Last major update issued on June 29, 2005 at 04:25 UTC.
geomagnetic data - last month (updated daily)]
[Solar wind and electron fluence charts (updated daily)]
[Solar cycles 21-23 (last update June 4, 2005)]
[Solar cycles 1-20]
[Graphical comparison of cycles 21, 22 and 23 (last update June 4, 2005)]
[Graphical comparison of cycles 2, 10, 13, 17, 20 and 23 (last update June 4, 2005)]
[Historical solar and geomagnetic data charts 1954-2004 (last update February 1, 2005)]
[Archived reports (last update June 21, 2005)]
The geomagnetic field was quiet on June 28. Solar wind speed ranged between 354 and 428 (all day average 378) km/sec.
Solar flux measured at 20h UTC on 2.8 GHz was 80.0. The planetary
index was 5 (STAR Ap - based on the mean of three hour interval ap
Three hour interval K indices: 11112222 (planetary), 12212222 (Boulder).
The background x-ray flux is at the class A7 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 10781 was quiet and didn't change significantly.
June 26: A symmetric full halo CME was observed in LASCO C3 images beginning at 08:18 UTC. No relevant activity was
observed on the visible disk during the hours before this observation, thus the source of the CME was most likely backsided.
June 27-28: No obvious fully or partly Earth directed CMEs were observed in available LASCO images.
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 large trans equatorial coronal hole (CH173) will be in an Earth facing position on June 28-30.
Processed SOHO/EIT 284 image at 01:06 UTC on June 29. The darkest areas on the solar disk are likely coronal holes.
The geomagnetic field is expected to be quiet on June 29-30 while a high speed stream from CH173 is likely to arrive on July 1 and cause unsettled to minor or major storm conditions that day and on July 2-3.
|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. Propagation along long distance north-south paths is poor. Trans Atlantic propagation conditions are normally monitored every night on 1470 kHz. Dominant stations tonight: Radio Cristal del Uruguay and Radio Vibración (Venezuela). There were signals on several other frequencies, however, most of them were weak or very weak.
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|
|10781||2005.06.27||10||5||N15E65||0090||EAO||classification was CAO at midnight, area 0050|
|Total spot count:||10||5|
flux at Earth
|International sunspot number||Smoothed sunspot number|
cycle 23 sunspot max.
|2004.12||94.5||17.9||(34.8 predicted, -0.5)|
|2005.01||102.2||31.3||(32.8 predicted, -2.0)|
|2005.02||97.2||29.1||(30.4 predicted, -2.4)|
|2005.03||89.9||24.8||(28.8 predicted, -1.6)|
|2005.04||86.0||24.4||(26.9 predicted, -1.9)|
|2005.05||99.3||42.6||(24.3 predicted, -2.6)|
|2005.06||93.6 (1)||54.7 (2)||(22.8 predicted, -1.5)|
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.