Solar Terrestrial Activity Report

Activity chart

Last major update issued on July 19, 2025 at 06:30 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 active levels on July 18 under the waning influence of effects associated with CH1306. Solar wind speed at SOHO ranged between 472 and 657 km/sec, averaging 553 km/sec (-95 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 155.7 - increasing 35.4 over the previous solar rotation. The 365 day average solar flux at 1 AU was 182.03 (183 days ago). The 81 day average solar flux at 1 AU was 136.8 (41 days ago, this is 42.8% 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 10 (STAR Ap - based on the mean of three hour interval ap indices: 10.4). Three hour interval K indices: 21224322 (planetary), 11333322 (Boulder), 22234332 (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 16 active regions using 2K resolution (SN: 316) and in 15 active regions using 1K resolution (SN: 235) SDO/HMI images.

AR 14135 [S08W79] decayed quickly and quietly.
AR 14136 [N20W48] decayed significantly and the magnetic delta disappeared. Still the region produced the large majority of the low level C flares recorded during the day. C1 flares: C1.2 @ 01:07, C1.3 @ 02:13, C1.4 @ 02:44, C1.8 @ 04:50, C1.5 @ 05:36, C1.5 @ 06:05, C1.5 @ 09:47, C1.6 @ 12:26, C1.5 @ 18:53, C1.5 @ 20:26, C1.4 @ 22:30, C1.6 @ 23:56 UT
AR 14139 [N21W67] was mostly quiet and stable.
AR 14140 [S15W21] decayed slowly and quietly.
AR 14142 [N01W07] decayed in the trailing spot section and was mostly quiet.
AR 14143 [N24W36] was mostly quiet and stable.
AR 14144 [S15E22] was quiet and stable.
AR 14145 [S24W19] decayed slowly and quietly.
AR 14147 [N06E29] was quiet and stable.
AR 14148 [S08W31] decayed slowly and quietly.

Spotted regions not observed (or interpreted differently) by SWPC/USAF:
S11257 [N17W32] reemerged with a tiny spot.
S11264 [N07W51] was quiet and stable.
New AR S11265 [N07W38] emerged with tiny spots.
New AR S11266 [N20W14] was observed with a tiny spot in an old plage area.
New AR S11267 [S14E79] rotated into view with a mature spot. C1 flares: C1.4 @ 19:49 UT
New AR S11268 [N17E83] rotated into view with a few spots. C1 flares: C1.3 @ 10:36, C1.5 @ 18:12 UT

C2+ flares

Magnitude Peak time (UT) Location Source Recorded by Comment
C2.2 03:42   14136 GOES18  
C2.2 07:13   14136 GOES18  
C3.5 08:13 N22W42 14136 GOES18  
C2.2 09:11   14136 GOES18  
C2.1 12:51 N24W40 14136 GOES18  
C2.4 13:09   14136 GOES18  
C2.1 16:39   14136 GOES18  

Coronal mass ejections (CMEs)

July 16-18: No obviously Earth directed CMEs.

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 trans equatorial positive polarity coronal hole (CH1306) was Earth facing on July 8-16. A recurrent negative polarity trans equatorial coronal hole (CH1307) will rotate across the central meridian on July 19-21.

Forecast

The geomagnetic field is expected to be at quiet to unsettled levels on July 19 due to lingering effects from CH1306. Quiet levels are likely on July 20-21 becoming unsettled to minor storm on July 22-23 due to effects associated with CH1307.

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
14135 2025.07.06
2025.07.07
2 3 2 S08W78 0020 AXX AXX was AR S11226
14136 2025.07.08
2025.07.09
10 17 12 N21W50 0280 DKC DKI beta-gamma

was AR S11232

location: N20W48

area: 0520

S11237 2025.07.09       S04W50            
14140 2025.07.10
2025.07.11
1 15 4 S16W19 0010 AXX BXO

 

was AR S11242

location: S15W21

area: 0025

14139 2025.07.11
2025.07.11
5 8 3 N22W68 0250 DKO EKO

was AR S11243

area: 0470

location: N21W67

S11247 2025.07.12       N28W47            
S11251 2025.07.13       S09W41            
14142 2025.07.13
2025.07.14
13 36 22 N01W05 0200 DAI EAI beta-gamma

was AR S11252

area: 0300

location: N01W07

14143 2025.07.14
2025.07.14
12 32 18 N25W38 0260 DKI EKI beta-gamma

was AR S11254

area: 0540

location: N24W36

14144 2025.07.14
2025.07.15
1 8 2 S15E22 0030 HSX HAX was AR S11255

area: 0040

14147 2025.07.14
2025.07.16
1 5 2 N06E28 0010 AXX BXO was AR S11256

location: N06E29

S11257 2025.07.14   1 1 N17W32 0004   AXX    
14145 2025.07.14
2025.07.15
5 9 6 S24W19 0010 BXO BXO was AR S11258

area: 0020

14148 2025.07.15
2025.07.17
5 10 5 S08W28 0030 CAO CRO was AR S11259

location: S08W31

S11260 2025.07.15       S13E20            
14146 2025.07.16 2     N20W58 0010 AXX       apparently a misinterpretation by SWPC. They split off the leader spot of AR 14136 on 2025.07.16. There is no obvious reason for this split
S11262 2025.07.16       N10E06            
S11263 2025.07.17       N06E52          
S11264 2025.07.17   1   N07W51 0001   AXX  
S11265 2025.07.18   5 3 N07W38 0010   BXO    
S11266 2025.07.18   2 1 N20W14 0005   AXX    
S11267 2025.07.18   1 1 S14E79 0170   HSX    
S11268 2025.07.18   3 3 N17E83 0160   DAO    
Total spot count: 57 156 85  
Sunspot number: 167 316 235  (total spot count + 10 * number of spotted regions)
Weighted SN: 102 209 138  (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): 183 174 188  

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
2025.07 130.5 (1)   67.9 (2A) / 117.0 (2B) / 135.2 (2C) (112.9 projected, -4.2) (14.1)
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.