Solar Terrestrial Activity Report

Activity chart

Last major update issued on January 7, 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 January 1, 2013)] [Cycle 24 progress (last update January 1, 2013) ]
[Solar cycles 1-20]
[Graphical comparison of cycles 21, 22, 23 and 24 (last update January 1, 2013)]
[Graphical comparison of cycles 10, 12, 13, 14, 16 and 24 (last update January 1, 2013)]
[Historical solar and geomagnetic data charts 1954-2006 (last update April 5, 2007)]
[Archived reports since January 2003 (last update January 2, 2013)]

[POES auroral activity level since October 2009 - updated October 7, 2012]
[Solar polar fields vs solar cycles - updated December 22, 2012]

Recent activity

The geomagnetic field was quiet on January 6. Solar wind speed at SOHO ranged between 280 and 362 km/s, gradually increasing throughout the day, likely under the influence of a low speed coronal hole stream.

Solar flux measured at 20h UTC on 2.8 GHz was 142.2 (increasing 38.2 over the last solar rotation). The Potsdam WDC planetary A index was 3 (STAR Ap - based on the mean of three hour interval ap indices: 2.8). Three hour interval K indices: 00011121 (planetary), 01001321 (Boulder).

The background x-ray flux was at the class B5 level.

At midnight UTC the visible solar disk had 16 spotted active regions (in 2K resolution SDO images).

Region 11638 [N12W60] was quiet and stable.
Region 11640 [N27W74] was quiet and stable.
Region 11641 [N02W33] decayed slowly and quietly.
Region 11642 [S24W03] was quiet and stable.
Region 11643 [S14W08] decayed slowly and could soon become spotless.
Region 11644 [N15E09] was quiet and stable.
Region 11645 [S13W43] decayed slowly and quietly.
Region 11646 [N13E18] was quiet and stable.
Region 11647 [N17W78] decayed slowly and quietly.
Region 11648 [N06E26] decayed slowly and quietly.
Region 11649 [S15E46] was quiet and stable.
Region 11650 [S29E55] was quiet but could produce at least C flares.
Region 11651 [N20E24] decayed slowly and quietly.
Region 11652 [N19E65] produced a single C class event and was otherwise quiet and stable.
Region 11653 [N08E63] produced a few C flares and was the most active region on the visible disk.

Spotted regions not numbered by SWPC:
New region S2160 [S17E12] emerged with tiny spots.

Coronal mass ejections (CMEs)

January 4-6: No obviously Earth directed CMEs were observed in LASCO and STEREO imagery.

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 small recurrent trans equatorial coronal hole (CH549) was in an Earth facing position on January 3-4.

Coronal hole map

The above coronal hole map is based on a method where coronal holes are detected automatically. While the method may need some fine tuning, it has significant advantages over detecting coronal holes manually. The main improvement is the ability to detect coronal holes at and just beyond the solar limbs. Early results using this method for SDO images over a span of several weeks indicate a good match between coronal holes observed over the visible disk and their extent and position at the east and west limbs. Note that the polar coronal holes are easily detected using this method, the extent and intensity of both CHs are consistent with other data sources.

Propagation

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

Forecast

The geomagnetic field is expected to be mostly quiet on January 7-9, there's a chance of unsettled intervals due to effects from CH549.

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 (blue-green) 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
11639 2012.12.26
2012.12.27
      S16W66           plage
11638 2012.12.26
2012.12.27
1 1 1 N13W61 0050 HSX HSX area: 0120
S2133 2012.12.28       N18W54           plage
11641 2012.12.29
2012.12.31
1 1 1 N02W33 0030 HSX HSX  
S2138 2012.12.29       N03W43           plage
11640 2012.12.29
2012.12.30
4 3 3 N28W75 0360 EHO EHO area: 0460
11642 2012.12.30
2012.12.31
1 5 3 S25W04 0090 HSX CSO

area: 0180

11643 2012.12.31
2013.01.02
  1   S14W11 0000   AXX location: S14W08
11644 2013.01.01
2013.01.02
3 8 3 N15E09 0040 CSO CSO area: 0070
11648 2013.01.02
2013.01.04
6 8 3 N05E26 0030 CRO BXO  
11646 2013.01.02
2013.01.03
1 4 2 N13E17 0040 HSX CSO area: 0070
11651 2013.01.02
2013.01.04
1 2 1 N20E23 0010 AXX AXX  
11645 2013.01.02
2013.01.03
4 2   S13W45 0010 BXO BXO  
11647 2013.01.02
2013.01.04
3 1   N16W81 0020 CRO AXX  
11649 2013.01.03
2013.01.04
1 3 1 S15E46 0070 HSX HSX area: 0100
S2156 2013.01.03       N17E19         plage
11650 2013.01.04 9 21 8 S29E54 0240 EAO EAO  
11652 2013.01.05 8 18 10 N20E61 0120 DAO EAO

location: N19E65

11653 2013.01.05 3 4 3 N09E63 0030 CSO DAO  
S2157 2013.01.05       S02E16         plage
S2158 2013.01.05       N15W25         plage
S2159 2013.01.05       N25W07         plage
S2160 2013.01.06   3   S17E12 0000   BXO    
Total spot count: 46 85 39  
Sunspot number: 186 245 159  (total spot count + 10 * number of spotted regions)
Weighted SN: 107 140 94  (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): 112 86 87 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)
2011.10 137.3 88.0 59.9 (+0.4) 8.28
2011.11 153.5 (cycle max) 96.7 (cycle max) 61.1 (+1.2) 5.55
2011.12 141.3 73.0 63.4 (+2.3) 3.78
2012.01 132.5 58.3 65.5 (+2.1) 7.15
2012.02 106.5 32.9 66.9 (+1.4)
possible cycle 24 max
8.81
2012.03 114.7 64.3 66.8 (-0.1) 16.08
2012.04 113.0 55.2 64.6 (-2.2) 10.10
2012.05 121.5 69.0 61.7 (-2.9) 7.06
2012.06 119.6 64.5 58.9 (-2.8) 10.08
2012.07 133.9 66.5 (57.4 projected, -1.5) 13.90
2012.08 115.4 63.1 (58.3 projected, +0.9) 7.96
2012.09 122.9 61.5 (58.9 projected, +0.6) 8.07
2012.10 123.3 53.3 (58.3 projected, -0.6) 9.97
2012.11 121.3 61.4 (57.6 projected, -0.7) 7.08
2012.12 108.6 40.8 (56.9 projected, -0.7) 3.44
2013.01 132.7 (1) 27.1 (2A) / 139.8 (2B) / 53.2 (2C) (56.2 projected, -0.7) (1.85)

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 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.