Solar Terrestrial Activity Report

Last major update issued on August 22, 2011 at 03:50 UTC. Minor update posted at 14:35 UTC

[Solar and geomagnetic data - last month (updated daily)]
[Solar wind and electron fluence charts (updated daily)
[Solar cycles 21-24 (last update August 2, 2011)]
[Solar cycles 1-20]
[Graphical comparison of cycles 21, 22, 23 and 24 (last update August 2, 2011)]
[Graphical comparison of cycles 10, 12, 13, 14, 16 and 24 (last update August 2, 2011)]
[Historical solar and geomagnetic data charts 1954-2006 (last update April 5, 2007)]
[Archived reports since January 2003 (last update August 2, 2011)]

[POES auroral activity level since October 2009 - updated August 19, 2011]
Annotated geomagnetic activity charts - Carrington rotation 2111 [June-July 2011]  - 2112 [July 2011] NEW
[Solar polar fields vs solar cycles - updated June 27, 2011]

Recent activity

The geomagnetic field was quiet on August 21. Solar wind speed ranged between 338 and 411 km/s.

Solar flux measured at 20h UTC on 2.8 GHz was 100.9 (increasing 13.9 over the last solar rotation). The planetary A index was 3 (STAR Ap - based on the mean of three hour interval ap indices: 3.4). Three hour interval K indices: 10002121 (planetary), 10012221 (Boulder).

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

At midnight UTC the visible solar disk had 5 spotted regions (in 2K resolution SDO images).

Region 11271 displayed no major changes and remains capable of producing C flares.
Region 11272 developed quickly in the trailing spot section. Opposite polarity spot separation is poor in the center of the region. Further development will increase the likelihood of minor M class flaring. Flares: C1.5 at 18:40, C1.2 at 23:16 UTC
Region 11274 was quiet and stable.
New region 11275 rotated partly into view on August 20 and was numbered the next day by SWPC.

Spotted regions not numbered by NOAA/SWPC:
[S1171] reemerged on August 20 (spots were included in the count for region 11271) with both polarity spots visible on August 21. Location at midnight: N07E04

Minor update added at 14:35 UTC on August 22: Region 11271 has changed a lot today with trailing polarity spots emerging near the center of the region, now classified as DKC. The new penumbra is already the largest in the region, and a magnetic delta structure could be forming at the southwestern edge. Region 11274 has added a trailing spot in the far eastern polarity area, further growth could change the classification of the region to FRO or FSO. Otherwise CH472 has decayed significantly over the last day or so and could close before rotating out of view. The latest high resolution CHARMAP.

Coronal mass ejections (CMEs)

August 19-21: No obviously Earth directed CMEs were observed in LASCO or STEREO imagery.

Coronal holes

Coronal hole history (since late 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 (CH472) was in an Earth facing position on August 19-20. A recurrent coronal hole (CH473) in the northern hemisphere could rotate into an Earth facing position on August 24-25.

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.

Propagation

Long distance low and medium frequency (below 2 MHz) propagation along paths north of due west over high and upper middle latitudes is fair. Propagation on long distance northeast-southwest paths is poor.

Forecast

The geomagnetic field is expected to be quiet to unsettled conditions with occasional active intervals on August 22-23 due to effects from CH472. Quiet conditions are likely on August 24-25.

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.

Active solar regions

(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 polarity overlay
Comment
SWPC STAR SDO SWPC STAR Current Previous
11270 2011.08.10
2011.08.11
    N23W83           plage
11271 2011.08.14
2011.08.15
15 36 N16W01 0240 EAO EAI

beta-gamma

area: 0400

11272 2011.08.15
2011.08.16
8 26 S21E03 0090 DAO DAI

location: S22E06

area: 0160

S1170 2011.08.15     N05W54           plage
S1171 2011.08.16   2 N07E04 0000   BXO    
11273 2011.08.16
2011.08.17
    S18W56         plage
S1173 2011.08.17     N24W14           plage
11274 2011.08.19
2011.08.20
2 4 N18E57 0030 CRO HRX location: N19E57
11275 2011.08.20
2011.08.21
1 5 N06E68 0030 CRO CSO formerly region S1176

SWPC combination of 1 spot and CRO classification is impossible

Total spot count: 26 73  
Sunspot number: 66 123  (total spot count + 10 * number of spotted regions)
Classification adjusted SN: 42 91  (Sum of total spot count + classification adjustment for each AR. Classification adjustment: X=0, R=3, A/S=5, H/K=10)
Relative sunspot number (Wolf number): 40 41  k * (sunspot number). k = 0.6 for SWPC. k = 0.33 for STAR SDO

Monthly solar cycle data

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
2010.05 73.8 8.7 15.5 (+1.5) 9.18 / 8.15
2010.06 72.5 13.6 16.4 (+0.9) 8.17 / 6.85
2010.07 79.8 16.1 16.7 (+0.3) 6.31 / 5.15
2010.08 79.2 19.6 17.4 (+0.7) 8.49 / 7.77
2010.09 81.1 25.2 19.6 (+2.2) 5.33 / 5.45
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 (33.6 predicted, +2.6) 5.41 / 6.44
2011.03 115.0 56.2 (36.6 predicted, +3.0) 7.79 / 8.18
2011.04 112.6 54.4 (39.4 predicted, +2.8) 9.71 / 8.83
2011.05 95.8 41.6 (42.7 predicted, +3.3) 9.18 / 8.94
2011.06 95.8 37.0 (46.5 predicted, +3.8) 8.96
2011.07 94.2 43.9 (50.6 predicted, +4.1) 9.14
2011.08 100.6 (1) 39.5 (2A) / 58.2 (2B) (54.8 predicted, +4.2) (9.41)

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.