Solar Terrestrial Activity Report

Activity chart

Last major update issued on August 16, 2023 at 06:35 UT.

Charts (* = updated daily) Data and archive
  Solar wind (*) Solar and geomagnetic data - last month (*)
  Electron fluence (*) Archived daily reports and monthly data since 2003.01 (August 5, 2023)
Solar cycle Solar cycles 23-25 (August 1, 2023) Historical solar and geomagnetic data charts 1954-2006 (April 5, 2007)
  Cycle 24-25 progress (August 1, 2023) Noon SDO sunspot count 1K image / 4K (*)
  Solar cycles 1-24 (July 1, 2020) POES auroral activity level [October 2009 - December 2012]
  Comparison of cycles 21-25 (August 1, 2023) 3rd SSN Workshop, Tucson, 2013
  Comparison of cycles 12-14, 16, 24-25 (August 1, 2023) 4th SSN Workshop, Locarno, 2014
  Solar polar fields vs. solar cycles (July 10, 2023) Cycle 25 spots (final update December 25, 2019)
  Solar cycles 24-25 transition using 365d smoothing Research: Solar Cycle 25 Started on November 17, 2019 with 365 Days Smoothing

Recent activity

The geomagnetic field was very quiet on August 15. Solar wind speed at SOHO ranged between 279 and 329 km/sec. The high latitude magnetometer at Andenes recorded quiet to unsettled levels.

Solar flux density measured at 20h UT on 2.8 GHz was 158.1 - decreasing 30.8 over the previous solar rotation. (Centered 1 year average SF at 1 AU - 183 days ago: 152.07. In comparison SC24 peaked on June 28, 2014 at 145.50). 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: 10011011 (planetary), 11112321 (Boulder), 21012133 (Andenes).

The background x-ray flux is at the class B8 level (GOES 16).

At the time of counting spots (see image time), spots were observed in 16 active regions using 2K resolution (SN: 277) and in 14 active regions using 1K resolution (SN: 190) SDO/HMI images.

Region 13395 [N13W82] decayed slowly and was mostly quiet. C1 flares: C1.1 @ 05:17 UT
Region 13397 [N19W57] decayed slowly and quietly.
Region 13403 [N26E05] developed further and could produce a minor M class flare. C1 flares: C1.4 @ 19:08, C1.6 @ 19:30 UT
Region 13404 [S08E47] was quiet and stable.
Region 13405 [N10E62] produced a few C flares and was mostly unchanged. C1 flares: C1.2 @ 02:17, C1.4 @ 11:16 UT
New region 13406 [S18W17] emerged on August 13 and was numbered by SWPC 2 days later as the region developed slowly.
New region 13407 [S18E23] emerged on August 14 and gained area and spots the following day when it was numbered by SWPC.

Spotted regions not observed (or interpreted differently) by SWPC/USAF:
S8848 [N21W18] was quiet and stable.
S8850 [N23E21] was mostly quiet and stable. C1 flares: C1.6 @ 01:56 UT
S8851 [N08W05] was quiet and stable.
S8856 [N19W03] developed slowly and quietly.
S8861 [S06E41] decayed slowly and quietly.
S8862 [N14W42] was quiet and stable.
S8863 [N27E66] was quiet and stable.
New region S8867 [N12E76] rotated into view with a mature spot.
New region S8868 [S18E09] emerged with a few spots.

AR 13394 produced a C1.8 flare from behind the southwest limb at 09:13 UT

C2+ flares:

Magnitude Peak time (UT) Location Source Recorded by Comment
C2.1 01:37 N21E32 S8850 GOES16  
C2.3 03:10   13405 GOES16  
C2.0 03:31   13405 GOES16  
C4.1 06:57 N12W80 13395 GOES16  
C2.9 11:33 N10E72 13405 GOES16  
C2.1 12:25   13405 GOES16  
C2.2 14:16   13395 GOES16  
C2.3 21:52 N10E63 13405 GOES16  

Coronal mass ejections (CMEs)

August 13-15: 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 northern hemisphere coronal hole (CH1164) was in an Earth facing position on August 12-13. A southern hemisphere coronal hole (CH1165) rotated across the central meridian on August 13-14.

Propagation

Long distance low and medium frequency (below 2 MHz) propagation along paths north of due west over upper middle and high latitudes is fair. Propagation on long distance northeast-southwest paths is poor.

Forecast

The geomagnetic field is expected to be quiet to unsettled on August 16-17 due to effects from CH1165, active intervals are possible. Quiet conditions are likely on August 18.

Coronal holes (1) Coronal mass ejections (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). 4K 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 officially numbered solar regions according to the Solar Region Summary provided by NOAA/SWPC, all other regions are numbered sequentially as they emerge using the STAR spot number. 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. SWPC data considered to be not sufficiently precise (location, area, classification) are colored red.

