Solar Terrestrial Activity Report

Activity chart

Last major update issued on September 22, 2025 at 05:35 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 (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 levels on September 21. Solar wind speed at SOHO ranged between 291 and 354 km/sec, averaging 327 km/sec (-59 km/sec compared to the previous day). A CIR associated with CH1317 is in progress early on September 22. The high latitude magnetometer at Andenes recorded quiet to unsettled 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 176.0 - increasing 1.1 over the previous solar rotation. The 365 day average solar flux at 1 AU was 169.09 (183 days ago). The 81 day average solar flux at 1 AU was 150.3 (41 days ago, this is 51.4% 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: 195.9 on October 13, 2024.

The Potsdam WDC planetary A index was 4 (STAR Ap - based on the average of three hour interval ap indices: 4.3). Three hour interval K indices: 11202111 (planetary), 12203222 (Boulder), 11112223 (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 19 active regions using 2K resolution (SN: 364) and in 16 active regions using 1K resolution (SN: 244) SDO/HMI images.

AR 14216 [N10W58] decayed slowly and quietly.
AR 14217 [S16W22] developed as new flux emerged around the large leading penumbra. C1 flares: C1.6 @ 03:13, C1.6 @ 10:01, C1.8 @ 20:24 UT
AR 14220 [S18W57] produced several low level C flares and was mostly unchanged.
AR 14221 [N03W26] decayed slowly and quietly.
AR 14223 [S18W02] decayed slowly and quietly.
AR 14224 [S11W27] decayed slowly and quietly.
AR 14225 [N09E14] decayed slowly and quietly.
AR 14226 [S10E59] developed slowly and was mostly quiet. C1 flares: C1.4 @ 01:35, C1.7 @ 03:34 UT
AR 14227 [S19E54] was mostly quiet and stable.
New AR 14228 [N04E68] rotated into view on September 20 and was numbered the next day by SWPC. C1 flares: C1.6 @ 12:03 UT

Spotted regions not observed (or interpreted differently) by SWPC/USAF:
S11435 [N24W47] reemerged with a tiny spot.
S11443 [S24W21] was quiet and stable.
S11444 [S14W09] matured and produced a few C flares. C1 flares: C1.4 @ 08:04, C1.7 @ 19:49 UT. Note that this is currently AR 14224 to SWPC.
S11445 [N08E33] was quiet and stable.
S11446 [S10E08] was quiet and stable.
S11450 [S27E24] was quiet and stable.
New AR S11454 [N01E12] emerged with a tiny spot.
New AR S11455 [N30E60] emerged with a tiny spot.

A C1.6 flare at 07:27 and a C1.4 flare at 13:04 UT had their origin behind the southeast limb.
A C1.5 flare at 08:36 UT was produced by AR 14219 at the northwest limb.

C2+ flares

Magnitude Peak time (UT) Location Source Recorded by Comment
C2.4 05:06   14217 GOES18  
C2.7 05:33   14220 GOES18  
C2.1 06:46   14220 GOES18  
C2.1 14:45 S16W14 14217 GOES18  
C2.3 17:08   14220 GOES18  
C3.3 17:43   S11444 GOES18  
C6.6 21:16   S11444 GOES18  
C2.7 21:31   S11444 GOES18  

Coronal mass ejections (CMEs)

September 19-21: 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 northern hemisphere negative polarity coronal hole (CH1317) was Earth facing on September 19-21.

Forecast

The geomagnetic field is expected to be at quiet to minor storm levels on September 22-24 due to effects related to CH1317.

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
14216 2025.09.10
2025.09.11
7 9 4 N11W59 0070 CSO CSO

was AR S11423

area: 0140

location: N10W58

14220 2025.09.12
2025.09.15
20 23 17 S18W55 0300 EKI EHI

was AR S11429

area: 0400

location: S18W57

14217 2025.09.13
2025.09.14
10 31 17 S17W19 0210 EAO DKI

was AR S11433

location: S16W22

area: 0320

S11435 2025.09.13   1 1 N24W47 0006   AXX    
14221 2025.09.14
2025.09.15
4 7 1 N04W25 0090 CSO CSO

was AR S11436

area: 0150

location: N03W26

S11437 2025.09.14       N23W54            
S11438 2025.09.14       S13W36            
14222 2025.09.16       N13W49           trailing spots of AR 14216
14223 2025.09.15
2025.09.16
1 12 4 S17W07 0040 CAO CRO

was AR S11439

location: S18W02

14224 2025.09.15
2025.09.16
7 5   S13W08 0050 DAI AXX was AR S11440

SWPC data correspond to that of AR S11444. The location of the original AR 14224 was S11E17 on 2025.09.18 and S11E02 on 2025.09.19.

actual location: S11W27

area:0007

S11441 2025.09.16   4 1 N14E07 0007   BXO  
14225 2025.09.16
2025.09.16
4 19 7 N09E14 0220 DAO CKO

was AR S11442

area: 0330

S11443 2025.09.18   4 2 S24W21 0010   BXO  
S11444 2025.09.18   23 11 S14W09 0180   DAI

SWPC has moved AR 14224 to this AR

S11445 2025.09.18   9 4 N08E33 0020   BXO  
S11446 2025.09.19   7 3 S08E19 0015   BXO  
14227 2025.09.19
2025.09.20
2 7 4 S19E53 0080 CAO HAX was AR S11448

area: 0150

location: S19E54

14226 2025.09.19
2025.09.20
2 8 6 S09E56 0060 DSO DSO was AR S11449

location: S10E59

area: 0270

S11450 2025.09.19   2   S27E24 0004   AXX  
S11451 2025.09.19       S31W16            
S11452 2025.09.20       N25E27          
14228 2025.09.20
2025.09.21
1 1 1 N04E66 0010 HSX HSX was AR S11453

area: 0090

location: N04E68

S11454 2025.09.21   1 1 N01E12 0003   AXX    
S11455 2025.09.21   1   N30E60 0001   AXX    
Total spot count: 57 174 84  
Sunspot number: 157 364 244  (total spot count + 10 * number of spotted regions)
Weighted SN: 107 237 147  (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): 173 200 195  

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) 9.97
2025.09 146.1 (1)   81.1 (2A) / 115.8 (2B) / 148.1 (2C)
ISN average to date: 122. At this level the SSN
for March 2025 will become 135.7
(109.7 projected, -4.4) (12.4)
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.