Solar Terrestrial Activity Report

Activity chart

Last major update issued on October 19, 2013 at 17:45 UTC. Updates are likely to be irregular or very late until October 25.

[Solar and geomagnetic data - last month (updated daily)]
[Solar wind and electron fluence charts (updated daily)]
[Solar cycles 23-24 (last update October 1, 2013)] [Cycle 24 progress (last update October 1, 2013) ]
[Solar cycles 1-20]
[Graphical comparison of cycles 21, 22, 23 and 24 (last update October 1, 2013)]
[Graphical comparison of cycles 10, 12, 13, 14, 16 and 24 (last update October 1, 2013)]
[Historical solar and geomagnetic data charts 1954-2006 (last update April 5, 2007)]
[Archived reports since January 2003 (last update October 9, 2013)]

[POES auroral activity level since October 2009 - updated January 26, 2013]
[Solar polar fields vs solar cycles - updated October 10, 2013]
[Presentation 3rd SSN Workshop, Tucson, 2013 (pdf)]

Recent activity

The geomagnetic field was quiet on October 18. Solar wind speed at SOHO ranged between 346 and 413 km/s.

Solar flux measured at 20h UTC on 2.8 GHz was 139.9 (increasing 29.6 over the last solar rotation). The 90 day 10.7 flux at 1 AU was 112.9. The Potsdam WDC planetary A index was 3 (STAR Ap - based on the mean of three hour interval ap indices: 3.0). Three hour interval K indices: 11100021 (planetary), 10112221 (Boulder).

The background x-ray flux was at the class B9 level.

At the time of counting spots (see image time) spots were observed in 16 active regions in 2K resolution (SN: 275) and 14 active regions in 1K resolution (SN: 207) SDO images on the visible solar disk.

Region 11861 [S08W80] failed to produce any major events despite the complexity of the region. C5+ flares: C5.0 at 10:34, C8.4 at 15:26 UTC.
Region 11864 [S22W71] was quiet and stable.

Region 11869 [N20W02] was quiet and stable.
Region 11870 [S15W59] was quiet and stable.
Region 11872 [S17E28] was quiet and stable.
Region 11873 [N11E36] lost all umbrae and had many penumbra spots.
Region 11874 [S11E07] decayed slowly and quietly.
Region 11875  [N07E59] developed slowly and has a small magnetic delta structure in the trailing spot section. A minor M class flare is possible.
New region 11877 [S12E77] rotated into view with a large spot.

Spotted regions not numbered by SWPC:
S2753 [N18E10] was quiet and stable.
S2760 [S10W34] reemerged with a penumbra spot.
S2764 [N22W16] developed as new flux emerged. The region has an east-west oriented inversion line.
New region S2769 [N17E54] emerged with penumbra spots.
New region S2770 [S22E06] emerged with penumbra spots.
New region S2771 [S13W08] emerged with a penumbra spot.
New region S2772 [N13W18] emerged with a penumbra spot.

Coronal mass ejections (CMEs)

October 16-18: 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 coronal hole (CH591) in the northern hemisphere rotated across the central meridian on October 17. CH591 may be too far to the north to cause geomagnetic effects.

Coronal hole map

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 to fair. Propagation on long distance northeast-southwest paths is poor.

Forecast

The geomagnetic field is expected to be quiet on October 19. There's a chance of weak coronal hole effects and quiet to unsettled conditions due to CH591 on October 20-21.

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 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 STAR SDO SWPC STAR Current Previous
2K 1K
11861 2013.10.06
2013.10.07
16 15 10 S07W79 0410 EKI FKC

beta-gamma

area: 0600

11864 2013.10.07
2013.10.08
1 2 2 S23W73 0020 HSX CSO

location: S22W71

11865 2013.10.08       S23W64           part of AR 11864
11876 2013.10.10
2013.10.17
      N05W75         plage
11868 2013.10.11
2013.10.13
4     N23W17 0010   BXO     actual location: N17W19, SWPC has moved this region to the location of AR S2764
11869 2013.10.12
2013.10.13
1 4 1 N19E07 0010 HSX BXO location: N20W02
S2753 2013.10.13   9 6 N18E10 0040   CRO  
11870 2013.10.13
2013.10.14
3 7 1 S15W58 0030 CAO CRO  
S2756 2013.10.13       S08W08           plage
11871 2013.10.14       N16E08           plage
11872 2013.10.14
2013.10.15
1 4 3 S16E28 0080 HSX HSX

area: 0120

11873 2013.10.14
2013.10.16
9 18 11 N11E36 0040 CSO BXI area: 0060
S2759 2013.10.14       S27W27           plage
S2760 2013.10.14   1   S10W34 0003   AXX    
11874 2013.10.16
2013.10.17
8 12 6 S10E07 0050 DAO DAO  
11875 2013.10.16
2013.10.17
10 23 16 N07E60 0150 CAO ESC area: 0250
S2764 2013.10.16   12 6 N22W16 0050   DRI  
S2767 2013.10.17       S05E40         plage
11877 2013.10.18 1 1 1 S11E75 0120 HSX HKX   area: 0320

location: S12E77

S2769 2013.10.18   2 2 N17E54 0008   BXO    
S2770 2013.10.18   3 1 S22E06 0009   AXX    
S2771 2013.10.18   1 1 S13W08 0004   AXX    
S2772 2013.10.18   1   N13W18 0002   AXX    
Total spot count: 54 115 67  
Sunspot number: 154 275 207  (total spot count + 10 * number of spotted regions)
Weighted SN: 104 164 116  (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): 92 96 114 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)
2011.11 153.5 (cycle peak) 96.7 (cycle peak) 61.1 (+1.2) 5.55
2012.02 106.5 32.9 66.9 (+1.4)
likely cycle 24 max
8.81
2012.06 119.6 64.5 58.9 (-2.8) 10.08
2012.07 133.9 66.5 57.8 (-1.1) 13.90
2012.08 115.4 63.0 58.2 (+0.4) 7.96
2012.09 122.9 61.4 58.1 (-0.1) 8.07
2012.10 123.3 53.3 58.6 (+0.5) 9.97
2012.11 121.3 61.8 59.7 (+1.1) 7.08
2012.12 108.6 40.8 59.6 (-0.1) 3.44
2013.01 127.1 62.9 58.7 (-0.9) 4.69
2013.02 104.3 38.0 58.4 (-0.3) 6.11
2013.03 111.3 57.9 57.5 (-0.9) 10.56
2013.04 124.8 72.4 (56.2 projected, -1.3) 5.40
2013.05 131.4 78.7 (55.8 projected, -0.4) 9.73
2013.06 110.1 52.5 (56.0 projected, +0.2) 12.60
2013.07 115.5 57.0 (56.1 projected, +0.1) 9.47
2013.08 114.6 66.0 (55.9 projected, -0.2) 8.27
2013.09 102.6 36.9 (55.4 projected, -0.5) 5.23
2013.10  119.3 (1) 60.3 (2A) / 103.8 (2B) / 60.2 (2C) (53.9 projected, -1.5) (10.78)

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) 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 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.