Solar Terrestrial Activity Report

Activity chart

Last major update issued on January 29, 2026 at 16:50 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 (January 1, 2026)
Solar cycle Solar cycles 23-25 (January 1, 2026) Historical solar and geomagnetic data charts 1954-2006 (April 5, 2007)
  Cycle 24-25 progress (January 1, 2026) 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 (January 1, 2026) 3rd SSN Workshop, Tucson, 2013
  Comparison of cycles 12-14, 16, 24-25 (January 1, 2026) 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 unsettled to minor storm levels on January 28 under the influence of effects associated with CH1341. Solar wind speed at SOHO ranged between 450 and 730 km/sec, averaging 565 km/sec (+136 km/sec compared to the previous day). The high latitude magnetometer at Andenes was at unsettled to major 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 133.1 - decreasing 36.1 over the previous solar rotation.

The 365 day average solar flux at 1 AU was 151.23 (183 days ago). The 81 day average solar flux at 1 AU was 146.6 (41 days ago, this is 49.1% 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 24 (STAR Ap - based on the average of three hour interval ap indices: 24.1). Three hour interval K indices: 33334435 (planetary), 32234433 (Boulder), 33121455 (Andenes).

The background x-ray flux is at the class B7 level (GOES 19).

At the time of counting spots (see image time), spots were observed in 13 active regions using 2K resolution (SN: 212) and in 14 active regions using 1K resolution (SN: 163) SDO/HMI images.

AR 14347 [N10W84] was quiet and stable.
AR 14349 [S14W45] decayed slowly and quietly.
AR 14351 [S05W73] decayed slowly and quietly.
AR 14353 [N17W68] decayed slowly and quietly.
AR 14355 [S14W04] decayed slowly and was mostly quiet. C1 flares: C1.3 @ 07:07 UT
AR 14357 [S13W19] decayed slowly and was mostly quiet. C1 flares: C1.0 @ 02:00, C1.0 @ 07:41, C1.0 @ 09:06, C1.0 @ 21:10, C1.3 @ 21:23 UT
AR 14358 [N14E50] was quiet and stable.
New AR 14359 [N19E29] emerged on January 27 and was numbered by SWPC the next day.
New AR 14360 [S14E25] emerged with several spots.
New AR 14361 [N19W25] emerged on January 24, then became spotless before reemerging with spots on January 27 and SWPC numbered the region the following day.

Spotted regions not observed (or interpreted differently) by SWPC/USAF:
AR S11806 [N25E14] decayed slowly and quietly.
New AR S11822 [S17E84] rotated into view with a mature spot.
New AR S11823 [S24E83] rotated into view with a few spots.

A C1.4 flare at 12:47 UT had its origin behind the southwest limb.

C2+ flares

Magnitude Peak time (UT) Location Source Recorded by Comment

Coronal mass ejections (CMEs)

January 26-28: 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 recurrent trans equatorial negative polarity coronal hole (CH1341) rotated across the central meridian on January 24-25.

Forecast

The geomagnetic field is expected to be at quiet to minor storm levels on January 29 due to effects associated with CH1341. Quiet to unsettled conditions are likely on January 30-31.

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
14347 2026.01.16
2026.01.16
2 1 1 N11W86 0050 HSX HSX was AR S11781

area: 0090

location: N10W84

14350 2026.01.18
2026.01.19
      N18W56           was AR S11786

location: N22W60

14351 2026.01.18
2026.01.19
7 4 4 S04W74 0060 DAO DRO

was AR S11787

area: 0040

location: S05W73

14349 2026.01.18
2026.01.19
1 6 2 S14W46 0120 HSX CSO was AR S11789

area: 0130

location: S14W45

S11793 2026.01.20       N18W48            
14353 2026.01.21
2026.01.22
7 4 3 N17W71 0030 CRO CRO

was AR S11797

location: N17W68

14355 2026.01.21
2026.01.24
1 16 2 S13W07 0010 AXX BXO was AR S11798

area: 0025

location: S14W06

14354 2026.01.22
2026.01.22
      S11W69           was AR 11800

location: S11W57

S11806 2026.01.23   4 1 N25E14 0008   BXO  
14361 2026.01.24
2026.01.28
2 5 1 N19W29 0010   BXO   was AR S11809

location: N19W25

S11810 2026.01.24       N08W41            
14356 2026.01.25
2026.01.26
      S12W33         was AR S11810

location: S11W27

S11813 2026.01.25       N17E09            
14357 2026.01.26
2026.01.27
7 22 9 S13W20 0030 CRO DRI was AR S11816

area: 0100

location: S13W19

14358 2026.01.26
2026.01.27
3 5 2 N14E50 0010 BXO BXO was AR S11817
S11818 2026.01.26       S32W13            
14360 2026.01.27
2026.01.28
3 5 2 S15E57 0030 CRO CRO was AR S11819

location: S14E55

14359 2026.01.27
2026.01.28
2 7 3 N18E27 0010 BXO CRO was AR S11820

area: 0015

location: N19E29

S11821 2026.01.27       S04W16          
S11822 2026.01.28   1 1 S17E84 0120   HSX    
S11823 2026.01.28   2 2 S24E83 0040   HAX    
Total spot count: 35 82 33  
Sunspot number: 135 212 163  (total spot count + 10 * number of spotted regions)
Weighted SN: 59 117 68  (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): 149 117 130  

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
2024.10 221.0 219.6 165.8 160.9 (+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 78.5 128.6 (-4.7) 17.26
2025.06 131.3 135.4 114.6 124.7 (-3.9) 21.43
2025.07 137.8 142.3 125.9 (122.4 projected, -2.3) 11.80
2025.08 154.9 158.7 133.7 (119.3 projected, -3.1) 9.97
2025.09 154.4 156.0 129.7 (115.8 projected, -3.5) 14.02
2025.10 139.5 138.6 114.6 (111.8 projected, -4.0) 15.64
2025.11 140.3 137.3 91.7 (109.6 projected, -2.2) 21.01
2025.12 160.8 155.8 124.0 (108.0 projected, -1.6) 13.35
2026.01 151.2 (1)   107.8 (2A) / 119.4 (2B) / 142.7 (2C)
ISN to date: 119. At this level SSN
for July 2025 will become: 122.7
(104.0 projected, -4.0) (24.3)
2026.02       (99.9 projected, -4.1)  
2026.03       (95.5 projected, -4.4)  
2026.04       (91.8 projected, -3.7)  
2026.05       (90.5 projected, -1.3)  
2026.06       (88.4 projected, -2.1)  

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 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.