The geomagnetic field was at quiet to unsettled levels on April 24. Solar wind speed at SOHO ranged between 385 and 470 km/sec, averaging 407 km/sec (-52 km/sec compared to the previous day). A CIR associated with CH1360 began influencing the geomagnetic field after 15h UT. The high speed stream associated with the coronal hole was observed beginning early on April 25. The high latitude magnetometer at Andenes was at quiet to major storm levels. The above 10 MeV proton flux was at background levels until 09:40 UT, then increased slowly and was just above background levels for the remainder of the day.
Solar flux density measured at 20h UT on 2.8 GHz was 146.3 - decreasing 18.5 over the previous solar rotation.
The 365 day average solar flux at 1 AU was 141.06 (183 days ago). The 81 day average solar flux at 1 AU was 125.3 (41 days ago, this is 35.6% 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 9 (STAR Ap - based on the average of three hour interval ap indices: 8.8). Three hour interval K indices: 21212233 (planetary), 21212222 (Boulder), 31112265 (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 13 active regions using 2K resolution (SN: 267) and in 11 active regions using 1K resolution (SN: 185) SDO/HMI images.
AR 14419 [N15W81] developed early in the day
and a magnetic delta configuration formed in the northern part of the main
penumbra. After the major flares the region decayed slowly and lost its
magnetic delta. C1 flares: C1.4 @ 03:07, C1.7 @ 03:50, C1.9 @ 23:28 UT
AR 14420 [N17E13] developed further gaining spots and area. The
region has 2 magnetic delta configurations and could produce a major flare.
C1 flares: C1.3 @ 00:20, C1.4 @ 00:27 UT
AR 14421 [S11E24] was quiet and stable.
AR 14422 [N08W73] decayed slowly and quietly.
New AR 14423 [S04E31] emerged with many spots on April 23 and was
numbered the next day by SWPC as development continued. A magnetic delta
configuration formed and further M class flares are possible.
New AR 14424 [N17E45] emerged on April 23 and received its NOAA
number the next day.
New AR 14425 [N06E76] rotated into view with several spots. C1
flares: C1.2 @ 00:45 UT
Spotted regions not observed (or interpreted
differently) by SWPC/USAF:
AR S12003 [N26W02] was quiet and stable.
New AR S12012 [N13W23] emerged with several spots.
New AR S12013 [S30E79] rotated into view with a mature spot.
New AR S12014 [N20E34] was observed with tiny spots in an old
plage area.
New AR S12015 [N12E67] rotated into view with a
tiny spot.
New AR S12016 [S23W11] was observed with tiny spots in an old
plage area.
C2+ flares
| Magnitude | Peak time (UT) | Location | Source | Recorded by | Comment |
| X2.5 | 01:07 | 14419 | GOES18 | CME | |
| C7.9 | 04:01 | 14423 | GOES18 | ||
| C2.8 | 04:40 | 14423 | GOES18 | ||
| C3.1 | 05:30 | 14419 | GOES18 | ||
| C2.8 | 05:37 | 14423 | GOES18 | ||
| C3.9 | 07:11 | 14423 | GOES18 | ||
| C2.6 | 07:27 | 14419 | GOES18 | ||
| C3.0 | 07:44 | 14425 | GOES18 | ||
| C3.7 | 07:57 | 14423 | GOES18 | ||
| X2.5/2B | 08:13 | 14419 | GOES18 | CME, strong type II radio sweep | |
| M2.0 | 09:07 | 14423 | GOES18 | ||
| M1.8 | 09:11 | 14423 | GOES18 | ||
| C7.8 | 09:52 | 14423 | GOES18 | ||
| C4.5 | 10:57 | 14420 | GOES18 | ||
| C2.9 | 11:24 | 14420 | GOES18 | ||
| C3.1 | 12:04 | 14425 | GOES18 | ||
| C4.4 | 12:09 | 14423 | GOES18 | ||
| C3.9 | 12:21 | 14425 | GOES18 | ||
| C4.3 | 12:25 | 14423 | GOES18 | ||
| C6.8 | 12:44 | 14425 | GOES18 | ||
| M1.7 | 13:01 | S04E37 | 14423 | GOES18 | |
| M1.5 | 13:11 | 14425 | GOES18 | ||
| C4.1 | 13:37 | 14425 | GOES18 | ||
| C3.9 | 13:48 | 14423 | GOES18 | ||
| C2.5 | 14:18 | 14425 | GOES18 | ||
| C2.3 | 14:22 | 14420 | GOES18 | ||
| C3.5 | 14:38 | S06E37 | 14423 | GOES18 | |
| C2.5 | 14:51 | 14420 | GOES18 | ||
| C2.4 | 15:19 | 14425 | GOES18 | ||
| C2.0 | 15:40 | 14420 | GOES18 | ||
| C3.4 | 16:03 | 14420 | GOES18 | ||
| C3.7 | 16:06 | 14423 | GOES18 | ||
| C2.3 | 16:36 | 14425 | GOES18 | ||
| C3.4 | 16:44 | S05E34 | 14423 | GOES18 | |
| C2.7 | 17:03 | 14425 | GOES18 | ||
| C7.0 | 17:15 | S06E35 | 14423 | GOES18 | |
| M6.4/1F | 18:15 | N18W80 | 14419 | GOES18 | |
| C2.4 | 20:31 | 14420 | GOES18 | ||
| C2.4 | 20:44 | 14420 | GOES18 | ||
| C2.4 | 21:52 | 14419 | GOES18 | ||
| C2.4 | 22:04 | 14420 | GOES18 | ||
| C2.1 | 22:31 | 14420 | GOES18 |
April 22: No obviously Earth directed CMEs were observed in
available coronagraph imagery.
