Solar Terrestrial Activity Report

Activity chart

Last major update issued on December 15, 2013 at 06:20 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 to active on December 14. Solar wind speed at SOHO ranged between 310 and 614 km/s under the influence of a high speed stream from CH597.

Solar flux measured at 20h UTC on 2.8 GHz was 164.2 (decreasing 12.8 over the last solar rotation). The 90 day 10.7 flux at 1 AU was 134.8. The Potsdam WDC planetary A index was 13 (STAR Ap - based on the mean of three hour interval ap indices: 12.6). Three hour interval K indices: 34211342 (planetary), 35312332 (Boulder).

The background x-ray flux was at the class B6 level.

At the time of counting spots (see image time) spots were observed in 12 active regions in 2K resolution (SN: 288) and 8 active regions in 1K resolution (SN: 171) SDO images on the visible solar disk.

Region 11917 [S15W22] developed further in the northern part with a weak magnetic delta structure forming. C and minor M class flares are possible.
Region 11918 [S10W03] decayed slowly and quietly.
Region 11920 [N07E09] was quiet and stable.
Region 11922 [N10W74] decayed slowly and quietly.
Region 11923 [N17W24] decayed slowly and quietly.
Region 11925 [S07E42] was quiet and stable.
New region 11926 [N08W01] has been slowly emerging for the last few days and finally developed a trailing polarity spot, thus making it possible to split this off from AR 11920.

Spotted regions not numbered by SWPC:
S2897 [N15W37] was quiet and stable.
S2911 [N17W15] was quiet and stable.
New region S2918 [S25E32] emerged with a penumbra spot.
New region S2919 [N33E08] emerged with a penumbra spot in an old plage area.
New region S2920 [S26W47] emerged with a penumbra spot.

Coronal mass ejections (CMEs)

December 13-14: No obviously Earth directed CMEs were observed in LASCO and STEREO imagery.
December 12: A partial halo CME (full halo in STEREO-B) was observed after the C4 event in AR 11912. This CME could have an Earth directed extension. A filament eruption the the south of 11917 was associated with a partial halo CME, possibly with 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) was in 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 fair.

Forecast

The geomagnetic field is expected to be quiet to active on December 15 due to effects from CH597 and a possible contribution from CMEs. Quiet to unsettled is likely on December 16 becoming quiet on December 17-18.

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
11912 2013.12.01
2013.12.02
1     S21W90 0060 HSX     rotated out of view
S2892 2013.12.04       S13W61         plage
11917 2013.12.06
2013.12.07
26 59 31 S15W24 0260 DKC DAC beta-gamma-delta

area: 0480

11923 2013.12.07
2013.12.10
11 26 16 N17W23 0040 DAO CRI  
S2897 2013.12.07   2 1 N15W52 0012   BXO  
11918 2013.12.08 8 23 16 S10W02 0180 DAO CSI beta-gamma

area: 0250

11920 2013.12.08
2013.12.09
5 31 12 N12E05 0070 HAX CKI

location: N07E09

area: 0750

11922 2013.12.08
2013.12.10
3 2 2 N10W71 0060 DAO DAO area: 0120

location: N10W74

S2906 2013.12.08       N09W13           plage
11921 2013.12.09 9     N07E10 0380 CKO       magnetically part of AR 11920
S2908 2013.12.10       S08W24           plage
S2909 2013.12.10       S27W34           plage
11925 2013.12.11
2013.12.13
4 10 6 S07E42 0030 CRO CRI  
S2911 2013.12.11   1   N17W15 0002   AXX  
S2912 2013.12.12       S25W06         plage
S2913 2013.12.12       N03W48           plage
S2914 2013.12.13       N08W30         plage
S2916 2013.12.13       S19W40         plage
11926 2013.12.14 6 11 7 N09W01 0020 CRO DRI   area: 0040
S2918 2013.12.14   1   S25E32 0002   AXX    
S2919 2013.12.14   1   N33E08 0003   AXX    
S2920 2013.12.14   1   S26W47 0001   AXX    
Total spot count: 73 168 91  
Sunspot number: 163 288 171  (total spot count + 10 * number of spotted regions)
Weighted SN: 124 202 125  (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): 98 101 94 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)
possible 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 (62.2 projected, +2.3) 12.60
2013.07 115.5 57.0 (63.9 projected, +1.7) 9.47
2013.08 114.6 66.0 (64.8 projected, +0.9) 8.27
2013.09 102.6 36.9 (65.6 projected, +0.8) 5.23
2013.10  132.1 85.6 (64.9 projected, -0.7) 7.71
2013.11  148.3 77.6 (63.0 projected, -1.9) 5.68
2013.12 154.7 (1) 56.1 (2A) / 124.1 (2B) / 83.5 (2C) (61.7 projected, -1.3) (5.9)

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.