Solar Terrestrial Activity Report

Activity chart

Last major update issued on September 17, 2026 at 09:30 UT. Active region table to be updated

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, 2026)
Solar cycle Solar cycles 23-25 (September 1, 2026) Historical solar and geomagnetic data charts 1954-2006 (April 5, 2007)
  Cycle 24-25 progress (September 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 (September 1, 2026) 3rd SSN Workshop, Tucson, 2013
  Comparison of cycles 12-14, 16, 24-25 (September 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 quiet to unsettled levels under the influence of effects associated with CH1399. Solar wind speed at SOHO ranged between 451 and 620 km/sec, averaging 556 km/sec (+85 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.

Solar flux density measured at 20h UT on 2.8 GHz was 99.7 - decreasing 25.0 over the previous solar rotation.

The 365 day average solar flux at 1 AU was 135.47 (183 days ago). The 81 day average solar flux at 1 AU was 127.7 (41 days ago, this is 37.1% 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 8 (STAR Ap - based on the average of three hour interval ap indices: 7.8). Three hour interval K indices: 33222102 (planetary), 4331221 (Boulder), 52223114 (Andenes).

The background x-ray flux is at the class B2 level (GOES 19).

At the time of counting spots (see image time), spots were observed in 6 active regions using 2K resolution (SN: 75) and in 4 active regions using 1K resolution (SN: 44) SDO/HMI images.

AR 14527 [N03W84] was quiet and stable.
AR 14528 [S11W69] was quiet and stable.
AR 14529 [N12W69] was quiet and stable.

Spotted regions not observed (or interpreted differently) by SWPC/USAF:
AR S12356 [N07W54] was quiet and stable.
AR S12362 [S10E24] was quiet and stable.
AR S12365 [N08E26] was quiet and stable.

C2+ flares

Magnitude Peak time (UT) Location Source Recorded by Comment

Coronal mass ejections (CMEs)

September 14-16: 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 negative polarity northern hemisphere coronal hole (CH1399) rotated across the central meridian on September 12-14. A recurrent positive polarity southern hemisphere coronal hole (CH1400) will likely become Earth facing on September 20.

Forecast

The geomagnetic field is expected to be at quiet to unsettled levels on September 17 due to effects associated with CH1399. Quiet levels are likely on September 18-19.

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
14527 2026.09.03
2026.09.04
2 3 2 N05W74 0150 HAX HKX was AR S12339

area: 0250

location: N03W71

14525 2026.09.03
2026.09.04
      N11W80           was AR S12340
14529 2026.09.05
2026.09.06
  6   N14W42 0010   AXX was AR S12346

location: N13W54

14528 2026.09.05
2026.09.06
1 2 1 S11W57 0120 HSX CSO area: 0180

location: S11W55

S12354 2026.09.09       S10W29            
S12356 2026.09.10   3 1 N06W39 0005   BXO  
S12357 2026.09.12       N04W12            
S12358 2026.09.12       S27W08            
S12359 2026.09.12       N18E16            
S12360 2026.09.12   7 2 S07W08 0010   AXX  
S12361 2026.09.13   4 2 S11E25 0010   BXO  
S12362 2026.09.14   2   S03E40 0002   BXO  
S12363 2026.09.15   8 2 N17E15 0015   AXX    
S12364 2026.09.15   2   N30W06 0004   AXX    
S12365 2026.09.15   4 3 N08E39 0015   BXO    
Total spot count: 3 41 13  
Sunspot number: 23 141 83  (total spot count + 10 * number of spotted regions)
Weighted SN: 13 56 28  (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): 25 78 66  

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
2025.06 131.3 135.4 114.6 124.7 (-3.9) 21.43
2025.07 137.8 142.3 125.9 122.5 (-2.2) 11.80
2025.08 154.9 158.7 133.7 118.4 (-4.1) 9.97
2025.09 154.4 156.0 129.7 113.1 (-5.3) 14.02
2025.10 139.5 138.6 114.6 108.5 (-4.6) 15.64
2025.11 140.3 137.3 91.7 106.9 (-1.6) 21.01
2025.12 160.8 155.8 124.0 107.0 (-0.1) 13.35
2026.01 148.7 144.0 115.0 104.2 (-2.8) 22.47
2026.02 136.4 133.1 77.4 99.8 (-4.4) 12.88
2026.03 131.0 129.7 86.6 (94.7 projected, -5.1) 15.44
2026.04  120.0 120.9 79.3 (90.8 projected, -3.9) 12.10
2026.05 125.4 128.2 101.4 (89.6 projected, -1.2) 9.80
2026.06 137.9 142.2 94.3 (87.4 projected, -2.2) 9.57
2026.07 134.7 139.0 78.1 (82.9 projected, -4.5) 10.16
2026.08 116.1 119.0 76.0 (80.7 projected, -2.2) 8.67
2026.09 107.9 (1)   37.3 (2A) / 74.5 (2B) / 84.8 (2C) (79.8 projected, -0.9) (8.7)
2026.10       (77.7 projected, -2.1)  
2026.11       (74.9 projected, -2.8)  
2026.12       (71.7 projected, -3.2)  
2027.01       (69.3 projected, -2.4)  
2027.02       (67.5 projected, -1.8)  

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 March 2026

Solar activity appears to have exited the solar max phase as of February 2026 with a strong decrease in the number of sunspots observed. The northern polar field has weakened considerably over the last months, and although there is a chance the the field could recover over the next 1-2 years, there is an increasing chance that solar cycle 26 will be very weak. The southern polar field is not impressive either, however, a southern polar coronal hole has formed early in 2026 and appears to be growing.

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.