The geomagnetic field was quiet to unsettled on September 23 under the influence of effects associated with CH1101. Solar wind speed at SOHO ranged between 368 and 503 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 146.3 - increasing 18.8 over the previous solar rotation. (Centered 1 year average SF at 1 AU - 183 days ago: 113.01). The Potsdam WDC planetary A index was 10 (STAR Ap - based on the mean of three hour interval ap indices: 9.9). Three hour interval K indices: 21332323 (planetary), 32433322 (Boulder), 30134334 (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 10 active regions using 2K resolution (SN: 285) and in 8 active regions using 1K resolution (SN: 183) SDO/HMI images.
Region 13102 [S27W67] decayed slowly and
produced a few C flares.
Region 13105 [S16E22] decayed in the leading spot section as the
largest penumbra split into smaller penumbrae and lost area. The region was
mostly quiet.
Region 13107 [S23E38] developed significantly and gained many spots
in the trailing spot section. There is quite a bit of polarity intermixing
and M flares are possible.
Region 13108 [S12W10] was mostly quiet and stable.
Region 13109 [N09W26] developed slowly and produced a few C flares.
New region 13110 [N17E71] rotated into view on September 22 and
developed quickly on September 23. The region is compact and has a magnetic
delta structure. Further M class flares are possible. C1 flares: C1.9 @
02:38, C1.8 @ 12:41 UT
Spotted regions not observed (or interpreted
differently) by SWPC:
New region S7885 [N12W10] emerged early in the day, then decayed
slowly after noon.
New region S7886 [N30E15] emerged with a tiny
spot.
New region S7887 [N20E23] emerged with a tiny spot.
C2+ flares:
| Magnitude | Peak time (UT) | Location | Source | Recorded by | Comment |
| C3.5 | 00:23 | N10W13 | 13109 | GOES16 | |
| C2.2 | 02:37 | 13110 | GOES16 | ||
| C6.0 | 03:39 | S23E49 | 13107 | GOES16 | |
| C2.6 | 04:28 | N15E88 | 13110 | GOES16 | |
| C5.0 | 05:10 | 13110 | GOES16 | ||
| C4.0 | 05:34 | 13110 | GOES16 | ||
| C2.6 | 06:20 | 13105 | GOES16 | ||
| C2.7 | 06:40 | 13110 | GOES16 | ||
| C2.5 | 08:38 | N16E85 | 13110 | GOES16 | |
| C2.8 | 08:55 | N10W16 | 13109 | GOES16 | |
| C2.7 | 09:38 | 13107 | GOES16 | ||
| C2.2 | 09:59 | 13110 | GOES16 | ||
| C2.2 | 11:01 | 13110 | GOES16 | ||
| C7.2 | 11:33 | 13110 | GOES16 | simultaneous flare in AR 13109 | |
| C4.7 | 14:23 | S22E45 | 13107 | GOES16 | |
| C5.6 | 14:52 | 13102 | GOES16 | ||
| C3.6 | 17:16 | 13107 | GOES16 | incorrectly attributed to AR 13102 by SWPC | |
| M1.7 | 18:10 | N19E77 | 13110 | GOES16 | CME, moderate type II and weak type IV radio sweep |
| C8.5 | 18:55 | 13107 | GOES16 | ||
| C2.4 | 20:40 | 13110 | GOES16 | ||
| C2.0 | 21:55 | 13107 | GOES16 | ||
| C2.6 | 22:15 | 13110 | GOES16 | ||
| C3.0 | 22:27 | S24E41 | 13107 | GOES16 | |
| C3.0 | 22:43 | 13107 | GOES16 | ||
| C3.6 | 23:29 | N10W24 | 13109 | GOES16 |
September 21-23: 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 trans equatorial coronal hole (CH1101) was in an Earth facing position on September 19-20. A recurrent southern hemisphere coronal hole (CH1102) will rotate across the central meridian on September 22-24.
Long distance low and medium frequency (below 2 MHz) propagation along paths north of due west over upper middle and high latitudes is poor. Propagation on long distance northeast-southwest paths is poor.
