The geomagnetic field was at quiet levels on April 28. Solar wind speed at SOHO ranged between 384 and 455 km/sec, averaging 404 km/sec (-16 km/sec compared to the previous day). The high latitude magnetometer at Andenes recorded quiet to minor storm levels. The above 10 MeV proton flux was at background levels.
Solar flux density measured at 20h UT on 2.8 GHz was 153.6 - decreasing 28.3 over the previous solar rotation. The 365 days average solar flux at 1 AU was 194.36 (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 3 (STAR Ap - based on the mean of three hour interval ap indices: 3.4). Three hour interval K indices: 20011001 (planetary), 21122312 (Boulder), 51012001 (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 14 active regions using 2K resolution (SN: 241) and in 11 active regions using 1K resolution (SN: 157) SDO/HMI images.
AR 14064 [N10W81] rotated mostly out of view.
AR 14065 [S32W76] was quiet and stable.
AR 14068 [S25W27] was quiet and stable.
AR 14070 [S12W44] decayed slowly and quietly.
AR 14072 [S18W03] was mostly quiet and stable.
AR 14073 [N12W14] was quiet and stable.
AR 14075 [S09E07] was mostly quiet and stable. C1 flares: C1.6 @
12:42 UT
AR 14076 [N05E18] was quiet and stable.
AR 14077 [S17E19] was mostly quiet and stable. C1 flares: C1.4 @
18:02 UT
New AR 14078 [N16W46] has been observed with spots since April 19.
New flux emerged on April 28 and the region was numbered by SWPC. C1 flares:
C1.5 @ 07:07, C1.5 @ 07:53, C1.4 @ 10:27, C1.7 @ 17:08, C1.4 @ 20:10 UT
New AR 14079 [N07E79] rotated into view with a huge leading penumbra.
An M1.7 flare was recorded at 05:13 UT on April 29. C1 flares: C1.3 @ 12:12,
C1.7 @ 13:02, C1.4 @ 18:57, C1.3 @ 19:37, C1.4 @ 20:57, C1.6 @ 22:23, C1.7 @
23:11, C1.6 @ 23:23 UT
Spotted regions not observed (or interpreted
differently) by SWPC/USAF:
S11021 [N19E26] was quiet and stable.
S11022 [N23W12] was quiet and stable.
S11025 [S11W06] reemerged with tiny spots.
C2+ flares
| Magnitude | Peak time (UT) | Location | Source | Recorded by | Comment |
| C2.2 | 06:02 | 14069 | GOES19 | ||
| C2.1 | 21:45 | 14079 | GOES19 | ||
| C3.2 | 21:52 | 14079 | GOES19 | ||
| C3.9 | 23:55 | 14070 | GOES19 |
April 26-28: 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 northern hemisphere negative polarity coronal hole (CH1289) will rotate across the central meridian on April 28-29.
Long distance low and medium frequency (below 2 MHz) propagation along paths north of due west over upper middle and high latitudes is fair. Propagation on long distance northeast-southwest paths is poor.
The geomagnetic field is expected to be at quiet on April 29-30. Quiet to unsettled levels are possible on May 1-2 due to effects associated with CH1288.
