The geomagnetic field was at quiet to active levels on April 10 due to effects associated with CH1283 before noon and CH1284 after noon. Solar wind speed at SOHO ranged between 427 and 574 km/sec, averaging 490 km/sec (-41 km/sec compared to the previous day). The high latitude magnetometer at Andenes recorded quiet to major storm levels. The above 10 MeV proton flux was at background levels.
Solar flux density measured at 20h UT on 2.8 GHz was 152.6 - decreasing 27.5 over the previous solar rotation. (Centered 1 year average SF at 1 AU - 183 days ago: 195.74. In comparison SC24 peaked on June 28, 2014 at 145.50 while SC23 peaked on February 23, 2002 at 198.15. Current SC25 peak: 195.74 on October 10, 2024 (subtracting a baseline solar flux level of 65, this is +62.41% compared to the SC24 peak and -1.81% compared to the SC23 peak). The Potsdam WDC planetary A index was 16 (STAR Ap - based on the mean of three hour interval ap indices: 16.4). Three hour interval K indices: 44422234 (planetary), 44422323 (Boulder), 55432366 (Andenes).
The background x-ray flux is at the class C1 level (GOES 18).
At the time of counting spots (see image time), spots were observed in 12 active regions using 2K resolution (SN: 245) and in 11 active regions using 1K resolution (SN: 177) SDO/HMI images.
AR 14048 [S16W74] rotated partly out of view
and was mostly quiet as decay continued. C1 flares: C1.8 @ 01:46, C1.2 @
21:10 UT
AR 14054 [S12W56] decayed slowly and was mostly quiet. C1 flares:
C1.3 @ 15:42 UT
AR 14055 [N08W36] developed further gaining area and spots. The
region still has polarity intermixing and an M flare is possible. C1 flares:
C1.5 @ 03:49, C1.2 @ 13:56 UT
AR 14056 [S06E18] was mostly quiet and stable. C1 flares: C1.6 @
10:34 UT
AR 14057 [N08E16] was quiet and stable.
AR 14058 [N18W38] decayed slowly and quietly.
AR 14059 [N11E43] was quiet and stable.
New AR 14060 [N07E64] rotated into view on April 9 and was numbered
by SWPC the next day as the region decayed slowly. C1 flares: C1.5 @ 12:40,
C1.2 @ 15:03 UT
Spotted regions not observed (or interpreted
differently) by SWPC/USAF:
S10969 [N17E25] gained tiny spots and was mostly quiet.
S10970 [S21W25] was quiet and stable.
S10971 [S16E05] was quiet and stable.
New region S10979 [N01W62] emerged with tiny spots.
C2+ flares
| Magnitude | Peak time (UT) | Location | Source | Recorded by | Comment |
| C2.5 | 03:05 | 14048 | GOES19 | ||
| C2.3 | 04:50 | 14060 | GOES18 | ||
| C2.2 | 05:37 | 14055 | GOES19 | ||
| C2.1 | 05:47 | 14055 | GOES19 | ||
| C3.2 | 06:28 | 14055 | GOES19 | ||
| C3.1 | 06:43 | N07W26 | 14055 | GOES19 | |
| C5.4 | 07:52 | 14060 | GOES19 | ||
| C2.8 | 08:18 | N07W24 | 14055 | GOES19 | |
| C3.7 | 16:51 | 14048 | GOES19 |
April 8-10: No obviously Earth directed CMEs.
[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 (CH1284) was Earth facing on April 7-9.
Long distance low and medium frequency (below 2 MHz) propagation along paths north of due west over upper middle and high latitudes is poor. Propagation on long distance northeast-southwest paths is poor to fair.
The geomagnetic field is expected to be at quiet to active levels on April 11-13 due to effects from CH1284.
