The geomagnetic field was at quiet to active levels on November 29 under the influence of effects associated with CH1332. Solar wind speed at SOHO ranged between 613 and 690 km/sec, averaging 649 km/sec (-19 km/sec compared to the previous day). The high latitude magnetometer at Andenes was at active to major storm levels. The above 10 MeV proton flux was at background levels all day.
Solar flux density measured at 18h UT on 2.8 GHz was 155.3 - increasing 32.3 over the previous solar rotation. The measurement at 20h UT was significantly higher than expected given the measurements at 18 and 22h UT and suspected faulty, therefore using the 18h UT measurement.
The 365 day average solar flux at 1 AU was 157.27 (183 days ago). The 81 day average solar flux at 1 AU was 141.8 (41 days ago, this is 46.0% 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 19 (STAR Ap - based on the average of three hour interval ap indices: 18.6). Three hour interval K indices: 23434433 (planetary), 23444322 (Boulder), 45444465 (Andenes).
The background x-ray flux is at the class C2 level (GOES 19).
At the time of counting spots (see image time), spots were observed in 9 active regions using 2K resolution (SN: 198) and in 7 active regions using 1K resolution (SN: 125) SDO/HMI images.
AR 14287 [N00W65] decayed slowly and quietly.
AR 14288 [N18W45] was mostly quiet and stable.
AR 14290 [S09W33] was mostly quiet and stable.
AR 14291 [S12W29] decayed slowly. There's still polarity intermixing
and C flares are likely.
AR 14294 [S16E73] rotated fully into view revealing a very large spot
group with a huge trailing spot section and several magnetic delta
configurations. The spot groups spans 22 degrees longitude and X class flaring is possible. The region produced many C and
M flares.
Spotted regions not observed (or interpreted
differently) by SWPC/USAF:
AR S11640 [S10E19] was quiet and stable.
New AR S11646 [N10W60] emerged before noon with
several tiny spots.
New AR S11647 [S13E84] rotated partly into view with a huge leader
spot trailing AR 14294.
New AR S11648 [N05E80] rotated into view with a single spot.
C2+ flares
| Magnitude | Peak time (UT) | Location | Source | Recorded by | Comment |
| C9.0 | 01:45 | 14294 | GOES18 | ||
| C2.9 | 02:30 | 14294 | GOES18 | ||
| C2.9 | 02:59 | 14294 | GOES18 | ||
| C2.7 | 03:48 | 14294 | GOES18 | ||
| C3.0 | 04:04 | 14288 | GOES18 | ||
| M1.5 | 04:20 | 14294 | GOES18 | ||
| C4.5 | 05:09 | 14294 | GOES18 | simultaneous flare behind northeast limb | |
| C3.5 | 05:36 | behind northeast limb | GOES18 | ||
| C3.8 | 05:46 | 14294 | GOES18 | ||
| C3.7 | 06:16 | 14288 | GOES18 | ||
| C3.4 | 06:31 | 14294 | GOES18 | ||
| C3.2 | 06:42 | 14294 | GOES18 | ||
| C3.7 | 07:00 | 14294 | GOES18 | ||
| C6.3 | 07:10 | 14294 | GOES18 | ||
| C3.3 | 08:00 | 14294 | GOES18 | ||
| C7.0 | 09:08 | 14294 | GOES18 | simultaneous flare in AR behind the northeast limb | |
| C4.7 | 09:39 | 14294 | GOES18 | ||
| C2.5 | 10:21 | 14294 | GOES18 | ||
| C2.6 | 10:30 | 14294 | GOES18 | ||
| C3.2 | 10:45 | S11647 | GOES18 | ||
| C3.4 | 10:50 | S11647 | GOES18 | ||
| C3.4 | 11:19 | 14294 | GOES18 | ||
| C2.9 | 11:52 | 14294 | GOES18 | ||
| C3.0 | 12:06 | 14294 | GOES18 | ||
| C3.6 | 12:27 | 14294 | GOES18 | ||
| M1.1 | 13:16 | S13E90 | S11647 | GOES18 | |
| C4.1 | 13:57 | 14294 | GOES18 | ||
| C3.2 | 14:21 | 14294 | GOES18 | ||
| C3.5 | 14:48 | 14294 | GOES18 | ||
| C3.9 | 15:02 | 14294 | GOES18 | ||
| M2.9 | 16:06 | behind northeast limb at N20E90 | GOES18 | ||
| M1.1 | 17:15 | S11647 | GOES18 | ||
| M1.0 | 17:27 | 14294 | GOES18 | ||
| C5.0 | 18:39 | 14294 | GOES18 | ||
| C4.4 | 19:16 | 14294 | GOES18 | ||
| C3.7 | 19:41 | 14294 | GOES18 | ||
| M1.4 | 20:14 | S18E80 | 14294 | GOES18 | |
| C3.8 | 20:30 | 14294 | GOES18 | ||
| C3.4 | 21:27 | 14294 | GOES18 | ||
| M1.4/1N | 21:48 | S18E72 | 14294 | GOES18 | |
| C3.3 | 22:31 | 14294 | GOES18 |
November 27-29: No obviously Earth directed CMEs were observed in available coronagraph imagery. Many CMEs were observed from active regions at or behind the east limb.
