Solar Terrestrial Activity Report

Activity chart

Last major update issued on December 10, 2013 at 05:55 UTC.

[Solar and geomagnetic data - last month (updated daily)]
[Solar wind and electron fluence charts (updated daily)]
[Solar cycles 23-24 (last update December 1, 2013)] [Cycle 24 progress (last update December 1, 2013) ]
[Solar cycles 1-20]
[Graphical comparison of cycles 21, 22, 23 and 24 (last update December 1, 2013)]
[Graphical comparison of cycles 10, 12, 13, 14, 16 and 24 (last update December 1, 2013)]
[Historical solar and geomagnetic data charts 1954-2006 (last update April 5, 2007)]
[Archived reports since January 2003 (last update December 1, 2013)]

[POES auroral activity level since October 2009 - updated January 26, 2013]
[Solar polar fields vs solar cycles - updated December 3, 2013]
[Presentation 3rd SSN Workshop, Tucson, 2013 (pdf)]

Recent activity

The geomagnetic field was quiet on December 9. Solar wind speed at SOHO ranged between 377 and 610 km/s under the weakening influence of a CME related disturbance.

Solar flux measured at 20h UTC on 2.8 GHz was 168.1 (increasing 0.6 over the last solar rotation). The 90 day 10.7 flux at 1 AU was 131.0. The Potsdam WDC planetary A index was 3 (STAR Ap - based on the mean of three hour interval ap indices: 3.3). Three hour interval K indices: 10001211 (planetary), 10012211 (Boulder).

The background x-ray flux was at the class C1 level.

At the time of counting spots (see image time) spots were observed in 13 active regions in 2K resolution (SN: 305) and 11 active regions in 1K resolution (SN: 190) SDO images on the visible solar disk.

Region 11912 [S20W25] was quiet and stable.
Region 11916 [S12W51] was mostly quiet and stable. The region has many spots but is currently not complex magnetically.
Region 11917 [S16E43] developed slowly and quietly.
Region 11918 [S09E64] was quiet and stable.
New region 11919 [S05W23] emerged on December 8 and was numbered the next day by SWPC.
New region 11920 [N08E76] rotated partly into view on December 8 and got its NOAA number the next day. The region has a very extensive trailing positive polarity field with hardly any spots. SWPC has numbered the southern spots as a region on its own. Currently the spots belong magnetically to one region.

Spotted regions not numbered by SWPC:
S2876 [S15W67] reemerged with a penumbra spot.
S2892 [S15E12] was quiet and stable and has many penumbra spots.
S2896 [N17E42] was quiet and stable.
S2897 [N16E13] was quiet and stable. The region has reversed polarities.
S2903 [N12W03] developed slowly and quietly.
S2906 [N10E50] decayed slowly and quietly.
New region S2907 [S12W33] emerged with a penumbra spot.

Coronal mass ejections (CMEs)

December 8-9: No obviously Earth directed CMEs were observed in LASCO and STEREO imagery.
December 7: A CME was observed in STEREO imagery after an M1 event in AR 11909. The partial halo CME was wide and could have an Earth directed extension.

Coronal holes

Coronal hole history (since October 2002)
Compare today's report to the situation one solar rotation ago: 28 days ago 27 days ago 26 days ago

A large northern hemisphere coronal hole (CH597) will likely rotate into an Earth facing position on December 11.

Coronal hole map

Propagation

Long distance low and medium frequency (below 2 MHz) propagation along paths north of due west over high and upper middle latitudes is poor. Propagation on long distance northeast-southwest paths is poor.

Forecast

The geomagnetic field is expected to be quiet to unsettled on December 10 due to weak CME effects and quiet on December 11-13. A high speed stream from CH597 could cause unsettled and active intervals on December 14-15.

Coronal holes (1) Coronal mass ejection (2) M and X class flares (3)
     

1) Effects from a coronal hole could reach Earth within the next 5 days. When the high speed stream has arrived the color changes to green.
2) Effects from a CME are likely to be observed at Earth within 96 hours.
3) There is a possibility of either M or X class flares within the next 48 hours.

Green: 0-20% probability, Yellow: 20-60% probability, Red: 60-100% probability.

Active solar regions

(Click on image for 2K resolution) Compare to the previous day's image. 0.5K image

When available the active region map has a coronal hole polarity overlay where red (pink) is negative and blue is positive.

Data for all numbered solar regions according to the Solar Region Summary provided by NOAA/SWPC. Comments are my own, as is the STAR spot count (spots observed at or inside a few hours before midnight) and data for regions not numbered by SWPC or where SWPC has observed no spots. SWPC active region numbers in the table below and in the active region map above are the historic SWPC/USAF numbers.

