Last major update issued on October 27, 2010 at 03:40 UTC.
[Solar and geomagnetic data - last month (updated daily)]
[Solar wind and electron fluence charts (updated daily)
[Solar cycles 21-24 (last update October 2, 2010)]
[Solar cycles 1-20]
[Graphical comparison of cycles 21, 22, 23 and 24 (last update
October 2, 2010)]
[Graphical comparison of cycles 10, 12, 13, 14, 16 and 24 (last update
October 2, 2010)]
[Historical solar and geomagnetic data charts 1954-2006 (last update April 5, 2007)]
[Archived reports from January 2003 (last update October
9, 2010)]
NEW [POES auroral activity level charts since October 2009]
The geomagnetic field was quiet to unsettled on October 26. Solar wind speed ranged between 495 and 640 km/s, under the influence of a high speed stream from CH426.
Solar flux measured at 20h UTC on 2.8 GHz was 86.1 (down 4.6 over the last solar rotation). The planetary A index was 8 (STAR Ap - based on the mean of three hour interval ap indices: 7.6). Three hour interval K indices: 32221222 (planetary), 32331221 (Boulder).
The background x-ray flux is at the class B1 level.
At midnight UTC the visible solar disk had 3 spotted regions.
Region 11115 was quiet and stable and is rotating over the southwest
limb.
Region 11117 saw lots of changes during the day. A large spot east of the
leader spot developed quickly and moved fast westwards eventually merging with
the leader spot and forming a large symmetrical penumbra. A large spot formed in
the western part of the trailing spot section. Magnetically the region appears
to be a little less complex than it was a day ago, however, there is still a
chance of an M class flare.
Flare: C1.1 at 01:13 UTC.
Region 11119 developed early in the day, then decayed and coudl soon
become spotless.
Flare: C1.0 at 08:14 UTC.
October 24-25: No obviously Earth directed CMEs were seen in LASCO or STEREO
images.
October 26: A CME was observed starting at about 09h UTC following
activity near region 11115. Although the CME will likely not reach Earth,
there's a chance of a glancing blow.
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 obvious coronal holes are currently in or near Earth facing positions.
Image courtesy of SDO (NASA) and the AIA consortium. Annotations are my own. 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 on October 27-28. On October 29 there's a slight chance of unsettled intervals should the CME observed on October 26 reach Earth.
| 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 (NASA) / AIA 4500 image |
Comment | |||
|---|---|---|---|---|---|---|---|---|---|---|
| SWPC | STAR | SWPC | STAR | Current | Previous | |||||
| 11113 | 2010.10.13 | 1 | N17W92 | 0060 | HSX |
 |
rotated out of view | |||
| 11115 | 2010.10.15 | 1 | 1 | S31W75 | 0120 | HSX | HSX |
 |
 |
|
| 11118 | 2010.10.19 | N14W31 | plage | |||||||
| 11117 | 2010.10.19 | 31 | 38 | N21W15 | 0120 | EHI | EHI |
 |
 |
area: 0600 |
| 11119 | 2010.10.19 | 1 | 1 | N22W49 | 0020 | AXX | AXX |
 |
 |
|
| S828 | 2010.10.25 | N22W61 | plage | |||||||
| Total spot count: | 34 | 40 | ||||||||
| SSN: | 74 | 70 | ||||||||
| 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 |
| 2009.07 | 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 (+1.7) | 4.58 / 4.65 |
| 2010.04 | 75.9 | 8.0 | (13.9 predicted, +1.6) | 10.22 / 10.24 |
| 2010.05 | 73.8 | 8.7 | (15.2 predicted, +1.3) | 9.18 / 8.15 |
| 2010.06 | 72.5 | 13.6 | (16.7 predicted, +1.5) | 8.17 / 6.85 |
| 2010.07 | 79.8 | 16.1 | (18.3 predicted, +1.6) | 6.31 / 5.15 |
| 2010.08 | 79.2 | 19.6 | (19.5 predicted, +1.2) | 8.49 / 7.77 |
| 2010.09 | 81.1 | 25.2 | (20.7 predicted, +1.2) | 5.33 |
| 2010.10 | 81.0 (1) | 29.3 (2A) / 34.9 (2B) | (23.1 predicted, +2.4) | (6.64) |
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.