Northern Lights Now – Occassionally when there is a strong aurora predicted, and we feel there is a good chance for an evolving storm, we’ll start up the live blog! As the storm transpires over the next couple days keep checking back. We will talk about the source of the storm, give updates on it’s progression, and hopefully share some of the photos our followers share with us. If you’d like to have your photo featured please tag NLN on Twitter
August 19, 3:45 UTC
Reminent activity from the initial CME impact shock, and the high speed solar winds from the coronal hole have produced intermitent activity over the last 6-9 hours. With Bz variable, there hasn’t been a long duraction aurora event yet. Even with the Bz uncooperative, the strong winds and high proton density in the tail end of the first CME have been enough to produce occasional G1 conditions. Some aurora photographers have gotten lucky and captured a show. If you have a great aurora photo and would like us to share it in the live blog, tag it with #NLNLiveBlog
August 18, 09:00 UTC
Fairly quiet since the last update. Solar wind speeds remain high around 575km/s as a result of the Coronal Hole High Speed Stream. Most forcasters are still anticipating the arrival of the next CME. When it arrives, the data on the solar wind page will show a jump in values. Keep an eye on the Bz, if it dives south at that point (negative), we should be in for a good show.
August 18, 04:30 UTC
The first round of activity brought a period G2 activity across two three hours periods. The timing of this storm meant that mostly aurora hunters in northern Europe got to see a show. Viewers in North America and Au/NZ will need to wait until later in this storm.
A series of Six storms on the surface of the Sun launched solar plasma and other CME material towards earth between August 13 and August 16. As these arrive they will activate the magnetosphere and produce aurora. SWPC is predicting a long period of G1 storming, with chances for KP=7+ over this period.