Last major update issued on May 29, 2006 at 04:00 UTC.
[Solar and
geomagnetic data - last month (updated daily)]
[Solar wind and
electron fluence charts (updated daily)]
[Solar cycles 21-23
(last update April 1, 2006)]
[Solar cycles 1-20]
[Graphical comparison
of cycles 21, 22 and 23 (last update April 1, 2006)]
[Graphical
comparison of cycles 2, 10, 13, 17, 20 and 23 (last update April 1, 2006)]
[Historical solar and
geomagnetic data charts 1954-2005 (last update March 3, 2006)]
[Archived reports (last update
May 3, 2006)]
The geomagnetic field was quiet to unsettled on May 28. Solar wind speed ranged between 279 and 333 (all day average 309) km/sec under the influence of a weak low speed, high density disturbance.
Solar flux measured at 20h UTC on 2.8 GHz was 84.7. The planetary A index
was 7 (STAR Ap - based on the mean of three hour interval ap
indices: 6.9).
Three hour interval K indices: 22112123 (planetary), 23220112 (Boulder).
The background x-ray flux is at the class A5 level.
At midnight there were 4 spotted regions on the visible solar disk. The solar flare activity level was very low. No C class events were recorded during the day.
Region 10886 decayed slowly and quietly.
Region 10887 developed penumbra on the leader spot.
Region 10889 was quiet and stable.
New region 10890 emerged in the southwest quadrant on May 27 and was
numbered the next day by NOAA/SEC. The region developed slowly on May 28 with
penumbra forming on both polarities.
May 27-28: No partly or fully Earth directed CMEs were observed in
limited LASCO
imagery.
May 25/26: A very faint halo CME was observed in LASCO images early on
May 26. Its source was likely a B class event in region 10885 late on May 25.
This CME could reach Earth on May 29.
Coronal hole history (since late October 2002)
Compare today's report with the situation one solar rotation ago:
28 days ago
27 days ago
26 days ago
A recurrent trans equatorial coronal hole (CH226) will likely rotate into an Earth facing position on May 29-30.
Processed SOHO/EIT 284 image at 19:06 UTC on May 26. The darkest areas on the solar disk are likely coronal holes.
The geomagnetic field is expected to be quiet to active on May 29-30 due to the possible arrival of a CME observed on May 25/26. Quiet to unsettled conditions are likely on May 31, becoming quiet to active on June 1-3 due to a high speed stream from CH226.
| 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.
Long distance low and medium frequency (below 2 MHz) propagation along east-west paths over high and upper middle latitudes is very poor. Propagation on long distance northeast-southwest paths is fair. Trans Atlantic propagation conditions are normally monitored every night on 1470 kHz. As is usual this time of the year Radio Cristal del Uruguay was the dominant signal. Stations from the São Paulo area were better than they've been in a long time with the best signals noted on 1230 and 1600 kHz.
Compare to the previous day's image.
Data for all numbered solar regions according to the Solar Region Summary provided by NOAA/SEC. 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 SEC or where SEC has observed no spots. SEC active region numbers in the table below and in the active region map above are the historic SEC/USAF numbers.
| Active region | Date numbered | SEC spot count |
STAR spot count |
Location at midnight | Area | Classification | Comment |
|---|---|---|---|---|---|---|---|
| 10884 | 2006.05.19 | S12W70 | plage | ||||
| 10885 | 2006.05.20 | S12W67 | plage | ||||
| 10886 | 2006.05.23 | 5 | 3 | N07W24 | 0030 | CSO | |
| 10887 | 2006.05.26 | 5 | 3 | S12E38 | 0030 | CAO | |
| 10888 | 2006.05.26 | 2 | N05W91 | 0060 | CAO | rotated out of view | |
| 10889 | 2006.05.27 | 6 | 3 | S02W06 | 0040 | CSO | |
| 10890 | 2006.05.28 | 10 | 10 | S14W29 | 0040 | CSO | formerly region S657 |
| Total spot count: | 28 | 19 | |||||
| SSN: | 78 | 59 | |||||
| Month | Average solar flux at Earth |
International sunspot number | Smoothed sunspot number |
|---|---|---|---|
| 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) |
| 2005.02 | 97.2 | 29.2 | 33.9 (-0.7) |
| 2005.03 | 89.9 | 24.5 | 33.5 (-0.4) |
| 2005.04 | 86.0 | 24.2 | 31.6 (-1.9) |
| 2005.05 | 99.3 | 42.7 | 28.9 (-2.7) |
| 2005.06 | 93.7 | 39.3 | 28.8 (-0.1) |
| 2005.07 | 96.4 | 40.1 | 29.1 (+0.3) |
| 2005.08 | 90.5 | 36.4 | 27.4 (-1.7) |
| 2005.09 | 91.1 | 21.9 | 25.8 (-1.6) |
| 2005.10 | 77.0 | 8.5 | 25.5 (-0.3) |
| 2005.11 | 86.3 | 18.0 | (24.5 predicted, -1.0) |
| 2005.12 | 90.7 | 41.2 | (21.8 predicted, -2.7) |
| 2006.01 | 83.4 | 15.4 | (18.7 predicted, -3.1) |
| 2006.02 | 76.5 | 4.7 | (15.6 predicted, -3.1) |
| 2006.03 | 75.4 | 10.8 | (13.4 predicted, -2.2) |
| 2006.04 | 89.0 | 30.2 | (12.7 predicted, -0.7) |
| 2006.05 | 81.0 (1) | 34.7 (2) | (12.2 predicted, -0.5) |
1) Running average based on the
daily 20:00 UTC observed solar flux
value at 2800 MHz.
2) Unofficial, accumulated value based on the Boulder (NOAA/SEC)
sunspot number. The official international sunspot number is typically
30-50% lower.
This report has been prepared by Jan Alvestad. It is based partly on my own observations and analysis, and partly on data from some of these solar data sources. All time references are to the UTC day. Comments and suggestions are always welcome.
| [DX-Listeners' Club] |