Solar Terrestrial Activity Report

Activity chart

Last major update issued on December 26, 2025 at 06:20 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 (December 1, 2025)
Solar cycle Solar cycles 23-25 (December 1, 2025) Historical solar and geomagnetic data charts 1954-2006 (April 5, 2007)
  Cycle 24-25 progress (December 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 (December 1, 2025) 3rd SSN Workshop, Tucson, 2013
  Comparison of cycles 12-14, 16, 24-25 (December 1, 2025) 4th SSN Workshop, Locarno, 2014
  Solar polar fields vs. solar cycles (December 21, 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 unsettled levels on December 25 under the decreasing influence of effects associated with CH1336. Solar wind speed at SOHO ranged between 555 and 665 km/sec, averaging 594 km/sec (-94 km/sec compared to the previous day). The high latitude magnetometer at Andenes was at 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 162.5 - increasing 24.3 over the previous solar rotation.

The 365 day average solar flux at 1 AU was 155.24 (183 days ago). The 81 day average solar flux at 1 AU was 140.4 (41 days ago, this is 45.1% 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 11 (STAR Ap - based on the average of three hour interval ap indices: 10.6). Three hour interval K indices: 33322212 (planetary), 24432321 (Boulder), 54422324 (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: 302) and in 12 active regions using 1K resolution (SN: 201) SDO/HMI images.

AR 14312 [N18W33] decayed slowly and was mostly quiet.
AR 14316 [S07W31] decayed slowly and quietly.
AR 14317 [N10E04] decayed significantly in the intermediate and trailing spot sections. The region became mostly quiet. C1 flares: C1.6 @ 02:00, C1.6 @ 09:06, C1.8 @ 14:21, C1.7 @ 14:50 UT
AR 14318 [N05E12] decayed slowly and quietly.
AR 14319 [S10E29] was mostly quiet and stable.
AR 14320 [N04E41] gained a few spots and was quiet.
AR 14321 [S11W22] still has a magnetic delta configuration and could produce M flares. Most spots are within a single, large penumbra. C1 flares: C1.6 @ 11:01 UT
New AR 14322 [N13W63] emerged on December 24 and was numbered the next day by SWPC.

Spotted regions not observed (or interpreted differently) by SWPC/USAF:
AR S11701 [S09W48] reemerged with a tiny spot.
AR S11712 [S16E23] was quiet and stable.
AR S11715 [S19W30] decayed slowly and quietly.
New AR S11718 [N09W29] emerged with tiny spots.
New AR S11719 [S14E80] rotated into view with tiny spots. C1 flares: C1.6 @ 04:58, C1.6 @ 13:17 UT

An active region behind the northeast limb produced C1 flares: C1.6 @ 05:43, C1.8 @ 08:44, C1.9 @ 16:00 UT
An active region behind the southeast limb was the source of C1 flares: C1.9 @ 17:36, C1.9 @ 19:03 UT

C2+ flares

Magnitude Peak time (UT) Location Source Recorded by Comment
C2.6 04:24 S10E42 14319 GOES18 simultaneous flare in AR 14317
C2.3 06:09   14321 GOES18  
C2.2 08:02 behind northeast limb (N23E90)   GOES18  
C2.0 16:31   14312 GOES18  
C2.1 20:29 behind southeast limb   GOES18  
C2.4 21:53 behind northeast limb (N23E90)   GOES18  
C2.3 23:10 behind northeast limb (N23E90)   GOES18  
C2.3 23:25   14312 GOES18  

Coronal mass ejections (CMEs)

December 23-25: No obviously Earth directed CMEs were observed in available coronagraph imagery.

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 huge recurrent positive polarity trans equatorial coronal hole (CH1336) will be Earth facing on December 19-27. A recurrent northern hemisphere negative polarity coronal hole (CH1337) will likely rotate across the central meridian on December 28-29.

Forecast

The geomagnetic field is expected to be at quiet to unsettled levels on December 26-30 due to weak effects associated with CH1336.

