Solar Terrestrial Activity Report

Activity chart

Last major update issued on August 29, 2015 at 06:00 UT.

Charts (* = updated daily) Data and archive
  Solar wind (*) Solar and geomagnetic data - last month (*)
  Electron fluence (*) Archived daily reports and monthly data from 2003.01 (August 1, 2015)
Solar cycle Solar cycles 23-24 (August 1, 2015) Historical solar and geomagnetic data charts 1954-2006 (April 5, 2007)
  Cycle 24 progress (August 1, 2015) Noon SDO sunspot count 1K Reference: 4K (large file) (*)
  Solar cycles 1-24 (July 17, 2015) POES auroral activity level October 2009 - December 2012
  Comparison of cycles 21, 22, 23 and 24 (August 1, 2015) 3rd SSN Workshop, Tucson, 2013
  Comparison of cycles 12, 13, 14, 16 and 24 (August 1, 2015) 4th SSN Workshop, Locarno, 2014
  Solar polar fields vs solar cycles (August 18, 2015)  

Recent activity

The geomagnetic field was unsettled to major storm on August 28. Solar wind speed at SOHO ranged between 313 and 433 km/s. A moderately high speed stream associated with CH685 became the dominant solar wind source after 16h UT in a clear transition from the disturbance which began on August 26. No co-rotating interaction region effects were observed.

Solar flux at 20h UTC on 2.8 GHz was 109.1 (increasing 6.2 over the last solar rotation). The 90 day 10.7 flux at 1 AU was 115.2. The Potsdam WDC planetary A index was 39 (STAR Ap - based on the mean of three hour interval ap indices: 38.9). Three hour interval K indices: 54335564 (planetary), 44335554 (Boulder).

The background x-ray flux is at the class B7 level.

At the time of counting spots (see image time), spots were observed in 8 active regions using 2K resolution (SN: 142) and 7 active regions using 1K resolution (SN: 100) SDO images on the visible solar disk.

Region 12403 [S15W70] decayed further losing spots and penumbral area. The magnetic delta in the leading spot section is still present and further M class flaring is possible while the region rotates over the southwest limb.
Region 12405 [S22E36] decayed slowly and quietly.

Spotted regions not numbered (or interpreted differently) by SWPC:
S4703 [N14W09] was quiet and stable.
S4714 [S05E03] was quiet and stable.
S4715 [N12E17] was quiet and stable.
New region S4717 [N02E50] emerged with a few spots.
New region S4720 [S17E38] emerged with a few spots to the north of AR 12405.
New region S4721 [S20E20] emerged with a penumbra spot.

C2+ flares:

Magnitude Peak time (UTC) Location AR Recorded by Comment
C8.0 02:51 S13W59 12403 GOES15  
C4.5 06:28   12403 GOES15  
C3.7 08:19 S14W63 12403 GOES15  
C5.3 11:44   12403 GOES15  
C2.6 12:55   12403 GOES15  
M2.2/1F 13:16 S14W65 12403 GOES15  
C2.0 17:38   12403 GOES15  
M2.1/1N 19:03 S13W70 12403 GOES15  
C4.6 19:39 S13W70 12403 GOES15  
C2.1 20:29   12403 GOES15  
C4.8 23:47 S14W75 12403 GOES15  

Flare activity (SDO/EVE/ESP XRS-B proxy)

Coronal mass ejections (CMEs)

August 26-28: No obviously Earth directed CMEs were observed.

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 coronal hole (CH685) was in an Earth facing position on August 25-26. Another recurrent trans equatorial coronal hole (CH686) will rotate across the central meridian on August 29-30.

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 active on August 29 becoming quiet to unsettled on August 30-31 due to effects from CH685. Quiet conditions are likely on September 1 while a disturbance associated with CH686 could cause quiet to active conditions on September 2-3.

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 overlays
Comment
SWPC Magnetic
(SDO)
SWPC STAR Current Previous
2K 1K
12403 2015.08.17
2015.08.18
27 26 15 S15W69 0840 FKC FKC beta-gamma-delta

area: 0650

location: S14W70

12404 2015.08.19
2015.08.20
      N14W88            
S4703 2015.08.22   12 6 N14W09 0025   BXO images/AR_S4703_20150828_2345.png images/AR_S4703_20150827_2345.png  
S4704 2015.08.22       S23W56            
S4706 2015.08.23       S15W35            
S4711 2015.08.25       S02W54            
S4712 2015.08.25       S13W46            
12405 2015.08.26
2015.08.27
3 10 3 S23E35 0010 BXO BXO area: 0025
S4714 2015.08.27   1 1 S03E05 0003   AXX  
S4715 2015.08.27   2 2 N12E17 0007   AXX  
S4717 2015.08.28   4 1 N02E50 0014   CRO    
S4720 2015.08.28   6 2 S17E38 0024   DRO    
S4721 2015.08.28   1   S20E20 0002   AXX    
Total spot count: 30 62 30  
Sunspot number: 50 142 100  (total spot count + 10 * number of spotted regions)
Weighted SN: 40 78 46  (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): 55 78 85 k * (sunspot number)
As of July 1, 2015: k = 1.1 for SWPC, k = 0.55 for MSN 2K, k = 0.85 for MSN 1K (MSN=Magnetic Sunspot Number)

Monthly solar cycle data

Month Average solar flux International sunspot number
(WDC-SILSO) (4)
Smoothed sunspot number (4) Average ap
(3)
Measured 1 AU
2014.02 170.3
(cycle peak)
166.3 146.1 (cycle peak) 110.5 (+1.2) 10.70
2014.03 149.9 148.5 128.7 114.3 (+3.8) 4.88
2014.04 143.9 144.8 112.5 116.4 (+2.1) (solar max) 7.88
2014.05 129.7 132.9 112.5 115.0 (-1.4) 5.75
2014.06 122.0 125.8 102.9 114.1 (-0.9) 6.72
2014.07 137.4 141.8 100.2 112.6 (-1.5) 4.50
2014.08 124.7 127.9 106.9 108.3 (-4.3) 7.71
2014.09 146.6 148.1 130.0 101.9 (-6.4) 9.78
2014.10 153.4 152.9 90.0 97.4 (-4.5) 8.96
2014.11 154.8 151.4 103.6 95.0 (-2.4) 9.33
2014.12 158.7 153.8 112.9 92.6 (-2.4) 11.24
2015.01 141.9 137.3 93.0 89.8 (-2.8) 9.46
2015.02 129.1 126.0 66.7 (86.8 projected, -3.0) 9.92
2015.03 125.9 124.6 54.5 (83.1 projected, -3.7) 16.14
2015.04 128.8 129.7 78.0 (79.8 projected, -3.3) 10.73
2015.05 120.0 122.6 90.0 (77.4 projected, -2.4) 8.29
2015.06 122.3 126.1 68.3 (73.9 projected, -3.5) 13.15
2015.07 107.0 110.8 66.4 (70.2 projected, -3.7) 8.83
2015.08 (106.6)   56.6 (2A) / 62.6 (2B) / 76.5 (2C) (69.0 projected, -1.2) (14.6)

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).
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.
4) Updated to new data set from WDC-SILSO on July 1, 2015

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 Universal Time. Comments and suggestions are always welcome.

SDO images are courtesy of NASA/SDO and the AIA, EVE, and HMI science teams.