Last major update issued on June 27, 2012 at 04:50 UTC.
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June 2, 2012)]
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[Graphical comparison of cycles 10, 12, 13, 14, 16 and
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(last update April 5, 2007)]
[Archived reports since January 2003 (last update
June 24, 2012)]
[POES auroral activity level since October
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[Solar polar fields vs solar cycles - updated
June 27, 2011]
The geomagnetic field was quiet to unsettled on June 26. Solar wind speed at SOHO ranged between 349 and 489 km/s.
Solar flux measured at 20h UTC on 2.8 GHz was 99.2 (decreasing 11.8 over the last solar rotation). The Potsdam WDC planetary A index was 8 (STAR Ap - based on the mean of three hour interval ap indices: 8.3). Three hour interval K indices: 23321112 (planetary), 23222212 (Boulder).
The background x-ray flux is at the class B3 level.
At midnight UTC the visible solar disk had 9 spotted active regions (in 2K resolution SDO images).
Region 11512 [S16E26] developed further and has many spots and a
magnetic delta structure in a central penumbra. An M class flare is possible.
New region 11513 [N15E73] rotated into view on June 25 and developed
slowly on June 26 when it was numbered by SWPC.
Spotted active regions not numbered or interpreted differently by NOAA/SWPC:
S1747 [S26W07] lost the leader spot while a new trailing polarity spot
emerged.
S1754 [S19E10] was quiet and stable.
New region S1756 [S16E70] rotated into view with several spots.
New region S1757 [S16E84] rotated into view with a single spot.
New region S1758 [N14E24] emerged with a single tiny spot.
New region S1759 [N19E10] emerged with tiny spots.
New region S1760 [N07E09] emerged with a tiny spot.
June 24-26: No obvious 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 large recurrent trans equatorial coronal hole (CH521) will rotate into an Earth facing position on June 29 - July 1.
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 poor to fair.
The geomagnetic field is expected to be quiet on June 27-30. A high speed stream from CH521 could cause unsettled to minor storm conditions on July 1-3.
| Coronal holes (1) | Coronal mass ejection (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 | ||||||
| 2K | 1K | ||||||||||
| 11511 | 2012.06.20 2012.06.22 |
N15W72 | plage | ||||||||
| S1744 | 2012.06.20 | S32W45 | plage | ||||||||
| S1745 | 2012.06.21 | N20E16 | plage | ||||||||
| S1747 | 2012.06.22 | 1 | S26W07 | 0000 | AXX |
 |
 |
||||
| S1748 | 2012.06.23 | S12W28 |
 |
plage | |||||||
| 11512 | 2012.06.24 2012.06.25 |
7 | 39 | 22 | S16E25 | 0130 | DAI | DAC |
 |
 |
beta-gamma-delta area: 0280 |
| S1751 | 2012.06.24 | S13E03 |
 |
plage | |||||||
| S1752 | 2012.06.24 | S18W53 | plage | ||||||||
| S1753 | 2012.06.25 | S27E54 |
 |
plage | |||||||
| S1754 | 2012.06.25 | 3 | 1 | S19E10 | 0000 | BXO |
 |
 |
|||
| 11513 | 2012.06.25 2012.06.26 |
1 | 6 | 4 | N16E71 | 0030 | HAX | CAO |
 |
 |
|
| S1756 | 2012.06.26 | 6 | 3 | S16E70 | 0020 | CRO |
 |
||||
| S1757 | 2012.06.26 | 1 | 1 | S16E84 | 0100 | HSX |
 |
||||
| S1758 | 2012.06.26 | 1 | 1 | N14E24 | 0000 | AXX |
 |
||||
| S1759 | 2012.06.26 | 2 | 1 | N19E10 | 0000 | BXO |
 |
||||
| S1760 | 2012.06.26 | 1 | N07E09 | 0000 | AXX |
 |
|||||
| Total spot count: | 8 | 60 | 33 | ||||||||
| Sunspot number: | 28 | 150 | 113 | (total spot count + 10 * number of spotted regions) | |||||||
| Weighted penumbral SN: | 18 | 78 | 51 | (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): | 17 | 53 | 62 | k * (sunspot number). k = 0.6 for SWPC, k = 0.35 (changed from 0.45 on March 1, 2011) for STAR SDO 2K, k = 0.55 for STAR SDO 1K | |||||||
| 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 |
|
| 2011.03 | 115.0 | 56.2 | 36.9 (+3.5) | 8.18 |
| 2011.04 | 112.6 | 54.4 | 41.8 (+4.9) | 8.83 |
| 2011.05 | 95.8 | 41.6 | 47.6 (+5.8) | 8.94 |
| 2011.06 | 95.8 | 37.0 | 53.2 (+5.6) | 8.06 |
| 2011.07 | 94.2 | 43.9 | 57.2 (+4.0) | 8.16 |
| 2011.08 | 101.7 | 50.6 | 59.0 (+1.8) | 7.26 |
| 2011.09 | 133.8 | 78.0 | 59.5 (+0.5) | 12.27 |
| 2011.10 | 137.3 | 88.0 | 59.9 (+0.4) | 8.28 |
| 2011.11 | 153.5 | 96.7 | 61.1 (+1.2) | 5.55 |
| 2011.12 | 141.3 | 73.0 | (64.3 projected, +3.2) | 3.78 |
| 2012.01 | 132.5 | 58.3 | (68.0 projected, +3.7) | 7.15 |
| 2012.02 | 106.5 | 33.1 | (71.3 projected, +3.3) | 8.81 |
| 2012.03 | 114.7 | 64.2 | (73.0 projected, +1.7) | 16.08 |
| 2012.04 | 113.0 | 55.2 | (73.2 projected, +0.2) | 10.10 |
| 2012.05 | 121.5 | 69.0 | (73.2 projected, +0.0) | 8.75 |
| 2012.06 | 120.4 (1) | 76.9 (2A) / 88.7 (2B) | (73.9 projected, +0.7) | (12.57) |
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 quicklook and definitive Potsdam WDC ap indices.
Values in red are based on the definitive
international Potsdam
WDC
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.
