Last major update issued on May 11, 2012 at 05:05 UTC.
[Solar and geomagnetic data - last month (updated
[Solar wind and electron fluence charts (updated daily)
[Solar cycles 21-24 (last update May 3, 2012)]
[Solar cycles 1-20]
[Graphical comparison of cycles 21, 22, 23 and 24 (last update May 3, 2012)]
[Graphical comparison of cycles 10, 12, 13, 14, 16 and 24 (last update May 3, 2012)]
[Historical solar and geomagnetic data charts 1954-2006 (last update April 5, 2007)]
[Archived reports since January 2003 (last update May 3, 2012)]
[POES auroral activity level since October
2009 - updated May 5, 2012]
Annotated geomagnetic activity charts - Carrington rotation 2118 [December 2011 - January 2012] - 2119 [January-February 2012]
[Solar polar fields vs solar cycles - updated June 27, 2011]
The geomagnetic field was quiet to active on May 10. Solar wind speed at SOHO ranged between 557 and 603 km/s under the influence of a high speed stream from CH515.
Solar flux measured at 20h UTC on 2.8 GHz was 130.7 (increasing 33.0 over the last solar rotation). The Potsdam WDC planetary A index was 15 (STAR Ap - based on the mean of three hour interval ap indices: 15.3). Three hour interval K indices: 33322234 (planetary), 33222233 (Boulder).
The background x-ray flux is at the class B7 level.
At midnight UTC the visible solar disk had 8 spotted active regions (in 2K resolution SDO images).
Region 11474 [N17W33] was quiet and stable.
Region 11476 [N12E08] has a very complex magnetic delta structure in the southern part of the huge penumbra (spanning about 6 degrees latitudinally and longitudinally). There are several layers of opposite polarities in the most complex parts. The region has the potential to produce an X5+ flare. Flares: M5.7/2B at 04:18, C7.9 at 05:10, C8.3 at 05:22, M1.7 at 20:26 UTC and numerous sub C5 level flares.
Region 11477 [S22E47] added a few spots and was quiet.
New region 11478 [S24E56] rotated into view at the southeast limb on May 8 and was numbered by SWPC two days later.
Spotted active regions not numbered by NOAA/SWPC:
S1636 [S16E04] was quiet and stable.
S1642 [S15E26] developed slowly and quietly.
New region S1644 [N14E81] rotated into view at the northeast limb with a single penumbra.
New region S1645 [S12E22] was split off from S1642.
May 8: A filament eruption beginning at 09:45 UTC near AR 11474 across
the central meridian was the source of a small CME observed in both STEREO-A and
B imagery after 11h UTC. While most of the ejected material was over the
northern limbs, it appears that a part of the CME is Earth directed.
May 9-10: No obviously Earth directed significant CMEs were observed in STEREO imagery.
Coronal hole history (since October
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 (CH515) was in an Earth facing position on May 5-7. A southern hemisphere coronal hole (CH516) was Earth facing on May 9-10.
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 good.
The geomagnetic field is expected to be quiet to active on May 11 due to a high speed stream from CH515. The CME observed on May 8 could reach Earth on May 11. Starting late on May 12 or early on May 13 a high speed stream from CH516 could cause quiet to active conditions until May 14.
|Coronal holes (1)||Coronal mass ejection (2)||M and X class flares (3)|
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.
|Active region||Date numbered
|Spot count||Location at midnight||Area||Classification||SDO / HMI 4K continuum
image with magnetic polarity overlay
rotated out of view
|Total spot count:||53||158||77|
|Sunspot number:||93||238||157||(total spot count + 10 * number of spotted regions)|
|Weighted penumbral SN:||88||186||105||(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):||56||83||86||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
|2008.07||65.7 (SF minimum)||0.5||2.8 (-0.4)|
|2011.11||153.5||96.7||(61.2 projected, +1.3)||5.55|
|2011.12||141.3||73.0||(63.9 projected, +2.7)||3.78|
|2012.01||132.5||58.3||(67.4 projected, +3.5)||7.15|
|2012.02||106.5||33.1||(71.4 projected, +4.0)||8.81|
|2012.03||114.7||64.2||(73.5 projected, +2.1)||16.08|
|2012.04||113.0||55.2||(74.5 projected, +1.0)||10.10|
|2012.05||118.9 (1)||30.6 (2A) / 94.9 (2B)||(75.8 projected, +1.3)||(10.06)|
1) Running average based on the daily 20:00 UTC observed solar flux value at
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.