April 23: Multiple CMEs were observed in conjunction with the M
flares. One of them, produced by an M1.2 flare in AR 14420 peaking at 04:58
UT, appears to have some Earth directed components.
April 24: Partial halo CMEs were observed after the major flares in
AR 14419. While the main ejecta are not headed towards Earth, there is a
chance of solar wind shocks on April 26.
[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 northern hemisphere coronal hole (CH1359) will likely become Earth facing on April 22-23. A positive polarity southern hemisphere coronal hole (CH1360) will rotate across the central meridian on April 21-22.
The geomagnetic field is expected to be at quiet to minor levels on April 24-26 due to effects associated with CH1360 and CH1359. The April 23 CME could conmtribute to the disturbance on April 26.
| 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 | ||||||||||
| 14419 | 2026.04.12 2026.04.13 |
7 | 3 | 3 | N15W79 | 0230 | ESO | DSO |
 |
 |
beta-gamma was AR S11991 area: 0180 location: N15W81 |
| S11996 | 2026.04.17 | N00W48 | |||||||||
| S11998 | 2026.04.17 | S14W53 | |||||||||
| S12003 | 2026.04.20 | 10 | 2 | N26W02 | 0020 | BXO |
 |
 |
|||
| 14420 | 2026.04.20 2026.04.21 |
20 | 54 | 28 | N17E10 | 0280 | EKI | FKC |
 |
 |
beta-gamma-delta was AR S12004 area: 0850 location: N17E13 |
| 14421 | 2026.04.20 2026.04.21 |
1 | 3 | 2 | S11E24 | 0045 | HSX | CAO |
 |
 |
was AR S12005 area: 0110 |
| 14422 | 2026.04.21 2026.04.21 |
1 | 1 | 1 | N08W73 | 0015 | HRX | HRX |
 |
 |
was AR S12006 area: 0006 |
| S12007 | 2026.04.21 | N11W21 | |||||||||
| 14423 | 2026.04.23 2026.04.24 |
13 | 27 | 18 | S05E30 | 0100 | DAI | DAC |
 |
 |
beta-delta was AR S12009 area: 0140 location: S04E31 |
| 14424 | 2026.04.23 2026.04.24 |
6 | 12 | 7 | N17E45 | 0030 | CRO | DAO |
 |
 |
was AR S12010 |
| 14425 | 2026.04.24 2026.04.24 |
5 | 8 | 6 | N06E76 | 0075 | DSO | DAC |
 |
was AR S12011 area: 0250 |
|
| S12012 | 2026.04.24 | 9 | 6 | N13W23 | 0040 | DRO |
 |
||||
| S12013 | 2026.04.24 | 1 | 1 | S30E79 | 0050 | HAX |
 |
||||
| S12014 | 2026.04.24 | 4 | N20E34 | 0006 | BXO |
 |
|||||
| S12015 | 2026.04.24 | 1 | 1 | N12E67 | 0002 | AXX |
 |
||||
| S12016 | 2026.04.24 | 4 | S23W11 | 0005 | AXX |
 |
|||||
| Total spot count: | 53 | 137 | 75 | ||||||||
| Sunspot number: | 123 | 267 | 185 | (total spot count + 10 * number of spotted regions) | |||||||
| Weighted SN: | 89 | 183 | 121 | (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): | 135 | 147 | 148 | ||||||||
| 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 |
| 2025.01 | 190.3 | 184.2 | 137.0 | 146.2 (-5.0) | 13.17 |
| 2025.02 | 184.2 | 179.7 | 155.7 | 139.8 (-6.4) | 14.42 |
| 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 | (108.9 projected, -4.0) | 15.64 |
| 2025.11 | 140.3 | 137.3 | 91.7 | (106.9 projected, -2.0) | 21.01 |
| 2025.12 | 160.8 | 155.8 | 124.0 | (105.4 projected, -1.5) | 13.35 |
| 2026.01 | 148.7 | 144.0 | 112.6 | (101.5 projected, -3.9) | 22.47 |
| 2026.02 | 136.4 | 133.1 | 78.2 | (97.3 projected, -4.2) | 12.88 |
| 2026.03 | 131.0 | 129.7 | 85.9 | (92.7 projected, -4.6) | 15.44 |
| 2026.04 | 113.2 (1) | 63.6 (2A) / 79.5 (2B) / 88.9 (2C) ISN month to date: 75. At this level the SSN for October 2025 will become 108.2 |
(88.7 projected, -4.0) | (13.2) | |
| 2026.05 | (87.5 projected, -1.2) | ||||
| 2026.06 | (85.4 projected, -2.1) | ||||
| 2026.07 | (81.0 projected, -4.4) | ||||
| 2026.08 | (78.8 projected, -2.2) | ||||
| 2026.09 | (77.9 projected, -0.9) | ||||
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.