Quiet to unsettled conditions are likely on September 24 due to effects from CH1101. Quiet to active conditions are possible on September 25-27 due to effects from CH1102.
| Coronal holes (1) | Coronal mass ejection (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 | ||||||||||
| 13102 | 2022.09.12 2022.09.13 |
4 | 7 | 6 | S25W66 | 0160 | DAO | DSO |
 |
 |
location: S27W67 |
| S7872 | 2022.09.15 | S19W54 | |||||||||
| S7875 | 2022.09.17 | N33W45 | |||||||||
| 13105 | 2022.09.19 2022.09.19 |
20 | 57 | 36 | S16E21 | 0370 | DKI | EAI |
 |
 |
location: S16E22 |
| 13106 | 2022.09.19 2022.09.20 |
3 | S12E10 | 0005 |
 |
location: S12E09 |
|||||
| 13108 | 2022.09.20 2022.09.21 |
6 | 20 | 9 | S12W10 | 0090 | CSO | DSI |
 |
 |
|
| 13107 | 2022.09.20 2022.09.21 |
10 | 48 | 28 | S24E37 | 0230 | CAO | FAI |
 |
 |
beta-gamma location: S23E38 |
| 13109 | 2022.09.21 2022.09.22 |
7 | 32 | 13 | N09W26 | 0040 | DRO | DRI |
 |
 |
area: 0070 |
| 13110 | 2022.09.22 2022.09.23 |
4 | 15 | 9 | N16E72 | 0160 | CAO | DAC |
 |
 |
beta-delta location: N17E71 |
| S7885 | 2022.09.23 | 1 | N12W10 | 0001 | AXX |
 |
|||||
| S7886 | 2022.09.23 | 1 | 1 | N30E15 | 0003 | AXX |
 |
||||
| S7887 | 2022.09.23 | 1 | 1 | N20E23 | 0002 | AXX |
 |
||||
| Total spot count: | 51 | 185 | 103 | ||||||||
| Sunspot number: | 111 | 285 | 183 | (total spot count + 10 * number of spotted regions) | |||||||
| Weighted SN: | 84 | 213 | 131 | (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): | 122 | 157 | 146 | ||||||||
| 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 (solar max) | 7.88 |
| 2017.09 | 91.3 | 92.3 | 43.6 | 18.2 (-1.3) | 18.22 (cycle 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 |
| 2021.02 | 74.3 | 72.4 | 8.2 | 19.0 (+1.7) | 9.50 |
| 2021.03 | 76.0 | 75.2 | 17.2 | 21.7 (+2.7) | 10.17 |
| 2021.04 | 75.9 | 76.4 | 24.5 | 24.8 (+3.1) | 8.40 |
| 2021.05 | 75.3 | 77.1 | 21.2 | 25.8 (+1.0) | 6.50 |
| 2021.06 | 79.4 | 81.8 | 25.0 | 27.6 (+1.8) | 5.52 |
| 2021.07 | 81.0 | 83.6 | 34.3 | 31.4 (+3.8) | 5.51 |
| 2021.08 | 77.7 | 79.7 | 22.0 | 35.4 (+4.0) | 6.19 |
| 2021.09 | 87.0 | 88.2 | 51.3 | 40.2 (+4.8) | 6.33 |
| 2021.10 | 88.9 | 88.3 | 37.4 | 45.2 (+5.0) | 7.38 |
| 2021.11 | 86.2 | 84.4 | 34.8 | 50.8 (+5.6) | 9.83 |
| 2021.12 | 103.0 | 99.8 | 67.5 | 55.9 (+5.1) | 6.40 |
| 2022.01 | 103.8 | 100.5 | 55.3 | 60.1 (+4.2) | 8.92 |
| 2022.02 | 109.1 | 106.5 | 60.9 | 64.8 (+4.7) | 10.46 |
| 2022.03 | 117.0 | 115.8 | 78.6 | (68.7 projected, +3.9) | 10.20 |
| 2022.04 | 130.8 | 131.7 | 84.1 | (73.9 projected, +5.2) | 11.79 |
| 2022.05 | 133.8 | 136.8 | 96.5 | (80.3 projected, +6.4) | 7.48 |
| 2022.06 | 116.1 | 119.8 | 70.5 | (86.2 projected, +5.9) | 8.20 |
| 2022.07 | 125.4 | 129.5 | 91.4 | (93.4 projected, +7.2) | 9.51 |
| 2022.08 | 114.2 | 117.1 | 75.4 | (100.0 projected, +6.6) | 10.92 |
| 2022.09 | 134.5 (1) | 61.0 (2A) / 79.6 (2B) / 105.8 (2C) | (104.9 projected, +4.9) | (13.1) | |
| 2022.10 | (108.1 projected, +3.2) | ||||
| 2022.11 | (110.9 projected, +2.8) | ||||
| 2022.12 | (115.7 projected, +4.8) | ||||
| 2023.01 | (121.7 projected, +6.0) | ||||
| 2023.02 | (126.7 projected, +5.0) | ||||
| 2023.11 | (142.5 projected max SC25) | ||||
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: SIDC-SILSO.
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.
