Last major update issued on January 30, 2011 at 07:15 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
The geomagnetic field was quiet to unsettled on January 29. Solar wind speed ranged between 287 and 335 km/s.
Solar flux measured at 20h UTC on 2.8 GHz was 81.4 (decreasing 9.7 over the last solar rotation). The planetary A index was 4 (STAR Ap - based on the mean of three hour interval ap indices: 3.9). Three hour interval K indices: 31011101 (planetary), 21121201 (Boulder).
The background x-ray flux is at the class A6 level.
At midnight UTC the visible solar disk had 1 spotted region.
Region 11150 was mostly unchanged during the day. Early on January 30 many new small spots have become visible.
January 27-29: 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 large recurrent coronal hole (CH435) in the northern hemisphere will rotate into an Earth facing position on January 30-February 1.
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 to fair.
The geomagnetic field is expected to be quiet to unsettled on January 29-30 due to an area of weak corona which was Earth facing on January 25-26. Quiet conditions are likely on January 31 and February 1. A high speed stream from CH435 could cause unsettled to minor storm conditions on February 2-4.
| 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.
(Click on image for higher resolution image) 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 | |||||
| 11151 | 2011.01.26 | 1 | N11W71 | 0005 | AXX |
 |
spotless | |||
| 11150 | 2011.01.26 | 6 | 7 | S22E50 | 0020 | BXO | BXO |
 |
 |
|
| Total spot count: | 7 | 7 | ||||||||
| Sunspot number: | 27 | 17 | ||||||||
| 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 | 83.7 (1) | 30.8 (2A) / 33.0 (2B) | (27.7 predicted, +2.4) | (4.43) |
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.