Active region SWPC date numbered
STAR detected
Spot count Location at midnight Area Classification SDO / HMI 4K continuum
image with magnetic polarity overlays
Comment
SWPC/
USAF
Magnetic
(SDO)
SWPC STAR Current Previous
2K 1K
13395 2023.08.03 2 3 1 N12W87 0010 AXX AXX

location: N13W82

13397 2023.08.06
2023.08.07
2 3 2 N18W58 0060 DSO DSO area: 0090

location: N19W57

13399 2023.08.06
2023.08.09
      S15W48         location: S16W34
S8837 2023.08.07       N04W48            
S8838 2023.08.07       S14W56            
S8839 2023.08.08       S28W24            
13400 2023.08.10
2023.08.11
      S14W62            
S8845 2023.08.10       S19W32            
S8847 2023.08.10       N12W44            
S8848 2023.08.10   6   N21W18 0010   BXO  
S8850 2023.08.11   5 2 N23E21 0010   BXO  
S8851 2023.08.11   8   N08W05 0020   BXO  
13402 2023.08.12
2023.08.13
      S18W75            
13403 2023.08.13
2023.08.13
18 30 17 N26E05 0200 DAO DAI

area: 0420

13406 2023.08.13
2023.08.15
3 12 5 S17W18 0010 BXO DRO location: S18W17

area: 0050

13404 2023.08.13
2023.08.14
3 4 2 S07E45 0060 CAO HAX area: 0080

location: S08E47

S8856 2023.08.13   12 5 N19W03 0040   DRO  
13405 2023.08.13
2023.08.14
3 6 3 N10E65 0160 DSO ESO area: 0220

location: N10E62

13407 2023.08.14
2023.08.15
6 11 6 S18E22 0030 CRO DAO area: 0280
S8861 2023.08.14   4 2 S06E41 0008   AXX  
S8862 2023.08.14   3 1 N14W42 0005   AXX  
S8863 2023.08.14   3 1 N27E66 0007   BXO  
S8864 2023.08.14       N19E22          
S8865 2023.08.14       S09E05          
S8866 2023.08.14       S33E23          
S8867 2023.08.15   1 1 N12E76 0120   HSX    
S8868 2023.08.15   6 2 S18E09 0030   CRO    
Total spot count: 37 117 50  
Sunspot number: 107 277 190  (total spot count + 10 * number of spotted regions)
Weighted SN: 60 156 89  (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): 118 152 152  

Monthly solar cycle data

Month Average solar flux International sunspot number
(WDC-SILSO)
Smoothed sunspot number (4) Average ap
(3)
Measured 1 AU
2014.02 170.3
(cycle peak)
166.3 146.1 (SC24 peak) 110.5 10.70
2014.04 143.9 144.8 112.5 116.4 (SC24 solar max) 7.88
2017.09 91.3 92.3 43.6 18.2 (-1.3) 18.22
(SC24 peak)
2019.11 70.2 68.7 0.5 2.0 (-0.6)
(Solar minimum using 365d smoothing:
November 17, 2019)
4.19
2019.12 70.8 68.6 1.6 1.8 (-0.2)
(ISN 13 months smoothed
solar minimum)
3.22
2022.01 103.8 100.5 55.3 60.1 (+4.2) 8.92
2022.02 109.1 106.5 60.9 64.7 (+4.6) 10.46
2022.03 117.0 115.8 78.6 68.7 (+4.0) 10.20
2022.04 130.8 131.7 84.0 73.0 (+4.3) 11.79
2022.05 133.8 136.8 96.5 77.4 (+4.4) 7.48
2022.06 116.1 119.8 70.3 81.1 (+3.7) 8.20
2022.07 125.4 129.5 91.4 86.7 (+5.6) 9.51
2022.08 114.2 117.1 74.6 92.5 (+5.8) 10.92
2022.09 135.1 136.5 96.0 96.4 (+3.9) 12.18
2022.10 133.5 132.7 95.5 98.7 (+2.3) 11.16
2022.11 123.4 120.7 80.5 101.0 (+2.3) 9.33
2022.12 147.9 143.4 112.8 106.6 (+5.6) 10.99
2023.01 182.4 176.6 143.6 113.3 (+6.7) 8.73
2023.02 167.2 163.2 110.9 (119.1 projected, +5.8) 14.48
(current
SC25 peak)
2023.03 157.2 155.6 122.6 (124.4 projected, +5.3) 14.42
2023.04 145.4 146.4 96.4 (130.5 projected, +6.1) 13.40
2023.05 155.6 159.2 137.9 (136.1 projected, +5.6) 10.67
2023.06 161.7 166.8 163.4 (139.3 projected, +3.2) 8.95
2023.07  176.4 182.2 159.1 (139.7 projected, +0.4) 8.15
2023.08  162.1 (1)   50.4 (2A) / 104.3 (2B) / 140.4 (2C) (141.5 projected, +1.8) (8.3)
2023.09       (145.0 projected, +3.5)  
2023.10       (146.8 projected, +1.8)  
2023.11       (149.4 projected max SC25, +2.6)  
2023.12       (148.6 projected, -0.8)  
2024.01       (145.7 projected, -2.9)  
2024.02       (144.3 projected, -1.4)  

1) Running average based on the daily 20:00 UTC observed solar flux value at 2800 MHz and any corrections applied to that measurement.
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) Source: WDC-SILSO, Royal Observatory Of Belgium, Brussels

Solar cycles 24-25

Smoothed SF and sunspot numbers

 

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.