Last major update issued on January 25, 2007 at 05:50 UTC. The next update will be on January 29.
geomagnetic data - last month (updated daily)]
[Solar wind and electron fluence charts (updated daily)
[Solar cycles 21-23 (last update January 11, 2007)]
[Solar cycles 1-20]
[Graphical comparison of cycles 21, 22 and 23 (last update January 11, 2007)]
[Graphical comparison of cycles 2, 10, 13, 17, 20 and 23 (last update January 11, 2007)]
[Historical solar and geomagnetic data charts 1954-2005 (last update March 3, 2006)]
[Archived reports (last update December 18, 2006)]
The geomagnetic field was very quiet on January 24. Solar wind speed ranged between 336 and 394 km/s (all day average 352 km/s - decreasing 55 km/s compared to the previous day).
Solar flux measured at 20h UTC on 2.8 GHz was 80.4. The planetary A index was 1 (STAR Ap - based on the mean of three hour interval ap indices: 1.3). Three hour interval K indices: 00001101 (planetary), 00101210 (Boulder).
The background x-ray flux is at the class A3 level.
At midnight there was 1 spotted region on the visible solar disk. The solar flare activity level was very low. No C class events were recorded during the day.
Region 10939 decayed significantly and was mostly quiet.
An active region just behind the central east limb will likely rotate into view today or tomorrow. This region produced a long duration B9 event peaking at 14:52 UTC on January 24. The event was associated with a bright CME observed over most of the east limbs. The region may be capable of M class flaring.
January 22-24: No obvious partly or fully Earth directed CMEs were detected in LASCO imagery.
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 recurrent coronal hole (CH256) in the southern hemisphere will likely rotate into an Earth facing position on January 26-27.
Processed SOHO/EIT 195 image at 17:48 UTC on January 24. The darkest areas on the solar disk are likely coronal holes.
The geomagnetic field is expected to be mostly quiet on January 25-28. A high speed stream from CH256 will likely cause unsettled to minor storm conditions on January 29-30.
|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.
Monitoring has been temporarily suspended (as of January 1, 2007).
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
|Location at midnight||Area||Classification||Comment|
|10939||2007.01.20||5||5||S04W69||0160||DAO||classification was DSO at midnight, area 0050|
|Total spot count:||5||5|
flux at Earth
|International sunspot number||Smoothed sunspot number|
cycle 23 sunspot max.
|2006.07||75.7||12.2||(15.0 predicted, -1.3)|
|2006.08||79.0||12.9||(14.9 predicted, -0.1)|
|2006.09||77.8||14.5||(14.7 predicted, -0.2)|
|2006.10||74.3||10.4||(13.5 predicted, -1.2)|
|2006.11||86.3||21.5||(12.1 predicted, -1.4)|
|2006.12||84.5||13.6||(11.7 predicted, -0.4)|
|2007.01||83.2 (1)||23.7 (2)||(11.9 predicted, +0.2)|
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.