The geomagnetic field was very quiet on November 18. Solar wind speed at SOHO ranged between 302 and 337 km/sec. The high latitude magnetometer at Andenes recorded quiet to unsettled levels.
Solar flux density measured at 20h UT on 2.8 GHz was 127.1 - increasing 8.3 over the previous solar rotation. (Centered 1 year average SF at 1 AU - 183 days ago: 156.23. In comparison SC24 peaked on June 28, 2014 at 145.50). The Potsdam WDC planetary A index was 2 (STAR Ap - based on the mean of three hour interval ap indices: 1.5). Three hour interval K indices: 00000011 (planetary), 00002211 (Boulder), 00000023 (Andenes).
The background x-ray flux is at the class C1 level (GOES 16).
At the time of counting spots (see image time), spots were observed in 9 active regions using 2K resolution (SN: 139) and in 7 active regions using 1K resolution (SN: 91) SDO/HMI images.
Region 13488 [N27E19] reemerged with tiny
spots.
Region 13489 [S15E58] developed slowly and produced several C flares
after noon. A minor
M class flare is possible.
Spotted regions not observed (or interpreted
differently) by SWPC/USAF:
S9147 [N19W15] was quiet and stable.
S9154 [S19W02] was quiet and stable.
New region S9155 [N18E73] rotated into view
early in the day.
New region S9156 [N23E78] rotated into view with several spots. M
class flares are possible. C1 flares: C1.4 @ 00:07, C1.9 @ 05:05 UT
New region S9157 [N13E32] was observed with a tiny spot in an old
plage area.
New region S9158 [N19E85] rotated partly into view. The leading
penumbra appears to have both negative and positive polarity spots, however,
limb proximity prevented an accurate analysis. A major flare is possible.
New region S9159 [N11E84] rotated partly into view and may be capable
of minor M class flaring.
C2+ flares:
| Magnitude | Peak time (UT) | Location | Source | Recorded by | Comment |
| C2.5 | 04:32 | S9156 | GOES18 | incorrectly attributed by SWPC to smaller simultaneous flare in AR 13489 | |
| M1.2 | 05:42 | S9156 | GOES18 | ||
| C2.2 | 08:37 | S9156 | GOES18 | ||
| C4.0 | 10:43 | S9156 | GOES18 | ||
| C2.8 | 11:52 | S9156 | GOES18 | ||
| C2.2 | 12:55 | S9156 | GOES18 | ||
| C2.1 | 15:27 | 13489 | GOES18 | ||
| M1.2 | 16:44 | S9158 | GOES18 | ||
| C2.9 | 17:09 | 13489 | GOES18 | ||
| C2.4 | 17:38 | S9156 | GOES18 | ||
| C2.1 | 18:06 | 13489 | GOES18 | ||
| C3.3 | 19:59 | S9158 | GOES18 | ||
| M1.0 | 22:33 | S9158 | GOES16 | ||
| C4.3 | 23:03 | 13489 | GOES18 | ||
| C3.3 | 23:28 | 13489 | GOES18 | ||
| C3.6 | 23:48 | 13489 | GOES18 |
November 17-18: No obviously Earth directed CMEs were observed.
November 16: A filament eruption began near 01:30 UT, peaked near
04:15 UT and covered parts of the northwestern quadrant from the central
meridian. A slow moving partial halo CME was observed in LASCO imagery, the
CME could reach Earth on November 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 positive polarity northern hemisphere coronal hole (CH1187) is well defined and was Earth facing on November 17-18. A positive polarity trans equatorial coronal hole (CH1188) formed just west of the central meridian on November 16. It is uncertain if CH1188 will cause any disturbance. A positive polarity northern hemisphere coronal hole (CH1189) will likely become Earth facing on November 23.
Long distance low and medium frequency (below 2 MHz) propagation along paths north of due west over upper middle and high latitudes is good. Propagation on long distance northeast-southwest paths is poor.
The geomagnetic field is expected to be quiet to minor storm on November 19-20 due to the November 16 CME. Quiet to active is likely on November 20-21 due to effects from CH1187.
