The geomagnetic field was very quiet. Solar wind speed at SOHO ranged between 389 and 458 km/sec, averaging 413 km/sec (-76 km/sec compared to the previous day). The high latitude magnetometer at Andenes was at very quiet levels. The above 10 MeV proton flux was at background levels all day.
Solar flux density measured at 20h UT on 2.8 GHz was 119.3 - decreasing 12.3 over the previous solar rotation.
The 365 day average solar flux at 1 AU was 129.02 (183 days ago). The 81 day average solar flux at 1 AU was 109.6 (41 days ago, this is 25.7% 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 3 (STAR Ap - based on the average of three hour interval ap indices: 2.8). Three hour interval K indices: 10110010 (planetary), 00112211 (Boulder), 00000001 (Andenes).
The background x-ray flux is at the class B5 level (GOES 19).
At the time of counting spots (see image time), spots were observed in 13 active regions using 2K resolution (SN: 233) and in 11 active regions using 1K resolution (SN: 161) SDO/HMI images.
AR 14566 [S09W77] decayed quickly and quietly.
AR 14568 [S08W52] decayed slowly and quietly.
AR 14572 [N12E17] developed slowly and quietly.
AR 14573 [N07E08] decayed slowly and quietly.
AR 14574 [N17E33] developed slowly and was
mostly quiet.
AR 14575 [S09E39] developed slowly and quietly.
AR 14576 [S17W24] developed slowly and was mostly quiet. C1 flares:
C1.0 @ 22:30 UT
New AR 14577 [S07E19] emerged on November 12 and developed slowly the
next day when it was numbered by SWPC.
New AR 14578 [S11W19] emerged on November 12 and received its NOAA
number the next day. The region developed slowly and produced a few C
flares. C1 flares: C1.1 @ 14:21, C1.5 @ 22:01 UT
Spotted regions not observed (or interpreted
differently) by SWPC/USAF:
AR S12475 [N08W07] was quiet and stable.
New AR S12480 [N02E49] emerged with tiny spots.
New AR S12481 [N14E84] rotated into view with a large, mature spot.
The region produced the largest flare of the day, and may be capable of M
class flaring. C1 flares: C1.1 @ 17:40 UT
New AR S12482 [N12W47] emerged with a tiny spot.
C2+ flares
| Magnitude | Peak time (UT) | Location | Source | Recorded by | Comment |
| C5.5 | 18:21 | northeast limb | S12481 | GOES18 | LDE |
| C2.6 | 18:59 | 14578 | GOES18 | ||
| C2.0 | 23:40 | 14578 | GOES18 |
November 11-13: No obviously Earth directed CMEs were observed.
[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 southern hemisphere positive polarity coronal hole (CH1411) will be Earth facing on November 13-14.
The geomagnetic field is expected to be quiet on November 13-15. Quiet to active levels are possible on November 16-17 due to effects associated with CH1411.
| 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 | ||||||||||
| 14566 | 2026.11.01 2026.11.02 |
24 | 16 | 8 | S08W62 | 0240 | EAI | EAO |
 |
 |
was AR S12450 location: S09W64 area: 0100 SWPC spot count is much higher than expected |
| S12456 | 2026.11.02 | N05W49 | |||||||||
| 14568 | 2026.11.03 2026.11.05 |
4 | 6 | 2 | S09W42 | 0030 | CSO | CAO |
 |
 |
was AR S12457 location: S09W38 |
| 14570 | 2026.11.05 2026.11.06 |
