Thursday, 2 October 2014 19:36 UTC
Sunspot region 2173 decayed rapidly the past few days and only a couple of sunspots remain as it approaches the west limb. This however didn't stop it from producing two M-class solar flares in rapid succesion: M1.5 (NOAA R1-minor) at 17:44 UTC and M7.3 (NOAA R2-moderate) at 19:01 UTC.
The M7.3 solar flare looks eruptive but it is too early to tell if there really is a coronal mass ejection (CME) associated with this event. Type II and IV sweeps were detected as well as eruptive signatures on SDO imagery which makes it likely that a coronal mass ejection (CME) has been launched. We do need to note that the coronal mass ejection (CME) will likely be directed away from Earth as this sunspot region is already near the west limb. We will await coronagraph imagery and post more information regarding any coronal mass ejection (CME) when we can.
Images: NASA SDO/SIDC.
One thing to note is that this eruption could produce a space radiation storm here at Earth as this eruption is in a favourable location for high energy protons to reach Earth along the magnetic field lines of the interplanetary magnetic field. This could degrade HF radio communications at high latitudes.
ALERT: X-Ray Flux exceeded M5 Threshold Reached: 2014 Oct 02 1857 UTC NOAA Scale: R2 - Moderate
ALERT: Type II Radio Emission Begin Time: 2014 Oct 02 1858 UTC Estimated Velocity: 713 km/s
ALERT: Type IV Radio Emission Begin Time: 2014 Oct 02 1859 UTC
ALERT: Type II Radio Emission Begin Time: 2014 Oct 02 1931 UTC Estimated Velocity: 449 km/s
SUMMARY: X-ray Event exceeded M5 Begin Time: 2014 Oct 02 1849 UTC Maximum Time: 2014 Oct 02 1901 UTC End Time: 2014 Oct 02 1914 UTC X-ray Class: M7.3 Optical Class: 1f Location: S17W82 NOAA Scale: R2 - Moderate
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Coronagraph imagery are now available and show that the coronal mass ejection associated with the M7.3 event is as expected heading south-west and away from Earth.
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