Solar Terrestrial Activity Report

Activity chart

Last major update issued on September 26, 2014 at 05:20 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 25. Solar wind speed at SOHO ranged between 427 and 508 km/s under the influence of a high speed stream from CH636.

Solar flux at 20h UTC on 2.8 GHz was 158 (increasing 38.1 over the last solar rotation). The 90 day 10.7 flux at 1 AU was 136.8. The Potsdam WDC planetary A index was 11 (STAR Ap - based on the mean of three hour interval ap indices: 10.8). Three hour interval K indices: 42232123 (planetary), 43423324 (Boulder).

The background x-ray flux is at the class B8 level.

At the time of counting spots (see image time), spots were observed in 11 active regions using 2K resolution (SN: 306) and 11 active regions using 1K resolution (SN: 230) SDO images on the visible solar disk.

Region 12169 [N06W42] decayed slowly and quietly.
Region 12170 [N10W38] decayed  further and could soon become spotless.
Region 12171 [S12W11] developed in the trailing spot section as new flux emerged. The new spots could be a region by itself.
Region 12172 [S11E12] displayed no major changes and still has a weak magnetic delta structure in a central penumbra. M class flares are possible.
Region 12173 [S16E02] reformed with new flux emerging quickly.
New region 12175 [N14W11] was first observed with spots on September 21 with SWPC numbering the region 4 days later. Quick growth started on September 24 and continued the next day with a small magnetic delta structure forming in a trailing penumbra. The magnetic layout of the region suggests that this is actually two closely spaced regions with the smallest region in the north.
New region 12176 [N07E44] rotated into view on September 22 and was numbered by SWPC 3 days later.
New region 12177 [N12E80] rotated into view and may be capable of M class flaring.

Spotted regions not numbered (or interpreted differently) by SWPC:
S3837 [N15W26] reemerged with a penumbra spot.
New region S3847 [N01W22] emerged with a penumbra spot.
New region S3848 [S13E66] emerged with penumbra spots.

C2+ flares (GOES):

Magnitude Peak time (UTC) Location AR Comment
C2.5 13:53   12175  
C3.2 (LDE) 20:32   12171  
C5.6 22:09 N13W10 12175  

Coronal mass ejections (CMEs)

September 23-25: No obviously Earth directed CMEs were observed in LASCO and STEREO imagery. A large backsided northern hemisphere CME was observed late on September 24, this CME was associated with a minor enhancement in proton levels.

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 fair to good.

Forecast

The geomagnetic field is expected to be quiet to unsettled with a chance of active intervals on September 26-28 due to coronal hole effects.

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 3 3 N06W43 0010 AXX AXX

 

12170 2014.09.16
2014.09.17
1 4 1 N11W40 0010 AXX HRX

location: N10W38

12168 2014.09.16
2014.09.17
      S22W66           plage
12171 2014.09.18
2014.09.19
11 32 19 S12W15 0100 EAO FAC area: 0260
12173 2014.09.19
2014.09.20
  20 15 S15W00     DRI   location: S16E02
12172 2014.09.20 29 72 40 S11E09 0450 EKC EKC beta-gamma-delta

area: 0960

location: S11E12

12175 2014.09.21
2014.09.25
25 48 30 N15W12 0080 CAI DAC beta-gamma-delta

area: 0420

location: N14W11 

S3836 2014.09.22       S11W31           plage
S3837 2014.09.22   1 1 N15W26 0003   AXX    
12176 2014.09.22
2014.09.25
1 8 5 N06E41 0010 AXX BXO location: N07E44
S3842 2014.09.23       S20W29           plage
S3843 2014.09.24       N11E10         plage
S3844 2014.09.24       N17W15         plage
S3845 2014.09.24       S24W32         plage
12177 2014.09.25 1 5 4 N12E75 0030 HSX DAO   location: N12E80

area: 0230

S3847 2014.09.25   1 1 N01W22 0004   AXX    
S3848 2014.09.25   2 1 S13E66 0013   BXO    
Total spot count: 69 196 120  
Sunspot number: 139 306 230  (total spot count + 10 * number of spotted regions)
Weighted SN: 94 227 100  (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): 83 107 127 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
2014.09 140.7 (1)   100.4 (2A) / 120.4 (2B) / 85.8 (2C) (65.9 projected, -4.2) (9.4)

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.