A strong, long duration, solar flare measuring M5.2 erupted from 'beta-gamma' Region 2056 on May 8, 2014. The event started at 09:20, peaked at 10:07, and ended at 10:18 UTC. This region is located near the eastern limb.Radio blackout levels
Departing region 2051 produced 2 M-class and several C-class solar flares in last 24 hours. Newly numbered Region 2055 showed minor penumbral development in its trailer portion and should be on the watch.At 22:09 UTC on May 6 Region 2051 erupted with M1.0 sola
Moderately strong solar flare measuring M1.8 at its peak time erupted on May 6, 2014. The event started at 08:41, peaked at 09:03 and ended at 09:21 UTC.The source was Active Region 2051 located on the western limb. CME was not Earth directed. [Updates]Solar wind parame
Solar activity has been low in last 24 hours, however, that might change today and in the coming days. New Active Region 2051 (S10W44, Dac/beta-gamma-delta) is growing rapidly and is now harboring energy for X-class solar flares. Eruptions from this regio
Major solar flare measuring X1.3 erupted on April 25, 2014 from Region 2035 located behind the western limb. The event started at 00:17, peaked at 00:27, and ended at 00:38 UTC. Because of the location of this region CME was not Earth directed.R3 (strong) Radio Blac
Earth is currently under the influence of S1 (minor) solar radiation storm created as a result of yesterday's M7.3 solar flare. Our planet is showered with highly energetic solar particles (primarily protons) released from the flare site. Extende
A strong, long duration, solar flare measuring M7.3 erupted from Region 2036 on April 18, 2014. This event started at 12:31, peaked at 13:03 and ended at 13:20 UTC.R2 Moderate radio blackout threshold was reached at 12:55 UTC – limited black
Moderately strong solar flare measuring M1.0 erupted from Region 2035 (S17E18, Fkc/beta-gamma) on April 16, 2014. This event started at 19:54, peaked at 19:59 and ended at 20:04 UTC. A Type II Radio Emission with estimated velocity of 1071 km/s was a
A coronal hole high-speed stream (CH HSS) from a pair of coronal holes straddling the Sun's equator is predicted to become geoeffective beginning around midday on April 12 with an increase in solar wind speed expected along with enhancements in the In
Strong, long duration, solar flare measuring M6.5 erupted from Region 2027 on April 2, 2014. The event started at 13:18, peaked at 14:05 and ended at 14:28 UTC.
A Type II and IV Radio Emission with estimated velocity of 903 km/h were observed