S09W33 |
was AR S12459 location: S09W38 |
||||||||
| S12460 | 2026.11.05 | S21W34 | |||||||||
| S12463 | 2026.11.05 | N17W45 |
 |
||||||||
| 14569 | 2026.11.06 | S06W74 | |||||||||
| S12465 | 2026.11.07 | N06W07 | |||||||||
| S12466 | 2026.11.07 | S04W01 | |||||||||
| S12467 | 2026.11.07 | 5 | S08W13 | 0006 | BXO |
 |
 |
split off the southern section into AR 14576 on 2026.11.12 | |||
| 14572 | 2026.11.08 2026.11.09 |
2 | 7 | 2 | N12E30 | 0030 | HSX | CRO |
 |
 |
was AR S12468 area: 0015 |
| 14573 | 2026.11.09 2026.11.10 |
3 | 6 | 4 | N08E22 | 0010 | BXO | CRO |
 |
 |
was AR S12469 location: N08E19 |
| 14574 | 2026.11.10 2026.11.11 |
3 | 5 | 4 | N16E47 | 0030 | DRO | DRO |
 |
 |
was AR S12470 |
| 14575 | 2026.11.10 2026.11.11 |
1 | 7 | 3 | S09E52 | 0030 | HSX | CAO |
 |
 |
was AR S12471 area: 0080 |
| S12473 | 2026.11.11 | S12E12 |
 |
||||||||
| S12474 | 2026.11.11 | 1 | S05W02 | 0002 | AXX |
 |
 |
||||
| S12475 | 2026.11.11 | 9 | 3 | N07E08 | 0020 | BXO |
 |
 |
|||
| 14576 | 2026.11.12 2026.11.12 |
8 | 15 | 7 | S18W12 | 0010 | BXO | CRI |
 |
split off from AR S12467 area: 0030 location: S18W09 |
|
| S12476 | 2026.11.12 | 8 | 5 | S07E33 | 0025 | CRO |
 |
||||
| S12477 | 2026.11.12 | 10 | 5 | S11W05 | 0020 | BXI |
 |
||||
| S12478 | 2026.11.12 | 2 | 1 | N05W54 | 0004 | BXO |
 |
||||
| S12479 | 2026.11.12 | 3 | 1 | N25E04 | 0005 | BXO |
 |
||||
| Total spot count: | 45 | 100 | 45 | ||||||||
| Sunspot number: | 115 | 240 | 165 | (total spot count + 10 * number of spotted regions) | |||||||
| Weighted SN: | 68 | 130 | 75 | (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): | 115 | 120 | 124 | (Effective 2026.09.19: SWPC adjustment changed from 1.1 to 1.0, STAR 2K adjustment changed from 0.55 to 0.5, STAR 1K adjustment changed from 0.8 to 0.75) | |||||||
| 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 |
| 2025.08 | 154.9 | 158.7 | 133.7 | 118.4 (-4.1) | 9.97 |
| 2025.09 | 154.4 | 156.0 | 129.7 | 113.1 (-5.3) | 14.02 |
| 2025.10 | 139.5 | 138.6 | 114.6 | 108.5 (-4.6) | 15.64 |
| 2025.11 | 140.3 | 137.3 | 91.7 | 106.9 (-1.6) | 21.01 |
| 2025.12 | 160.8 | 155.8 | 124.0 | 107.0 (-0.1) | 13.35 |
| 2026.01 | 148.7 | 144.0 | 115.0 | 104.1 (-2.9) | 22.47 |
| 2026.02 | 136.4 | 133.1 | 77.4 | 99.7 (-4.4) | 12.88 |
| 2026.03 | 131.0 | 129.7 | 86.6 | 94.4 (-5.3) | 15.44 |
| 2026.04 | 120.0 | 120.9 | 79.0 | 88.6 (-5.8) | 12.10 |
| 2026.05 | 125.4 | 128.2 | 101.8 | (84.4 projected, -4.2) | 9.80 |
| 2026.06 | 137.9 | 142.2 | 93.3 | (80.3 projected, -4.1) | 9.57 |
| 2026.07 | 134.7 | 139.0 | 78.1 | (75.1 projected, -5.2) | 10.16 |
| 2026.08 | 116.1 | 119.0 | 76.0 | (71.7 projected, -3.4) | 8.67 |
| 2026.09 | 105.0 | 106.1 | 60.3 | (69.6 projected, -2.1) | 7.54 |
| 2026.10 | 108.7 | 108.0 | 45.7 | (67.6 projected, -2.0) | 10.73 |
| 2026.11 | 117.8 (1) | 32.0 (2A) / 80.1 (2B) / 69.7 (2C) | (64.4 projected, -3.2) | (10.1) | |
| 2026.12 | (60.9 projected, -3.5) | ||||
| 2027.01 | (58.0 projected, -2.9) | ||||
| 2027.02 | (55.7 projected, -2.3) | ||||
| 2027.03 | (54.4 projected, -1.3) | ||||
| 2027.04 | (53.5 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.
