Solar Terrestrial Activity Report

Activity chart

Last major update issued on September 26, 2012 at 04:10 UTC.

[Solar and geomagnetic data - last month (updated daily)]
[Solar wind and electron fluence charts (updated daily)]
[Solar cycles 21-24 (last update September 8, 2012)] [Cycle 24 progress (last update September 2, 2012) ]
[Solar cycles 1-20]
[Graphical comparison of cycles 21, 22, 23 and 24 (last update September 8, 2012)]
[Graphical comparison of cycles 10, 12, 13, 14, 16 and 24 (last update September 8, 2012)]
[Historical solar and geomagnetic data charts 1954-2006 (last update April 5, 2007)]
[Archived reports since January 2003 (last update September 3, 2012)]

[POES auroral activity level since October 2009 - updated September 8, 2012]
[Solar polar fields vs solar cycles - updated June 27, 2011]

Recent activity

The geomagnetic field was very quiet on September 25. Solar wind speed at SOHO ranged between 298 and 374 km/s.

Solar flux measured at 20h UTC on 2.8 GHz was 139.8 (increasing 21.5 over the last solar rotation). The Potsdam WDC planetary A index was 2 (STAR Ap - based on the mean of three hour interval ap indices: 2.4). Three hour interval K indices: 11101000 (planetary), 11001200 (Boulder).

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

At midnight UTC the visible solar disk had 15 spotted active regions (in 2K resolution SDO images).

Region 11573 [N14W55] developed slowly and produced a single small C flare.
Region 11575 [N07W17] decayed slowly and was mostly quiet.
Region 11576 [S21W10] decayed slowly and quietly.
Region 11577 [N08E03] decayed further and was mostly quiet.
Region 11578 [N20W04] decayed significantly and was quiet.
Region 11579 [S10E60] was quiet and stable.
New region 11580 [N16E69] rotated into view on September 24 and was numbered the next day by SWPC.
New region 11581 [N20E05] emerged on September 19 and got its NOAA number 6 days later.

Spotted regions not numbered by NOAA/SWPC:
S1924 [S26W45] was quiet and stable.
S1929 [N08E12] was quiet and stable.
S1936 [N07E26] was quiet and stable.
S1937 [S22E56] was quiet and stable.
S1939 [N08W48] was quiet and stable.
New region S1941 [S12E85] rotated into view with a large spot.
New region S1942 [S23W60] emerged with tiny spots.

Coronal mass ejections (CMEs)

September 22-24: 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

No obvious coronal holes are currently in or near Earth facing positions.

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 good. Propagation on long distance northeast-southwest paths is poor.

Forecast

The geomagnetic field is expected to be quiet on September 26-28.

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 higher resolution image) 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
11573 2012.09.15
2012.09.16
8 18 10 N15W56 0050 CAI DRI

area: 0030

11575 2012.09.17
2012.09.18
11 17 11 N08W16 0180 ESO CHO

area: 0320

S1924 2012.09.17   2   S26W45 0000   AXX  
11576 2012.09.18
2012.09.19
3 18 7 S21W09 0030 CRO DRO  
11581 2012.09.19
2012.09.25
3 10 4 N22E03 0020 CAO CRO area: 0050

location: N20E05

S1928 2012.09.20       N02W53           plage
S1929 2012.09.21   3 1 N08E12 0000   AXX  
S1930 2012.09.21       S16W57           plage
11577 2012.09.22 7 15 7 N09E03 0060 CSO CRO area: 0030
S1933 2012.09.22       N18W15           plage
S1934 2012.09.22       S17W29           plage
11579 2012.09.23
2012.09.24
3 8 2 S09E58 0180 CSO DHO area: 0320

location: S10E60

S1936 2012.09.23   1   N07E26 0000   AXX  
11578 2012.09.24 3 5 1 N21W04 0010 BXO BXO  
S1937 2012.09.24   2 1 S22E56 0010   AXX  
11580 2012.09.24
2012.09.25
3 6 5 N17E67 0030 CRO DRO location: N16E69
S1939 2012.09.24   3   N08W48 0000   BXO  
S1940 2012.09.24       N28E08         plage
S1941 2012.09.25   1 1 S12E85 0400   HHX    
S1942 2012.09.25   2   S23W60 0000   BXO    
Total spot count: 41 111 50  
Sunspot number: 121 261 160  (total spot count + 10 * number of spotted regions)
Weighted SN: 72 156 95  (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): 73 91 88 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)
2011.05 95.8 41.5 47.6 (+5.8) 8.94
2011.06 95.8 37.0 53.2 (+5.6) 8.06
2011.07 94.2 43.8 57.2 (+4.0) 8.16
2011.08 101.7 50.6 59.0 (+1.8) 7.26
2011.09 133.8 78.0 59.5 (+0.5) 12.27
2011.10 137.3 88.0 59.9 (+0.4) 8.28
2011.11 153.5 96.7 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) 8.81
2012.03 114.7 64.3 (67.3 projected, +0.4) 16.08
2012.04 113.0 55.2 (66.5 projected, -0.8) 10.10
2012.05 121.5 69.0 (64.4 projected, -2.1) 7.06
2012.06 119.6 64.5 (63.6 projected, -0.8) 10.08
2012.07 133.9 66.5 (64.6 projected, +1.0) 13.90
2012.08 115.4 63.1 (67.2 projected, +2.6) 7.96
2012.09 120.2 (1)  68.6 (2A) / 82.4 (2B) / 60.5 (2C) (70.0 projected, +2.8) (9.21)

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) Month average to date. 2C) STAR SDO 1K Wolf number month to date.
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.