Solar Terrestrial Activity Report

Activity chart

Last major update issued on September 27, 2014 at 06:00 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)]

[New: Noon SDO count 1K 4K (large file)]

[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 active on September 26. Solar wind speed at SOHO ranged between 427 and 477 km/s under the influence of a high speed stream from CH636.

Solar flux at 20h UTC on 2.8 GHz was 170 (increasing 46.9 over the last solar rotation). The 90 day 10.7 flux at 1 AU was 137.4. The Potsdam WDC planetary A index was 13 (STAR Ap - based on the mean of three hour interval ap indices: 13.0). Three hour interval K indices: 33224323 (planetary), 34333423 (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 13 active regions using 2K resolution (SN: 350) and 10 active regions using 1K resolution (SN: 219) SDO images on the visible solar disk.

Region 12169 [N06W42] decayed slowly and quietly.
Region 12171 [S11W24] developed slowly and was mostly quiet.
Region 12172 [S11W02] gained a few spots while the central magnetic delta structure disappeared. A major flare is possible.
Region 12173 [S17W12] developed further and could produce a minor M class flare.
Region 12175 [N14W24] developed quickly and a magnetic delta structure in the southern part of a central penumbra formed. A major flare is possible.
Region 12176 [N07E31] decayed and could soon become spotless.
Region 12177 [N12E69] is a compact region which has minor M class flare potential. The region apparently had a magnetic delta structure early in the day.

Spotted regions not numbered (or interpreted differently) by SWPC:
S3848 [S14E52] was quiet and stable.
New region S3850 [S16E25] emerged with a penumbra spot.
New region S3851 [N10W03] emerged with a penumbra spot.
New region S3852 [S09W21] emerged with a few spots close to AR 12171.
New region S3853 [N29W19] emerged with a penumbra spot.
New region S3854 [N23W22] emerged with penumbra spots.

A region behind the southeast limb produced the most interesting flare of the day, this event was associated with a fast and impressive CME.

C2+ flares (GOES):

Magnitude Peak time (UTC) Location AR Comment
C8.6 (LDE) 05:44 behind SE limb   CME
C3.7 12:55   12177  
C4.2/1N 13:54 S11E04 12172  
C7.9 16:18 N13E75 12177  
C3.5 23:10 SE limb    

Coronal mass ejections (CMEs)

September 24-26: 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 southern hemisphere coronal hole was in an Earth facing position on September 22-25.

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 good.

Forecast

The geomagnetic field is expected to be quiet to unsettled with a chance of active intervals on September 27-28 due to coronal hole effects and quiet on September 29.

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
12169 2014.09.16
2014.09.17
1 1   N07W56 0000 AXX AXX

area: 0002

12170 2014.09.16
2014.09.17
2     N12W52 0010 AXX    

spotless

12168 2014.09.16
2014.09.17
      S22W80           plage
12171 2014.09.18
2014.09.19
10 23 9 S11W28 0130 EAO FAO location: S11W24
12173 2014.09.19
2014.09.20
16 34 21 S17W10 0050 CAO DAC area: 0170

location: S17W12

12172 2014.09.20 55 85 44 S11W05 0500 EKC EKC beta-gamma

area: 0910

location: S11W02

12175 2014.09.21
2014.09.25
30 45 31 N16W25 0240 DAC DKC beta-gamma-delta

area: 0790

location: N14W24 

S3836 2014.09.22       S11W44           plage
S3837 2014.09.22       N15W39         plage
12176 2014.09.22
2014.09.25
4 4 1 N07E28 0010 BXO AXX location: N07E31
S3842 2014.09.23       S20W42           plage
S3844 2014.09.24       N17W28           plage
S3845 2014.09.24       S24W45           plage
12177 2014.09.25 5 13 7 N12E67 0080 DAO EAC beta-gamma

location: N12E69

S3847 2014.09.25       N01W35         plage
S3848 2014.09.25   6 2 S14E52 0015   CRO  
S3850 2014.09.26   1   S16E25 0003   AXX    
S3851 2014.09.26   1 1 N10W03 0003   AXX    
S3852 2014.09.26   4 2 S09W21 0012   CRO    
S3853 2014.09.26   1   N29W19 0002   AXX    
S3854 2014.09.26   2 1 N23W22 0004   BXO    
Total spot count: 123 220 119  
Sunspot number: 203 350 219  (total spot count + 10 * number of spotted regions)
Weighted SN: 153 261 160  (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): 122 123 121 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
2014.08 124.7 127.9 74.7 (70.1 projected, -3.5) 7.71
2014.09 141.8 (1)   107.1 (2A) / 123.6 (2B) / 87.6 (2C) (65.9 projected, -4.2) (9.6)

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.