The geomagnetic field was quiet on October 16. Solar wind speed at SOHO ranged between 330 and 413 km/sec. The high latitude magnetometer at Andenes recorded quiet to active levels.
Solar flux density measured at 20h UT on 2.8 GHz was 144.0 - decreasing 22.1 over the previous solar rotation. (Centered 1 year average SF at 1 AU - 183 days ago: 155.41. 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: 2.0). Three hour interval K indices: 20101000 (planetary), 20101100 (Boulder), 40002000 (Andenes).
The background x-ray flux is at the class B6 level (GOES 16).
At the time of counting spots (see image time), spots were observed in 12 active regions using 2K resolution (SN: 213) and in 10 active regions using 1K resolution (SN: 141) SDO/HMI images.
Region 13463 [S18W31] decayed slowly and
quietly.
Region 13464 [N04W20] was mostly quiet and stable.
Region 13465 [N11E03] gained spots and was mostly quiet. C1 flares:
C1.8 @ 03:53, C1.1 @ 18:01 UT
Region 13466 [N07W65] decayed slowly and was mostly quiet. C1 flares:
C1.7 @ 14:42 UT
Region 13467 [N13E41] has only tiny spots and still managed to
produce a few notable C flares, one of them associated with a partial halo
CME.
New region 13468 [S10E69] rotated into view on October 15 and was
numbered the next day by SWPC.
Spotted regions not observed (or interpreted
differently) by SWPC/USAF:
S9053 [N19W22] was quiet and stable.
S9061 [S14W72] was quiet and mostly stable. C1 flare: C1.8 @ 20:20 UT
S9063 [N04E57] was quiet and stable.
S9064 [S13E03] was quiet and stable.
New region S9067 [N24E79] rotated into view
with small and tiny spots. The region was the source of the largest flare of
the day. C1 flares: C1.1 @ 07:28, C1.4 @ 15:14 UT
New region S9068 [S07W58] emerged with a tiny spot.
C2+ flares:
| Magnitude | Peak time (UT) | Location | Source | Recorded by | Comment |
| C7.5 | 10:51 | 13467 | GOES16 | ||
| C4.9 | 11:15 | 13467 | GOES16 | partial halo CME | |
| C4.8 | 12:33 | 13465 | GOES16 | ||
| C9.8 | 16:06 | S9067 | GOES16 |
October 14-15: No obviously Earth directed CMEs were observed.
October 16: A partial halo CME was observed after C flares in AR
13467 around 11 UT. This CME could reach Earth on October 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 small southern hemisphere positive polarity coronal hole (CH1179) rotated across the central meridian on October 12-13. A small southern hemisphere negative polarity coronal hole (CH1180) was Earth facing on October 16.
Long distance low and medium frequency (below 2 MHz) propagation along paths north of due west over upper middle and high latitudes is good to very good. Propagation on long distance northeast-southwest paths is poor.
The geomagnetic field is expected to be quiet on October 17-18. There is still a chance of weak effects from CH1179 on October 17 if the coronal hole stream arrives. Quiet to unsettled is likely on October 19-20 due to effects from CH1180. If the October 16 CME reaches Earth, we could see unsettled to minor storm conditions on October 19.
