Solar Terrestrial Activity Report

Activity chart

Last major update issued on August 22, 2023 at 07:25 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 quiet to unsettled on August 21 under the influence of high speed (negative polarity) coronal hole effects. Solar wind speed at SOHO ranged between 519 and 682 km/sec. The high latitude magnetometer at Andenes recorded quiet to active levels.

Solar flux density measured at 20h UT on 2.8 GHz was 148.7 - decreasing 20.3 over the previous solar rotation. (Centered 1 year average SF at 1 AU - 183 days ago: 152.73. In comparison SC24 peaked on June 28, 2014 at 145.50). The Potsdam WDC planetary A index was 8 (STAR Ap - based on the mean of three hour interval ap indices: 8.0). Three hour interval K indices: 22323121 (planetary), 21322222 (Boulder), 41233133 (Andenes).

The background x-ray flux is at the class B9 level (GOES 16).

At the time of counting spots (see image time), spots were observed in 10 active regions using 2K resolution (SN: 159) and in 9 active regions using 1K resolution (SN: 118) SDO/HMI images.

Region 13403 [N26W79] decayed slowly and was mostly quiet. C1 flares: C1.3 @ 01:23 UT
Region 13405 [N10W20] decayed slowly and quietly.
Region 13407 [S18W56] decayed slowly and quietly.
Region 13411 [N13W02] decayed slowly and quietly.
Region 13412 [N30E33] was quiet and stable.
New region 13413 [N10E71] rotated into view on August 20 and was numbered by SWPC the next day. C1 flares: C1.5 @ 05:28 UT
New region 13414 [S10E33] rotated into view on August 18 and received its NOAA number 3 days later.

Spotted regions not observed (or interpreted differently) by SWPC/USAF:
S8877 [N27W10] reemerged with tiny spots.
S8883 [N21E08] was quiet and stable.
S8884 [S13W34] developed slowly and quietly.

AR S8886 was numbered as it rotated into view early on August 22 at S11E88. The region produced several C flares during the day. C1 flares: C1.3 @ 07:30, C1.6 @ 10:21, C1.1 @ 11:37, C1.3 @ 19:09, C1.2 @ 19:34, C1.3 @ 20:45 UT

C2+ flares:

Magnitude Peak time (UT) Location Source Recorded by Comment
C2.0 05:44   S8886 GOES16  
C4.3 07:53   S8886 GOES16  
C3.1 08:47   S8886 GOES16  
C3.1 12:38 N26W76 13403 GOES16 simultaneous flare in AR S8886
C2.0 22:05   S8886 GOES16  
C4.7 23:43 N08E69 13413 GOES16  
C5.7 23:59   S8886 GOES16  

Coronal mass ejections (CMEs)

August 19-21: 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 southern hemisphere coronal hole (CH1166) will likely rotate across the central meridian on August 23.

Propagation

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

Forecast

The geomagnetic field is expected to be quiet on August 21-23.

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
S8850 2023.08.11       N25W58            
13403 2023.08.13
2023.08.13
3 3 1 N26W75 0110 CSO HSX

area: 0180

location: N26W79

13404 2023.08.13
2023.08.14
2     S11W33 0020 CAO     spotless

location: S09W31

apparently SWPC is counting the spots of AR S8844

13409 2023.08.13
2023.08.16
      N22W84        

location: N20W81

13405 2023.08.13
2023.08.14
1 6 4 N10W20 0110 HSX HSX area: 0200
13407 2023.08.14
2023.08.15
8 10 7 S19W58 0120 DAI DAO

location: S18W56

S8861 2023.08.14       S06W37            
S8864 2023.08.14       N19W56            
S8866 2023.08.14       S33W55            
13411 2023.08.15
2023.08.17
1 6 2 N13W02 0060 HSX HSX

area: 0090

13408 2023.08.15
2023.08.16
      S18W74          

location: S19W70

S8869 2023.08.16       N12W4|            
S8870 2023.08.16       N14W48            
S8872 2023.08.16       S25W54            
S8873 2023.08.16       N15W20            
13412 2023.08.17
2023.08.18
1 1 1 N30E34 0070 HSX HSX area: 0110

location: N30E33

S8875 2023.08.17       S22W41            
13414 2023.08.18
2023.08.21
5 15 6 S09E32 0020 CRO BXO location: S10E33
S8877 2023.08.18   3 1 N27W10 0007   BXO    
S8879 2023.08.18       N32W35            
S8880 2023.08.18       S01W05            
13413 2023.08.20
2023.08.21
1 5 2 N10E73 0150 HSX DHO area: 0430
S8883 2023.08.20   3   N21E08 0004   BXO  
S8884 2023.08.20   7 4 S13W34 0050   DRO  
S8885 2023.08.20       S26W11          
Total spot count: 22 59 28  
Sunspot number: 102 159 118  (total spot count + 10 * number of spotted regions)
Weighted SN: 60 97 66  (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): 112 87 94  

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  159.1 (1)   72.9 (2A) / 107.7 (2B) / 136.1 (2C) (141.5 projected, +1.8) (8.2)
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

Update on the progress of solar cycle 25 as of August 20, 2023

Looking back 6 months, the 365d smoothed values for solar flux and all sunspot numbers with the exception of NOAA's, are all above their solar cycle 24 peak. The first peak of solar cycle 25 is projected to be between July 7 and 10, 2023 (solar flux on July 7, ISN and STAR 1K and 2K all have that peak on July 9, while NOAA peaks on July 10). This is unlikely to be the final peak of SC25, there is only a small chance that it is the actual sunspot and solar flux maximum.

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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.