The geomagnetic field was at quiet to severe storm levels on June 3 under the influence of strong CME effects. Solar wind speed at SOHO ranged between 548 and 694 km/sec, averaging 617 km/sec (-80 km/sec compared to the previous day). The high latitude magnetometer at Andenes recorded unsettled to very severe storm levels. The above 10 MeV proton flux was at 0.7 pfu at the end of the day.
Solar flux density measured at 20h UT on 2.8 GHz was 134.8 - decreasing 19.4 over the previous solar rotation. The 365 day average solar flux at 1 AU was 189.52 (183 days ago). SC25 peak: 195.86 on October 13, 2024 (subtracting a baseline solar flux level of 65, this is +62.6% compared to the SC24 peak and -1.7% compared to the SC23 peak). The Potsdam WDC planetary A index was 56 (STAR Ap - based on the mean of three hour interval ap indices: 56.4). Three hour interval K indices: 67656522 (planetary), 56644*32 (Boulder), 68755533 (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 10 active regions using 2K resolution (SN: 201) and in 8 active regions using 1K resolution (SN: 126) SDO/HMI images.
AR 14099 [S13W50] decayed slowly and was mostly
quiet. C1 flares: C1.9 @ 21:44 UT
AR 14100 [N09W39] decayed slowly and was mostly quiet.
AR 14101 [N03W58] decayed slowly and quietly.
AR 14104 [N07W11] decayed slowly and quietly.
New AR 14105 [S14E75] rotated partly into view on June 2 and was
numbered the next day by SWPC. The region was somewhat unstable and could
produce further M class flaring. C1 flares: C1.3 @ 00:26, C1.5 @ 03:27, C1.1
@ 05:24, C1.1 @ 06:45, C1.3 @ 08:39, C1.5 @ 11:36, C1.4 @ 11:46 UT
Spotted regions not observed (or interpreted
differently) by SWPC/USAF:
S11113 [S11E07] reemerged with tiny spots.
S11115 [S11E20] reemerged with tiny spots.
S11116 [N11E47] was quiet and stable.
New region S11123 [N12E26] emerged with tiny spots.
New region S11124 [N19E09] emerged with a tiny spot.
C2+ flares
| Magnitude | Peak time (UT) | Location | Source | Recorded by | Comment |
| C2.2 | 02:09 | 14105 | GOES18 | ||
| C2.7 | 04:27 | 14105 | GOES18 | ||
| C2.1 | 05:57 | 14105 | GOES18 | ||
| C2.3 | 06:20 | 14105 | GOES18 | ||
| M1.4 | 13:03 | 14105 | GOES18 | LDE | |
| C2.8 | 15:10 | 14100 | GOES18 |
June 1-2: No obviously Earth directed CMEs.
June 3: A filament eruption in the northern hemisphere began early in
the day with a positive polarity coronal hole forming after 17h UT. The
associated slow moving CME may have an Earth direct component and could
reach Earth on June 6-7.
[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) will be Earth facing on June 2-4.
The geomagnetic field is expected to be at quiet to unsettled levels on June 4. June 5-7 could see quiet to active levels due to effects from CH1299, maybe with some effects from the June 3 CME on June 6-7.
| 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.
(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 | ||||||||||
| 14099 | 2025.05.24 | 13 | 14 | 7 | S14W50 | 0210 | DAI | DAO |
 |
 |
was AR S11093 area: 0240 location: S13W50 |
| 14100 | 2025.05.25 2025.05.26 |
24 | 45 | 22 | N10W41 | 0320 | EKI | CAI |
 |
 |
beta-gamma was AR S11095 location: N09W39 area: 0380 |
| 14101 | 2025.05.26 2025.05.27 |
1 | 3 | 2 | N04W60 | 0020 | HRX | HRX |
 |
 |
was AR S11098 location: N03W58 |
| S11099 | 2025.05.26 | N13W54 | |||||||||
| 14103 | 2025.05.27 2025.05.28 |
S17W86 |
was AR S11101 location: S17W80 |
||||||||
| S11103 | 2025.05.28 | S08W48 | |||||||||
| 14104 | 2025.05.29 2025.05.30 |
2 | 7 | 2 | N06W12 | 0010 | AXX | BXO |
 |
 |
was AR S11107 location: N07W11 |
| S11112 | 2025.05.30 | S23W33 | |||||||||
| S11113 | 2025.05.31 | 2 | 1 | S11E07 | 0004 | BXO |
 |
||||
| S11114 | 2025.05.31 | N11E27 | |||||||||
| S11115 | 2025.06.01 | 3 | S11E20 | 0006 | BXO |
 |
|||||
| S11116 | 2025.06.01 | 4 | 2 | N11E47 | 0007 | BXO |
 |
 |
|||
| 14105 | 2025.06.02 2025.06.03 |
5 | 18 | 9 | S14E73 | 0030 | DAI | EAC |
 |
was AR S11119 location: S14E75 area: 0200 |
|
| S11120 | 2025.06.02 | N11E69 |
 |
||||||||
| S11121 | 2025.06.02 | S09W13 |
 |
||||||||
| S11122 | 2025.06.02 | S07W17 |
 |
||||||||
| S11123 | 2025.06.03 | 4 | 1 | N12E26 | 0012 | BXO |
 |
||||
| S11124 | 2025.06.03 | 1 | N19E09 | 0002 | AXX |
 |
|||||
| Total spot count: | 45 | 101 | 46 | ||||||||
| Sunspot number: | 95 | 201 | 126 | (total spot count + 10 * number of spotted regions) | |||||||
| Weighted SN: | 68 | 119 | 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): | 105 | 111 | 101 | ||||||||
| 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 | 141.7 (1) | 9.8 (2A) / 98.3 (2B) / 107.1 (2C) | (114.4 projected, -4.9) | (74.6) | |
| 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
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.
