Solar Terrestrial Activity Report

Last major update issued on September 17, 2010 at 03:50 UTC.

[Solar and geomagnetic data - last month (updated daily)]
[Solar wind and electron fluence charts (updated daily)
[Solar cycles 21-24 (last update September 4, 2010)]
[Solar cycles 1-20]
[Graphical comparison of cycles 21, 22, 23 and 24 (last update September 4, 2010)]
[Graphical comparison of cycles 10, 12, 13, 14, 16 and 24 (last update September 4, 2010)]
[Historical solar and geomagnetic data charts 1954-2006 (last update April 5, 2007)]
[Archived reports (last update September 4, 2010)]

Recent activity

The geomagnetic field was quiet to unsettled on September 16. Solar wind speed ranged between 332 and 462 km/s under the influence of a coronal hole stream.

Solar flux measured at 20h UTC on 2.8 GHz was 82.5 (up 5.4 over the last solar rotation). The planetary A index  was 6 (STAR Ap - based on the mean of three hour interval ap indices: 6.4). Three hour interval K indices: 10101332 (planetary), 10112332 (Boulder).

The background x-ray flux is at the class B2 level.

At midnight UTC the visible solar disk had 2 spotted regions.

Region 11106 developed slowly with some positive polarity flux emerging inside the trailing negative polarity area. C flares are possible.
New region 11108 rotated fully into view at the southeast limb. C flares and minor M class flares are possible.

Coronal mass ejections (CMEs)

September 14-16: No obviously Earth directed CMEs were seen in LASCO or STEREO images.

Coronal holes

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

A large recurrent coronal hole (CH422) in the northern hemisphere will likely be Earth facing on September 18-20.

Image courtesy of SDO (NASA) and the AIA consortium. Annotations are my own. The darkest areas on the solar disk are likely coronal holes.

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 unsettled on September 17 and quiet on September 18-19. A high speed stream from CH422 could cause quiet to minor storm conditions on September 21-23.

Coronal holes (1) Coronal mass ejections (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 (Recent map)

Compare to the previous day's image

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 Spot count Location at midnight Area Classification SDO (NASA) / AIA 4500
image
Comment
SWPC STAR SWPC STAR Current Previous
S811 2010.09.09     S33W54           plage
11106 2010.09.11 21 31 S20E05 0090 FSO FSI  
11107 2010.09.12     N33E10           plage
S814 2010.09.13     S30E41           plage
11108 2010.09.16 5 5 S28E69 0290 CKO DKO formerly region S815
Total spot count: 26 36  
SSN: 46 56  

Monthly solar cycle data

Month Average measured solar flux International sunspot number (SIDC) Smoothed sunspot number Average ap
(3)
2000.04 184.2 125.5 120.8
cycle 23 sunspot max.
 
2000.07 202.3 170.1 119.8  
2001.12 235.1 132.2 114.6 (-0.9)  
2008.07 65.7 (SF minimum) 0.5 2.8 (-0.4)  
2008.12 69.2 0.8 1.7 (-)
sunspot minimum
3.25
2009.06 68.6 2.9 2.7 (+0.4) 5.22
2009.07 68.2 3.2 3.6 (+0.9) 5.49 / 4.55
2009.08 67.3 0.0 4.8 (+1.2) 5.70 / 4.89
2009.09 70.5 4.3 6.2 (+1.4) 3.88 / 3.61
2009.10 72.6 4.8 7.1 (+0.9) 3.66 / 3.56
2009.11 73.6 4.1 7.6 (+0.5) 2.45 / 2.63
2009.12 76.7 10.8 8.3 (+0.7) 1.41 / 1.92
2010.01 81.1 13.2 9.3 (+1.0) 2.93 / 3.07
2010.02 84.7 18.8 10.6 (+1.3) 4.15 / 4.61
2010.03 83.4 15.4 (12.3 predicted, +1.7) 4.58 / 4.65
2010.04 75.9 7.9 (13.9 predicted, +1.6) 10.22 / 10.24
2010.05 73.8 8.8 (15.2 predicted, +1.3) 9.18 / 8.15
2010.06 72.5 13.5 (16.6 predicted, +1.4) 8.17 / 6.85
2010.07 79.8 16.1 (18.3 predicted, +1.7) 6.31 / 5.15
2010.08 79.2 19.6 (19.5 predicted, +1.2) 8.49 / 7.77
2010.09 78.4 (1) 15.4 (2A) / 28.9 (2B) (20.7 predicted, +1.2) (5.20)

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 international sunspot number is typically 30-50% lower. 2B) Month average to date.
3) Running average based on the daily SWPC ap indices. Values in red are based on the official NGDC 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.