Last major update issued on November 7, 2005 at 05:10 UTC.
geomagnetic data - last month (updated daily)]
[Solar wind and electron fluence charts (updated daily)]
[Solar cycles 21-23 (last update October 2, 2005)]
[Solar cycles 1-20]
[Graphical comparison of cycles 21, 22 and 23 (last update October 2, 2005)]
[Graphical comparison of cycles 2, 10, 13, 17, 20 and 23 (last update October 2, 2005)]
[Historical solar and geomagnetic data charts 1954-2004 (last update February 1, 2005)]
[Archived reports (last update November 2, 2005)]
The geomagnetic field was quiet to unsettled on November 6. Solar wind speed ranged between 575 and 695 (all day average 601) km/sec under the influence of a high speed stream from CH195.
Solar flux measured at 20h UTC on 2.8 GHz was 81.7. The planetary
index was 10 (STAR Ap - based on the mean of three hour interval ap
Three hour interval K indices: 33222232 (planetary), 42233322 (Boulder).
The background x-ray flux is at the class A5 level.
At midnight there were 4 spotted regions on the visible solar disk. The solar flare activity level was low. A single C class event was recorded during the day.
Region 10819 was quiet and stable.
Region 10820 decayed slightly but could produce further C class flares. Flare: C1.1 at 14:43 UTC.
Spotted regions not numbered by NOAA/SEC:
[S602] This region emerged in the southeast quadrant on November 6. Location at midnight: S06E04.
[S603] A new region emerged in the northeast quadrant on November 6. Location at midnight: N05E16.
November 4-6: No obvious fully or partly Earth directed CMEs were observed.
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 recurrent coronal hole (CH196) in the northern hemisphere will likely be in an Earth facing position on November 7-8.
Processed SOHO/EIT 284 image at 01:06 UTC on November 7. The darkest areas on the solar disk are likely coronal holes.
The geomagnetic field is expected to be quiet to unsettled on November 7-8 and quiet on November 9. A high speed stream from CH196 could cause unsettled to active conditions on November 10-11.
|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 on long distance northeast-southwest paths is fair. Trans Atlantic propagation conditions are normally monitored every night on 1470 kHz. Dominant stations tonight: Radio Vibración (Venezuela).
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:||14||18|
flux at Earth
|International sunspot number||Smoothed sunspot number|
cycle 23 sunspot max.
|2005.05||99.3||42.6||(28.9 predicted, -2.7)|
|2005.06||93.7||39.6||(27.3 predicted, -1.6)|
|2005.07||96.4||39.9||(26.1 predicted, -1.2)|
|2005.08||90.5||36.4||(24.3 predicted, -1.8)|
|2005.09||91.1||22.1||(22.2 predicted, -2.1)|
|2005.10||77.0||8.5||(20.2 predicted, -2.0)|
|2005.11||78.4 (1)||5.6 (2)||(17.8 predicted, -2.4)|
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.