The geomagnetic field was at quiet to minor storm levels on August 30. Solar wind speed at SOHO ranged between 304 and 416 km/sec. The high latitude magnetometer at Andenes recorded quiet to major storm levels. The above 10 MeV proton flux was at background levels at the end of the day. A solar wind shock was recorded at SOHO at 06:46 UT with a sudden increase in solar wind speed from 314 to 388 km/s
Solar flux density measured at 20h UT on 2.8 GHz was 214.2 - decreasing 32.9 over the previous solar rotation. (Centered 1 year average SF at 1 AU - 183 days ago: 172.85. In comparison SC24 peaked on June 28, 2014 at 145.50. Current SC25 peak: 172.85 on March 1, 2024). The Potsdam WDC planetary A index was 23 (STAR Ap - based on the mean of three hour interval ap indices: 23.4). Three hour interval K indices: 11435445 (planetary), 21434432 (Boulder), 32364334 (Andenes).
The background x-ray flux is at the class C3 level (GOES 16).
At the time of counting spots (see image time), spots were observed in 17 active regions using 2K resolution (SN: 368) and in 15 active regions using 1K resolution (SN: 231) SDO/HMI images.
AR 13798 [N07W72] decayed slowly and quietly.
AR 13799 [S11W59] decayed slowly and was mostly quiet.
AR 13800 [S27W76] decayed slowly and quietly.
AR 13801 [N08W41] decayed slowly and quietly.
AR 13803 [N14E17] decayed slowly and quietly.
AR 13804 [S24E10] was quiet and stable.
AR 13805 [N09E07] decayed slowly and quietly.
AR 13806 [S11E44] has a small magnetic delta in the southern part of
the main penumbra.
Further M class flaring is likely.
New AR 13807 [S16W05] emerged on August 27 and was noticed by SWPC 3
days later as rapid development continued. M flares are possible.
New AR 13808 [S09E57] rotated into view on August 29 and was numbered
by SWPC the next day. An M flare was recorded early in the day.
Spotted regions not observed (or interpreted
differently) by SWPC/USAF:
S10066 [N23E32] decayed slowly and quietly.
S10067 [N25W36] reemerged with tiny spots.
S10072 [S08E22] was quiet and stable
New region S10075 [S20E06] emerged with tiny spots to the northwest
of AR 13804.
New region S10076 [S08E78] rotated into view with tiny spots.
New region S10077 [S14W12] emerged with tiny spots.
New region S10078 [S20E51] emerged with tiny
spots.
C2+ flares
| Magnitude | Peak time (UT) | Location | Source | Recorded by | Comment |
| C3.6 | 01:15 | 13805 | GOES16 | simultaneous flare at the southeast limb | |
| C6.5/1F | 01:26 | N10E24 | 13805 | GOES16 | 2 flare centers |
| C7.3 | 01:47 | 13796 | GOES16 | incorrectly attributred to AR 13803 by SWPC | |
| M1.2 | 02:06 | S09E70 (SDO/AIA) | 13808 | GOES16 | incorrectly attributred to AR 13806 by SWPC |
| C4.2 | 02:52 | southeast limb | NN | GOES16 | |
| C2.9 | 03:44 | 13806 | GOES16 | ||
| C3.2 | 04:09 | 13807 | GOES16 | ||
| C3.1 | 06:53 | 13807 | GOES16 | ||
| C3.6 | 07:14 | southeast limb | GOES16 | ||