| 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 |
Magnetic (SDO) |
SWPC | STAR | Current | Previous | ||||||
| 2K | 1K | ||||||||||
| 13486 | 2023.11.11 2023.11.12 |
1 | S09W90 | 0080 | HSX |
 |
rotated out of view | ||||
| S9141 | 2023.11.13 | N25E15 | |||||||||
| S9142 | 2023.11.13 | N09W17 | |||||||||
| 13488 | 2023.11.14 2023.11.14 |
6 | 2 | N31E24 | 0012 | BXO |
 |
location: N27E19 |
|||
| S9145 | 2023.11.14 | S11W46 | |||||||||
| S9147 | 2023.11.15 | 4 | N19W15 | 0010 | BXO |
 |
 |
||||
| S9148 | 2023.11.15 | S15W46 | |||||||||
| S9149 | 2023.11.16 | S08E16 | |||||||||
| 13489 | 2023.11.16 2023.11.17 |
3 | 20 | 10 | S15E58 | 0180 | DAO | EAI |
 |
 |
area: 0220 |
| S9151 | 2023.11.16 | S24E33 | |||||||||
| S9152 | 2023.11.16 | S14W01 | |||||||||
| S9153 | 2023.11.17 | N22E02 |
 |
||||||||
| S9154 | 2023.11.17 | 6 | S19W02 | 0010 | BXO |
 |
 |
||||
| S9155 | 2023.11.18 | 3 | 2 | N18E73 | 0060 | HAX |
 |
||||
| S9156 | 2023.11.18 | 6 | 4 | N23E78 | 0200 | DAO |
 |
||||
| 13490 | 2023.11.18 | 5 | N18E69 | 0080 | DAO | SWPC apparently consider all the northeast limb spots as one region | |||||
| S9157 | 2023.11.18 | 1 | 1 | N13E32 | 0004 | AXX |
 |
||||
| S9158 | 2023.11.18 | 2 | 1 | N19E85 | 0200 | DAC |
 |
beta-delta? tentative classification |
|||
| S9159 | 2023.11.18 | 1 | 1 | N11E84 | 0130 | HSX |
 |
||||
| Total spot count: | 9 | 49 | 21 | ||||||||
| Sunspot number: | 39 | 139 | 91 | (total spot count + 10 * number of spotted regions) | |||||||
| Weighted SN: | 24 | 74 | 46 | (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): | 43 | 76 | 73 | ||||||||
| 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 |
| 2022.04 | 130.8 | 131.7 | 84.0 | 73.0 (+4.3) | 11.79 |
| 2022.05 | 133.8 | 136.8 | 96.5 | 77.4 (+4.4) | 7.48 |
| 2022.06 | 116.1 | 119.8 | 70.3 | 81.1 (+3.7) | 8.20 |
| 2022.07 | 125.4 | 129.5 | 91.4 | 86.7 (+5.6) | 9.51 |
| 2022.08 | 114.2 | 117.1 | 74.6 | 92.6 (+5.9) | 10.92 |
| 2022.09 | 135.1 | 136.5 | 96.0 | 96.5 (+3.9) | 12.18 |
| 2022.10 | 133.5 | 132.7 | 95.5 | 98.9 (+2.4) | 11.16 |
| 2022.11 | 123.4 | 120.7 | 80.5 | 101.2 (+2.3) | 9.33 |
| 2022.12 | 147.9 | 143.4 | 112.8 | 106.7 (+5.5) | 10.99 |
| 2023.01 | 182.4 | 176.6 | 144.4 | 113.3 (+6.6) | 8.73 |
| 2023.02 | 167.2 | 163.2 | 111.3 | 117.8 (+3.5) | 14.48 (current SC25 peak) |
| 2023.03 | 157.2 | 155.6 | 123.3 | 121.0 (+3.2) | 14.42 |
| 2023.04 | 145.4 | 146.4 | 97.6 | 122.7 (+1.7) | 13.40 |
| 2023.05 | 155.6 | 159.2 | 137.4 | (124.7 projected, +2.0) | 10.67 |
| 2023.06 | 161.7 | 166.8 | 160.5 | (127.9 projected, +3.2) | 8.95 |
| 2023.07 | 176.4 | 182.2 | 159.1 | (128.3 projected, +0.4) | 8.15 |
| 2023.08 | 153.7 | 157.6 | 114.8 | (130.1 projected, +1.8) | 7.19 |
| 2023.09 | 154.4 | 156.0 | 133.6 | (133.5 projected, +3.4) | 14.26 |
| 2023.10 | 142.8 | 141.9 | 99.4 | (135.2 projected, +1.7) | 8.16 |
| 2023.11 | 140.1 (1) | 45.8 (2A) / 76.4 (2B) / 93.1 (2C) | (137.8 projected max SC25, +2.6) | (13.0) | |
| 2023.12 | (137.1 projected, -0.7) | ||||
| 2024.01 | (134.4 projected, -2.7) | ||||
| 2024.02 | (134.2 projected, -0.2) | ||||
| 2024.03 | (133.7 projected, -0.5) | ||||
| 2024.04 | (134.5 projected, +0.8) | ||||
| 2024.05 | (135.8 projected, +1.3) | ||||
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 30 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
Looking back 6 months, the 365d smoothed values for solar flux and all sunspot numbers with the exception of NOAA's, are all above their solar cycle 24 peak. The first peak of solar cycle 25 is forecast to be between July 7 and 10, 2023 (solar flux on July 7, ISN and STAR 1K and 2K all have that peak on July 9, while NOAA peaks on July 10). This is unlikely to be the final peak of SC25, however, there is a small probability that it is the actual sunspot and solar flux maximum.
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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.