| 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 | ||||||||||
| 14048 | 2025.03.28 2025.03.29 |
12 | 10 | 6 | S16W79 | 0180 | FAO | CRO |
 |
 |
was AR S10940 location: S16W74 |
| 14055 | 2025.04.04 2025.04.05 |
14 | 41 | 25 | N08W36 | 0120 | DAI | DAC |
 |
 |
beta-gamma was AR S10959 area: 0430 |
| 14054 | 2025.04.04 2025.04.05 |
4 | 13 | 8 | S12W57 | 0150 | DSO | DAO |
 |
 |
was AR S10960 area: 0200 location: S12W56 |
| S10961 | 2025.04.04 | N06W18 | |||||||||
| 14057 | 2025.04.05 2025.04.07 |
4 | 3 | N08E13 | 0010 | AXX |
 |
 |
was AR S10964 location: N08E16 |
||
| 14056 | 2025.04.05 2025.04.06 |
1 | 3 | 2 | S07E17 | 0070 | HSX | CSO |
 |
 |
was AR S10966 area: 0140 location: S06E18 |
| S10968 | 2025.04.06 | N20W16 | |||||||||
| S10969 | 2025.04.06 | 11 | 5 | N17E25 | 0030 | CRO |
 |
 |
|||
| S10970 | 2025.04.07 | 4 | S21W25 | 0005 | BXO |
 |
 |
||||
| S10971 | 2025.04.07 | 9 | 1 | S16E05 | 0020 | BXO |
 |
 |
|||
| 14058 | 2025.04.08 2025.04.09 |
8 | 15 | 8 | N18W40 | 0050 | DAO | DRI |
 |
 |
beta-gamma was AR S10972 location: N18W38 |
| S10973 | 2025.04.08 | N07W04 |
 |
||||||||
| S10975 | 2025.04.08 | S08W24 | |||||||||
| 14059 | 2025.04.09 2025.04.09 |
1 | 4 | 2 | N11E39 | 0010 | CRO | DRO |
 |
 |
was AR S10976 location: N11E43 area: 0020 |
| 14060 | 2025.04.09 2025.04.10 |
2 | 9 | 6 | N07E57 | 0100 | DAO | CAO |
 |
 |
was AR S10977 area: 0300 location: N07E64 SWPC location is way off |
| S10979 | 2025.04.10 | 2 | 1 | N01W62 | 0004 | BXO |
 |
||||
| Total spot count: | 42 | 125 | 67 | ||||||||
| Sunspot number: | 112 | 245 | 177 | (total spot count + 10 * number of spotted regions) | |||||||
| Weighted SN: | 75 | 157 | 99 | (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): | 123 | 135 | 142 | ||||||||
| Month | Average solar flux | International sunspot number (WDC-SILSO) |
Smoothed sunspot number (4) | Average
ap (3) |
|
|---|---|---|---|---|---|
| Measured | 1 AU | ||||
| 2014.02 | 170.3 (cycle peak) |
166.3 | 146.1 (SC24 peak) | 110.5 | 10.70 |
| 2014.04 | 143.9 | 144.8 | 112.5 | 116.4 (SC24 solar max) | 7.88 |
| 2017.09 | 91.3 | 92.3 | 43.6 | 18.2 (-1.3) | 18.22 (SC24 peak) |
| 2019.11 | 70.2 | 68.7 | 0.5 | 2.0 (-0.6) (Solar minimum using 365d smoothing: November 17, 2019) |
4.19 |
| 2019.12 | 70.8 | 68.6 | 1.6 | 1.8 (-0.2) (ISN 13 months smoothed solar minimum) |
3.22 |
| 2023.10 | 142.8 | 141.9 | 99.9 | 124.8 (+0.8) | 8.16 |
| 2023.11 | 153.5 | 150.2 | 107.1 | 127.9 (+3.1) | 12.20 |
| 2023.12 | 151.1 | 146.4 | 113.5 | 129.5 (+1.6) | 9.60 |
| 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 | 152.7 (+3.6) | 10.24 |
| 2024.07 | 196.6 | 203.0 | 196.8 | 154.9 (+2.3) | 7.13 |
| 2024.08 | 246.1 (cycle peak) |
252.2 | 216.0 (SC25 peak) | 156.7 (+1.8) | 15.96 |
| 2024.09 | 195.7 | 197.8 | 141.1 | 159.3 (+1.6) | 15.36 |
| 2024.10 | 221.0 | 219.6 | 166.4 | (160.2 projected, +0.9) | 18.99 |
| 2024.11 | 199.6 | 195.3 | 152.5 | (157.6 projected, -2.6) | 9.33 |
| 2024.12 | 197.3 | 191.2 | 154.5 | (153.8 projected, -3.8) | 8.42 |
| 2025.01 | 190.3 | 184.2 | 137.0 | (148.3 projected, -5.5) | 13.17 |
| 2025.02 | 184.2 | 179.7 | 154.7 | (139.8 projected, -8.5) | 14.42 |
| 2025.03 | 163.7 | 162.1 | 134.2 | (133.4 projected, -6.4) | 15.96 |
| 2025.04 | 171.2 (1) | 47.1 (2A) / 141.4 (2B) / 167.6 (2C) | (128.8 projected, -4.6) | (20.8) | |
| 2025.05 | (123.5 projected, -5.3) | ||||
| 2025.06 | (118.6 projected, -4.9) | ||||
| 2025.07 | (114.5 projected, -4.1) | ||||
| 2025.08 | (109.8 projected, -4.7) | ||||
| 2025.09 | (105.5 projected, -4.3) | ||||
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). Currently all 365 days smoothed indices are still indicating that a peak occurred on October 12 or 13, 2024. Should sunspot activity decrease even further then there is a possibility that the peak may have taken place in September 2024. Any peak outside of September-October 2024 appears unlikely. The 365 days average solar flux is likely to max out ~2% below the peak of solar cycle 23. The maximum 365d smoothed solar flux of SC23 and SC25 are similar, however, sunspot numbers were significantly lower during SC25 compared to SC23.
--------------------------------------------------------------------------------------
This report has been prepared by Jan Alvestad. It is based on the analysis of data from whatever 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.
