The geomagnetic field was at quiet levels on March 17. Solar wind speed at SOHO ranged between 425 and 521 km/sec, averaging 491 km/sec (-69 km/sec compared to the previous day). The high latitude magnetometer at Andenes was at quiet to unsettled 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 111.1 - decreasing 5.3 over the previous solar rotation.
The 365 day average solar flux at 1 AU was 145.71 (183 days ago). The 81 day average solar flux at 1 AU was 138.8 (41 days ago, this is 44.1% 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 4 (STAR Ap - based on the average of three hour interval ap indices: 3.8). Three hour interval K indices: 21111011 (planetary), 12121211 (Boulder), 30111111 (Andenes).
The background x-ray flux is at the class B3 level (GOES 19).
At the time of counting spots (see image time), spots were observed in 7 active regions using 2K resolution (SN: 125) and in 6 active regions using 1K resolution (SN: 85) SDO/HMI images.
AR 14391 [N07W47] was quiet and stable.
AR 14392 [S16E02] lost a few spots and appears to be in slow decay. Another M flare is possible
as there is still polarity intermixing. C1 flares: C1.1 @ 05:35 UT
AR 14393 [N14W31] decayed slowly and quietly.
AR 14395 [S06E13] decayed slowly and quietly.
AR 14396 [N20E28] decayed slowly and could soon become
spotless.
Spotted regions not observed (or interpreted
differently) by SWPC/USAF:
New AR S11933 [S26E68] emerged with tiny spots.
C1 flares: C1.0 @ 22:57 UT
New AR S11934 [N16E80] rotated into view with tiny spots.
C2+ flares
| Magnitude | Peak time (UT) | Location | Source | Recorded by | Comment |
| M1.3 | 09:04 | S14E12 | 14392 | GOES18 |
March 15, 17: No obviously Earth directed CMEs were observed in
available coronagraph imagery.
March 16: An asymmetric partial halo CME was observed after the M2 flare in
AR 14392. The CME could reach Earth on March 19.
[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 (CH1349) rotated across the central meridian on March 11-18. A recurrent trans equatorial negative polarity coronal hole (CH1351) will likely become Earth facing on March 19-21.
The geomagnetic field is expected to be at quiet levels on March 18. On March 19 there is a chance a CME could reach Earth and cause some unsettled to minor storm intervals. Weak effects associated with the southernmost part of CH1349 are possible on March 18-21. Unsettled to major storm conditions are likely on March 22-24 due to effects associated with CH1351.
| 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 | ||||||||||
| 14387 | 2026.03.07 2026.03.08 |
N08W61 |
was AR S11914 location: N10W56 |
||||||||
| 14389 | 2026.03.09 2026.03.10 |
N12W43 |
was AR S11915 location: N14W41 |
||||||||
| 14390 | 2026.03.09 | N26W68 |
 |
was AR S11918 location: N26W62 |
|||||||
| 14393 | 2026.03.09 2026.03.11 |
5 | 5 | 5 | N14W31 | 0030 | CRO | DRO |
 |
 |
was AR S11919/AR 14389 |
| 14391 | 2026.03.10 2026.03.11 |
1 | 5 | 3 | N07W47 | 0010 | AXX | BXO |
 |
 |
was AR S11921 area: 0020 |
| 14392 | 2026.03.11 2026.03.11 |
16 | 27 | 8 | S16E01 | 0200 | CSI | DSI |
 |
 |
beta-gamma was AR S11922 area: 0270 |
| S11925 | 2026.03.12 | S11W35 | |||||||||
| 14394 | 2026.03.12 2026.03.14 |
S12E04 |
was AR S11926 merged with AR 14392 on 2026.03.16 |
||||||||
| S11928 | 2026.03.13 | N07W11 | |||||||||
| 14395 | 2026.03.14 2026.03.14 |
10 | 12 | 7 | S06E13 | 0030 | CRO | CRO |
 |
 |
was AR S11929 area: 0050 |
| S11930 | 2026.03.14 | N25W46 | |||||||||
| S11931 | 2026.03.14 | S01W40 | |||||||||
| 14396 | 2026.03.15 2026.03.15 |
2 | N20E27 | 0003 | AXX |
 |
 |
was AR S11932 location: N20E28 |
|||
| S11933 | 2026.03.17 | 2 | 1 | S26E68 | 0006 | BXO |
 |
||||
| S11934 | 2026.03.17 | 2 | 1 | N16E80 | 0020 | CRO |
 |
||||
| Total spot count: | 32 | 55 | 25 | ||||||||
| Sunspot number: | 72 | 125 | 85 | (total spot count + 10 * number of spotted regions) | |||||||
| Weighted SN: | 43 | 69 | 39 | (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): | 79 | 69 | 68 | ||||||||
| 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 |
| 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 | 128.6 (-4.7) | 17.26 |
| 2025.06 | 131.3 | 135.4 | 114.6 | 124.7 (-3.9) | 21.43 |
| 2025.07 | 137.8 | 142.3 | 125.9 | 122.4 (-2.3) | 11.80 |
| 2025.08 | 154.9 | 158.7 | 133.7 | 118.2 (-4.2) | 9.97 |
| 2025.09 | 154.4 | 156.0 | 129.7 | (113.5 projected, -4.7) | 14.02 |
| 2025.10 | 139.5 | 138.6 | 114.6 | (110.0 projected, -3.5) | 15.64 |
| 2025.11 | 140.3 | 137.3 | 91.7 | (108.3 projected, -1.7) | 21.01 |
| 2025.12 | 160.8 | 155.8 | 124.0 | (107.1 projected, -1.2) | 13.35 |
| 2026.01 | 148.7 | 144.0 | 112.6 | (103.2 projected, -3.9) | 22.47 |
| 2026.02 | 136.4 | 133.1 | 78.2 | (98.9 projected, -4.2) | 12.88 |
| 2026.03 | 129.4 (1) | 45.2 (2A) / 82.4 (2B) / 85.9 (2C) | (94.3 projected, -4.6) | (12.4) | |
| 2026.04 | (90.4 projected, -3.9) | ||||
| 2026.05 | (89.2 projected, -1.2) | ||||
| 2026.06 | (87.1 projected, -2.1) | ||||
| 2026.07 | (82.7 projected, -4.4) | ||||
| 2026.08 | (80.5 projected, -2.2) | ||||
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.
