Last major update issued on June 22, 2007 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 3, 2007)]
[Solar cycles 1-20]
[Graphical comparison of cycles 21, 22 and 23 (last update June 3, 2007)]
[Graphical comparison of cycles 2, 10, 13, 17, 20 and 23 (last update June 3, 2007)]
[Historical solar and geomagnetic data charts 1954-2006 (last update April 5, 2007)]
[Archived reports (last update May 18, 2007)]
The geomagnetic field was quiet to active on June 21. Solar wind speed ranged between 348 and 553 km/s (average speed was 441 km/s, increasing 10 km/s over the previous day). A high speed stream from CH273 arrived at approximately 08h UTC.
Solar flux measured at 20h UTC on 2.8 GHz was 65.5. The planetary A index was 14 (STAR Ap - based on the mean of three hour interval ap indices: 13.5). Three hour interval K indices: 12333334 (planetary), 12233234 (Boulder).
The background x-ray flux is below the class A1 level.
At midnight the visible solar disk was spotless. The solar flare activity level was very low. No C class events were recorded during the day.
June 19-21: No obvious fully or partially Earth directed CMEs were observed 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 (CH273) in the southern hemisphere was in an Earth facing position on June 17-19. A small trans equatorial coronal hole (CH274) will rotate into an Earth facing position on June 22.
Processed SOHO/EIT 195 image at 00:00 UTC on June 22. The darkest areas on the solar disk are likely coronal holes.
The geomagnetic field is expected to be quiet to active on June 22 due to a high speed stream from CH273 and quiet to unsettled on June 23-24. Some unsettled and active intervals are possible late on June 25 and on June 26 due to effects from CH274.
|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.
Daily monitoring will not resume until a local noise problem (related to construction work on a neighboring property) has been fixed. Occasional monitoring reports will be submitted when propagation is good.
April 8, 2007: Stations from the Canadian Atlantic provinces had strong signals during the night. Some stations from the northeastern USA and from Florida did well too, in particular 1510 WWZN was impressive.
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|
|Total spot count:||0||0|
flux at Earth
|International sunspot number||Smoothed sunspot number|
cycle 23 sunspot max.
|2006.12||84.5||13.6||(12.1 predicted, -0.6)|
|2007.01||83.3||16.9||(11.7 predicted, -0.4)|
|2007.02||77.7||10.6||(11.1 predicted, -0.6)|
|2007.03||72.2||4.8||(10.7 predicted, -0.4)|
|2007.04||72.4||3.7||(10.9 predicted, +0.2)|
|2007.05||74.4||11.7||(11.0 predicted, +0.1)|
|2007.06||75.1 (1)||16.4 (2)||(11.3 predicted, +0.3)|
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.