M9.2 solar flare from sunspot region 2297

Saturday, 7 March 2015 23:20 UTC

M9.2 solar flare from sunspot region 2297

Sunspot region 2297 is active again after a relative calm past 36 hours. It produced the strongest solar flare thus far in 2015: a near X-class event that peaked at M9.2 (R2-moderate) around 22:22 UTC. This was a long duration event which means it likely produced a coronal mass ejection. When looking at difference imagery from SDO we can conclude that a massive coronal mass ejection was launched, something the latest LASCO coronagraph imagery confirms.

Image: Difference imagery from NASA SDO showing coronal dimming, a sign that a coronal mass ejection was launched.

Image: Latest SOHO/LASCO C2 image showing a bright coronal mass ejection leaving the blast site.

A solar radiation storm is not expected as this sunspot region is not located in a prime position to cause such an event and this coronal mass ejection will also certainly not come directly towards Earth. We will have to wait for more coronagraph imagery before we can make a definitive conclusion regarding the exact trajectory of this CME. A glancing blow could be expected at most but it is also possible that the plasma cloud will miss Earth completly.

NOAA SWPC alerts

ALERT: X-Ray Flux exceeded M5
Threshold Reached: 2015 Mar 07 2203 UTC
NOAA Scale: R2 - Moderate
ALERT: Type II Radio Emission
Begin Time: 2015 Mar 07 2157 UTC
Estimated Velocity: 704 km/s
ALERT: Type IV Radio Emission
Begin Time: 2015 Mar 07 2204 UTC
SUMMARY: 10cm Radio Burst
Begin Time: 2015 Mar 07 2236 UTC
Maximum Time: 2015 Mar 07 2239 UTC
End Time: 2015 Mar 07 2246 UTC
Duration: 10 minutes
Peak Flux: 260 sfu
Latest Penticton Noon Flux: 138 sfu
SUMMARY: X-ray Event exceeded M5
Begin Time: 2015 Mar 07 2145 UTC
Maximum Time: 2015 Mar 07 2222 UTC
End Time: 2015 Mar 07 2258 UTC
X-ray Class: M9.2
Location: S19E60
NOAA Scale: R2 - Moderate

We will provide more news regarding this solar flare and it's coronal mass ejection tomorrow as more coronagraph imagery becomes available. Keep an eye on this website!

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.

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! Never want to miss out on a space weather event or one of our news articles again? Subscribe to our mailing list, follow us on Twitter and Facebook and download the SpaceWeatherLive app for Android and iOS!

Latest news

Support SpaceWeatherLive.com!

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!

100%
Support SpaceWeatherLive with our merchandise
Check out our merchandise

Latest alerts

Get instant alerts!

Space weather facts

Last X-flare2024/11/06X2.39
Last M-flare2024/11/22M1.0
Last geomagnetic storm2024/11/10Kp5+ (G1)
Spotless days
Last spotless day2022/06/08
Monthly mean Sunspot Number
October 2024166.4 +25
November 2024144.1 -22.3
Last 30 days158 +10.7

This day in history*

Solar flares
11998X3.24
21998M4.53
32013M1.69
42000M1.56
52013M1.54
DstG
11997-108G3
21982-101G2
31959-95G2
41991-84G1
51981-81
*since 1994

Social networks