Last major update issued on November 14, 2011 at 05:25 UTC.
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The geomagnetic field was very quiet on November 13. Solar wind speed ranged between 346 and 440 km/s.
Solar flux measured at 20h UTC on 2.8 GHz was 155.3 (increasing 2.7 over the last solar rotation). The planetary A index was 0 (STAR Ap - based on the mean of three hour interval ap indices: 0.4). Three hour interval K indices: 00000001 (planetary), 00111101 (Boulder).
The background x-ray flux is at the class B7 level.
At midnight UTC the visible solar disk had 13 spotted regions (in 2K resolution SDO images).
Region 11339 [N19W77] decayed further and rotated quietly to the
Region 11340 [S08W42] was quiet and stable.
Region 11341 [N11W22] developed slowly and could produce further C flares. There's minor polarity intermixing. Flare: C1.2 at 16:48 UTC
Region 11342 [N16W33] decayed slowly and quietly.
Region 11343 [N29W12] was quiet and stable.
Region 11345 [S24W58] decayed slowly and quietly.
Region 11346 [S20E56] was quiet and stable.
New region 11347 [N08E45] emerged in the northeast quadrant on November 12 and got an SWPC number the next day. Slow development was observed on November 13. The region has polarity intermixing. Flares: C2.6 at 09:21, C1.9 at 15:05 UTC.
Spotted regions not reported by NOAA/SWPC:
[S1317] emerged in the southern hemisphere near the central meridian on November 8 and developed slowly on Nov.9-11. Quick decay was observed on November 13. (SWPC has this as region 11344, a separate region further south and which is now spotless). Location at midnight: S18W75. Flares: C1.7 at 03:57, C2.4 at 04:59, C1.4 at 06:44, C1.9 at 08:20, C1.1 at 20:16 UTC.
[S1321] emerged in the northeast quadrant on November 12. Location at midnight: N13E17
[S1322] emerged in the northeast quadrant on November 13. Location at midnight: N11E62
[S1323] emerged in the northeast quadrant on November 13. Location at midnight: N18E39
[S1324] emerged in the northwest quadrant on November 13. C flares are possible. Location at midnight: N20W57
November 11: A small partial halo CME was observed following a long
duration event in region S1317 early in the day.
November 12-13: 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
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 good. Propagation on long distance northeast-southwest paths is poor.
The geomagnetic field is expected to be quiet on November 14-16.
|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
rotated out of view
SWPC is reusing 11344 instead of assigning a new number to to S1317
|Total spot count:||42||88|
|Sunspot number:||142||218||(total spot count + 10 * number of spotted regions)|
|Classification adjusted SN:||86||134||(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):||85||98||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||168.8 (1)||61.4 (2A) / 141.7 (2B)||(74.9 predicted, +4.4)||(5.04)|
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.