Last major update issued on July 6, 2010 at 03:20 UTC.
[Solar and geomagnetic data - last month (updated daily)]
[Solar wind and electron fluence charts (updated daily)
[Solar cycles 21-24 (last update July 2, 2010)]
[Solar cycles 1-20]
[Graphical comparison of cycles 21, 22, 23 and 24 (last update July 3, 2010)]
[Graphical comparison of cycles 10, 12, 13, 14, 16 and 24 (last update July 4, 2010)]
[Historical solar and geomagnetic data charts 1954-2006 (last update April 5, 2007)]
[Archived reports (last update July 3, 2010)]
The geomagnetic field was quiet on July 5. Solar wind speed ranged between 405 and 523 km/s.
Solar flux measured at 20h UTC on 2.8 GHz was 72.7. The planetary A index was 5 (STAR Ap - based on the mean of three hour interval ap indices: 4.8). Three hour interval K indices: 21111112 (planetary), 11101112 (Boulder).
The background x-ray flux is at the class A9 level.
At midnight there were 2 spotted regions on the visible solar disk.
Region 11084 was quiet and stable.
New region 11086 emerged in the northwest quadrant on July 4 and was numbered the next day by NOAA/SWPC.
A region 2-3 days behind the northeast limb was the source of a CME and a subsequent increase in the background x-ray flux during the last quarter of the day.
July 3-5: No obviously Earth directed CMEs were seen in LASCO or STEREO images.
Coronal hole 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 coronal hole (CH412) was in an Earth facing position on July 5-6.
Image courtesy of SDO (NASA) and the AIA consortium. Annotations are my own. The darkest areas on the solar disk are likely coronal holes.
Long distance low and medium frequency (below 2 MHz) propagation along paths north of due west over high and upper middle latitudes is poor. Propagation on long distance northeast-southwest paths is poor to fair.
The geomagnetic field is expected to be quiet on July 6-8. On July 9-10 there's a chance of unsettled conditions due to effects from CH412.
|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/SWPC. 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 SWPC or where SWPC has observed no spots. SWPC active region numbers in the table below and in the active region map above are the historic SWPC/USAF numbers.
|Active region||Date numbered||Spot count||Location at midnight||Area||Classification||SDO (NASA) / AIA 4500
|11086||2010.07.05||2||4||N18W53||0010||BXO||CSO||formerly region S785|
|Total spot count:||3||5|
|Month||Average measured solar flux||International sunspot number (SIDC)||Smoothed sunspot number||Average ap
cycle 23 sunspot max.
|2008.07||65.7 (SF minimum)||0.5||2.8 (-0.4)|
|2009.07||68.2||3.2||3.6 (+0.9)||5.49 / 4.55|
|2009.08||67.3||0.0||4.8 (+1.2)||5.70 / 4.89|
|2009.09||70.5||4.3||6.2 (+1.4)||3.88 / 3.61|
|2009.10||72.6||4.8||7.1 (+0.9)||3.66 / 3.56|
|2009.11||73.6||4.1||7.6 (+0.5)||2.45 / 2.63|
|2009.12||76.7||10.8||8.3 (+0.6)||1.41 / 1.92|
|2010.01||81.1||13.2||(9.2 predicted, +1.0)||2.93 / 3.07|
|2010.02||84.7||18.8||(10.4 predicted, +1.2)||4.15 / 4.61|
|2010.03||83.4||15.4||(12.1 predicted, +1.7)||4.58 / 4.65|
|2010.04||75.9||7.9||(13.7 predicted, +1.6)||10.22 / 10.24|
|2010.05||73.8||8.8||(15.0 predicted, +1.3)||9.18 / 8.15|
|2010.06||72.5||13.5||(16.4 predicted, +1.4)||8.17|
|2010.07||72.6 (1)||2.2 (2)||(18.0 predicted, +1.6)||(7.65)|
1) Running average based on the
daily 20:00 UTC observed solar flux
value at 2800 MHz.
2) Current impact on the monthly sunspot number based on the Boulder (NOAA/SWPC) sunspot number (accumulated daily sunspots / month days). The official international sunspot number is typically 30-50% lower.
3) Running average based on the daily SWPC ap indices. Values in red are based on the official NGDC ap indices.
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.