Last major update issued on November 11, 2011 at 05:40 UTC.
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The geomagnetic field was quiet on November 10. Solar wind speed ranged between 334 and 402 km/s.
Solar flux measured at 20h UTC on 2.8 GHz was 178.6 (increasing 42.5 over the last solar rotation). The planetary A index was 3 (STAR Ap - based on the mean of three hour interval ap indices: 2.9). Three hour interval K indices: 00001211 (planetary), 10012222 (Boulder).
The background x-ray flux is at the class B7 level.
At midnight UTC the visible solar disk had 11 spotted regions (in 2K resolution SDO images).
Region 11338 [S13W51] decayed slowly and quietly.
Region 11339 [N20W35] lost penumbral area and still has many spots.
There's two minor magnetic delta structures in the largest penumbra.
Flare: C6.0/1F long duration event peaking
at 18:31 UTC.
Region 11340 [S08W03] was quiet and stable.
Region 11341 [N10E15] developed slowly and has polarity intermixing. C
flares are possible.
Region 11342 [N17E06] was quiet and stable.
Region 11343 [N28E26] was quiet and stable.
Region 11344 [S22W33] was quiet and stable.
Region 11345 [S25W15] developed further and has polarity intermixing. C
flares are possible.
Spotted regions not reported by NOAA/SWPC:
[S1315] emerged in the southeast quadrant on November 8. Location at midnight:
S20E15
[S1317] emerged in the southern hemisphere near the central meridian on
November 8 and developed slowly on Nov.9-10. SWPC apparantly considers this to
be part of region 11344. Location at midnight: S17W31
November 8, 10: No obviously Earth directed CMEs observed.
November 9: A full halo CME was observed after a
filament eruption in the northeast quadrant near region 11342.
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
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 fair. Propagation on long distance northeast-southwest paths is poor.
The geomagnetic field is expected to be quiet on November 11. The CME observed on Nov.9 could arrive late on Nov.11 or most likely on Nov.12 and cause unsettled to minor storm conditions. On Nov.13 quiet to unsettled conditions are likely.
| 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.
(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 detected |
Spot count | Location at midnight | Area | Classification | SDO / HMI 4K continuum image with polarity overlay |
Comment | |||
|---|---|---|---|---|---|---|---|---|---|---|
| SWPC | STAR SDO | SWPC | STAR | Current | Previous | |||||
| 11336 | 2011.10.29 2011.10.31 |
N14W83 | plage | |||||||
| 11337 | 2011.10.30 2011.10.31 |
N17W71 | plage | |||||||
| 11338 | 2011.10.31 2011.11.01 |
4 | 11 | S13W51 | 0190 | CSO | CSO |
 |
 |
|
| 11339 | 2011.11.01 | 45 | 69 | N19W33 | 1020 | FKC | EKC |
 |
 |
beta-gamma-delta |
| 11344 | 2011.11.03 2011.11.07 |
7 | 4 | S19W31 | 0060 | CRO | BXO |
 |
 |
area: 0000 SWPC is including S1317 in this region |
| 11340 | 2011.11.04 2011.11.05 |
1 | 2 | S09W04 | 0080 | HSX | CSO |
 |
 |
area: 0140 |
| S1311 | 2011.11.04 | N16W53 | plage | |||||||
| 11341 | 2011.11.05 | 3 | 17 | N08E14 | 0110 | CSO | DAI |
 |
 |
beta-gamma location: N10E15 area: 0220 |
| 11342 | 2011.11.05 | 5 | 13 | N15E15 | 0180 | CSO | CHO |
 |
 |
location: N17E06 |
| 11343 | 2011.11.05 2011.11.06 |
1 | 4 | N27E23 | 0180 | HSX | HSX |
 |
 |
location: N28E26 |
| S1314 | 2011.11.07 | N20W16 | plage | |||||||
| S1315 | 2011.11.08 | 3 | S20E15 | 0000 | BXO |
 |
 |
|||
| S1316 | 2011.11.08 | N03W18 | plage | |||||||
| S1317 | 2011.11.08 | 17 | S17W31 | 0130 | DSI |
 |
 |
|||
| 11345 | 2011.11.09 | 6 | 16 | S25W16 | 0090 | DRO | DAI |
 |
 |
beta-gamma area: 0120 |
| S1318 | 2011.11.10 | 1 | N15E37 | 0000 | AXX |
 |
|
|||
| Total spot count: | 72 | 157 | ||||||||
| Sunspot number: | 152 | 267 | (total spot count + 10 * number of spotted regions) | |||||||
| Classification adjusted SN: | 113 | 207 | (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): | 91 | 120 | 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 (3) |
|---|---|---|---|---|
| 2008.07 | 65.7 (SF minimum) | 0.5 | 2.8 (-0.4) | |
| 2008.12 | 69.2 | 0.8 | 1.7 (-) sunspot minimum |
3.25 |
| 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 | 169.7 (1) | 47.2 (2A) / 141.7 (2B) | (74.9 predicted, +4.4) | (6.13) |
1) Running average based on the daily 20:00 UTC observed solar flux value at
2800 MHz.
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.