Active region Date numbered
detected
Spot count Location at midnight Area Classification SDO / HMI 4K continuum
image with magnetic polarity overlay
Comment
SWPC STAR SDO SWPC STAR Current Previous
2K 1K
11909 2013.11.26
2013.11.27
1     S19W93 0040 HSX    

 

S2876 2013.12.01   1   S15W66 0002   AXX    
11912 2013.12.01
2013.12.02
2 7 1 S21W24 0110 HSX CSO area: 0160
11915 2013.12.01
2013.12.03
      S30W87           plage
S2887 2013.12.03       N08W53           plage
11916 2013.12.04 20 47 30 S13W51 0210 EAC EAC  

area: 0450

S2892 2013.12.04   30 8 S15E12 0060   BXI  
11917 2013.12.06
2013.12.07
10 32 16 S16E45 0240 CAI DAI beta-gamma

area: 0340

S2896 2013.12.07   10 5 N17E42 0035   CRO  
S2897 2013.12.07   8 4 N16E13 0040   CRO reversed polarities
S2898 2013.12.07       N20W08           plage
11918 2013.12.08 4 14 6 S08E63 0110 DAO CAO area: 0200
S2901 2013.12.08       N31W40         plage
11920 2013.12.08
2013.12.09
1 6 3 N12E71 0070 HSX CKO location: N08E76

area: 0500

S2903 2013.12.08   4 1 N12W03 0005   CRO  
11919 2013.12.08
2013.12.09
5 13 5 S06W25 0020 CRO DRO location: S05W23

area: 0060

S2906 2013.12.08   2   N10E50 0003   AXX  
11921 2013.12.09 2     N06E75 0120 HSX       magnetically part of AR 11920
S2907 2013.12.09   1 1 S12W33 0004   AXX    
Total spot count: 45 175 80  
Sunspot number: 125 305 190  (total spot count + 10 * number of spotted regions)
Weighted SN: 83 217 122  (Sum of total spot count + classification weighting for each AR. Classification weighting: X=0, R=3, A/S=5, H/K=10)
Relative sunspot number (Wolf number): 75 107 105 k * (sunspot number). k = 0.6 for SWPC, k = 0.35 for STAR SDO 2K, k = 0.55 for STAR SDO 1K

Monthly solar cycle data

Month Average measured solar flux International sunspot number (SIDC) Smoothed sunspot number Average ap
(3)
2011.11 153.5 (cycle peak) 96.7 (cycle peak) 61.1 (+1.2) 5.55
2012.02 106.5 32.9 66.9 (+1.4)
possibe cycle 24 max
8.81
2012.08 115.4 63.0 58.2 (+0.4) 7.96
2012.09 122.9 61.4 58.1 (-0.1) 8.07
2012.10 123.3 53.3 58.6 (+0.5) 9.97
2012.11 121.3 61.8 59.7 (+1.1) 7.08
2012.12 108.6 40.8 59.6 (-0.1) 3.44
2013.01 127.1 62.9 58.7 (-0.9) 4.69
2013.02 104.3 38.0 58.4 (-0.3) 6.11
2013.03 111.3 57.9 57.5 (-0.9) 10.56
2013.04 124.8 72.4 57.9 (+0.4) 5.40
2013.05 131.4 78.7 59.9 (+2.0) 9.73
2013.06 110.1 52.5 (61.5 projected, +1.6) 12.60
2013.07 115.5 57.0 (62.1 projected, +0.6) 9.47
2013.08 114.6 66.0 (62.3 projected, +0.2) 8.27
2013.09 102.6 36.9 (61.2 projected, -1.1) 5.23
2013.10  132.1 85.6 (59.0 projected, -2.2) 7.71
2013.11  148.3 77.6 (57.3 projected, -1.7) 5.68
2013.12 147.5 (1) 30.4 (2A) / 104.8 (2B) / 80.6 (2C) (56.1 projected, -1.2) (6.7)

1) Running average based on the daily 20:00 UTC observed solar flux value at 2800 MHz.
2A) Current impact on the monthly sunspot number based on the Boulder (NOAA/SWPC) sunspot number (accumulated daily sunspots / month days). The official SIDC international sunspot number is typically 30-50% lower. 2B) Boulder SN current month average to date. 2C) STAR SDO 1K Wolf number 30 day average.
3) Running average based on the quicklook and definitive Potsdam WDC ap indices. Values in red are based on the definitive international Potsdam WDC ap indices.

This report has been prepared by Jan Alvestad. It is based on the analysis of data from whatever sources are available at the time the report is prepared. All time references are to the UTC day. Comments and suggestions are always welcome.

SDO images are courtesy of NASA/SDO and the AIA, EVE, and HMI science teams.