| C4.0 | 07:33 | 13807 | GOES16 | ||
| C5.0 | 07:40 | 13807 | GOES16 | simultaneous flare at the southeast limb | |
| C7.2 | 08:54 | 13806 | GOES16 | ||
| C6.1 | 09:07 | S10E59 | 13806 | GOES16 | |
| C4.3 | 09:54 | 13806 | GOES16 | ||
| C3.4 | 11:07 | 13807 | GOES16 | ||
| M3.8 | 12:20 | 13806 | GOES16 | ||
| C6.3 | 12:53 | southeast limb | S10076 | GOES16 | |
| C6.2 | 13:08 | northeast limb | NN | GOES16 | |
| C3.5 | 14:31 | 13799 | GOES16 | ||
| C3.6 | 14:47 | 13807 | GOES16 | simultaneous flare in AR S10076 | |
| C5.5 | 15:17 | 13807 | GOES16 | ||
| C6.9 | 15:37 | 13807 | GOES16 | ||
| C4.2 | 16:48 | 13807 | GOES16 | ||
| C4.7 | 16:57 | 13806 | GOES16 | ||
| C5.1 | 17:48 | 13807 | GOES16 | ||
| C3.7 | 19:14 | northeast limb | NN | GOES16 | |
| C5.8 | 20:57 | 13806 | GOES16 | ||
| C5.5 | 21:04 | 13807 | GOES16 | ||
| C4.3 | 21:34 | 13807 | GOES16 | ||
| C4.6 | 22:33 | 13807 | GOES16 | simultaneous flare in AR 13806 | |
| C5.4 | 22:44 | 10073 | GOES16 | ||
| C6.4 | 23:07 | 13807 | GOES16 |
August 28-30: 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 narrow trans equatorial negative polarity coronal hole (CH1239) was in an Earth facing position on August 29-30. A positive polarity northern hemisphere coronal hole (CH1240) could rotate into an Earth facing position on September 3.
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 fair.
The geomagnetic field is expected to be at quiet to unsettled levels on August 30 - September 1.
| 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 | ||||||||||
| 13798 | 2024.08.19 2024.08.19 |
1 | 2 | 1 | N04W73 | 0010 | AXX | HRX |
 |
 |
location: N07W72 |
| 13799 | 2024.08.20 2024.08.21 |
4 | 12 | 6 | S11W56 | 0270 | CKO | CHO |
 |
 |
area: 0440 location: S11W59 |
| 13800 | 2024.08.20 2024.08.22 |
4 | 6 | 4 | S28W74 | 0260 | FKO | FHO |
 |
 |
location: S27W76 area: 0380 |
| 13801 | 2024.08.21 2024.08.22 |
4 | 12 | 4 | N07W39 | 0100 | CAO | CAO |
 |
 |
area: 0130 location: N08W41 |
| S10046 | 2024.08.22 | N13W47 | |||||||||
| S10047 | 2024.08.22 | N21W43 | |||||||||
| S10048 | 2024.08.22 | N13W58 | |||||||||
| S10049 | 2024.08.22 | S20W46 | |||||||||
| 13803 | 2024.08.25 2024.08.26 |
1 | 21 | 7 | N13E18 | 0010 | AXX | CRO |
 |
 |
location: N14E17 area: 0050 |
| 13804 | 2024.08.25 2024.08.26 |
1 | 12 | 2 | S26E11 | 0050 | HSX | CAO |
 |
 |
location: S24E10 area: 0070 |
| 13805 | 2024.08.26 | 5 | 1 | N08E07 | 0010 | BXO |
 |
 |
location: N09E07 | ||
| S10060 | 2024.08.26 | S07E28 | |||||||||
| 13807 | 2024.08.27 2024.08.30 |
10 | 33 | 18 | S18W04 | 0070 | DSI | DAI |
 |
 |
beta-gamma location: S16W05 area: 0430 |
| 13806 | 2024.08.27 2024.08.28 |
11 | 53 | 25 | S11E40 | 0450 | FKC | EKC |
 |
 |
beta-gamma-delta location: S11E44 area: 0720 SWPC claims the region spans 24 degrees, in reality it is close to 12 degrees |
| S10063 | 2024.08.27 | N09W15 | |||||||||
| S10064 | 2024.08.27 | S08E08 | |||||||||
