Updated 05/13/2013 @ 02:10 UTC
X-Class Solar Flare
A major X-Class Solar Flare peaking at X1.7 was observed around an active region hiding off the east limb at 02:15 UTC. This event was also responsible for a strong R3 Level Radio Blackout on the sunlit side of Earth. This region is currently seething with activity and should begin to rotate into view within the next 24 hours. Because of the sunspot location, any associated Coronal Mass Ejection (CME) should be directed away from Earth. Stay Tuned to SolarHam.com for the latest and most up to date Space Weather information.
X-Class Solar Flare
A major X-Class Solar Flare peaking at X1.7 was observed around an active region hiding off the east limb at 02:15 UTC. This event was also responsible for a strong R3 Level Radio Blackout on the sunlit side of Earth. This region is currently seething with activity and should begin to rotate into view within the next 24 hours. Because of the sunspot location, any associated Coronal Mass Ejection (CME) should be directed away from Earth. Stay Tuned to SolarHam.com for the latest and most up to date Space Weather information.
SUMMARY: 10cm Radio Burst
Begin Time: 2013 May 13 0208 UTC
Maximum Time: 2013 May 13 0219 UTC
End Time: 2013 May 13 0222 UTC
Duration: 14 minutes
Peak Flux: 320 sfu
Description: A 10cm radio burst indicates that the electromagnetic burst associated with a solar flare at the 10cm wavelength was double or greater than the initial 10cm radio background. This can be indicative of significant radio noise in association with a solar flare. This noise is generally short-lived but can cause interference for sensitive receivers including radar, GPS, and satellite communications.
http://www.solarham.net/
https://www.facebook.com/SolarHam?hc_location=streamBegin Time: 2013 May 13 0208 UTC
Maximum Time: 2013 May 13 0219 UTC
End Time: 2013 May 13 0222 UTC
Duration: 14 minutes
Peak Flux: 320 sfu
Description: A 10cm radio burst indicates that the electromagnetic burst associated with a solar flare at the 10cm wavelength was double or greater than the initial 10cm radio background. This can be indicative of significant radio noise in association with a solar flare. This noise is generally short-lived but can cause interference for sensitive receivers including radar, GPS, and satellite communications.
http://www.solarham.net/
http://sohowww.nascom.nasa.gov/data/realtime/mpeg/
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