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Growing region 1967 produced strong M6.6 solar flare, glancing blow from CME possible

growing-region-1967-produced-strong-m6-6-solar-flare-hurled-cme-into-space

Image credit: NASA SDO / AIA 304 - January 30, 2014 at 16:11 UTC.

At 16:11 UTC today Region 1967 (S14E48, Fkc/beta-gamma-delta) unleashed its 13th and strongest M-class solar flare since it returned from the farside of the Sun. The region is rotating toward the center of the disk and is showing a trend of slight growth. Earth directed Coronal Mass Ejections (CME) from this region are possible in the days ahead.

After M2.1 at 06:44 and M1.1 at 08:41 UTC today, a strong solar flare measuring M6.6 erupted. A Type II Radio Emission, indicating a CME, was associated with a flare event. Its estimated velocity was 2161 km/s.

A 10cm Radio Burst (TenFlare) lasting 29 minutes was also reported. 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.

Update (SWPC, January 31, 2014 – 00:30 UTC):

"An asymmetric halo CME was observed in SOHO/LASCO C2 coronagraph imagery emerging from the southeast limb at 16:24 UTC.

Analysis suggests the CME was moving at approximately 1400-1500 km/s and may have an earthward component. WSA-Enlil model run is underway to determine the geoeffectiveness.

CME associated with the M2.1 flare was first observed in Lasco C2 imagery at 08:24 UTC. Analysis suggests this CME was moving around 500 km/s with very little of the ejecta being Earth-directed. It has been included in the model run mentioned above to determine the extent of any interaction."

Update (SWPC, January 31, 2014 – 12:30 UTC):

"WSA-ENLIL model analysis [for M6.6 solar flare] indicates a glancing blow from the CME is likely mid to late on February 02."

*** end of updates ***

ENameStartStopPeakGOES ClassDerived Position
gev_20140127_01052014/01/27 01:05:0001:39:0001:22:00M1.0S16E88 ( 1967 )
gev_20140127_02022014/01/27 02:02:0002:18:0002:11:00M1.1S13E88 ( 1967 )
gev_20140127_22052014/01/27 22:05:0022:15:0022:10:00M4.9S14E88 ( 1967 )
gev_20140128_04022014/01/28 04:02:0004:13:0004:09:00M1.5S14E88 ( 1967 )
gev_20140128_07252014/01/28 07:25:0007:34:0007:31:00M3.6S10E75 ( 1967 )
gev_20140128_11342014/01/28 11:34:0011:41:0011:38:00M1.4S10E72 ( 1967 )
gev_20140128_12332014/01/28 12:33:0012:50:0012:46:00M1.3S15E79 ( 1967 )
gev_20140128_15242014/01/28 15:24:0015:30:0015:26:00M3.5S13E88 ( 1967 )
gev_20140128_19002014/01/28 19:00:0019:46:0019:40:00M4.9S14E75 ( 1967 )
gev_20140128_22042014/01/28 22:04:0022:20:0022:16:00M2.6S14E74 ( 1967 )
gev_20140130_06332014/01/30 06:33:0006:44:0006:39:00M2.1S14E54 ( 1967 )
gev_20140130_07542014/01/30 07:54:0008:41:0008:11:00M1.1S11E54 ( 1967 )
gev_20140130_15482014/01/30 15:48:0016:28:0016:11:00M6.6S11E64

Data source: http://www.lmsal.com/solarsoft/latest_events/

Space Weather Message Code: SUM10R
Serial Number: 607
Issue Time: 2014 Jan 30 1642 UTC

SUMMARY: 10cm Radio Burst
Begin Time: 2014 Jan 30 1553 UTC
Maximum Time: 2014 Jan 30 1605 UTC
End Time: 2014 Jan 30 1622 UTC
Duration: 29 minutes
Peak Flux: 220 sfu

Latest Penticton Noon Flux: 156 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.

***

Space Weather Message Code: ALTTP2
Serial Number: 904
Issue Time: 2014 Jan 30 1639 UTC

ALERT: Type II Radio Emission
Begin Time: 2014 Jan 30 1601 UTC
Estimated Velocity: 2161 km/s
Description: Type II emissions occur in association with eruptions on the sun and typically indicate a coronal mass ejection is associated with a flare event.

***

Space Weather Message Code: SUMXM5
Serial Number: 112
Issue Time: 2014 Jan 30 1633 UTC

SUMMARY: X-ray Event exceeded M5
Begin Time: 2014 Jan 30 1548 UTC
Maximum Time: 2014 Jan 30 1611 UTC
End Time: 2014 Jan 30 1628 UTC
X-ray Class: M6.6
Location: S12E61
NOAA Scale: R2 – Moderate
Potential Impacts: Area of impact centered primarily on sub-solar point on the sunlit side of Earth.
Radio – Limited blackout of HF (high frequency) radio communication for tens of minutes.

Sunspots

There are currently 5 numbered sunspot groups on the Earth side of the Sun.

1959 S23W75 242 90 2 HAX 1 A
1960 S15W70 237 70 3 HSX 3 A
1965 S13W43 210 20 2 CRO 2 B
1967 S14E55 111 980 18 FKC 29 BGD
1968 N09E54 112 210 11 EAO 11 B

Sunspots on January 30, 2014. Image credit: NASA SDO / HMI

Region 1967 (S14E48, Fkc/beta-gamma-delta) continues its trend of slight growth. Region 1968 (N09E48,Eao/beta-gamma) exhibited mixed polarities in the leader spots, yet remained fairly inactive. The remaining three numbered sunspot groups are stable or showing signs of decay.

I'm a dedicated researcher, journalist, and editor at The Watchers. With over 20 years of experience in the media industry, I specialize in hard science news, focusing on extreme weather, seismic and volcanic activity, space weather, and astronomy, including near-Earth objects and planetary defense strategies. You can reach me at teo /at/ watchers.news.

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