Last major update issued on February 2, 2005 at 04:35 UTC.
geomagnetic data - last month (updated daily)]
[Solar wind and electron fluence charts (updated daily)]
[Solar cycles 21-23 (last update January 2, 2005)]
[Solar cycles 1-20]
[Graphical comparison of cycles 21, 22 and 23 (last update January 2, 2005)]
[Graphical comparison of cycles 2, 10, 13, 17, 20 and 23 (last update January 2, 2005)]
[Historical solar and geomagnetic data charts 1954-2004 (last update February 1, 2005)]
[Archived reports (last update February 1, 2005)]
The geomagnetic field was inactive to unsettled on February 1. Solar wind speed ranged between 484 and 600 km/sec.
Solar flux measured at 20h UTC on 2.8 GHz was 83.7. The planetary
index was 6 (STAR Ap - based on the mean of three hour interval ap
Three hour interval K indices: 30121222 (planetary), 30112321 (Boulder).
The background x-ray flux is at the class A3 level.
At midnight there were 2 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 10727 decayed slowly and quietly and will soon rotate out of view at the southwest limb.
January 30-February 1: No obvious fully or partly Earth directed CMEs were observed. A full halo CME observed during the afternoon and early evening on January 30 most likely had a backsided source. Another full halo CME observed near noon on February 1 had a source behind the northeast limb, possibly in returning old region 10720.
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 small recurrent coronal hole (CH143) in the southern hemisphere will likely rotate to a geoeffective position on February 3.
Processed SOHO/EIT 284 image at 01:06 UTC on February 2. The darkest areas on the solar disk are likely coronal holes.
The geomagnetic field is expected to be inactive to quiet on February 2-5. A low speed stream from coronal hole CH143 could reach Earth on February 6 and cause a few unsettled and active intervals.
|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) Material from a CME is likely to impact 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 poor to fair. Propagation along long distance north-south paths is very poor. Trans Atlantic propagation conditions are normally monitored every night on 1470 kHz. Dominant stations tonight: WLAM Lewiston ME and Radio Vibración (Venezuela). Quite a few stations from the easternmost parts of North America were heard on other frequencies, the best signals were coming from stations located on Newfoundland.
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|
|10727||2005.01.24||2||1||S09W68||0110||CAO||classification was HAX at midnight, area 0070|
area was 0040 at midnight
|Total spot count:||7||4|
flux at Earth
|International sunspot number||Smoothed sunspot number|
cycle 23 sunspot max.
|2004.08||109.6||40.9||(38.9 predicted, -1.4)|
|2004.09||103.1||27.7||(36.6 predicted, -2.3)|
|2004.10||105.9||48.4||(34.4 predicted, -2.2)|
|2004.11||113.2||43.7||(32.5 predicted, -1.9)|
|2004.12||94.5||17.9||(30.2 predicted, -2.3)|
|2005.01||102.2||31.3||(27.6 predicted, -2.6)|
|2005.02||83.7 (1)||1.0 (2)||(25.2 predicted, -2.4)|
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% less.
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.