6 solar #flare from #sunspot region 12371 - Follow live on http://t.co/XHATH0OOfT pic.twitter.com/5u8YejiCyB

— SpaceWeatherLive (@_SpaceWeather_) 22 juni 2015

It didn't took long to come to the conclusion that this M6.6 solar flare also launched a coronal mass ejection with an earth-directed component. More about that here in our news update from yesterday evening. SOHO imagery shows us a very nice halo coronal mass ejection which is guaranteed to arrive at Earth. The animations below from SOHO shows us the full expanding halo as the plasma cloud leaves the Sun.

Animations: SOHO/LASCO C2 and C3 coronagraph animations showing the M6.6 coronal mass ejection as it leaves the Sun.

While this coronal mass ejection does not expand like a perfect symmetrical halo event as the 21 June coronal mass ejection did (this coronal mass ejection has it's bulk heading a bit north-west) we still expect a very decent impact from this event as the full halo is still well defined.

CACtus reports a speed of about 1000km/s which is only a fraction slower than the coronal mass ejection of 21 June. Considering this coronal mass ejection is traveling trough a portion of space which has pretty much been cleared of ambient solar wind by the 21 June coronal mass ejection it is possible that this coronal mass ejection does not decelerate all that much. Using the same method that we used to predict the arrival time of the June 21 CME (which arrived close to our predicted arrival time) we come to the conclusion that this plasma cloud will arrive at Earth on Wednesday 24 June at 17:00 UTC with a plus/minus of 6 hours. The solar wind speed could again increase to about 700km/s and if the direction of the IMF again turns southward (Bz) we could again experience a strong G3 geomagnetic storm with aurora displays possible at middle latitude locations like southern England, Belgium and northern parts of Germany and Poland in Europe and many of the northernmost states in the USA. With a bit of luck, even sky watchers in southern parts of New South Wales in Australia will need to be alert for possible aurora displays.