[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 trans equatorial positive polarity coronal hole (CH1332) was Earth facing on November 22-24. A recurrent trans equatorial negative polarity coronal hole (CH1333) will be Earth facing on November 30 - December 2.
The geomagnetic field is expected to be at quiet to active levels on November 30-December 1 due to lingering effects from CH1332. Mostly quiet levels are likely on December 2. Quiet to minor storm levels are likely on December 3-5 due to effects associated with CH1333.
| 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 | ||||||||||
| 14287 | 2025.11.18 2025.11.19 |
2 | N01W70 | 0002 | AXX |
 |
 |
was AR S11622 location: N00W65 |
|||
| 14289 | 2025.11.19 2025.11.21 |
S02W62 |
was AR S11623 location: S03W55 |
||||||||
| 14288 | 2025.11.20 2025.11.20 |
7 | 21 | 11 | N18W45 | 0090 | DAO | DAI |
 |
 |
beta-gamma was AR S11626 area: 0130 |
| 14290 | 2025.11.20 2025.11.21 |
1 | 7 | 2 | S10W34 | 0040 | HSX | HSX |
 |
 |
was AR S11627 area: 0060 location: S09W33 |
| 14291 | 2025.11.21 2025.11.22 |
14 | 29 | 17 | S14W28 | 0150 | EAI | DAI |
 |
 |
beta-gamma was AR S11630 area: 0190 location: S12W29 |
| 14293 | 2025.11.22 2025.11.24 |
N08W26 |
was AR S11633 location: N08W21 |
||||||||
| S11634 | 2025.11.23 | S18W53 | |||||||||
| S11638 | 2025.11.25 | N26W48 | |||||||||
| S11639 | 2025.11.25 | N09E16 |
|
||||||||
| S11640 | 2025.11.26 | 3 | S10E19 | 0005 | AXX |
 |
 |
||||
| 14294 | 2025.11.28 2025.11.28 |
12 | 36 | 19 | S16E64 | 0800 | FKC | FKC |
 |
 |
beta-gamma-delta was AR S11642 area: 2300 location: S16E73 |
| S11643 | 2025.11.28 | N16W23 |
 |
||||||||
| S11644 | 2025.11.28 | N18E42 |
 |
||||||||
| S11645 | 2025.11.28 | S05W30 |
 |
||||||||
| S11646 | 2025.11.29 | 8 | 4 | N10W60 | 0020 | BXI |
 |
||||
| S11647 | 2025.11.29 | 1 | 1 | S13E84 | 0760 | HHX |
 |
||||
| S11648 | 2025.11.29 | 1 | 1 | N05E80 | 0090 | HAX |
 |
||||
| Total spot count: | 34 | 108 | 55 | ||||||||
| Sunspot number: | 74 | 198 | 125 | (total spot count + 10 * number of spotted regions) | |||||||
| Weighted SN: | 59 | 148 | 95 | (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): | 81 | 109 | 100 | ||||||||
| 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) |
| 2024.07 | 196.6 | 203.0 | 196.8 | 155.0 (+2.3) | 7.13 |
| 2024.08 | 246.1 (SC25 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 | 160.9 (+1.5) (SC25 solar max) | 18.99 |
| 2024.11 | 199.6 | 195.3 | 154.1 | 157.2 (-3.7) | 9.33 |
| 2024.12 | 197.3 | 191.2 | 154.6 | 151.2 (-6.0) | 8.42 |
| 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 | (128.5 projected, -4.8) | 17.26 |
| 2025.06 | 131.3 | 135.4 | 114.6 | (123.8 projected, -4.7) | 21.43 |
| 2025.07 | 137.8 | 142.3 | 125.6 | (120.6 projected, -3.2) | 11.80 |
| 2025.08 | 154.9 | 158.7 | 133.5 | (117.0 projected, -3.6) | 9.97 |
| 2025.09 | 154.4 | 156.0 | 129.8 | (113.1 projected, -3.9) | 14.02 |
| 2025.10 | 139.5 | 138.6 | 114.6 | (109.1 projected, -4.0) | 15.64 |
| 2025.11 | 139.0 (1) | 85.0 (2A) / 88.0 (2B) / 112.4 (2C) ISN average to date: 95 At this level the May 2025 SSN will become 128.7 |
(106.8 projected, -2.3) | (21.5) | |
| 2025.12 | (105.3 projected, -1.5) | ||||
| 2026.01 | (101.2 projected, -4.1) | ||||
| 2026.02 | (97.1 projected, -4.1) | ||||
| 2026.03 | (92.8 projected, -4.3) | ||||
| 2026.04 | (89.0 projected, -3.8) | ||||
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
Sunspot activity was on a decreasing trend from September
2024 until mid August 2025 (using the average solar flux over 3 solar rotations as a proxy).
Then a strong surge in activity saw solar flux peak in late August 2025 just
below the largest peaks seen in 2024. A slow decrease in activity from the
August level has been observed in September and October 2025.
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.
