Solar Terrestrial Activity Report

Activity chart

Last major update issued on July 26, 2025 at 06:00 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 (July 1, 2025)
Solar cycle Solar cycles 23-25 (July 1, 2025) Historical solar and geomagnetic data charts 1954-2006 (April 5, 2007)
  Cycle 24-25 progress (July 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 (July 1, 2025) 3rd SSN Workshop, Tucson, 2013
  Comparison of cycles 12-14, 16, 24-25 (July 1, 2025) 4th SSN Workshop, Locarno, 2014
  Solar polar fields vs. solar cycles (April 21, 2025) Cycle 25 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 July 25 under the weakening influence of effects associated with CH1307. Solar wind speed at SOHO ranged between 489 and 630 km/sec, averaging 557 km/sec (-70 km/sec compared to the previous day). The high latitude magnetometer at Andenes recorded quiet to active 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 148.0 - increasing 26.2 over the previous solar rotation. The 365 day average solar flux at 1 AU was 181.29 (183 days ago). The 81 day average solar flux at 1 AU was 136.7 (41 days ago, this is 42.7% 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: 195.86 on October 13, 2024. The Potsdam WDC planetary A index was 8 (STAR Ap - based on the average of three hour interval ap indices: 8.1). Three hour interval K indices: 23222322 (planetary), 22232323 (Boulder), 43333324 (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 16 active regions using 2K resolution (SN: 307) and in 14 active regions using 1K resolution (SN: 210) SDO/HMI images.

AR 14149 [N16W12] decayed further and was mostly quiet. C1 flares: C1.1 @ 04:44, C1.1 @ 05:19 UT
AR 14150 [S13W12] gained a few spots and was mostly quiet.
AR 14152 [N11E15] was quiet and stable.
AR 14153 [S29E17] was mostly quiet and stable. C1 flares: C1.4 @ 02:57, C1.1 @ 14:31 UT
AR 14154 [S13E32] was mostly quiet and stable. C1 flares: C1.0 @ 17:54 UT
AR 14155 [S08E47] lost some area and the tiny magnetic delta configuration, however, there are many small spots and C flares are likely. C1 flares: C1.2 @ 00:27, C1.2 @ 04:58, C1.7 @ 05:56, C1.6 @ 08:13, C1.1 @ 14:53, C1-1 @ 18:07 UT
AR 14156 [N10E47] was quiet and stable.
AR 14157 [S19E41] was quiet and stable.
AR 14158 [S16W60] was quiet and stable.

Spotted regions not observed (or interpreted differently) by SWPC/USAF:
S11263 [N08W34] was quiet and stable.
S11276 [N08E22] was quiet and stable.
S11277 [S02E20] was quiet and stable.
S11285 [S07E06] developed slowly and quietly.
S11286 [S08E61] was quiet and stable.
S11287 [S04E47] was quiet and stable.
New AR S11288 [N20E09] emerged before noon, then decayed slowly.

A C1.8 flare with an unidentified origin was recorded at 03:14 UT

C2+ flares

Magnitude Peak time (UT) Location Source Recorded by Comment
C7.4 01:01 N15E08 14149 GOES18  
C2.2 08:05 S08E58 14155 GOES18  

Coronal mass ejections (CMEs)

July 24-25: No obviously Earth directed CMEs.
July 23: A faint partial halo CME was observed following a filament eruption in the northwest quadrant near the central meridian and the equator. The eruption began shortly after 02h and peaked near 05h UT. The CME could reach Earth on July 26 and cause some unsettled and active intervals.

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 negative polarity northern hemisphere coronal hole (CH1308) will rotate across the central meridian on July 26-27, however, CH1308 may be too far to the north to cause any geomagnetic disturbance.

Forecast

The geomagnetic field is expected to be at quiet to unsettled levels on July 26-27 due to possible effects from the July 23 CME, active intervals are possible. Mostly quiet levels are likely on July 28. Some unsettled and active intervals are possible on July 29-30 due to effects from CH1308.

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
14144 2025.07.14
2025.07.15
      S15W76           was AR S11255

location: S12W73

14147 2025.07.14
2025.07.16
      N06W74           was AR S11256

location: N07W60

S11263 2025.07.17   5 1 N08W35 0008   BXO  
14150 2025.07.18
2025.07.19
1 13 4 S13W13 0060 CSO DSO was AR S11267

location: S13W12

area: 0120

14149 2025.07.18
2025.07.19
20 22 10 N17W10 0280 EKO EAO beta-gamma

was AR S11268

location: N16W12

area: 0330

S11270 2025.07.19       S20W08            
14158 2025.07.20 3 12 8 S15W61 0010 CAO DRI was AR S11274

area: 0040

14152 2025.07.20
2025.07.21
  11 5 N09E05 0025   BXO was AR S11275

location: N11E15

area: 0030

S11276 2025.07.21   3 1 N08E22 0007   BXO  
S11277 2025.07.21   2   S02E20 0003   AXX  
14153 2025.07.22
2025.07.22
15 22 13 S30E20 0210 DAI EAO

was AR S11278

location: S29E17

area: 0300

14154 2025.07.22
2025.07.23
4 9 6 S14E32 0060 CAO CAO was AR S11279

area: 0100

location: S13E32

14157 2025.07.22
2025.07.24
2 1 1 S19E40 0050 HSX HSX was AR S11280

area: 0090

location: S19E41

S11281 2025.07.22       S25W39            
14155 2025.07.23
2025.07.24
7 25 13 S10E46 0010 CAI DRI beta-gamma

was AR S11282

area: 0150

14156 2025.07.23 1 2 1 N10E46 0000 HRX HAX was AR S11283

area: 0050

location: N10E47

S11284 2025.07.23       S13E02          
S11285 2025.07.24   10 3 S07E06 0025   CRI  
S11286 2025.07.24   5 3 S08E61 0030   CRO  
S11287 2025.07.24   4 1 S04E47 0006   BXO  
S11288 2025.07.25   1   N20E09 0003   AXX    
Total spot count: 53 147 70  
Sunspot number: 133 307 210  (total spot count + 10 * number of spotted regions)
Weighted SN: 96 189 107  (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): 146 169 168  

Monthly solar cycle data

Month Average solar flux International sunspot number
(WDC-SILSO)
Smoothed sunspot number (4) Average ap
(3)
Measured 1 AU
2024.01 164.6 159.3 126.0 131.2 (+1.7) 5.46
2024.02 172.5 168.3 123.0 136.9 (+5.7) 5.31
2024.03 154.4 152.9 103.7 141.4 (+4.5) 11.03
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 (146.1 projected, -5.2) 13.17
2025.02  184.2 179.7 155.7 (138.3 projected, -7.8) 14.42
2025.03 163.7 162.1 134.2 (131.9 projected, -6.4) 15.96
2025.04 162.5 163.6 140.6 (127.3 projected, -4.6) 17.62
2025.05  135.3 138.3 79.2 (122.0 projected, -5.3) 17.26
2025.06 131.3 135.4 116.3 (117.1 projected, -4.9) 21.43
2025.07 135.8 (1)   95.8 (2A) / 118.8 (2B) / 145.5 (2C)
ISN average: 130.2. At this level the SSN
for January 2025 will become 146.5
(112.9 projected, -4.2) (13.3)
2025.08       (108.1 projected, -4.8)  
2025.09       (103.8 projected, -4.3)  
2025.10       (99.9 projected, -3.9)  
2025.11       (97.6 projected, -2.3)  
2025.12       (96.0 projected, -1.6)  

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.