Last major update issued on November 23, 2011 at 05:20 UTC.
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The geomagnetic field was quiet to unsettled on November 22. Solar wind speed ranged between 285 and 437 km/s under the influence of a weak disturbance. After 21h UTC a fairly low speed stream from CH485 became the dominant solar wind source.
Solar flux measured at 20h UTC on 2.8 GHz was 142.4 (increasing 10.2 over the last solar rotation). The planetary A index was 6 (STAR Ap - based on the mean of three hour interval ap indices: 6.5). Three hour interval K indices: 21223212 (planetary), 32222212 (Boulder).
The background x-ray flux is at the class B5 level.
At midnight UTC the visible solar disk had 10 spotted regions (in 2K resolution SDO images).
Region 11346 [S17W69] decayed significantly and was mostly quiet.
Region 11352 [S25W12] decayed slowly and quietly.
Region 11353 [N07E06] was quiet and stable.
Region 11354 [S17E06] decayed further and was mostly quiet. Flare: C1.2 at 00:37 UTC
Region 11355 [N14E21] was quiet and has minor polarity intermixing.
Region 11356 [N15E44] still has a magnetic delta structure in the southernmost penumbra. An M class flare is possible. Flares: C4.9 at 04:04, C1.9 at 07:29, C3.2 at 09:54, C1.0 at 14:53, C1.6 at 17:12, C1.0 at 21:38, C1.9 at 23:39 UTC
Region 11357 [N18W43] developed slowly and quietly, the region has polarity intermixing.
New region 11358 [N19E80] rotated into view at the northeast limb.
Spotted regions not reported by NOAA/SWPC:
[S1333] emerged in the northeast quadrant on November 19. Location at midnight: N11W05
[S1334] emerged in the northeast quadrant on November 19, was spotless the next day and reemerged on Nov.21. Location at midnight: N16W18
November 20-21: No obviously Earth directed CMEs observed.
November 22: A filament eruption between regions 11356 and 11355 began near 06:24 UTC and caused a weak partial halo CME as observed by SOHO/LASCO.
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 poorly defined trans equatorial coronal hole (CH485) was in an Earth facing position on November 19-20.
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. Propagation on long distance northeast-southwest paths is fair.
The geomagnetic field is expected to be quiet to unsettled on November 23 due to effects from CH485. Quiet conditions are likely on Nov.24-25. On Nov.26 there's a possibility of weak CME effects from the CME observed on Nov.22.
|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
|11351||2011.11.14||S24W59||region should be deleted, was the trailing spots of region 11346|
|Total spot count:||52||102|
|Sunspot number:||132||202||(total spot count + 10 * number of spotted regions)|
|Classification adjusted SN:||92||141||(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):||79||91||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||159.2 (1)||100.0 (2A) / 136.3 (2B)||(74.9 predicted, +4.4)||(4.21)|
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.