The geomagnetic field was at quiet to unsettled levels. Solar wind speed at SOHO ranged between 376 and 452 km/sec, averaging 417 km/sec (+8 km/sec compared to the previous day). A solar wind shock was observed at ACE at 04:23 UT on June 5, the arrival of the first of the June 3 CMEs. The high latitude magnetometer at Andenes was at quiet to minor 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 147.9 - increasing 28.4 over the previous solar rotation.
The 365 day average solar flux at 1 AU was 140.14 (183 days ago). The 81 day average solar flux at 1 AU was 126.7 (41 days ago, this is 36.4% 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 5 (STAR Ap - based on the average of three hour interval ap indices: 5.1). Three hour interval K indices: 32002101 (planetary), 33112312 (Boulder), 45113211 (Andenes).
The background x-ray flux is at the class B9 level (GOES 19).
At the time of counting spots (see image time), spots were observed in 14 active regions using 2K resolution (SN: 296) and in 9 active regions using 1K resolution (SN: 170) SDO/HMI images.
AR 14455 [N14W34] was less active than during
the previous days and lost a few spots. There's still significant polarity
intermixing to the north and southwest of the main penumbra. M flares are
possible. C1 flares: C1.1 @ 12:01, C1.1 @ 12:35, C1.5 @ 12:58, C1.4 @ 19:45
UT
AR 14456 [N14W15] decayed slowly and quietly.
AR 14457 [S09W71] developed slowly and produced a few C flares. C1
flares: C1.4 @ 15:44, C1.6 @ 19:53, C1.6 @ 21:45, C1.5 @ 23:42 UT
AR 14458 [S06W21] gained area and could produce a minor M class
flare. C1 flares: C1.8 @ 02:00, C1.2 @ 03:31, C1.3 @ 04:36, C1.2 @ 05:50,
C1.2 @ 11:30. C1.3 @ 22:35, C1.3 @ 23:07 UT
AR 14459 [N13E25] decayed, lost spots and simplified. C1 flares: C1.6
@ 00:31 UT
AR 14460 [S22W83] rotated mostly out of view.
AR 14461 [S21E46] was mostly quiet and stable.
C1 flares: C1.2 @ 06:23, C1.2 @ 10:36, C1.5 @ 11:00 UT
AR 14462 [N16E46] was mostly quiet and stable. C1 flares: C1.2 @
05:11, C1.1 @ 13:55 UT
Spotted regions not observed (or interpreted
differently) by SWPC/USAF:
AR S12114 [N19E14] decayed slowly and quietly.
New AR S12116 [N17W06] emerged with many tiny
spots and polarity intermixing.
New AR S12117 [N16E79] rotated into view at noon with a mature spot.
New AR S12118 [S09W56] emerged with a tiny spot.
New AR S12119 [N19E37] was observed with a tiny spot in an old plage
area.
New AR S12120 [S13E80] rotated into view with a tiny spot.
AR 14446 produced a C1.5 flare at 06:38 and a C1.4
flare at 10:06 UT while rotating over the southwest limb.
A C1.6 flare at 15:58 and a C1.8 flare at 16:34 UT had their origin just
behind the northwest limb.
C2+ flares
| Magnitude | Peak time (UT) | Location | Source | Recorded by | Comment |
| C2.5 | 03:53 | 14457 | GOES18 | ||
| C2.6 | 03:57 | 14458 | GOES18 | ||
| C2.0 | 07:27 | 14462 | GOES18 | ||
| C2.1 | 07:42 | 14455 | GOES18 | ||
| C2.0 | 21:06 | 14458 | GOES18 | LDE |
June 2, 4: No obviously Earth directed CMEs were observed in
available coronagraph imagery.
June 3: CMEs were observed with each of the 3 major flares in AR
14455, all of them are expected to have some Earth directed components.
However, none of the CMEs were particularly impressive and there's
significant uncertainty as to when they will reach Earth and how strong the
disturbances will be.
[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 positive polarity trans equatorial coronal hole (CH1372) was Earth facing on May 31-June 1.
