Last major update issued on January 14, 2012 at 06:00 UTC.
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The geomagnetic field was quiet to unsettled on January 13. Solar wind speed ranged between 445 and 583 km/s under the influence of a high speed stream from CH492.
Solar flux measured at 20h UTC on 2.8 GHz was 124.1 (increasing 4.5 over the last solar rotation). The planetary A index was 7 (STAR Ap - based on the mean of three hour interval ap indices: 6.9). Three hour interval K indices: 23310111 (planetary), 13322221 (Boulder).
The background x-ray flux is at the class B6 level.
At midnight UTC the visible solar disk had 7 spotted regions (in 2K resolution SDO images).
Region 11391 [N12W67] decayed slowly and was mostly quiet.
Flare: C2.2 at 06:05 UTC
Region 11395 [N22W04] decayed slowly and quietly.
Region 11396 [N26E19] developed quickly and has a weak magnetic delta
structure in the southeastern part of the leading penumbra. C flares are likely.
New region 11397 [S19E29] emerged in the southeast quadrant on January 12
and got an SWPC number the next day.
New region 11398 [N13W08] emerged in the northeast quadrant on January 11
and was numbered by SWPC two days later. The region has polarity intermixing. C
flares are possible.
Spotted regions not reported (or interpreted differently) by NOAA/SWPC:
[S1428] rotated into view at the southeast limb on January 13. Location at midnight:
S23E84
[S1429] emerged in the southeast quadrant on January 13. Location at
midnight: S13E11
Two interesting regions behind the northeast limb culd rotate into view today and tomorrow.
January 11-13: 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 recurrent trans equatorial coronal hole (CH493) was in an Earth facing position on January 12-13.
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 to good. Propagation on long distance northeast-southwest paths is poor.
The geomagnetic field is expected to be quiet on January 14 becoming quiet to unsettled on January 15-16 with a chance of active intervals due to effects from CH493.
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 | |||||
11391 | 2012.01.02 | 11 | 7 | N12W67 | 0120 | DAO | DAO | |||
11394 | 2012.01.05 2012.01.06 |
N18W56 | plage | |||||||
S1411 | 2012.01.06 | S20W31 | plage | |||||||
11395 | 2012.01.07 2012.01.08 |
2 | 8 | N21W06 | 0040 | HSX | HSX |
location: N22W04 |
||
S1415 | 2012.01.07 | N12W38 | plage | |||||||
S1419 | 2012.01.08 | S22W42 | plage | |||||||
S1420 | 2012.01.09 | N30W54 | plage | |||||||
11396 | 2012.01.09 2012.01.12 |
10 | 22 | N26E18 | 0070 | DAI | DAI |
beta-gamma-delta area: 0180 |
||
S1422 | 2012.01.10 | S16W17 | plage | |||||||
S1423 | 2012.01.10 | S26W08 | plage | |||||||
S1424 | 2012.01.11 | S16E47 | plage | |||||||
11398 | 2012.01.11 2012.01.13 |
4 | 14 | N13W08 | 0015 | DAO | DAI | area: 0070 | ||
11397 | 2012.01.12 2012.01.13 |
4 | 5 | S20E48 | 0040 | DAO | DSO | |||
S1427 | 2012.01.12 | S24E21 | plage | |||||||
S1428 | 2012.01.13 | 1 | S23E84 | 0040 | HSX | |||||
S1429 | 2012.01.13 | 4 | S13E11 | 0010 | BXO | |||||
Total spot count: | 31 | 61 | ||||||||
Sunspot number: | 81 | 131 | (total spot count + 10 * number of spotted regions) | |||||||
Weighted penumbral SN: | 56 | 91 | (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): | 49 | 59 | 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 | 132.4 (1) | 34.5 (2A) / 82.4 (2B) | (84.4 projected, +5.8) | (4.65) |
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.