The geomagnetic field was at quiet to active levels on April 14 due to effects associated with CH1284. Solar wind speed at SOHO ranged between 398 and 498 km/sec, averaging 443 km/sec (-63 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 152.7 - decreasing 31.3 over the previous solar rotation. (Centered 365d average SF at 1 AU - 183 days ago: 195.79. In comparison SC24 peaked on June 28, 2014 at 145.50 while SC23 peaked on February 23, 2002 at 198.15. SC25 smoothed 365d solar flux max: 195.86 on October 13, 2024 (subtracting a baseline solar flux level of 65, this is +62.56% compared to the SC24 peak and -1.72% compared to the SC23 peak). The Potsdam WDC planetary A index was 17 (STAR Ap - based on the mean of three hour interval ap indices: 17.0). Three hour interval K indices: 34322334 (planetary), 35322322 (Boulder), 46223546 (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 10 active regions using 2K resolution (SN: 184) and in 8 active regions using 1K resolution (SN: 120) SDO/HMI images.
AR 14055 [N09W85] rotated mostly out of view.
Less flares were produced compared to the previous days, however, there is
still a chance of a major flare.
AR 14056 [S07W34] decayed slowly and quietly.
AR 14060 [N07E13] developed further and could be forming magnetic
delta structures. M class flaring is possible.
AR 14061 [N17W29] decayed slowly and quietly.
Spotted regions not observed (or interpreted
differently) by SWPC/USAF:
S10971 [S13W52] was quiet and stable.
S10982 [S17E09] was quiet and stable.
New region S10983 [N24E12] emerged with tiny spots.
New region S10984 [S03E79] rotated into view with large spots.
New region S10985 [N05E73] rotated into view with a tiny spot.
New region S10986 [S20W16] was observed with tiny spots in an old
plage area.
C2+ flares
| Magnitude | Peak time (UT) | Location | Source | Recorded by | Comment |
| C6.4 | 00:20 | 14055 | GOES19 | ||
| C5.3 | 00:44 | 14055 | GOES19 | ||
| C5.5 | 01:27 | behind SW limb | 14054 | GOES19 | |
| C5.6 | 01:40 | 14054 | GOES19 | ||
| C5.6 | 02:07 | 14055 | GOES19 | ||
| C6.1 | 02:13 | 14055 | GOES19 | ||
| C3.0 | 02:53 | 14055 | GOES19 | ||
| C3.2 | 03:05 | 14055 | GOES19 | ||
| C3.7 | 03:23 | 14055 | GOES19 | ||
| C2.8 | 03:38 | 14055 | GOES19 | ||
| C2.8 | 03:44 | 14055 | GOES19 | ||
| C3.1 | 03:51 | 14055 | GOES19 | ||
| C3.0 | 04:15 | 14055 | GOES19 | ||
| C5.0 | 04:49 | 14055 | GOES19 | ||
| C8.1 | 05:56 | 14055 | GOES19 | ||
| M1.4 | 06:05 | 14055 | GOES19 | ||
| M4.2 | 06:50 | N06W82 | 14055 | GOES19 | |
| C4.6 | 07:25 | 14055 | GOES19 | ||
| C3.9 | 07:48 | 14055 | GOES19 | ||
| C2.7 | 08:15 | 14055 | GOES19 | ||
| C2.2 | 10:27 | 14055 | GOES19 | ||
| C2.2 | 11:00 | 14055 | GOES19 | ||
| C3.2 | 14:50 | 14055 | GOES19 | ||
| C4.9 | 15:40 | 14055 | GOES19 | ||
| C2.5 | 16:44 | S10984 | GOES19 | ||
| C2.8 | 17:50 | 14055 | GOES19 | ||
| C6.2 | 18:42 | 14055 | GOES19 | ||
| C3.8 | 18:59 | 14055 | GOES19 | ||
| C6.8 | 20:00 | 14055 | GOES19 | ||
| C2.7 | 21:10 | S10984 | GOES19 | ||
| C2.7 | 22:40 | 14055 | GOES19 |
April 14: No obviously Earth directed CMEs.
April 13: A full halo CME was observed after a very large filament
eruption in the southwestern quadrant (with extensions from just north of
the equator into high latitudes in the southeastern quadrant). This CME will
likely reach Earth on April 16. The eruption caused a large coronal hole to
form in the southwestern quadrant.
April 12: A filament eruption in the southeast quadrant late in the
day was associated with a partial halo CME. There is a chance effects from
this CME could reach Earth early on April 16.
[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 trans equatorial coronal hole (CH1285) was Earth facing on April 14. A positive polarity southern hemisphere coronal hole (CH1286) will likely rotate across the central meridian on April 17-20, however, the associated high speed stream may be too far to the south to cause a geomagnetic disturbance.
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 unsettled levels on April 15. CME effects could cause unsettled to major storm levels on April 16-17.
| 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 | ||||||||||
| 14055 | 2025.04.04 2025.04.05 |
14 | 2 | 1 | N07W92 | 0820 | EKC | HKX |
 |
 |
was AR S10959 location: N09W85 SWPC data is a copy from the previous day |
| 14057 | 2025.04.05 2025.04.07 |
N09W40 |
was AR S10964 location: N07W38 |
||||||||
| 14056 | 2025.04.05 2025.04.06 |
1 | 5 | 3 | S09W36 | 0060 | HSX | CSO |
 |
 |
was AR S10966 area: 0100 location: S07W34 |
| 14061 | 2025.04.06 2025.04.11 |
2 | 7 | 4 | N18W29 | 0010 | BXO | CRO |
 |
 |
was AR S10969 area: 0020 location: N17W29 |
| S10971 | 2025.04.07 | 3 | S13W52 | 0006 | BXO |
 |
 |
||||
| 14058 | 2025.04.08 2025.04.09 |
7 | N16W90 | 0040 | CAO |
 |
was AR S10972 location: N18W89 rotated out of view |
||||
| S10973 | 2025.04.08 | N07W55 |
 |
||||||||
| 14059 | 2025.04.09 2025.04.09 |
N13W15 |
 |
was AR S10976 location: N14W12 |
|||||||
| 14060 | 2025.04.09 2025.04.10 |
12 | 48 | 22 | N08E07 | 0140 | DAI | DAC |
 |
 |
beta-gamma was AR S10977 area: 0380 location: N07E13 SPWC location is way off |
| S10980 | 2025.04.11 | S12W06 | |||||||||
| S10981 | 2025.04.11 | N29W15 | |||||||||
| S10982 | 2025.04.13 | 6 | 1 | S17E09 | 0015 | BXO |
 |
 |
|||
| S10983 | 2025.04.14 | 4 | 3 | N24E12 | 0020 | BXO |
 |
||||
| S10984 | 2025.04.14 | 3 | 3 | S03E79 | 0490 | HKX |
 |
||||
| S10985 | 2025.04.14 | 1 | N05E73 | 0001 | AXX |
 |
|||||
| S10986 | 2025.04.14 | 5 | 3 | S20W16 | 0012 | AXX |
 |
||||
| Total spot count: | 36 | 84 | 40 | ||||||||
| Sunspot number: | 86 | 184 | 120 | (total spot count + 10 * number of spotted regions) | |||||||
| Weighted SN: | 61 | 117 | 73 | (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): | 95 | 101 | 96 | ||||||||
| 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 | 168.9 (1) | 57.2 (2A) / 128.6 (2B) / 148.1 (2C) | (128.8 projected, -4.6) | (19.5) | |
| 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). 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: 364.3, NOAA SN 365d peak: 156.0, ISN 365d peak: 163.5. 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 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.
