Sunday, 19 April 2015 14:32 UTC
The Sun released an asymmetrical full halo coronal mass ejection yesterday (as seen by SOHO) due to a C5.2 solar flare in combination with a filament eruption near sunspot region 2321.
A slow, faint, asymmetrical full halo coronal mass ejection raced away from the Sun at a speed of about 400km/s which is only slightly faster than the background solar wind. We expect this coronal mass ejection to arrive at Earth on 22 April with likely no or only a very minimal increase in the solar wind speed. No geomagnetic storming is expected from this event due to the slow speed of the CME but high latitude sky watchers should be alert for possible enhanced auroral displays on 22 and 23 April if the parameters of the IMF are favourable. Kp-values up to 4 (active geomagnetic conditions) are possible.
Images: SOHO/LASCO C2 (left) and C3 (right) coronagraph animations.
Thank you for reading this article! Did you have any trouble with the technical terms used in this article? Our help section is the place to be where you can find in-depth articles, a FAQ and a list with common abbreviations. Still puzzled? Just post on our forum where we will help you the best we can!
A lot of people come to SpaceWeatherLive to follow the Sun's activity or if there is aurora to be seen, but with more traffic comes higher server costs. Consider a donation if you enjoy SpaceWeatherLive so we can keep the website online!
Last X-flare | 2024/11/06 | X2.39 |
Last M-flare | 2024/11/20 | M1.1 |
Last geomagnetic storm | 2024/11/10 | Kp5+ (G1) |
Spotless days | |
---|---|
Last spotless day | 2022/06/08 |
Monthly mean Sunspot Number | |
---|---|
October 2024 | 166.4 +25 |
November 2024 | 142.7 -23.8 |
Last 30 days | 156.1 +4.7 |