Last major update issued on December 1, 2011 at 04:50 UTC.
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The geomagnetic field was quiet to unsettled on November 30. Solar wind speed ranged between 378 and 513 km/s. There was a solar wind sector transition at 07:51 UTC at SOHO. After the transition a relatively low speed stream from CH486 was the dominant solar wind source.
Solar flux measured at 20h UTC on 2.8 GHz was 144.0 (decreasing 16.4 over the last solar rotation). The planetary A index was 10 (STAR Ap - based on the mean of three hour interval ap indices: 10.4). Three hour interval K indices: 30033332 (planetary), 31034332 (Boulder).
The background x-ray flux is at the class B7 level.
At midnight UTC the visible solar disk had 9 spotted regions (in 2K resolution SDO images).
Region 11355 [N15W87] decayed slowly and quietly as it rotated to the
northwest limb.
Region 11356 [N17W65] was mostly quiet and stable, new positive polarity
spots emerged in the northwestern part of the reigon.
Flare: C3.6 at 22:32 UTC
Region 11358 [N22W25] decayed slowly and quietly.
Region 11361 [N20E08] developed slowly and quietly. The region has minor
polarity intermixing.
Region 11362 [N08E37] developed further and has polarity intermixing.
Flare: C1.2 at 02:10 UTC
Region 11363 [S17E56] added a few spots to the north of the single
penumbra.
Region 11364 [N20E62] was mostly unchanged.
Flare: C3.8 at 20:28 UTC
Spotted regions not reported by NOAA/SWPC:
[S1342] rotated into view at the southeast limb on Nov.28. Location at midnight:
S22E59.
Flares: C2.0 at 00:11, C1.1 at 09:17 UTC
[S1344] emerged in the northeast quadrant on November 30. Location at midnight:
N25E34
November 28-30: No obviously Earth directed CMEs observed.
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
A coronal hole (CH486) in the southern hemisphere was in an Earth facing position on November 26-27.
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 December 1 due to coronal hole effects and quiet on December 2-3.
| 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 magnetic polarity overlay |
Comment | |||
|---|---|---|---|---|---|---|---|---|---|---|
| SWPC | STAR SDO | SWPC | STAR | Current | Previous | |||||
| 11355 | 2011.11.17 2011.11.18 |
1 | 1 | N15W87 | 0060 | HSX | AXX |
 |
 |
area: 0010 |
| 11356 | 2011.11.19 | 4 | 8 | N17W62 | 0060 | ESO | CSO |
 |
 |
|
| 11358 | 2011.11.22 | 8 | 13 | N22W24 | 0120 | CSO | CSO |
 |
 |
location: N22W12 |
| 11361 | 2011.11.24 2011.11.25 |
17 | 23 | N18W06 | 0080 | DSI | DSI |
 |
 |
beta-gamma area: 0170 location: N20W05 |
| 11360 | 2011.11.24 2011.11.25 |
N17W59 | plage | |||||||
| S1337 | 2011.11.25 | S17E14 | plage | |||||||
| S1338 | 2011.11.26 | N17E04 |
 |
|||||||
| 11362 | 2011.11.27 | 7 | 25 | N07E36 | 0130 | DSI | DSI |
 |
 |
beta-gamma area: 0370 |
| 11363 | 2011.11.28 2011.11.29 |
3 | 4 | S19E55 | 0110 | DSO | CSO |
 |
 |
location: S17E56 SWPC includes S1342 in this region |
| 11364 | 2011.11.28 2011.11.29 |
1 | 1 | N18E60 | 0060 | HSX | CSO |
 |
 |
area: 0100 location: N20E62 |
| S1342 | 2011.11.28 | 11 | S22E59 | 0130 | DAI |
 |
 |
|||
| S1343 | 2011.11.29 | S10E40 |
 |
plage | ||||||
| S1344 | 2011.11.30 | 2 | N25E34 | 0000 | AXX |
 |
||||
| Total spot count: | 41 | 88 | ||||||||
| Sunspot number: | 111 | 178 | (total spot count + 10 * number of spotted regions) | |||||||
| Weighted penumbral SN: | 76 | 123 | (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): | 67 | 80 | 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 |
| 2010.09 | 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 | 47.6 (+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 | 1) | (2A/2B) | (82.1 projected, +5.5) | () |
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.
