Solar Terrestrial Activity Report

Activity chart

Last major update issued on September 4, 2025 at 02:50 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 (September 1, 2025)
Solar cycle Solar cycles 23-25 (September 1, 2025) Historical solar and geomagnetic data charts 1954-2006 (April 5, 2007)
  Cycle 24-25 progress (September 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 (September 1, 2025) 3rd SSN Workshop, Tucson, 2013
  Comparison of cycles 12-14, 16, 24-25 (September 1, 2025) 4th SSN Workshop, Locarno, 2014
  Solar polar fields vs. solar cycles (August 17, 2025) Cycle 25 initial spots (final update December 25, 2019)
  Solar cycles 24-25 transition using 365d smoothing  

Recent activity

The geomagnetic field was at quiet to active levels on September 3 under the decreasing influence of CME effects.  Solar wind speed at SOHO ranged between 446 and 621 km/sec. The high latitude magnetometer at Andenes recorded quiet to minor storm levels. The above 10 MeV proton flux was at background levels all day.

Solar flux density measured at 20h UT on 2.8 GHz was 179.6 - increasing 28.0 over the previous solar rotation. The 365 day average solar flux at 1 AU was 171.91 (183 days ago). The 81 day average solar flux at 1 AU was 148.7 (41 days ago, this is 50.4% 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 11 (STAR Ap - based on the average of three hour interval ap indices: 10.8). Three hour interval K indices: 43222121 (planetary), 33221221 (Boulder), 54222241 (Andenes).

The background x-ray flux is at the class C1 level (GOES 19).

At the time of counting spots (see image time), spots were observed in 13 active regions using 2K resolution (SN: 269) and in 12 active regions using 1K resolution (SN: 185) SDO/HMI images.

AR 14197 [S18W67] decayed slowing and produced some low level C flares. C1 flares: C1.8 @ 02:27, C1.8 @ 16:50 UT
AR 14199 [N03W49] decayed slowly and was mostly quiet. C1 flares: C1.8 @ 22:53 UT
AR 14201 [S21W49] decayed slowly and quietly.
AR 14202 [S15W43] decayed slowly and quietly.
AR 14205 [N17E00] decayed slowly losing mature penumbra.
AR 14206 [N09E04] was quiet and stable.
AR 14207 [N29E20] displayed both decay and development. New intermediate spots emerged while both the leading and trailing penumbra lost area. C1 flares: C1.6 @ 12:36 UT
AR 14210 [N08E42] developed slowly and produced several C flares.
AR 14211 [S13E58] produced a few C flares and was otherwise unremarkable. C1 flares: C1.7 @ 14:05, C1.9 @ 16:57, C1.7 @ 17:28, C1.7 @ 19:08 UT

Spotted regions not observed (or interpreted differently) by SWPC/USAF:
S11400 [N18W29] was quiet and stable.
New AR S11404 [N10E25] was observed with tiny spots.
New AR S11405 [N28E06] was observed with tiny spots in an old plage area.
New AR S11406 [S03E37] was observed with tiny spots in an old plage area.

C2+ flares

Magnitude Peak time (UT) Location Source Recorded by Comment
C2.7 00:09   14197 GOES18  
C2.7 00:19   14197 GOES18  
C3.0 00:35   14197 GOES18  
C2.7 00:56   14210 GOES18  
C2.8 02:41 N09E54 14210 GOES18  
C2.9 03:59 N09E52 14210 GOES18  
C2.8 04:42   14211 GOES18  
C2.5 05:42   14197 GOES18  
C2.1 05:56   14211 GOES18  
C2.0 07:26   14210 GOES18  
C3.7 15:23 S13E73 14211 GOES18  
C2.4 15:51   14199 GOES18  
C2.8 18:00   14207 GOES18 simultaneous flare in AR 14197
C2.4 18:17   14197 GOES18  
C2.9 19:21 N32E23 14207 GOES18  
C2.3 21:30   14211 GOES18  
C3.4 00:01   14211 GOES18 flare started at 23:52 UT

Coronal mass ejections (CMEs)

September 1-3: No obviously Earth directed CMEs.

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 positive polarity southern hemisphere coronal hole (CH1315) will rotate into an Earth facing position on September 2-7. CH1315 has a poorly defined trans equatorial extension.

Forecast

The geomagnetic field is expected to be at mostly quiet levels on September 4. Quiet to minor storm levels are possible on September 5-9 due to effects associated with CH1315.

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
14195 2025.08.22
2025.08.2?
      S18W85           was AR S11374

location: S13W78

14197 2025.08.23
2025.08.24
14 26 12 S18W65 0480 FHI EHO

was AR S11375

area: 0630

location: S18W67

14196 2025.08.23
2025.08.24
      S11W71           was AR 11376

location: S12W64

14199 2025.08.24
2025.08.25
6 14 7 N04W51 0170 CSO CKO

was AR S11381

location: N03W49

area: 0270

14201 2025.08.24
2025.08.26
1 2 1 S21W51 0050 HSX HAX

was AR S11382

location: S21W49

14202 2025.08.25
2025.08.26
2 8 3 S14W46 0080 HSX CSO

was AR S11385

location: S15W43

14204 2025.08.27       N03W46           trailing part of AR 14199
14205 2025.08.28 2 9 4 N18W03 0040 HAX CRO was AR S11389

area: 0030

location: N17E00

14206 2025.08.28
2025.08.29
1 4 3 N08E01 0080 HSX HSX was AR S11390

location: N08E04

area: 0150

S11391 2025.08.28       N21W44            
14207 2025.08.29
2025.08.30
6 33 17 N30E24 0300 FHO FAI was AR S11394

location: N29E20

area: 0370

14209 2025.08.29
2025.09.02
      N18W56         was AR S11395
S11398 2025.08.30       S08W20          
S11400 2025.08.31   3   N18W29 0005   BXO  
14211 2025.09.01
2025.09.02
1 4 2 S14E56 0210 HSX CSO was AR S11401

area: 0250

location: S13E58

14210 2025.09.01
2025.09.02
5 18 11 N08E41 0140 DSO DSI was AR S11402

location: N08E42

area: 0280

S11404 2025.09.03   13 2 N10E25 0025   BXO    
S11405 2025.09.03   2 1 N28E06 0005   AXX    
S11406 2025.09.03   3 2 S03E37 0005   AXX    
Total spot count: 38 139 65  
Sunspot number: 128 269 185  (total spot count + 10 * number of spotted regions)
Weighted SN: 93 192 118  (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): 141 148 148  

Monthly solar cycle data

Month Average solar flux International sunspot number
(WDC-SILSO)
Smoothed sunspot number (4) Average ap
(3)
Measured 1 AU
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  184.2 179.7 155.7 139.9 (-6.4) 14.42
2025.03 163.7 162.1 134.2 (135.6 projected, -4.3) 15.96
2025.04 162.5 163.6 140.6 (132.5 projected, -3.1) 17.62
2025.05  135.3 138.3 79.2 (127.6 projected, -4.9) 17.26
2025.06 131.3 135.4 116.3 (122.8 projected, -4.8) 21.43
2025.07 137.8 142.3 125.6 (118.9 projected, -3.9) 11.80
2025.08 154.9 158.7 133.6 (114.1 projected, -4.8) 9.8
2025.09 189.8 (1)   15.6 (2A) / 156.0 (2B) / 153.2 (2C) (109.7 projected, -4.4) (18.3)
2025.10       (105.8 projected, -3.9)  
2025.11       (103.6 projected, -2.2)  
2025.12       (101.9 projected, -1.7)  
2026.01       (97.8 projected, -4.1)  
2026.02       (93.7 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.