Solar Terrestrial Activity Report

Activity chart

Last major update issued on August 24, 2025 at 16:10 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 3, 2025)
Solar cycle Solar cycles 23-25 (August 1, 2025) Historical solar and geomagnetic data charts 1954-2006 (April 5, 2007)
  Cycle 24-25 progress (August 1, 2025) Noon SDO sunspot count 1K image / 4K (*)
  Solar cycles 1-24 (August 1, 2020) POES auroral activity level [October 2009 - December 2012]
  Comparison of cycles 21-25 (August 1, 2025) 3rd SSN Workshop, Tucson, 2013
  Comparison of cycles 12-14, 16, 24-25 (August 1, 2025) 4th SSN Workshop, Locarno, 2014
  Solar polar fields vs. solar cycles (August 17, 2025) Cycle 25 spots (final update December 25, 2019)
  Solar cycles 24-25 transition using 365d smoothing  

Recent activity

The geomagnetic field was at quiet levels on August 23. Solar wind speed at SOHO ranged between 396 and 497 km/sec, averaging 450 km/sec (-68 km/sec compared to the previous day). The high latitude magnetometer at Andenes recorded quiet to minor storm levels. The above 10 MeV proton flux increased slowly and was at 1.3 pfu at the end of the UT day.

Solar flux density measured at 17h UT on 2.8 GHz was 142.5 - decreasing 2.5 over the previous solar rotation. The 365 day average solar flux at 1 AU was 172.67 (183 days ago). The 81 day average solar flux at 1 AU was 139.2 (41 days ago, this is 44.4% of the total SC25 solar flux range from the max 81 day average peak on September 4, 2024 at 227.3 and an average 81 day flux of 69 at solar minimum). SC25 365d peak: 195.86 on October 13, 2024. The Potsdam WDC planetary A index was 4 (STAR Ap - based on the average of three hour interval ap indices: 4.5). Three hour interval K indices: 22111012 (planetary), 23122321 (Boulder), 53211123 (Andenes).

The background x-ray flux is at the class C2 level (GOES 19).

At the time of counting spots (see image time), spots were observed in 13 active regions using 2K resolution (SN: 196) and in 10 active regions using 1K resolution (SN: 128) SDO/HMI images.

AR 14187 [S20W47] decayed slowly and quietly.
AR 14188 [S09E06] was quiet and stable.
AR 14189 [N08W10] decayed slowly and quietly.
AR 14191 [N10E40] developed significantly as new flux emerged in the intermediate spot section. A major flare is possible even though only minor polarity intermixing was observed. C1 flares: C1.7 @ 05:29, C1.6 @ 07:14, C1.9 @ 12:52 UT

Note that SWPC/USAF has not published any SRS data the last days.

Spotted regions not observed (or interpreted differently) by SWPC/USAF:
S11356 [N22W27] reemerged with tiny spots.
S11358 [N10W23] reemerged with tiny spots.
S11368 [S27W03] developed slowly and quietly.
S11373 [N02E27] developed slowly and quietly.
S11374 [S18E68] was quiet and stable.
New AR S11375 [S15E80] rotated into view with a few spots. C1 flares: C1.6 @ 05:54 UT
New AR S11376 [S11E78] rotated into view with a small spot.
New AR S11377 [S09W08] emerged with a tiny spot.

There's a lot of activity behind the east limb as observed in SDO/AIA imagery. The AR that released the huge CME on August 21 could rotate into view on August 24-25.

C2+ flares

Magnitude Peak time (UT) Location Source Recorded by Comment
C2.2 02:04   14191 GOES18  
C2.8 06:29 N12E54 14191 GOES18  
C2.0 09:19 southeast limb S11375 GOES18 LDE
C2.3 11:35 southeast limb S11375 GOES18  
C2.1 12:10 southeast limb S11375 GOES18  
C3.2 13:32 N12E51 14191 GOES18  
C2.0 14:08 southeast limb S11375 GOES18  
C2.2 14:24 southeast limb S11375 GOES18  
C3.0 14:54 southeast limb S11375 GOES18  
C2.6 15:16 southeast limb S11375 GOES18  
C2.2 16:32 southeast limb S11375 GOES18  
C3.5 18:50 southeast limb S11375 GOES18  
C9.1 19:22 N12E46 14191 GOES18  
C8.3 19:32   14191 GOES18  
M1.9 20:06 southeast limb S11375 GOES18  
C5.7 20:44   14191 GOES18  
C6.0 20:49 southeast limb S11375 GOES18  
C4.8 21:10 southeast limb S11375 GOES18  
C5.5 22:56 southeast limb S11375 GOES18  
C6.2 23:19 southeast limb S11375 GOES18  
C3.7 00:04 southeast limb S11375 GOES18 flare started at 23:56

Coronal mass ejections (CMEs)

August 22-23: No obviously Earth directed CMEs.
August 21: One of the most impressive full halo CMEs of solar cycle 25 was observed in LASCO imagery starting at 08:24 UT. The source was 3-4 days behind the northeast limb based on mass distribution. The CME was very fast with no Earth directed components.

