Solar Terrestrial Activity Report

Activity chart

Last major update issued on August 25, 2012 at 04:50 UTC.

[Solar and geomagnetic data - last month (updated daily)]
[Solar wind and electron fluence charts (updated daily)]
[Solar cycles 21-24 (last update August 6, 2012)] [Cycle 24 progress (last update August 2, 2012) ]
[Solar cycles 1-20]
[Graphical comparison of cycles 21, 22, 23 and 24 (last update August 6, 2012)]
[Graphical comparison of cycles 10, 12, 13, 14, 16 and 24 (last update August 6, 2012)]
[Historical solar and geomagnetic data charts 1954-2006 (last update April 5, 2007)]
[Archived reports since January 2003 (last update August 5, 2012)]

[POES auroral activity level since October 2009 - updated August 5, 2012]
[Solar polar fields vs solar cycles - updated June 27, 2011]

Recent activity

The geomagnetic field was quiet to unsettled on August 24. Solar wind speed at SOHO ranged between 345 and 406 km/s. A high speed stream associated with CH530 arrived early on August 25.

Solar flux measured at 20h UTC on 2.8 GHz was 104.2 (decreasing 22.4 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: 7.9). Three hour interval K indices: 23212122 (planetary), 23232322 (Boulder).

The background x-ray flux is at the class B2 level.

At 20h UTC the visible solar disk had 8 spotted active regions (in 2K resolution SDO images).

Region 11546 [N15W33] decayed slowly and quietly.
Region 11548 [N18W04] decayed slowly and quietly.
Region 11551 [N12W51] reemerged with two tiny spots.
Region 11552 [S17E17] was quiet and stable.
Region 11553 [S22E48] developed slowly and quietly.
New region 11554 [N15E14] emerged on August 23 and was numbered the next day by SWPC. The region developed fairly quickly and was quiet.

Spotted regions not numbered by NOAA/SWPC:
New region S1874 [N08E83] rotated into view as a compact region which likely has minor M class flare potential.
New region S1875 [N10E07] emerged with a single spot.

Coronal mass ejections (CMEs)

August 22-24: No obviously Earth directed CMEs were observed in LASCO and STEREO imagery.

Coronal holes

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 (CH530) was in an Earth facing position on August 22-23.

Coronal hole map

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.

Propagation

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 to good.

Forecast

The geomagnetic field is expected to be quiet to active with a chance of minor storm intervals on August 25-26 and quiet to unsettled on August 27 due to effects from CH530.

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.

Active solar regions

Click on image for higher resolution image) Compare to the previous day's image. 0.5k image [NEW]

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
11546 2012.08.15
2012.08.16
1 2 1 N16W35 0010 AXX HRX location: N15W33
11547 2012.08.16
2012.08.17
      N05W71           plage
11548 2012.08.17
2012.08.18
5 9 2 N18W09 0020 CSO BXO area: 0005
11551 2012.08.19
2012.08.21
  2   N13W54 0000   AXX   location: N12W51
11552 2012.08.20
2012.08.21
1 7 2 S17E18 0020 HSX HSX area: 0050
S1870 2012.08.21       S00W43           plage
11553 2012.08.22
2012.08.23
1 5 4 S22E46 0090 HSX DSO area: 0180
S1872 2012.08.22       S21W41         plage
11554 2012.08.23
2012.08.24
11 15 8 N16E12 0060 DAI DSI area: 0300
S1874 2012.08.24   5 3 N08E83 0350   DAC    
S1875 2012.08.24   1 1 N10E07 0000   AXX    
Total spot count: 19 46 21  
Sunspot number: 69 126 91  (total spot count + 10 * number of spotted regions)
Weighted SN: 39 69 44  (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): 41 44 50 k * (sunspot number). k = 0.6 for SWPC, k = 0.35 for STAR SDO 2K, k = 0.55 for STAR SDO 1K

Monthly solar cycle data

Month Average measured solar flux International sunspot number (SIDC) Smoothed sunspot number Average ap
(3)
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 63.4 (+2.3) 3.78
2012.01 132.5 58.3 65.5 (+2.1) 7.15
2012.02 106.5 32.9 (67.4 projected, +1.9) 8.81
2012.03 114.7 64.3 (68.1 projected, +0.7) 16.08
2012.04 113.0 55.2 (67.5 projected, -0.6) 10.10
2012.05 121.5 69.0 (65.8 projected, -1.7) 7.06
2012.06 119.6 64.5 (65.0 projected, -0.8) 10.08
2012.07 133.9 66.5 (66.0 projected, +1.0) 13.90
2012.08 115.0 (1) 64.6 (2A) / 83.4 (2B) (68.6 projected, +2.6) (8.53)

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.