Solar Terrestrial Activity Report

Activity chart

Last major update issued on August 14, 2015 at 03:55 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 (July 18, 2015)  

Recent activity

The geomagnetic field was quiet to unsettled on August 13. Solar wind speed at SOHO ranged between 322 and 360 km/s.

Solar flux at 20h UTC on 2.8 GHz was 94.8 (decreasing 2.6 over the last solar rotation). The 90 day 10.7 flux at 1 AU was 114.9. The Potsdam WDC planetary A index was 9 (STAR Ap - based on the mean of three hour interval ap indices: 8.8). Three hour interval K indices: 33222111 (planetary), 34322211 (Boulder).

The background x-ray flux is at the class B2 level.

At the time of counting spots (see image time), spots were observed in 8 active regions using 2K resolution (SN: 129) and 6 active regions using 1K resolution (SN: 85) SDO images on the visible solar disk.

Region 12396 [S18W80] decayed very quickly with no spots retaining mature penumbra by the end of the day.
Region 12398 [N18W15] lost the leading polarity spots.
Region 12400 [N17E08] developed slowly and quietly.
New region 12401 [S11E51] emerged on August 12 with SWPC numbering the region the following day. The region is compact and a magnetic delta has formed. The region is small and growing and has produced several small C flares early on August 14. A minor M class event is possible.

Spotted regions not numbered (or interpreted differently) by SWPC:
S4686 [S02W22] developed early in the day, then decayed and lost the leading polarity spot.
New region S4687 [S07E54] emerged early in the day and decayed slowly towards the end of the day.
New region S4688 [N20E18] was observed with penumbra spots.
New region S4689 [S23E01] was observed with a penumbra spot.

C2+ flares:

Magnitude Peak time (UTC) Location AR Recorded by Comment
           

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

Coronal mass ejections (CMEs)

August 11, 13: No obviously Earth directed CMEs were observed.
August 12: A partial halo CME was observed after multiple filament eruptions in the southwest quadrant. The first eruption began after 14h UTC and likely triggered a second eruption close to CH682.

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 (CH682) was in an Earth facing position on August 12-13. An extension of a northern hemisphere coronal hole (CH683) will likely rotate across the central meridian on August 15-17. A co-rotating interaction region may be associated with CH683 and could cause a geomagnetic disturbance on August 17-19.

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 poor.

Forecast

The geomagnetic field is expected to be quiet on August 14. A high speed stream associated with CH682 could cause unsettled and active conditions on August 15-16. A CME associated with a filament eruption observed on August 12 could arrive late on August 15 and contribute to the ongoing disturbance.

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
12395 2015.08.02
2015.08.03
      N12W70            
12396 2015.08.03 9 13 8 S18W79 0230 EAC ERI area: 0080
S4667 2015.08.04       S18W50            
12398 2015.08.06
2015.08.07
  2 1 N16W22 0006   AXX location: N18W15
S4679 2015.08.09       S17W42            
12399 2015.08.10
2015.08.11
      S16W28          
12400 2015.08.11 7 12 6 N17E07 0050 DAO DAO area: 0120
S4683 2015.08.12       N03W45          
S4684 2015.08.12       N20W56          
12401 2015.08.12
2015.08.13
5 15 8 S11E50 0010 BXO DRI beta-delta

area: 0060

S4686 2015.08.12   1   S02W22 0002   AXX  
S4687 2015.08.13   1 1 S07E54 0003   AXX    
S4688 2015.08.13   4 1 N20E18 0010   BXO    
S4689 2015.08.13   1   S23E01 0002   AXX    
Total spot count: 21 49 25  
Sunspot number: 51 129 85  (total spot count + 10 * number of spotted regions)
Weighted SN: 31 60 36  (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): 56 71 72 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) 8.8
2015.08 (108.2)   30.6 (2A) / 73.0 (2B) / 74.9 (2C) (69.0 projected, -1.2) (8.3)

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.