Major solar flare measuring X1.6 erupts, sends Earth directed CME

A major solar flare measuring X1.6 at its peak time erupted on September 10, 2014. The source was geoeffective Active Region 2158 located almost at the center of the disk. The event started at 17:21, peaked at 17:45 and ended at 18:20 UTC.

Coronal Mass Ejection (CME) was generated and is headed directly toward our planet.

A Type II (velocity 3750 km/s) and Type IV radio emissions were associated with the event. Type IV emissions occur in association with major eruptions on the sun and are typically associated with strong coronal mass ejections and solar radiation storms.

Additionally, a 10cm Radio Burst (tenflare) lasting 57 minutes with peak flux of 1300 sfu was associated with the event. 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.

Region 2158, the source of today's X-class solar flare, has 'beta-gamma-delta' magnetic configuration and is capable of producing more strong to major eruptions on the Sun. It will remain in geoeffective position for the next couple of days. Any CME from that region will most likely be Earth directed. 

NOAA SWPC forecasters estimate 85% chance for M-class and 40% chance for X-class solar flares in the next two days.

Update, September 11:

The CME is expected to pass the Earth's magnetosphere mid to late day on September 12h. It follows the September 9th CME which is expected to arrive early on September 12.

A G3 (Strong) Geomagnetic Storm Watch has been issued for September 13th due to the combined influence of these two events with G1 (Minor) storming anticipated to continue into September 14th.

WSA-Enlil solar wind prediction. Check SWS-Solar Wind for updated model.

S1 (Minor) solar radiation storm is in progress as a result of the X1.6 eruption and is expected to persist for the next few days. 

Alerts issued during and after X1.6 flare:

Space Weather Message Code: SUMX01Serial Number: 103Issue Time: 2014 Sep 10 1827 UTC

SUMMARY: X-ray Event exceeded X1Begin Time: 2014 Sep 10 1721 UTCMaximum Time: 2014 Sep 10 1745 UTCEnd Time: 2014 Sep 10 1820 UTCX-ray Class: X1.6Optical Class: 2bLocation: N15E09NOAA Scale: R3 - StrongPotential Impacts: Area of impact consists of large portions of the sunlit side of Earth, strongest at the sub-solar point.Radio - Wide area blackout of HF (high frequency) radio communication for about an hour.

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Space Weather Message Code: SUM10RSerial Number: 627Issue Time: 2014 Sep 10 1903 UTC

SUMMARY: 10cm Radio BurstBegin Time: 2014 Sep 10 1723 UTCMaximum Time: 2014 Sep 10 1732 UTCEnd Time: 2014 Sep 10 1826 UTCDuration: 57 minutesPeak Flux: 1300 sfuLatest Penticton Noon Flux: 159 sfu

NOAA Space Weather Scale descriptions can be found atwww.swpc.noaa.gov/NOAAscales

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.

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Space Weather Message Code: ALTTP4Serial Number: 477Issue Time: 2014 Sep 10 1815 UTC

ALERT: Type IV Radio EmissionBegin Time: 2014 Sep 10 1728 UTCDescription: Type IV emissions occur in association with major eruptions on the sun and are typically associated with strong coronal mass ejections and solar radiation storms.

***Space Weather Message Code: ALTTP2Serial Number: 960Issue Time: 2014 Sep 10 1814 UTC

ALERT: Type II Radio EmissionBegin Time: 2014 Sep 10 1727 UTCEstimated Velocity: 3750 km/sDescription: Type II emissions occur in association with eruptions on the sun and typically indicate a coronal mass ejection is associated with a flare event.

Image credit: NASA/ESA SOHO LASCO C2

Image credit: NASA/ESA SOHO LASCO C3

Sunspots

There are currently 8 numbered sunspot regions on the disk. Regions 2157 and 2158 have 'beta-gamma-delta' magnetic configuration and continue to be areas of interest as they are still the largest and most magnetically complex regions on the visible disk. Both are almost directly facing Earth and should they produce CMEs they will most likely be Earth directed.

Sunspots on September 10, 2014. Image credit: NASA SDO / HMI

2152 - Alpha2155 - Beta2157 - Beta-Gamma-Delta2158 - Beta-Gamma-Delta2159 - Beta2161 - Alpha2162 - Beta2163 - Beta

Geospace

Geomagnetic field was mostly quiet today but this will likely rapidly change on September 12th when the CME from September 9 is expected to impact Earth's magnetospere. Quiet to major storm (G2/Moderate) conditions are expected as a result.

Update, September 11:

G2 (Moderate) geomagnetic storms remain in the forecast for September 12th as a result of the coronal mass ejection (CME) associated with the R1 (Minor) solar flare observed on the 9th. The latest WSA-Enlil model run has the CME associated with X1.6 - R3 (Strong) solar flare arriving mid to late day on that same day.

A G3 (Strong) Geomagnetic Storm Watch has been issued for September 13th due to the combined influence of these two events with G1 (Minor) storming anticipated to continue into September 14th.

Featured image: NASA SDO / AIA 304