Solar Terrestrial Activity Report

Activity chart

Last major update issued on October 9, 2025 at 03:30 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 (October 1, 2025)
Solar cycle Solar cycles 23-25 (October 1, 2025) Historical solar and geomagnetic data charts 1954-2006 (April 5, 2007)
  Cycle 24-25 progress (October 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 (October 1, 2025) 3rd SSN Workshop, Tucson, 2013
  Comparison of cycles 12-14, 16, 24-25 (October 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 October 8 under the influence of CME effects. Solar wind speed at SOHO ranged between 380 and 463 km/sec, averaging 413 km/sec (-34 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 was at background levels all day.

Solar flux density measured at 20h UT on 2.8 GHz was 119.6 - increasing 4.4 over the previous solar rotation.
The 365 day average solar flux at 1 AU was 166.30 (183 days ago). The 81 day average solar flux at 1 AU was 155.9 (41 days ago, this is 54.9% 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 10 (STAR Ap - based on the average of three hour interval ap indices: 10.0). Three hour interval K indices: 34222210 (planetary), 24324321 (Boulder), 55233432 (Andenes).

The background x-ray flux is at the class B5 level (GOES 19).

At the time of counting spots (see image time), spots were observed in 13 active regions using 2K resolution (SN: 201) and in 6 active regions using 1K resolution (SN: 90) SDO/HMI images.

AR 14232 [N03W88] rotated mostly out of view. C1 flares: C1.9 @ 04:37 UT
AR 14240 [N15W33] was quiet and stable.
AR 14241 [N12W55] decayed slowly and quietly.
AR 14242 [S12W34] produced a few low level C flares. C1 flares: C1.0 @ 05:15, C1.2 @ 12:48 UT
AR 14243 [N19W13] decayed slowly and quietly.
AR 14244 [S21E26] decayed slowly and quietly.
AR 14245 [S11W52] decayed slowly and quietly.
AR 14246 [N24E37] decayed slowly and quietly.
AR 14247 [S10E02] was quiet and displayed no significant development.

Spotted regions not observed (or interpreted differently) by SWPC/USAF:
S11504 [N12W44] was quiet and stable.
New AR S11508 [S20E78] rotated into view with a few spots.
New AR S11509 [N30E46] was observed with a tiny spot in an old plage area.
New AR S11510 [S02E09] emerged with a tiny spot.

C2+ flares

Magnitude Peak time (UT) Location Source Recorded by Comment

Coronal mass ejections (CMEs)

October 6-8: 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 negative polarity trans equatorial coronal hole (CH1322) will rotate across the central meridian on October 7-10.

Forecast

The geomagnetic field is expected to be at quiet to unsettled levels on October 9. Quiet to minor storm levels are possible on October 10-13 due to effects associated with CH1322.

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
14233 2025.09.25
2025.09.27
      N19W88          

was AR S11461

location: N19W80

14232 2025.09.26
2025.09.26
3 1   N02W91 0250 CHO HHX

was AR S11462

area: 0320

location: N03W88

14235 2025.09.27
2025.09.27
      N27W85        

location: N26W79

14240 2025.09.29
2025.09.30
  4   N17W46 0005   BXO was AR S11480

location: N15W33

14241 2025.09.30
2025.10.01
3 1   N12W52 0020 CRO AXX was AR S11484

area: 0001

location: N12W55

S11486 2025.09.30       N33W57            
S11489 2025.10.01       N03W30            
S11490 2025.10.02       N17W36            
14245 2025.10.02
2025.10.06
  2 1 S11W53 0003   BXO was AR S11491

location: S11W52

14243 2025.10.02
2025.10.03
1 8 2 N19W16 0010 AXX BXO was AR S11492

location: N19W13

14242 2025.10.02
2025.10.03
3 12 3 S11W37 0010 BXO CRO

was AR S11494

area: 0020

location: S12W34

S11496 2025.10.03       N09W21            
S11497 2025.10.03       N26W41            
S11498 2025.10.03       S19W32            
14244 2025.10.04
2025.10.05
  1   S21E20 0001   AXX was AR S11500

location: S21E26

S11501 2025.10.04       N08W46            
S11502 2025.10.04       N15W19            
S11503 2025.10.04       S01W21          
S11504 2025.10.05   10 6 N12W44 0030   CRO  
14246 2025.10.05
2025.10.06
  3   N24E38 0005   BXO was AR S11505

location: N24E37

14247 2025.10.05
2025.10.07
7 24 16 S11W00 0030 DRO DRI was AR S11506

area: 0120

location: S10E02

S11508 2025.10.08   3 2 S20E78 0020   CRO    
S11509 2025.10.08   1   N30E46 0001   AXX    
S11510 2025.10.08   1   S02E09 0002   AXX    
Total spot count: 17 71 30  
Sunspot number: 67 201 90  (total spot count + 10 * number of spotted regions)
Weighted SN: 33 93 52  (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): 74 111 72  

Monthly solar cycle data

Month Average solar flux International sunspot number
(WDC-SILSO)
Smoothed sunspot number (4) Average ap
(3)
Measured 1 AU
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
2025.03 163.7 162.1 134.2 136.0 (-3.9) 15.96
2025.04 162.5 163.6 140.6 (133.7 projected, -2.3) 17.62
2025.05  135.3 138.3 79.2 (130.1 projected, -3.6) 17.26
2025.06 131.3 135.4 116.3 (126.3 projected, -3.8) 21.43
2025.07 137.8 142.3 125.6 (123.0 projected, -3.3) 11.80
2025.08 154.9 158.7 133.6 (119.4 projected, -3.6) 9.97
2025.09 154.4 156.0 129.6 (115.5 projected, -3.9) 14.1
2025.10 150.1 (1)   33.8 (2A) / 131.0 (2B) / 155.4 (2C) (111.5 projected, -4.0) (22.3)
2025.11       (109.3 projected, -2.2)  
2025.12       (107.6 projected, -1.7)  
2026.01       (103.5 projected, -4.1)  
2026.02       (99.4 projected, -4.1)  
2026.03       (95.0 projected, -4.4)  

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 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.