Solar Terrestrial Activity Report

Last major update issued on January 27, 2011 at 05:45 UTC.

[Solar and geomagnetic data - last month (updated daily)]
[Solar wind and electron fluence charts (updated daily)
[Solar cycles 21-24 (last update January 2, 2011)]
[Solar cycles 1-20]
[Graphical comparison of cycles 21, 22, 23 and 24 (last update January 2, 2011)]
[Graphical comparison of cycles 10, 12, 13, 14, 16 and 24 (last update January 2, 2011)]
[Historical solar and geomagnetic data charts 1954-2006 (last update April 5, 2007)]
[Archived reports from January 2003 (last update January 1, 2011)]

[POES auroral activity level charts since October 2009]
Annotated geomagnetic activity charts - Carrington rotation 2104 [Nov-Dec.2010]- 2105 [Dec-Jan.2011] NEW

Recent activity

The geomagnetic field was quiet on January 26. Solar wind speed ranged between 280 and 319 km/s.

Solar flux measured at 20h UTC on 2.8 GHz was 80.0 (decreasing 2.9 over the last solar rotation). The planetary A index  was 3 (STAR Ap - based on the mean of three hour interval ap indices: 3.1). Three hour interval K indices: 11100111 (planetary), 11200220 (Boulder).

The background x-ray flux is at the class A7 level.

At midnight UTC the visible solar disk had 3 spotted regions.

Region 11147 was quiet and stable.
Region 11149 decayed further losing all trailing spots.

Spotted regions not numbered by NOAA/SWPC:
[S865] This region emerged in the northwest quadrant on January 26. Location at midnight: N11W31

Coronal mass ejections (CMEs)

January 24-26: No obviously Earth directed CMEs were observed 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

No significant coronal holes are currently Earth facing. A trans equatorial area with weak corona may be numbered today.

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

Forecast

The geomagnetic field is expected to be quiet on January 27-28. On January 29-30 there's a chance of a few unsettled intervals due to a weak trans equatorial coronal hole.

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

(Click on image for higher resolution image with polarity overlay) Compare to the previous day's 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 Spot count Location at midnight Area Classification SDO / HMI continuum
image with polarity overlay
Comment
SWPC STAR SWPC STAR Current Previous
11147 2011.01.15 1 1 N24W77 0150 HSX HSX area: 0100
11149 2011.01.21 4 4 N17W77 0130 DSO HSX area: 0130
S865 2011.01.26   1 N11W31 0010   AXX    
Total spot count: 5 6  
Sunspot number: 25 36  

Monthly solar cycle data

Month Average measured solar flux International sunspot number (SIDC) Smoothed sunspot number Average ap
(3)
2008.07 65.7 (SF minimum) 0.5 2.8 (-0.4)  
2008.12 69.2 0.8 1.7 (-)
sunspot minimum
3.25
2009.10 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 (+1.7) 4.58 / 4.65
2010.04 75.9 8.0 14.0 (+1.7) 10.22 / 10.24
2010.05 73.8 8.7 15.5 (+1.5) 9.18 / 8.15
2010.06 72.5 13.6 16.4 (+0.9) 8.17 / 6.85
2010.07 79.8 16.1 (17.0 predicted, +0.6) 6.31 / 5.15
2010.08 79.2 19.6 (17.9 predicted, +0.9) 8.49 / 7.77
2010.09 81.1 25.2 (19.0 predicted, +1.1) 5.33 / 5.45
2010.10 81.6 23.5 (20.7 predicted, +1.7) 6.07 / 6.27
2010.11 82.5 21.6 (23.0 predicted, +2.3) 4.80
2010.12 84.2 14.5 (25.3 predicted, +2.3) 3.41
2011.01 84.0 (1) 29.1 (2A) / 34.7 (2B) (27.7 predicted, +2.4) (4.51)

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 preliminary 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.

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