Last major update issued on April 18, 2007 at 03:05 UTC.
geomagnetic data - last month (updated daily)]
[Solar wind and electron fluence charts (updated daily)
[Solar cycles 21-23 (last update April 10, 2007)]
[Solar cycles 1-20]
[Graphical comparison of cycles 21, 22 and 23 (last update April 10, 2007)]
[Graphical comparison of cycles 2, 10, 13, 17, 20 and 23 (last update April 10, 2007)]
[Historical solar and geomagnetic data charts 1954-2006 (last update April 5, 2007)]
[Archived reports (last update April 7, 2007)]
The geomagnetic field was quiet to unsettled on April 17. Solar wind speed ranged between 288 and 351 km/s (average speed was 327 km/s, increasing 15 km/s over the previous day). A low speed stream from CH265 arrived early in the day.
Solar flux measured at 20h UTC on 2.8 GHz was 69.2. The planetary A index was 8 (STAR Ap - based on the mean of three hour interval ap indices: 8.4). Three hour interval K indices: 11122233 (planetary), 01233322 (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.
April 15-17: 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 small trans equatorial recurrent coronal hole (CH265) was in an Earth facing position on April 13-14. Another recurrent trans equatorial coronal hole (CH266) will face Earth on April 16-19.
Processed SOHO/EIT 195 image at 23:12 UTC on April 17. The darkest areas on the solar disk are likely coronal holes.
The geomagnetic field is expected to be quiet to unsettled on April 18 due to effects from CH265. A high speed stream from CH266 could cause unsettled to minor storm conditions on April 19-21.
|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.
|Active region||Date numbered||SEC
|Location at midnight||Area||Classification||Comment|
formerly region S698
|Total spot count:||2||0|
flux at Earth
|International sunspot number||Smoothed sunspot number|
cycle 23 sunspot max.
|2006.10||74.3||10.4||(14.3 predicted, -1.3)|
|2006.11||86.3||21.5||(12.6 predicted, -1.7)|
|2006.12||84.5||13.6||(11.6 predicted, -1.0)|
|2007.01||83.3||16.9||(11.2 predicted, -0.4)|
|2007.02||77.7||10.6||(11.1 predicted, -0.1)|
|2007.03||72.2||4.8||(11.3 predicted, +0.2)|
|2007.04||70.0 (1)||2.3 (2)||(11.9 predicted, +0.6)|
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% lower.