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 negative polarity northern hemisphere coronal hole (CH1313) was Earth facing on August 22-24.

Forecast

The geomagnetic field is expected to be at quiet levels on August 24. Quiet to active levels are possible on August 25-27 due to effects associated with CH1313.

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
STAR SWPC STAR Current Previous
2K 1K
14182 2025.08.12
2025.08.13
      N10W69          

was AR S11340

location: N09W65

S11354 2025.08.16   1   S20W32 0001   AXX  
14187 2025.08.17
2025.08.18
  2 1 S19W49 0010   HRX was AR S11355

location S20W47

S11356 2025.08.17   2   N22W27          
S11358 2025.08.17   6 2 N10W23 0010   AXX    
14188 2025.08.17
2025.08.18
  6 2 S09E04 0070   CSO was AR S11359

location: S09E06

14189 2025.08.18
2025.08.19
  4 2 N08W10 0020   HRX was AR S11360
14190 2025.08.19
2025.08.20
      N19E14         was AR S11362
14191 2025.08.20
2025.08.20
  29 12 N10E37 0670   EHC beta-gamma

was AR S11363

location: N10E40

S11364 2025.08.20       N19W58            
S11365 2025.08.20       N36W23            
S11368 2025.08.20   4 2 S27W03 0010   CRO  
14192 2025.08.21
2025.08.21
      N26W57           was AR S11369
S11371 2025.08.21       S40W17            
S11373 2025.08.22   7 4 N02E27 0040   DRO  
S11374 2025.08.22   1 1 S18E68 0030   HSX  
S11375 2025.08.23   2 1 S15E80 0090   HAX    
S11376 2025.08.23   1 1 S11E78 0030   HSX    
S11377 2025.08.23   1   S09W08 0001   AXX    
Total spot count:   66 28  
Sunspot number: 87 196 128  (total spot count + 10 * number of spotted regions)
Weighted SN:   108 70  (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): 96 108 102  

Monthly solar cycle data

Month Average solar flux International sunspot number
(WDC-SILSO)
Smoothed sunspot number (4) Average ap
(3)
Measured 1 AU
2024.02 172.5 168.3 123.0 136.9 (+5.7) 5.31
2024.03 154.4 152.9 103.7 141.4 (+4.5) 11.03
2024.04 161.3 162.6 137.0 144.5 (+3.1) 9.69
2024.05 187.7 191.9 172.1 149.1 (+4.6) 23.56
(SC25 peak)
2024.06 184.3 190.2 164.1 152.8 (+3.7) 10.24
2024.07 196.6 203.0 196.8 155.0 (+2.3) 7.13
2024.08  246.1
(cycle peak)
252.2 216.0  (SC25 peak) 156.8 (+1.8) 15.96
2024.09 195.7 197.8 141.1 159.4 (+1.6) 15.36
2024.10 221.0 219.6 165.8 160.9 (+1.5) (SC25 solar max) 18.99
2024.11 199.6 195.3 154.1 157.1 (-3.8) 9.33
2024.12 197.3 191.2 154.6 151.3 (-5.8) 8.42
2025.01 190.3 184.2 137.0 146.3 (-5.0) 13.17
2025.02  184.2 179.7 155.7 (139.4 projected, -6.9) 14.42
2025.03 163.7 162.1 134.2 (133.4 projected, -6.0) 15.96
2025.04 162.5 163.6 140.6 (129.3 projected, -4.1) 17.62
2025.05  135.3 138.3 79.2 (124.4 projected, -4.9) 17.26
2025.06 131.3 135.4 116.3 (119.6 projected, -4.8) 21.43
2025.07 137.8 142.3 125.6 (115.6 projected, -4.0) 11.80
2025.08 137.3 (1)   87.7 (2A) / 118.3 (2B) / 140.5 (2C) (110.9 projected, -4.7) (11.1)
2025.09       (106.5 projected, -4.4)  
2025.10       (102.6 projected, -3.9)  
2025.11       (100.3 projected, -2.3)  
2025.12       (98.7 projected, -1.6)  
2026.01       (94.6 projected, -4.1)  

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 27 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 June 23, 2025

Sunspot activity has been on a decreasing trend since September 2024 (using the average solar flux over 3 solar rotations as a proxy). Compared to the peak of SC25 solar flux has been at a low level in both May and June 2025. Taking a closer look at the 81 day (3 solar rotations) average solar flux proxy, its peak was in early September 2024 and had on May 12 decreased to less than half of the solar cycle flux range. Subtracting the 81 day average of approximately 69 at solar cycle minimum from all measurements, the SC25 range is 0 - 158.3.

All 365 day smoothed sunspot numbers peaked on October 11-12, 2024
, very likely making this the peak of SC25 (365 day smoothed peaks: STAR 1K: 236.1, STAR 2K: 364.3, NOAA SN: 156.0, ISN: 163.9). The 365d smoothed solar flux peaked on October 13, 2024, just 1.7% below the SC23 peak, and 62.6% above the SC24 peak.

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This report has been prepared by Jan Alvestad. It is based on the analysis of data from whichever 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.