| 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 | ||||||||||
| 13459 | 2023.10.05 | N07W86 | |||||||||
| 13461 | 2023.10.05 2023.10.08 |
N13W72 |
 |
location: N11W58 | |||||||
| 13460 | 2023.10.05 2023.10.07 |
1 | S10W87 | 0030 | HSX |
 |
rotated out of view |
||||
| S9031 | 2023.10.06 | N02W55 | |||||||||
| 13462 | 2023.10.06 2023.10.08 |
N20W41 | location: N19W39 | ||||||||
| 13463 | 2023.10.08 2023.10.09 |
12 | 11 | 4 | S17W30 | 0010 | AXX | CRO |
 |
 |
location: S18W31 SWPC spot count is probably a typo |
| 13466 | 2023.10.08 2023.10.11 |
5 | 5 | 2 | N08W62 | 0010 | BXO | HRX |
 |
 |
location: N07W65 |
| 13464 | 2023.10.09 2023.10.10 |
9 | 16 | 10 | N04W19 | 0100 | CSO | DSI |
 |
 |
area: 0140 location: N04W20 |
| 13465 | 2023.10.10 2023.10.11 |
6 | 27 | 14 | N11E03 | 0190 | HAX | DAO |
 |
 |
area: 0290 |
| S9051 | 2023.10.10 | S23W53 | |||||||||
| S9052 | 2023.10.12 | S25W23 | |||||||||
| S9053 | 2023.10.12 | 5 | 2 | N19W22 | 0010 | BXO |
 |
 |
|||
| S9054 | 2023.10.12 | S00E03 | |||||||||
| S9056 | 2023.10.12 | N18W57 | |||||||||
| 13467 | 2023.10.13 2023.10.14 |
2 | 10 | 2 | N13E42 | 0010 | AXX | BXO |
 |
 |
area: 0020 location: N13E41 |
| S9059 | 2023.10.14 | S20W42 | |||||||||
| S9061 | 2023.10.15 | 5 | 4 | S14W72 | 0020 | CRO |
 |
 |
|||
| 13468 | 2023.10.15 2023.10.16 |
1 | 2 | 1 | S09E69 | 0080 | HAX | CSO |
 |
 |
|
| S9063 | 2023.10.15 | 1 | 1 | N04E57 | 0002 | AXX |
 |
 |
|||
| S9064 | 2023.10.15 | 7 | S13E03 | 0012 | BXO |
 |
 |
||||
| S9065 | 2023.10.15 | N07E29 |
 |
||||||||
| S9066 | 2023.10.15 | N20E05 |
 |
||||||||
| S9067 | 2023.10.16 | 3 | 1 | N24E79 | 0010 | HRX |
 |
||||
| S9068 | 2023.10.16 | 1 | S07W57 | 0001 | AXX |
 |
|||||
| Total spot count: | 36 | 93 | 41 | ||||||||
| Sunspot number: | 106 | 213 | 141 | (total spot count + 10 * number of spotted regions) | |||||||
| Weighted SN: | 56 | 120 | 68 | (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): | 117 | 117 | 113 | ||||||||
| 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 |
| 2022.03 | 117.0 | 115.8 | 78.6 | 68.7 (+4.0) | 10.20 |
| 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 | 101.1 (+2.2) | 9.33 |
| 2022.12 | 147.9 | 143.4 | 112.8 | 106.7 (+5.6) | 10.99 |
| 2023.01 | 182.4 | 176.6 | 144.4 | 113.4 (+6.7) | 8.73 |
| 2023.02 | 167.2 | 163.2 | 111.3 | 117.9 (+3.5) | 14.48 (current SC25 peak) |
| 2023.03 | 157.2 | 155.6 | 123.3 | 121.2 (+3.3) | 14.42 |
| 2023.04 | 145.4 | 146.4 | 97.6 | (126.6 projected, +5.4) | 13.40 |
| 2023.05 | 155.6 | 159.2 | 137.4 | (132.2 projected, +5.6) | 10.67 |
| 2023.06 | 161.7 | 166.8 | 160.5 | (135.4 projected, +3.2) | 8.95 |
| 2023.07 | 176.4 | 182.2 | 159.1 | (135.8 projected, +0.4) | 8.15 |
| 2023.08 | 153.7 | 157.6 | 114.9 | (137.6 projected, +1.8) | 7.19 |
| 2023.09 | 154.4 | 156.0 | 133.6 | (141.0 projected, +3.4) | 14.26 |
| 2023.10 | 155.2 (1) | 68.0 (2A) / 131.7 (2B) / 149.8 (2C) | (142.8 projected, +1.8) | (6.) | |
| 2023.11 | (145.4 projected max SC25, +2.6) | ||||
| 2023.12 | (144.5 projected, -0.9) | ||||
| 2024.01 | (141.7 projected, -2.8) | ||||
| 2024.02 | (141.5 projected, -0.2) | ||||
| 2024.03 | (141.0 projected, -0.5) | ||||
| 2024.04 | (138.2 projected, -2.8) | ||||
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 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.
