Last major update issued on December 10, 2011 at 04:50 UTC.
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The geomagnetic field was quiet on December 9. Solar wind speed ranged between 274 and 373 km/s. The leading edge of a high speed stream, probably from CH487, was observed arriving at ACE near 21:30 UTC. Solar wind speed is slowly increasing early on December 10.
Solar flux measured at 20h UTC on 2.8 GHz was 143.5 (decreasing 25.3 over the last solar rotation). The planetary A index was 3 (STAR Ap - based on the mean of three hour interval ap indices: 3.0). Three hour interval K indices: 00112101 (planetary), 00112211 (Boulder).
The background x-ray flux is at the class B4 level.
At midnight UTC the visible solar disk had 14 spotted regions (in 2K resolution SDO images).
Region 11364 [N19W57] decayed slowly and quietly.
Region 11365 [N20W76] was quiet and stable.
Region 11366 [N19W14] was quiet and stable.
Region 11367 [S17W33] developed slowly and was quiet.
Region 11368 [S14W02] was quiet and stable.
Region 11369 [N23W07] was quiet and stable.
Region 11372 [N09E05] developed slowly and was quiet.
Region 11373 [S29W53] decayed slowly and quietly.
Region 11374 [S17E56] displayed no major changes and was mostly quiet. Flare: C3.1 at 13:20 UTC
Region 11375 [N10E54] matured and was quiet.
Spotted regions not reported by NOAA/SWPC:
[S1342] rotated into view at the southeast limb on Nov.28. The region developed quickly on Dec.1-3 while moderately quick decay has been observed since December 4. Location at midnight: S23W60.
[S1349] was split off from 11366 on December 4. Location at midnight: N29W11
[S1353] emerged in the northeast quadrant on December 4. Location at midnight: N15W03
[S1364] emerged in the northeast quadrant on December 9. Location at midnight: N14E26
December 7-9: No obviously Earth directed CMEs observed.
Coronal hole history (since late October
Compare today's report to the situation one solar rotation ago: 28 days ago 27 days ago 26 days ago
A small coronal hole (CH487) in the northern hemisphere was in an Earth facing position on December 7-8.
The above coronal hole map is based on a new method where coronal holes are detected automatically. The method may need some fine tuning, however, it has significant advantages over detecting coronal holes manually. The main improvement is the ability to detect coronal holes at and just beyond the solar limbs. Early results using this method for SDO images over a span of several weeks indicate a good match between coronal holes observed over the visible disk and their extent and position at the east and west limbs. Note that the polar coronal holes are easily detected using the new method, the extent and intensity of both holes are consistent with other data sources.
Long distance low and medium frequency (below 2 MHz) propagation along paths north of due west over high and upper middle latitudes is poor to fair. Propagation on long distance northeast-southwest paths is poor to fair.
The geomagnetic field is expected to be quiet to unsettled with a chance of active conditions on December 10-11 due to effects from CH487. Quiet conditions are likely on December 12-13
|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
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.
Click on image for higher resolution image) Compare to the previous day's image
When available the active region map has a coronal hole polarity overlay where red (pink) is negative and blue (blue-green) is positive.
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 / HMI 4K continuum
image with magnetic polarity overlay
|11362||2011.11.27||1||N07W85||0060||HSX||rotated out of view|
SWPC includes S1342 in this region
SWPC has reassigned 11365 to a new region 15 degrees further west
|Total spot count:||26||72|
|Sunspot number:||116||212||(total spot count + 10 * number of spotted regions)|
|Weighted penumbral SN:||71||110||(Sum of total spot count + classification weighting for each AR. Classification weighting: X=0, R=3, A/S=5, H/K=10)|
|Relative sunspot number (Wolf number):||70||95||k * (sunspot number). k = 0.6 for SWPC. k = 0.45 (changed from 0.33 on Nov.1) for STAR SDO|
|Month||Average measured solar flux||International sunspot number (SIDC)||Smoothed sunspot number||Average ap
|2008.07||65.7 (SF minimum)||0.5||2.8 (-0.4)|
|2010.10||81.6||23.5||23.2 (+3.6)||6.07 / 6.27|
|2010.11||82.5||21.5||26.5 (+3.3)||4.80 / 5.50|
|2010.12||84.2||14.4||28.8 (+2.3)||3.41 / 4.35|
|2011.01||83.6||19.1||31.0 (+2.2)||4.32 / 5.51|
|2011.02||94.6||29.4||33.4 (+2.4)||5.41 / 6.44|
|2011.03||115.0||56.2||36.9 (+3.5)||7.79 / 8.18|
|2011.04||112.6||54.4||41.8 (+4.9)||9.71 / 8.83|
|2011.05||95.8||41.6||47.6 (+5.8)||9.18 / 8.94|
|2011.06||95.8||37.0||(53.7 projected, +6.1)||8.96 / 8.06|
|2011.07||94.2||43.9||(60.0 projected, +6.3)||9.14 / 8.16|
|2011.08||101.7||50.6||(65.5 projected, +5.5)||8.16 / 7.26|
|2011.09||133.8||78.0||(68.8 projected, +3.3)||12.80 / 12.27|
|2011.10||137.3||88.0||(72.3 projected, +3.5)||7.52|
|2011.11||153.5||96.7||(76.6 projected, +4.3)||4.58|
|2011.12||153.7 (1)||38.5 (2A) / 132.8 (2B)||(82.1 projected, +5.5)||(3.85)|
1) Running average based on the daily 20:00 UTC observed solar flux value at
2A) Current impact on the monthly sunspot number based on the Boulder (NOAA/SWPC) sunspot number (accumulated daily sunspots / month days). The official SIDC international sunspot number is typically 30-50% lower. 2B) Month average to date.
3) Running average based on the preliminary 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 on analysis of data from whatever sources are available at the time the report is prepared. All time references are to the UTC day. Comments and suggestions are always welcome.
SDO images are courtesy of NASA/SDO and the AIA, EVE, and HMI science teams.