| 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 | ||||||||||
| 14064 | 2025.04.15 2025.04.16 |
2 | 2 | N11W86 | 0100 | DSO | AXX |
 |
 |
was AR S10989 location: N10W81 area: 0010 |
|
| 14065 | 2025.04.16 2025.04.17 |
1 | 1 | 1 | S31W79 | 0030 | HSX | HSX |
 |
 |
was AR S10990 location: S32W76 area: 0060 |
| 14067 | 2025.04.17 2025.04.18 |
S04W83 |
was AR S10994 location: S03W78 |
||||||||
| 14078 | 2025.04.19 2025.04.28 |
2 | 17 | 8 | N16W48 | 0030 | BXO | BXO |
 |
 |
was AR S10999 location: N16W46 |
| 14068 | 2025.04.20 2025.04.21 |
2 | 5 | 3 | S25W31 | 0010 | BXO | AXX |
 |
 |
was AR S11002 location: S25W27 |
| 14070 | 2025.04.20 2025.04.22 |
8 | 16 | 11 | S12W42 | 0060 | DSO | DSI |
 |
 |
beta-gamma was AR S11004 area: 0160 location: S12W44 |
| 14069 | 2025.04.20 2025.04.22 |
1 | S07W72 | 0010 | AXX |
 |
was AR S11006 location: S08W75 spotless |
||||
| S11009 | 2025.04.21 | S08W24 |
 |
||||||||
| 14072 | 2025.04.22 2025.04.23 |
9 | 20 | 10 | S19W05 | 0070 | DAI | DAI |
 |
 |
beta-gamma was AR S11011 area: 0140 location: S18W03 |
| S11012 | 2025.04.22 | S14W54 | |||||||||
| 14073 | 2025.04.23 2025.04.24 |
6 | 1 | N11W14 | 0010 | BXO |
 |
 |
was AR S11015 location: N12W14 |
||
| 14076 | 2025.04.23 2025.04.25 |
1 | 7 | 2 | N06E16 | 0090 | HSX | CSO |
 |
 |
was AR S11017 area: 0170 location: N05E18 |
| 14075 | 2025.04.23 2025.04.25 |
6 | 1 | S11E06 | 0010 | BXO |
 |
 |
was AR S11018 location: S09E07 |
||
| 14077 | 2025.04.24 2025.04.25 |
2 | 9 | 6 | S17E18 | 0010 | HRX | CRO |
 |
 |
was AR S11020 area: 0020 location: S17E19 |
| S11021 | 2025.04.24 | 2 | 1 | N19E26 | 0004 | BXO |
 |
 |
|||
| S11022 | 2025.04.24 | 3 | N23W12 | 0005 | BXO |
 |
 |
||||
| S11025 | 2025.04.25 | 2 | S11W06 | 0004 | AXX |
 |
|||||
| S11026 | 2025.04.26 | S23W15 | |||||||||
| S11027 | 2025.04.26 | S14E34 |
 |
||||||||
| 14079 | 2025.04.28 2025.04.28 |
2 | 5 | 3 | N08E74 | 0120 | DSO | DKC |
 |
was AR S11028 area: 1100 |
|
| Total spot count: | 30 | 101 | 47 | ||||||||
| Sunspot number: | 130 | 241 | 157 | (total spot count + 10 * number of spotted regions) | |||||||
| Weighted SN: | 63 | 134 | 80 | (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): | 143 | 133 | 126 | ||||||||
| 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 | 152.8 (+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 | (160.3 projected, +0.9) | 18.99 |
| 2024.11 | 199.6 | 195.3 | 154.1 | (157.7 projected, -2.6) | 9.33 |
| 2024.12 | 197.3 | 191.2 | 154.6 | (153.9 projected, -3.8) | 8.42 |
| 2025.01 | 190.3 | 184.2 | 137.0 | (148.4 projected, -5.5) | 13.17 |
| 2025.02 | 184.2 | 179.7 | 154.7 | (139.9 projected, -8.5) | 14.42 |
| 2025.03 | 163.7 | 162.1 | 134.2 | (133.5 projected, -6.4) | 15.96 |
| 2025.04 | 163.5 (1) | 117.8 (2A) / 126.3 (2B) / 146.4 (2C) ISN average: 139 |
(128.9 projected, -4.6) | (18.6) | |
| 2025.05 | (123.6 projected, -5.3) | ||||
| 2025.06 | (118.6 projected, -5.0) | ||||
| 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). All 365 days smoothed sunspot numbers peaked on October 11-12, 2024, very likely making this the solar max. SDO1K 365d peak: 236.1, SDO2K 365d peak: 364.4, NOAA SN 365d peak: 156.0, ISN 365d peak: 163.6. The 365d smoothed solar flux peaked on October 13, 2024, only 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.