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
14312 2025.12.17
2025.12.18
1 10 4 N19W34 0020 HSX HAX was AR S11695

area: 0080

location: N18W33

merged with AR 14314

14313 2025.12.18
2025.12.18
      S14W68           was AR S11696
14314 2025.12.19
2025.12.20
      N24W38           was AR S11698

location: N25W33

14315 2025.12.19
2025.12.20
      N21W21         was AR S11700

location: N21W14

S11701 2025.12.19   1   S09W48 0002   AXX    
S11702 2025.12.19       S12W51            
14316 2025.12.20
2025.12.20
1 7 4 S07W30 0020 HAX HAX

was AR S11704

area: 0060

location: S07W31

14317 2025.12.20
2025.12.20
12 42 20 N12E09 0240 EAI EKO

was AR S11705

area: 0420

location: N10E04

S11706 2025.12.20       N01W39            
14318 2025.12.21
2025.12.22
1 14 5 N05E15 0010 AXX BXO was S11707

area: 0030

location: N05E12

14319 2025.12.21
2025.12.22
4 31 14 S09E27 0030 CRO DRI was AR S11708

area: 0110

location: S10E29

14321 2025.12.22
2025.12.24
10 37 18 S10W23 0200 DAI DKC beta-delta

was AR S11709

area: 0650

14320 2025.12.22
2025.12.23
1 8 5 N05E41 0010 AXX CRO was AR S11710

area: 0030

location: N04E41

S11711 2025.12.22       N14W45            
S11712 2025.12.23   7 2 S16E23 0015   BXO  
S11713 2025.12.23       S20E40            
14322 2025.12.24
2025.12.25
3 7 5 N13W63 0020 CRO DRO was AR S11714

area: 0040

S11715 2025.12.24   1 1 S19W30 0007   HRX  
S11716 2025.12.24       S16W09          
S11717 2025.12.24       S16W18          
S11718 2025.12.25   5 2 N09W29 0013   BXO    
S11719 2025.12.25   2 1 S14E80 0010   HRX    
Total spot count: 33 172 81  
Sunspot number: 113 302 201  (total spot count + 10 * number of spotted regions)
Weighted SN: 59 217 126  (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): 124 166 161  

Monthly solar cycle data

Month Average solar flux International sunspot number
(WDC-SILSO)
Smoothed sunspot number (4) Average ap
(3)
Measured 1 AU
2024.05 187.7 191.9 172.1 149.1 (+4.6) 23.56
(SC25 peak)
2024.08  246.1
(SC25 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
2024.11 199.6 195.3 154.1 157.2 (-3.7) 9.33
2024.12 197.3 191.2 154.6 151.2 (-6.0) 8.42
2025.01 190.3 184.2 137.0 146.2 (-5.0) 13.17
2025.02  184.2 179.7 155.7 139.8 (-6.4) 14.42
2025.03 163.7 162.1 134.2 135.9 (-3.9) 15.96
2025.04 162.5 163.6 141.4 133.3 (-2.6) 17.62
2025.05  135.3 138.3 78.5 128.5 (-4.8) 17.26
2025.06 131.3 135.4 114.6 (124.4 projected, -4.1) 21.43
2025.07 137.8 142.3 125.6 (121.7 projected, -2.7) 11.80
2025.08 154.9 158.7 133.5 (118.0 projected, -3.7) 9.97
2025.09 154.4 156.0 129.8 (114.1 projected, -3.9) 14.02
2025.10 139.5 138.6 114.6 (110.1 projected, -4.0) 15.64
2025.11 140.3 137.3 91.7 (107.9 projected, -2.2) 21.01
2025.12 156.2 (1)   92.2 (2A) / 114.3 (2B) / 131.1 (2C)
ISN to date: 115. At this level the
SSN for June 2025 will become 124.3
(106.3 projected, -1.6) (15.4)
2026.01       (102.3 projected, -4.0)  
2026.02       (98.2 projected, -4.1)  
2026.03       (93.8 projected, -4.4)  
2026.04       (90.1 projected, -3.7)  
2026.05       (88.9 projected, -1.2)  

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 October 2025

Sunspot activity was on a decreasing trend from September 2024 until mid August 2025 (using the average solar flux over 3 solar rotations as a proxy). Then a strong surge in activity saw solar flux peak in late August 2025 just below the largest peaks seen in 2024. A slow decrease in activity from the August level has been observed in September and October 2025.

All 365 day smoothed sunspot numbers reached a maximum on October 11-12, 2024
. This became the peak of SC25 (365 day smoothed peaks: STAR 1K: 236.1, STAR 2K: 364.3, NOAA SN: 156.0, ISN: 163.9), while 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.