Limb eruption, S1 radiation storm, sunspot region 2371

Thursday, 18 June 2015 12:23 UTC

Limb eruption, S1 radiation storm, sunspot region 2371

Early this morning we observed an M1.2 solar flare (R1-minor) peaking at 01:27 UTC from sunspot region 2365 at the West limb. The solar flare was accompanied by a gorgeous prominence eruption and launched a stunning coronal mass ejection.

A closer look at imagery from SOHO reveals that the coronal mass ejection is not aimed at Earth which was to be expected considering the source location of this event. Coronagraph imagery show that the coronal mass ejection which leaves the Sun at a speed of about 650km/s only forms a partial halo that will pass well south-west of Earth.

Image: SOHO/LASCO C2 difference image showing the coronal mass ejection of this morning.

The eruption also caused a minor S1 solar radiation storm here at Earth which is still in progress at this time. This is nothing to be concerned about as it only affects HF radio signals through polar regions.

Note that this eruption also surged the low energy protons and electrons at ACE. This is caused by this morning eruption and does not indicate that the coronal mass ejection is directed at Earth.

Sunspot region 2371

We understand that amazing eruptions like these beg the question: could there be more eruptions like these in store for us?

Answer: maybe.

There is a sunspot region on the earth-facing disk right now which is moderately complex and that is sunspot region 2371. This sunspot region is showing signs of growth and is already a Beta-Gamma sunspot region. A closer look at SDO imagery shows however that a Beta-Gamma-Delta classification can already be made. An M-class (R1-R2) solar flare from this sunspot region is very much possible in the coming days. 

Images: SDO/HMI images showing the (magnetic) layout of sunspot region 2371.

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 Solar activity or if there is a chance to see the aurora, but with more traffic comes higher costs to keep the servers online. If you like SpaceWeatherLive and want to support the project you can choose a subscription for an ad-free site or consider a donation. With your help we can keep SpaceWeatherLive online!

No Ads on SWL Pro!
No Ads on SWL Pro! Subscriptions
Donations
Support SpaceWeatherLive.com! Donate
Support SpaceWeatherLive with our merchandise
Check out our merchandise

Latest alerts

Get instant alerts!

Space weather facts

Last X-flare2026/03/30X1.5
Last M-flare2026/04/09M1.0
Last geomagnetic storm2026/04/03Kp7- (G3)
Spotless days
Last 365 days3 days
20263 days (3%)
Last spotless day2026/02/24
Monthly mean Sunspot Number
March 202685.9 +7.7
April 202697.2 +11.3
Last 30 days95.6 +37.2

This day in history*

Solar flares
12025M3.24
22024M2.41
32025M2.31
42025M1.6
52025M1.41
DstG
11981-311G4
21990-108G1
31973-84G3
42001-77G3
51969-64
*since 1994

Aurora on this day in history

No observations submitted for this day in history. If you've observed the aurora and you have some amazing photos to show off, submit your observations now!
Submit your aurora observation

Social networks