Solar Terrestrial Activity Report

Activity chart

Last major update issued on September 7, 2014 at 05:50 UTC.

[Solar and geomagnetic data - last month (updated daily)]
[Solar wind and electron fluence charts (updated daily)]
[Solar cycles 23-24 (last update September 1, 2014)] [Cycle 24 progress (last update September 1, 2014) ]
[Solar cycles 1-20]
[Graphical comparison of cycles 21, 22, 23 and 24 (last update September 1, 2014)]
[Graphical comparison of cycles 10, 12, 13, 14, 16 and 24 (last update September 1, 2014)]
[Historical solar and geomagnetic data charts 1954-2006 (last update April 5, 2007)]
[Archived reports since January 2003 (last update September 6, 2014)]

[POES auroral activity level October 2009 - December 2012]
[Solar polar fields vs solar cycles - updated September 6, 2014]
[Presentations: 3rd SSN Workshop, Tucson, 2013 (pdf) / 4th SSN Workshop, Locarno, 2014]

Recent activity

The geomagnetic field was quiet to unsettled on September 6. Solar wind speed at SOHO ranged between 327 and 411 km/s, most of the day under the influence of weak CME effects.

Solar flux at 20h UTC on 2.8 GHz was 157 (increasing 49 over the last solar rotation). The 90 day 10.7 flux at 1 AU was 133.6. The Potsdam WDC planetary A index was 8 (STAR Ap - based on the mean of three hour interval ap indices: 8.4). Three hour interval K indices: 12312322 (planetary), 12323322 (Boulder).

The background x-ray flux is at the class C1 level.

At the time of counting spots (see image time), spots were observed in 11 active regions using 2K resolution (SN: 236) and 11 active regions using 1K resolution (SN: 180) SDO images on the visible solar disk.

Region 12152 [S14W68] decayed slowly and lost all trailing polarity umbrae. The region was mostly quiet.
Region 12154 [S19W20] decayed slowly and quietly.
Region 12155 [S19E34] decayed slowly and quietly.
Region 12157 [S14E47] still has a significant magnetic delta structure in the southeastern part of the largest penumbra. Further M class flares are likely, a major flare is possible.
Region 12158 [N15E56] was mostly unchanged and has a strong magnetic delta structure inside the large penumbra. An X class event is possible.
Region 12159 [S21E64] was quiet and stable.
New region 12160 [S09W52] emerged on September 5 and was numbered by SWPC the next day.
New region 12161 [S15W07] emerged with a few spots.
New region 12162 [N08W03] emerged on September 5 with SWPC numbering the region the following day.

Spotted regions not numbered (or interpreted differently) by SWPC:
New region S3804 [S16W13] emerged with penumbra spots to the northeast of AR 12154.
New region S3805 [S17E77] rotated into view.

C2+ flares (GOES):

Magnitude Peak time (UTC) Location AR Comment
C2.9 00:03 S16E61 12157  
C2.4 06:18   12157  
C8.0/1N (LDE) 08:14 S10E54 12157 CME
C2.5 11:29      
M1.1 17:09 S14E53 12157  
C4.7 17:48   12157  

Coronal mass ejections (CMEs)

September 4-6: 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 extension of a northern hemisphere coronal hole (CH634) was in an Earth facing position on September 5.

Propagation

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

Forecast

The geomagnetic field is expected to be quiet to unsettled on September 7-9 with a chance of active intervals due to CME effects on September 7 and under the influence of a high speed stream from CH634 on September 8-9.

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: 0-30% probability, Yellow: 30-70% probability, Red: 70-100% probability.

