Solar Terrestrial Activity Report

Activity chart

Last major update issued on June 8, 2025 at 07:30 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 (June 1, 2025)
Solar cycle Solar cycles 23-25 (June 1, 2025) Historical solar and geomagnetic data charts 1954-2006 (April 5, 2007)
  Cycle 24-25 progress (June 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 (June 1, 2025) 3rd SSN Workshop, Tucson, 2013
  Comparison of cycles 12-14, 16, 24-25 (June 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 Research: Solar Cycle 25 Started on November 17, 2019 with 365 Days Smoothing
Calculating the Strength of Solar Cycle 25 Using 365-day Smoothing

Recent activity

The geomagnetic field was at quiet to active levels on June 7 under the influence of CIR effects associated with CH1299. Solar wind speed at SOHO ranged between 371 and 479 km/sec, averaging 415 km/sec (-38 km/sec compared to the previous day). The phi angle was in a negative sector after 07h UT. The high latitude magnetometer at Andenes recorded quiet 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 120.9 - decreasing 4.9 over the previous solar rotation. The 365 day average solar flux at 1 AU was 188.79 (183 days ago). SC25 365d peak: 195.86 on October 13, 2024. The Potsdam WDC planetary A index was 17 (STAR Ap - based on the mean of three hour interval ap indices: 16.8). Three hour interval K indices: 22342244 (planetary), 23442333 (Boulder), 43442366 (Andenes).

The background x-ray flux is at the class B5 level (GOES 19).

At the time of counting spots (see image time), spots were observed in 12 active regions using 2K resolution (SN: 234) and in 5 active regions using 1K resolution (SN: 97) SDO/HMI images.

AR 14105 [S15E21] has many small spots, only the leader spot has mature penumbra. There's a chance of a minor M class flare as the region has significant polarity intermixing. C1 flares: C1.4 @ 12:01, C1.1 @ 21:15 UT
AR 14106 [N13W26] decayed slowly and quietly.
AR 14107 [S18W02] decayed slowly and quietly.
New AR 14108 [S20W19] emerged on June 6 and was numbered by SWPC the next day.
New AR 14109 [S15E38] rotated into view on June 5 and received its NOAA number 2 days later.

Spotted regions not observed (or interpreted differently) by SWPC/USAF:
S11115 [S11W32] decayed slowly and quietly.
S11116 [N09W08] decayed slowly and quietly.
S11120 [N10E18] decayed slowly and quietly.
S11128 [S04W05] decayed slowly and quietly.
New region S11136 [N25E05] emerged with tiny spots.
New region S11137 [N12W42] emerged with a tiny spot.
New region S11138 [S03E36] emerged with tiny spots.

AR 14100 at the northwest limb produced a few C1 flares: C1.0 @ 06:18, C1.3 @ 07:07, C1.7 @ 08:38 UT.

C2+ flares

Magnitude Peak time (UT) Location Source Recorded by Comment
C2.5 01:08   14100 GOES18  
C2.0 01:13   14100 GOES18  
C2.2 12:15   14100 GOES18  
C3.5 12:24   14100 GOES18  
C2.8 18:41 S12E21 14105 GOES18  

Coronal mass ejections (CMEs)

June 5-7: 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 negative polarity southern hemisphere coronal hole (CH1299) was Earth facing on June 2-5. A small negative polarity northern hemisphere coronal hole (CH1300) will rotated across the central meridian on June 8. A large recurrent positive polarity southern hemisphere coronal hole (CH1301) will likely become Earth facing on June 12-14.

Forecast

The geomagnetic field is expected to be at quiet to active levels on June 8 due to CIR effects associated with CH1299. Quiet to unsettled is likely on June 9-10.

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
14100 2025.05.25
2025.05.26
4     N09W95 0070 EAO    

was AR S11095

rotated out of view

14104 2025.05.29
2025.05.30
      N06W72          

was AR S11107

location: N08W67

S11113 2025.05.31       S12W45            
S11114 2025.05.31       N11W25            
S11115 2025.06.01   4   S11W32 0007   BXO  
S11116 2025.06.01   3   N09W08 0005   AXX  
14105 2025.06.02
2025.06.03
24 59 31 S15E21 0110 EAI EAI beta-gamma

was AR S11119

area: 0250

S11120 2025.06.02   2   N10E18 0003   BXO  
14106 2025.06.03
2025.06.04
2 6 1 N12W27 0010 AXX CRO was AR S11123

area: 0020

location: N13W26

S11124 2025.06.03       N19W43            
S11126 2025.06.04       S16W34            
S11128 2025.06.05   4   S04W05 0006   BXO  
14107 2025.06.05
2025.06.06
7 15 7 S18W03 0030 CRO DRO was AR S11129

location: S18W02

area: 0060

S11130 2025.06.05       S12W00            
14109 2025.06.05
2025.06.07
3 11 6 S16E40 0010 CRO DRI was AR S11131

location: S15E38

area: 0050

S11132 2025.06.06       S20W48          
14108 2025.06.06
2025.06.07
3 5 2 S21W17 0010 BXO CRO was AR S11133

area: 0020

location: S20W19

S11134 2025.06.06       N36W14          
S11135 2025.06.06       S14E05          
S11136 2025.06.07   2   N25E05 0002   BXO    
S11137 2025.06.07   1   N12W42 0001   AXX    
S11138 2025.06.07   2   S03E36 0002   BXO    
Total spot count: 43 114 47  
Sunspot number: 103 234 97  (total spot count + 10 * number of spotted regions)
Weighted SN: 59 131 64  (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): 113 129 78  

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
2024.10 221.0 219.6 165.8 160.8 (+1.4) (SC25 solar max) 18.99
2024.11 199.6 195.3 154.1 157.0 (-3.8) 9.33
2024.12 197.3 191.2 154.6 (150.7 projected, -6.3) 8.42
2025.01 190.3 184.2 137.0 (144.2 projected, -6.5) 13.17
2025.02  184.2 179.7 154.6 (135.6 projected, -8.6) 14.42
2025.03 163.7 162.1 134.2 (129.2 projected, -6.4) 15.96
2025.04 162.5 163.6 140.6 (124.6 projected, -4.6) 17.62
2025.05  135.3 138.3 79.2 (119.3 projected, -5.3) 16.9
2025.06 132.7 (1)   21.9 (2A) / 94.0 (2B) / 111.3 (2C) (114.4 projected, -4.9) (40.6)
2025.07       (110.2 projected, -4.2)  
2025.08       (105.5 projected, -4.7)  
2025.09       (101.2 projected, -4.3)  
2025.10       (97.3 projected, -3.9)  
2025.11       (95.0 projected, -2.3)  

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 May 13, 2025

Sunspot activity has been on a slowly decreasing trend since September 2024 (using the average solar flux over 3 solar rotations as a proxy). The decline has become more obvious during the first half of May 2025 with solar flux on May 12 at its lowest level since April 4, 2024. The solar max phase of solar cycle 25 was considerably shorter than that of the most recent solar cycles.

All 365 days smoothed sunspot numbers peaked on October 11-12, 2024
, very likely making this the peak of SC25 (STAR 1K 365d peak: 236.1, STAR 2K 365d peak: 364.3, NOAA SN 365d peak: 156.0, ISN 365d peak: 163.6). The 365d smoothed solar flux peaked on October 13, 2024, just 1.7% below the SC23 peak, and 62.6% above the SC24 peak.

--------------------------------------------------------------------------------------

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.