Last major update issued on January 19, 2011 at 05:30 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 chart - Carrington rotation 2104 - NEW]
The geomagnetic field was quiet on January 18. Solar wind speed ranged between 402 and 464 km/s, slowly decreasing until about 16h UTC when a high speed stream associated with CH434 began to dominate the solar wind.
Solar flux measured at 20h UTC on 2.8 GHz was 81.0 (increasing 3.3 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: 20100102 (planetary), 21210122 (Boulder).
The background x-ray flux is at the class A6 level.
At midnight UTC the visible solar disk had 2 spotted regions.
Region 11147 developed early in the day, then began to decay again.
Region 11148 displayed slow development early in the day, while slow
decay was observed during the latter half of the day.
January 16-18: No obviously Earth directed CMEs were observed in LASCO or STEREO images.
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 poorly defined coronal hole (CH434) was in an Earth facing position on January 15-16.
The darkest areas on the solar disk are likely coronal holes.
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.
The geomagnetic field is expected to be quiet on January 19-20 with a chance of occasional unsettled intervals due to effects from CH434. Quiet conditions are likely on January 21-22.
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.
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 / HMI continuum image |
Comment | |||
---|---|---|---|---|---|---|---|---|---|---|
SWPC | STAR | SWPC | STAR | Current | Previous | |||||
11146 | 2011.01.10 | N23W61 | plage | |||||||
11147 | 2011.01.15 | 12 | 9 | N26E37 | 0160 | CSO | CSO | |||
11148 | 2011.01.16 | 2 | 3 | S28W46 | 0030 | CRO | CRO |
|
||
Total spot count: | 14 | 12 | ||||||||
Sunspot number: | 34 | 32 |
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 | 84.5 (1) | 20.8 (2A) / 35.8 (2B) | (27.7 predicted, +2.4) | (5.03) |
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.