Last major update issued on January 31, 2012 at 04:55 UTC.
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(last update April 5, 2007)]
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Annotated geomagnetic activity charts - Carrington rotation
2117 [November-December 2011]
-
2118 [December 2011 - January 2012]
[Solar polar fields vs solar cycles - updated
June 27, 2011]
The geomagnetic field was quiet to unsettled on January 30. Solar wind speed ranged between 302 and 435 km/s. Solar wind density increased abruptly at SOHO at 15:22 UTC, the arrival of the CME observed on January 27.
Solar flux measured at 20h UTC on 2.8 GHz was 114.4 (decreasing 20.2 over the last solar rotation). The planetary A index was 7 (STAR Ap - based on the mean of three hour interval ap indices: 6.8). Three hour interval K indices: 00101333 (planetary), 00101332 (Boulder).
The background x-ray flux is at the class B2 level.
At midnight UTC the visible solar disk had 8 spotted regions (in 2K resolution SDO images).
Region 11408 [N08W50] decayed slowly and quietly.
Region 11410 [N19E23] developed slowly and currently has weak polarity
intermixing.
Region 11411 [S26W14] was quiet and stable.
Region 11413 [N09E23] developed slowly and has weak polarity intermixing.
Spotted regions not reported by NOAA/SWPC:
[S1441] reemerged on January 29. Location
at midnight: S18W22
[S1446] rotated into view at the southeast limb on January 24. Location
at midnight: S18W03
[S1453] emerged in the northeast quadrant on January 29. Location at midnight:
N21E09
[S1454] emerged in the northwest quadrant on January 30. Location at
midnight: N17W44
January 28-30: No obviously Earth directed CMEs were observed in LASCO and STEREO imagery.
Coronal hole history (since October
2002)
Compare today's report to the situation one solar rotation ago:
28 days ago
27 days ago
26 days ago
A trans equatorial coronal hole (CH498) will likely rotate into an Earth facing position on January 30-February 2.
The above coronal hole map is based on a method where coronal holes are detected automatically. While the method may need some fine tuning, 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 this method, the extent and intensity of both CHs 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 January 31 and quiet on February 1. A high speed stream from CH498 could cause quiet to active conditions on February 2-4.
| 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 | |||||
| 11409 | 2012.01.20 2012.01.21 |
N18W70 | plage | |||||||
| 11408 | 2012.01.20 2012.01.21 |
3 | 2 | N08W50 | 0060 | HSX | HSX |
 |
 |
|
| S1441 | 2012.01.22 | 1 | S18W22 | 0000 | AXX |
 |
 |
|||
| S1446 | 2012.01.24 | 10 | S18W03 | 0010 | AXX |
 |
 |
|||
| S1448 | 2012.01.25 | S17W59 | ||||||||
| 11410 | 2012.01.26 | 4 | 14 | N20E20 | 0170 | HSX | CHO |
 |
 |
beta-gamma area: 0290 location: N19E23 |
| 11411 | 2012.01.26 2012.01.28 |
6 | 9 | S27W16 | 0010 | BXO | DRI |
 |
 |
location: S26W14 area: 0040 |
| S1450 | 2012.01.26 | S20W48 | plage | |||||||
| 11413 | 2012.01.27 2012.01.29 |
11 | 21 | N08E22 | 0080 | DSO | DAI |
 |
 |
beta-gamma location: N09E23 |
| 11412 | 2012.01.28 2012.01.29 |
2 | S16W53 | 0010 | AXX |
 |
spotless | |||
| S1453 | 2012.01.29 | 3 | N21E07 | 0000 | AXX |
 |
 |
|||
| S1454 | 2012.01.30 | 1 | N17W44 | 0000 | AXX |
 |
||||
| Total spot count: | 26 | 61 | ||||||||
| Sunspot number: | 76 | 141 | (total spot count + 10 * number of spotted regions) | |||||||
| Weighted penumbral SN: | 41 | 84 | (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): | 46 | 63 | k * (sunspot number). k = 0.6 for SWPC. k = 0.45 (changed from 0.33 on Nov.1, 2011) 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 |
| 2010.10 | 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 | 53.2 (+5.6) | 8.96 / 8.06 |
| 2011.07 | 94.2 | 43.9 | (57.8 projected, +4.6) | 9.14 / 8.16 |
| 2011.08 | 101.7 | 50.6 | (62.0 projected, +4.2) | 8.16 / 7.26 |
| 2011.09 | 133.8 | 78.0 | (65.3 projected, +3.3) | 12.80 / 12.27 |
| 2011.10 | 137.3 | 88.0 | (68.8 projected, +3.5) | 7.52 |
| 2011.11 | 153.5 | 96.7 | (73.2 projected, +4.3) | 4.58 |
| 2011.12 | 141.3 | 73.0 | (78.6 projected, +5.5) | 3.32 |
| 2012.01 | 133.0 (1) | 87.5 (2A) / 90.4 (2B) | (84.4 projected, +5.8) | (6.69) |
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.
