Last major update issued on November 17, 2011 at 05:35 UTC.
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The geomagnetic field was quiet on November 16. Solar wind speed ranged between 372 and 500 km/s.
Solar flux measured at 20h UTC on 2.8 GHz was 142.3 (decreasing 16.9 over the last solar rotation). The planetary A index was 2 (STAR Ap - based on the mean of three hour interval ap indices: 1.9). Three hour interval K indices: 11000010 (planetary), 11012221 (Boulder).
The background x-ray flux is at the class B7 level.
At midnight UTC the visible solar disk had 15 spotted regions (in 2K resolution SDO images).
Region 11340 [S08W84] was quiet and stable.
Region 11341 [N10W65] decayed slowly and quietly.
Region 11342 [N17W76] was quiet and stable.
Region 11343 [N29W51] was quiet and stable.
Region 11346 [S17E13] lost the magnetic delta structure, however, the region is somewhat unstable and could produce further C class flares. Flare: C1.7 at 00:07, C2.8 at 13:37, C2.9/1F at 18:54, C1.6 at 21:43, C5.0 at 23:48 UTC
Region 11347 [N09E05] decayed and was quiet.
Region 11348 [behind the northwest limb] was unstable and produced lots of activity. Flares: C2.3 at 03:01, C3.0 at 03:43, C7.5 at 04:55, C4.0 at 06:25, C7.9/1F at 15:05 UTC.
Region 11349 [N17W30] decayed slowly and quietly.
Region 11350 [N26E44] was quiet and decayed slowly.
New region 11352 [S23E68] rotated into view at the southeast limb on Nov.15 and got an SWPC number the next day.
Spotted regions not reported by NOAA/SWPC:
[S1321] emerged in the northeast quadrant on November 12. Location at midnight: N12W22
[S1322] emerged in the northeast quadrant on November 13. Location at midnight: N10E19
[S1323] emerged in the northeast quadrant on November 13, was spotless the next day and reemerged on Nov.15. Location at midnight: N20E01
[S1327] emerged in the southeast quadrant on November 16. Location at midnight: S22E45
[S1328] rotated partly into view at the southeast limb on November 16. M class flaring is possible. Location at midnight: S16E87. Flare: C5.2 at 19:53 UTC
[S1329] rotated into view at the northeast limb on November 16. Location at midnight: N08E87
November 14-16: No obviously Earth directed CMEs observed.
Compare today's report to the situation one solar rotation ago: 28 days ago 27 days ago 26 days ago
No obvious coronal holes are near Earth facing positions.
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 on November 16-18.
|Coronal holes (1)||Coronal mass ejections (2)||M and X class flares (3)|
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.
|Active region||Date numbered
|Spot count||Location at midnight||Area||Classification||SDO / HMI 4K continuum
image with magnetic polarity overlay
|11351||2011.11.14||S24E23||region should be deleted, was trailing spots of region 11346|
|Total spot count:||23||66|
|Sunspot number:||113||216||(total spot count + 10 * number of spotted regions)|
|Classification adjusted SN:||58||112||(Sum of total spot count + classification adjustment for each AR. Classification adjustment: X=0, R=3, A/S=5, H/K=10)|
|Relative sunspot number (Wolf number):||68||97||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)|
|2010.07||79.8||16.1||16.7 (+0.3)||6.31 / 5.15|
|2010.08||79.2||19.6||17.4 (+0.7)||8.49 / 7.77|
|2010.09||81.1||25.2||19.6 (+2.2)||5.33 / 5.45|
|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||(47.4 predicted, +5.6)||9.18 / 8.94|
|2011.06||95.8||37.0||(52.5 predicted, +5.1)||8.96 / 8.06|
|2011.07||94.2||43.9||(58.2 predicted, +5.7)||9.14 / 8.16|
|2011.08||101.7||50.6||(63.7 predicted, +5.5)||8.16 / 7.26|
|2011.09||133.8||78.0||(67.0 predicted, +3.3)||12.80 / 12.27|
|2011.10||137.3||88.0||(70.5 predicted, +3.5)||7.52|
|2011.11||165.4 (1)||75.6 (2A) / 141.8 (2B)||(74.9 predicted, +4.4)||(4.57)|
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.