The geomagnetic field is expected to be at unsettled to major storm levels on June 5-6 due to effects related to the June 3 CMEs. Quiet conditions are likely on June 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 | ||||||||||
| 14446 | 2026.05.22 2026.05.23 |
3 | S14W88 | 0130 | CSO |
 |
was AR S12087 area: 0300 location: S14W89 rotated out of view |
||||
| 14449 | 2026.05.23 2026.05.25 |
S08W84 |
was AR S12089 location: S09W79 |
||||||||
| 14448 | 2026.05.23 2026.05.25 |
S05W85 |
was AR S12092 location: S04W78 |
||||||||
| 14454 | 2026.05.26 2026.05.27 |
S15W49 |
was AR S12099 location: S15W42 |
||||||||
| 14455 | 2026.05.26 2026.05.27 |
14 | 28 | 19 | N15W34 | 0325 | DKI | DKI |
 |
 |
beta-gamma was AR S12101 area: 0370 |
| 14457 | 2026.05.27 2026.05.30 |
6 | 13 | 7 | S09W72 | 0015 | CRO | DRI |
 |
 |
was AR S12104 area: 0040 location: S09W71 |
| 14456 | 2026.05.29 2026.05.30 |
2 | 1 | N14W13 | 0005 | AXX |
 |
 |
was AR S12105 location: N14W15 |
||
| 14458 | 2026.05.30 2026.06.01 |
14 | 33 | 18 | S05W21 | 0130 | DAI | DAI |
 |
 |
was AR S12108 area: 0320 location: S06W21 |
| S12109 | 2026.05.31 | S08W57 | |||||||||
| 14459 | 2026.05.31 2026.06.01 |
16 | 18 | 11 | N14E22 | 0130 | DAI | DAI |
 |
 |
was AR S12110 area: 0180 location: N13E25 |
| 14460 | 2026.06.01 2026.06.02 |
4 | 2 | S22W88 | 0090 | DSO | AXX |
 |
 |
was AR S12111 area: 0005 |
|
| 14461 | 2026.06.01 | 8 | 12 | 5 | S21E45 | 0025 | CRI | DRI |
 |
 |
was AR S12112 location: S21E46 |
| S12113 | 2026.06.01 | S24W05 | |||||||||
| S12114 | 2026.06.02 | 9 | N19E14 | 0010 | BXO |
 |
 |
||||
| 14462 | 2026.06.02 2026.06.02 |
12 | 19 | 10 | N17E47 | 0040 | DAO | DAI |
 |
 |
was AR S12115 area: 0080 location: N16E46 |
| S12116 | 2026.06.04 | 16 | 8 | N17W06 | 0060 | DRI |
 |
||||
| S12117 | 2026.06.04 | 1 | 1 | N16E79 | 0140 | HSX |
 |
||||
| S12118 | 2026.06.04 | 1 | S09W56 | 0002 | AXX |
 |
|||||
| S12119 | 2026.06.04 | 1 | N19E37 | 0002 | AXX |
 |
|||||
| S12120 | 2026.06.04 | 1 | S13E80 | 0001 | AXX |
 |
|||||
| Total spot count: | 77 | 156 | 80 | ||||||||
| Sunspot number: | 157 | 296 | 170 | (total spot count + 10 * number of spotted regions) | |||||||
| Weighted SN: | 118 | 195 | 119 | (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): | 173 | 163 | 136 | ||||||||
| 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 |
| 2025.03 | 163.7 | 162.1 | 134.2 | 135.9 (-3.9) | 15.96 |
| 2025.04 | 162.5 | 163.6 | 141.4 | 133.3 (-2.6) | 17.62 |
| 2025.05 | 135.3 | 138.3 | 78.5 | 128.6 (-4.7) | 17.26 |
| 2025.06 | 131.3 | 135.4 | 114.6 | 124.7 (-3.9) | 21.43 |
| 2025.07 | 137.8 | 142.3 | 125.9 | 122.4 (-2.3) | 11.80 |
| 2025.08 | 154.9 | 158.7 | 133.7 | 118.2 (-4.2) | 9.97 |
| 2025.09 | 154.4 | 156.0 | 129.7 | 112.9 (-5.3) | 14.02 |
| 2025.10 | 139.5 | 138.6 | 114.6 | 108.3 (-4.6) | 15.64 |
| 2025.11 | 140.3 | 137.3 | 91.7 | 106.7 (-1.6) | 21.01 |
| 2025.12 | 160.8 | 155.8 | 124.0 | (106.4 projected, -0.3) | 13.35 |
| 2026.01 | 148.7 | 144.0 | 112.6 | (102.7 projected, -3.7) | 22.47 |
| 2026.02 | 136.4 | 133.1 | 78.2 | (98.5 projected, -4.2) | 12.88 |
| 2026.03 | 131.0 | 129.7 | 85.9 | (93.9 projected, -4.6) | 15.44 |
| 2026.04 | 120.0 | 120.9 | 79.3 | (90.0 projected, -3.9) | 12.10 |
| 2026.05 | 125.4 | 128.2 | 101.4 | (88.7 projected, -1.3) | 9.8 |
| 2026.06 | 143.2 (1) | 19.2 (2A) / 144.3 (2B) / 113.1 (2C) | (86.6 projected, -2.1) | (6.8) | |
| 2026.07 | (82.2 projected, -4.4) | ||||
| 2026.08 | (80.1 projected, -2.1) | ||||
| 2026.09 | (79.1 projected, -1.0) | ||||
| 2026.10 | (77.1 projected, -2.0) | ||||
| 2026.11 | (74.3 projected, -2.8) | ||||
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 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.
--------------------------------------------------------------------------------------
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.