Active solar regions

(Click on image for 2K resolution) Compare to the previous day's image. 0.5K image

When available the active region map has a coronal hole polarity overlay where red (pink) is negative and blue 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 Magnetic
(SDO)
SWPC STAR Current Previous
2K 1K
12153 2014.08.26
2014.08.29
2     S09W92 0140 DSO     rotated out of view
12152 2014.08.26
2014.08.28
15 7 4 S15W65 0180 EAO CSO

location: S14W68

S3776 2014.08.30       N12W32         images/AR_S3776_20140905_2345.png plage
S3779 2014.08.30       N10W58           plage
S3781 2014.08.31       S08W05         plage
S3782 2014.08.31       N24W54           plage
12154 2014.09.01
2014.09.02
3 7 5 S18W19 0010 BXO BXO  
S3784 2014.09.01       S28W54           plage
S3786 2014.09.02       S19W43         plage
S3788 2014.09.02       S31W35           plage
S3791 2014.09.03       N09E11         plage
12155 2014.09.03 5 10 5 S20E33 0120 DAO CSO  
12157 2014.09.03
2014.09.04
17 41 21 S14E44 0540 EKC EKC beta-gamma-delta

location: S14E47

12156 2014.09.03
2014.09.04
      N15E28         plage
12158 2014.09.04 7 15 8 N15E54 0310 DKC DKC beta-delta

area: 0530

location: N15E56

S3796 2014.09.04       N08W13           plage
12159 2014.09.05 5 8 6 S20E60 0030 CRO DRO location: S21E64
12162 2014.09.05
2014.09.06
3 8 5 N08W04 0010 CAO CRO  
S3799 2014.09.05       S04E09         plage
12160 2014.09.05
2014.09.06
5 11 4 S09W55 0010 CRO DRO area: 0060

location: S09W52

S3801 2014.09.05       N02W27         plage
12161 2014.09.06 8 7 6 S16W07 0030 DAO DRO    
S3804 2014.09.06   8 4 S16W13 0030   BXO    
S3805 2014.09.06   4 2 S17E77 0030   BXO    
Total spot count: 70 126 70  
Sunspot number: 170 236 180  (total spot count + 10 * number of spotted regions)
Weighted SN: 121 168 112  (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): 102 83 99 k * (sunspot number). k = 0.6 for SWPC, k = 0.35 for MSN 2K, k = 0.55 for MSN 1K (MSN=Magnetic Sunspot Number)

Monthly solar cycle data

Month Average solar flux International sunspot number
(WDC-SILSO)
Smoothed sunspot number Average ap
(3)
Measured 1 AU
2013.05 131.4 134.3 78.7 59.9 (+2.0) 9.73
2013.06 110.1 113.7 52.5 62.6 (+2.7) 12.60
2013.07 115.5 119.3 57.0 65.5 (+2.9) 9.47
2013.08 114.6 118.3 66.0 69.0 (+3.5) 8.27
2013.09 102.6 103.7 36.9 73.1 (+4.1) 5.23
2013.10  132.1 131.2 85.6 75.0 (+1.9) 7.71
2013.11  148.3 145.1 77.6 75.4 (+0.4) 5.68
2013.12 147.7 143.1 90.3 76.0 (+0.6) 4.68
2014.01 157.4 152.4 81.8 77.3 (+1.3) 5.44
2014.02 170.3
(cycle peak)
166.3 102.3 (cycle peak) 78.4 (+1.1) 10.70
2014.03 149.9 148.5 91.9 (80.3 projected, +1.9) 4.88
2014.04 143.9 144.8 84.7 (81.0 projected, +0.7) 7.88
2014.05 129.7 132.9 75.2 (79.2 projected, -1.8) 5.75
2014.06 122.0 125.8 71.0 (76.6 projected, -2.6) 6.72
2014.07 137.4 141.8 72.5 (73.6 projected, -3.0) 4.50
2014.08 124.6   74.7 (70.1 projected, -3.5) 7.71
2014.09 141.0 (1)   24.4 (2A) / 122.2 (2B) / 71.7 (2C) (65.9 projected, -4.2) (7.5)

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 WDC-SILSO international sunspot number is typically 30-50% lower. 2B) Boulder SN current month average to date. 2C) STAR SDO 1K Wolf number 30 day average.
3) Running average based on the quicklook and definitive Potsdam WDC ap indices. Values in red are based on the definitive international GFZ Potsdam WDC ap indices.

This report has been prepared by Jan Alvestad. It is based on the 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.