Last major update issued on March 1, 2004 at 03:55 UTC.
[Solar and geomagnetic data - last month (updated daily)]
[Solar wind and electron fluence charts (updated daily)]
[Solar cycles 21-23 (last update February 2, 2004)]
[Solar cycles 1-20]
[Graphical comparison of cycles 21, 22 and 23 (last update February 2, 2004)]
[Graphical comparison of cycles 2, 10, 13, 17, 20 and 23 (last update February 2, 2004)]
[Historical solar and geomagnetic data charts 1954-2003 (last update January 16, 2004)]
[Archived reports (last update February 26, 2004)]
The geomagnetic field was quiet to minor storm on February 29. Solar wind speed ranged between 538 and 960 km/sec under the influence of a high speed stream from coronal hole CH83.
Solar flux measured at 20h UTC on 2.8 GHz was 110.0. The planetary A
index was 21 (STAR Ap - based on the mean of three hour interval ap indices: 22.0).
Three hour interval K indices: 23355433 (planetary), 23354343 (Boulder).
The background x-ray flux is at the class B2 level.
At midnight there were 3 spotted regions on the visible disk. Solar flare activity was very low. No C class events was recorded during the day.
Region 10564 decayed quickly and lost about half of its penumbral area. The region will be rotating partly out of view
Region 10565 decayed and lost all trailing spots.
Region 10567 decayed in the trailing spot section, however, penumbra developed on a couple of spots west of the main penumbra.
February 27-29: No partly or fully earth directed CMEs observed.
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 well defined recurrent trans equatorial coronal hole (CH83) was in a geoeffective position on February 26-29.
Processed SOHO/EIT 284 image at 19:06 UTC on February 29. The darkest areas on the solar disk are likely coronal holes.
The geomagnetic field is expected to be unsettled to minor storm on March 1-2 due to a high speed stream from coronal hole CH83, quiet to active is likely on March 3.
Long distance low and medium frequency (below 2 MHz) propagation along east-west paths over high and upper middle latitudes is poor. Propagation along long distance north-south paths is fair to poor. [Trans Atlantic propagation conditions are currently monitored every night on 1470 kHz. Dominant station tonight: Radio Vibración (Venezuela). Only 4 stations from North America noted: 590 VOCM, 930 CJYQ, 1030 WBZ and 1510 WWZN].
|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.
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|
classification was DAI
at midnight, area 0350
classification was HAX
classification was DSO
|Total spot count:||41||34|
flux at Earth
|International sunspot number||Smoothed sunspot number|
cycle 23 sunspot max.
|2003.08||122.1||72.7||(59.4 predicted, -2.4)|
|2003.09||112.2||48.7||(57.6 predicted, -1.8)|
|2003.10||151.7||65.5||(54.9 predicted, -2.7)|
|2003.11||140.8||67.3||(52.2 predicted, -2.7)|
|2003.12||114.9||46.5||(49.6 predicted, -2.6)|
|2004.01||114.1||37.2||(45.4 predicted, -4.2)|
|2004.02||107.0 (1)||75.5 (2)||(40.8 predicted, -4.6)|
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 sources noted in solar links. All time references are to the UTC day. Comments and suggestions are always welcome.