Last major update issued on August 2, 2007 at 02:40 UTC. /Charts updated on August 17, text and images will be updated on August 18./
geomagnetic data - last month (updated daily)]
[Solar wind and electron fluence charts (updated daily)
[Solar cycles 21-23 (last update July 23, 2007)]
[Solar cycles 1-20]
[Graphical comparison of cycles 21, 22 and 23 (last update July 23, 2007)]
[Graphical comparison of cycles 2, 10, 13, 17, 20 and 23 (last update July 23, 2007)]
[Historical solar and geomagnetic data charts 1954-2006 (last update April 5, 2007)]
[Archived reports (last update July 1, 2007)]
The geomagnetic field was quiet to active on August 1. Solar wind speed ranged between 476 and 700 km/s (average speed was 575 km/s, increasing 44 km/s over the previous day) under the influence of a high speed stream from CH281
Solar flux measured at 20h UTC on 2.8 GHz was 68.4. The planetary A index was 17 (STAR Ap - based on the mean of three hour interval ap indices: 15.6). Three hour interval K indices: 24432233 (planetary), 35542223 (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.
July 30 - August 1: No obvious fully or partly Earth directed CMEs were observed.
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 (CH282) in the southern hemisphere will likely rotate into an Earth facing position on August 2-3.
Processed SOHO/EIT 195 image at 00:00 UTC on August 2. The darkest areas on the solar disk are likely coronal holes.
Long distance low and medium frequency (below 2 MHz) propagation along east-west paths over high and upper middle latitudes is very poor. Propagation on long distance northeast-southwest paths is fair.
Monitoring remarks from a location near N58E06: August 1: Several stations from Argentina had fair to good signals during the night while stations from Brazil were mostly absent. Fair to good signals were noted from several North American stations including 590 VOCM, 800 VOWR, 1010 WINS, 1070 CBA, 1130 WBBR and 1510 WWZN.
The geomagnetic field is expected to be quiet to unsettled on August 2 due to effects from CH281. Quiet conditions could return on August 3-5, then become quiet to active again on August 6-7 due to a high speed stream from CH282.
|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.
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.
|2007.02||77.7||10.6||(11.6 predicted, -0.4)|
|2007.03||72.2||4.8||(11.1 predicted, -0.5)|
|2007.04||72.4||3.7||(10.8 predicted, -0.3)|
|2007.05||74.4||11.7||(10.4 predicted, -0.4)|
|2007.06||73.7||12.0||(10.3 predicted, -0.1)|
|2007.07||71.6||10.0||(10.5 predicted, +0.2)|
|2007.08||68.4 (1)||0.0 (2)||(11.0 predicted, +0.5)|
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.