Solar Terrestrial Activity Report

Activity chart

Last major update issued on November 22, 2025 at 07:45 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 (November 1, 2025)
Solar cycle Solar cycles 23-25 (November 1, 2025) Historical solar and geomagnetic data charts 1954-2006 (April 5, 2007)
  Cycle 24-25 progress (November 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 (November 1, 2025) 3rd SSN Workshop, Tucson, 2013
  Comparison of cycles 12-14, 16, 24-25 (November 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 unsettled levels on November 21, weakly under the influence of a high speed stream associated with CH1331. Solar wind speed at SOHO ranged between 396 and 501 km/sec, averaging 447 km/sec (+29 km/sec compared to the previous day). The above 10 MeV proton flux was slightly elevated all day.

Solar flux density measured at 20h UT on 2.8 GHz was 121.2 - decreasing 5.8 over the previous solar rotation.

The 365 day average solar flux at 1 AU was 159.07 (183 days ago). The 81 day average solar flux at 1 AU was 144.9 (41 days ago, this is 47.9% 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 7 (STAR Ap - based on the average of three hour interval ap indices: 7.3). Three hour interval K indices: 32121222 (planetary), 22111321 (Boulder), 32111442 (Andenes).

The background x-ray flux is at the class B6 level (GOES 19).

At the time of counting spots (see image time), spots were observed in 13 active regions using 2K resolution (SN: 186) and in 11 active regions using 1K resolution (SN: 135) SDO/HMI images.

AR 14284 [S07W72] decayed slowly and produced several low level C flares. C1 flares: C1.2 @ 00:41, C1.1 @ 00:54, C1.0 @ 08:03, C1.0 @ 12:00, C1.4 @ 16:51, C1.6 @ 17:50, C1.3 @ 19:54 UT
AR 14285 [S18W80] decayed slowly and quietly.
AR 14286 [S15E19] was quiet and stable.
AR 14287 [N02E40] was quiet and stable.
AR 14288 [N17E63] was mostly quiet and stable. C1 flares: C1.0 @ 01:24, C1.1 @ 02:45, C1.2 @ 03:02 UT
New AR 14289 [S01E49] rotated into view on November 19 and was numbered by SWPC 2 days later. C1 flares: C1.1 @ 04:25 UT
New AR 14290 [S10E73] began to rotate into view late on November 20 and received its NOAA number the following day.

Spotted regions not observed (or interpreted differently) by SWPC/USAF:
AR S11616 [S21E17] was quiet and stable.
AR S11620 [S14W14] was quiet and stable.
New AR S11629 [N22E08] was observed with tiny spots in an old plage area.
New AR S11630 [S13E81] rotated into view and may have a small magnetic delta configuration in the leading spot section. C1 flares: C1.2 @ 16:24 UT
New AR S11631 [N06W04] was observed with tiny spots in an old plage area.
New AR S11632 [N09E33] was observed with tiny spots in an old plage area.

A C1.0 flare was recorded at 01:09 UT from a spotless plage region in the southeast quadrant.

C2+ flares

Magnitude Peak time (UT) Location Source Recorded by Comment
C3.8 13:30   S11630 GOES18  
C2.1 22:37 S15E79 S11630 GOES18  

Coronal mass ejections (CMEs)

November 19-21: 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 positive polarity coronal hole (CH1332) will be Earth facing on November 22-24.

Forecast

The geomagnetic field is expected to be at quiet levels on November 22-24. Quiet to major storm levels are possible on November 25-27 due to effects from CH1332.

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
S11605 2025.11.12       S17W56            
S11609 2025.11.14       N24W41            
14283 2025.11.14
2025.11.15
      S19W80           was AR S11610

location: S19W76

14284 2025.11.16
2025.11.16
8 8 4 S07W72 0030 DAO DRO

was AR S11611

14286 2025.11.16
2025.11.18
  6 2 S15E09 0012   BXO was AR S11613

location: S15E19

S11614 2025.11.16       N06W56            
S11615 2025.11.16       N14W37            
S11616 2025.11.16   3 1 S21E17 0007   BXO  
S11617 2025.11.16       S02W46            
S11618 2025.11.16       S22W33          
14285 2025.11.17
2025.11.18
1 1   S17W82 0000 AXX AXX was AR S11619

area: 0002

location: S18W80

S11620 2025.11.17   6 3 S14W14 0012   BXO  
14287 2025.11.18
2025.11.19
1 2 2 N03E39 0020 HSX HSX was AR S11622

area: 0070

location: N02E40

S11623 2025.11.18       N35W27            
14289 2025.11.19
2025.11.21
1 3 2 S03E49 0010 AXX HRX was AR S11623

area: 0020

location: S01E49

S11625 2025.11.19       N15W28          
14288 2025.11.20
2025.11.20
1 5 3 N17E63 0030 HSX CAO was AR S11626

area: 0240

14290 2025.11.20
2025.11.21
3 3 2 S10E74 0040 CAO HSX was AR S11627

area: 0110

location: S10E73

S11628 2025.11.20       N11E15          
S11629 2025.11.21   4   N22E08 0007   BXO    
S11630 2025.11.21   7 4 S13E81 0110   DAI   beta-gamma
S11631 2025.11.21   3 1 N06W04 0005   AXX    
S11632 2025.11.21   5 1 N09E33 0010   BXO    
Total spot count: 15 56 25  
Sunspot number: 75 186 135  (total spot count + 10 * number of spotted regions)
Weighted SN: 35 82 51  (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): 83 102 108  

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)
2024.07 196.6 203.0 196.8 155.0 (+2.3) 7.13
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 projected, -4.8) 17.26
2025.06 131.3 135.4 114.6 (123.8 projected, -4.7) 21.43
2025.07 137.8 142.3 125.6 (120.6 projected, -3.2) 11.80
2025.08 154.9 158.7 133.5 (117.0 projected, -3.6) 9.97
2025.09 154.4 156.0 129.8 (113.1 projected, -3.9) 14.02
2025.10 139.5 138.6 114.6 (109.1 projected, -4.0) 15.64
2025.11 143.9 (1)   62.6 (2A) / 89.4 (2B) / 117.3 (2C)
ISN average to date: 96
At this level the May 2025 SSN
will become 128.7
(106.8 projected, -2.3) (22.4)
2025.12       (105.3 projected, -1.5)  
2026.01       (101.2 projected, -4.1)  
2026.02       (97.1 projected, -4.1)  
2026.03       (92.8 projected, -4.3)  
2026.04       (89.0 projected, -3.8)  

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.