Last major update issued on June 19, 2005 at 05:40 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 4, 2005)]
The geomagnetic field was very quiet to unsettled on June 18. Solar wind speed ranged between 457 and 643 km/sec.
Solar flux measured at 20h UTC on 2.8 GHz was 90.0. The planetary
index was 7 (STAR Ap - based on the mean of three hour interval ap
Three hour interval K indices: 12312221 (planetary), 23312121 (Boulder).
The background x-ray flux is at the class B1 level.
At midnight there were 2 spotted regions on the visible solar disk. The solar flare activity level was low. A total of 5 C class events was recorded during the day.
Region 10779 was mostly unchanged. Flares: C1.0 at 20:34 and C1.8 at 23:11 UTC.
Region 10780 developed slowly and produced a number of flares and sub flares. Flares: C1.6 at 00:26, C1.4 at 08:27 and C1.0 at 11:49 UTC.
June 16-18: 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
No obvious coronal holes are currently in or near Earth facing positions.
Processed SOHO/EIT 284 image at 01:06 UTC on June 6. The darkest areas on the solar disk are likely coronal holes.
The geomagnetic field is expected to be quiet to unsettled on June 19-22.
|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 very 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). A few stations from Brazil, Argentina and Uruguay were noted on other frequencies.
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|
|10779||2005.06.15||24||24||S18W32||0460||EKI||classification was EKO at midnight|
area was 0040 at midnight,
|Total spot count:||30||30|
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||101.0 (1)||46.1 (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.