| S10065 | 2024.08.28 | N21E24 |
 |
||||||||
| S10066 | 2024.08.28 | 4 | N23E32 | 0006 | BXO |
 |
 |
||||
| S10067 | 2024.08.28 | 3 | 2 | N25W26 | 0008 | AXX |
 |
||||
| S10068 | 2024.08.28 | N01E12 | |||||||||
| S10069 | 2024.08.28 | S16W19 | |||||||||
| 13808 | 2024.08.29 2024.08.30 |
4 | 3 | 2 | S08E60 | 0060 | DAO | DAO |
 |
 |
loction: S09E57 area: 0100 |
| S10071 | 2024.08.29 | N17E30 |
 |
||||||||
| S10072 | 2024.08.29 | 14 | 3 | S08E22 | 0025 | BXO |
 |
 |
|||
| S10073 | 2024.08.29 | N15E67 |
 |
||||||||
| S10074 | 2024.08.29 | S05W22 |
 |
||||||||
| S10075 | 2024.08.30 | 5 | 2 | S20E06 | 0012 | AXX |
 |
||||
| S10076 | 2024.08.30 | 4 | 2 | S08E78 | 0010 | BXO |
 |
||||
| S10077 | 2024.08.30 | 2 | S14W12 | 0003 | BXO |
 |
|||||
| S10078 | 2024.08.30 | 7 | 2 | S20E51 | 0010 | BXO |
 |
||||
| Total spot count: | 40 | 198 | 81 | ||||||||
| Sunspot number: | 130 | 368 | 231 | (total spot count + 10 * number of spotted regions) | |||||||
| Weighted SN: | 90 | 254 | 137 | (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): | 143 | 202 | 185 | ||||||||
| 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 |
| 2022.11 | 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 |
| 2023.03 | 157.2 | 155.6 | 123.3 | 121.1 (+3.3) | 14.42 |
| 2023.04 | 145.4 | 146.4 | 97.6 | 122.9 (+1.8) | 13.40 |
| 2023.05 | 155.6 | 159.2 | 137.4 | 124.2 (+1.3) | 10.67 |
| 2023.06 | 161.7 | 166.8 | 160.5 | 125.3 (+1.1) | 8.95 |
| 2023.07 | 176.4 | 182.2 | 160.0 | 124.6 (-0.7) | 8.15 |
| 2023.08 | 153.7 | 157.6 | 114.8 | 124.3 (-0.3) | 7.19 |
| 2023.09 | 154.4 | 156.0 | 134.2 | 124.0 (-0.3) | 14.26 |
| 2023.10 | 142.8 | 141.9 | 99.4 | 124.8 (+0.8) | 8.16 |
| 2023.11 | 153.5 | 150.2 | 105.4 | 127.8 (+3.0) | 12.20 |
| 2023.12 | 151.1 | 146.4 | 114.2 | 129.4 (+1.6) | 9.60 |
| 2024.01 | 164.6 | 159.3 | 126.0 | 131.1 (+1.7) | 5.46 |
| 2024.02 | 172.5 | 168.3 | 123.0 | (137.4 projected, +6.3) | 5.31 |
| 2024.03 | 154.4 | 152.9 | 103.7 | (144.1 projected, +6.7) | 11.03 |
| 2024.04 | 161.3 | 162.6 | 136.5 | (148.2 projected, +4.1) | 9.69 |
| 2024.05 | 187.7 | 191.9 | 171.7 | (152.9 projected, +4.7) | 23.56 (SC25 peak) |
| 2024.06 | 184.3 | 190.2 | 164.2 | (156.9 projected, +4.0) | 10.24 |
| 2024.07 | 196.6 (cycle peak) |
203.0 | 196.5 (SC25 peak) | (158.7 projected, +1.8) | 7.13 |
| 2024.08 | 246.5 (1) | 195.9 (2A) / 202.4 (2B) / 219.9 (2C) [projected ISN: 217] |
(159.1 projected, +0.4) | (15.5) | |
| 2024.09 | (161.0 projected, +1.9) | ||||
| 2024.10 | (162.8 projected, +1.8) | ||||
| 2024.11 | (160.8 projected, -2.0) | ||||
| 2024.12 | (156.4 projected, -4.4) | ||||
| 2025.01 | (150.3 projected, -6.1) | ||||
| 2025.02 | (143.0 projected, -7.3) | ||||
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
Sunspot counts in July 2024 were the highest we've seen for a single month during solar cycle 25. The first part of August has seen very high sunspot counts, and there more than a remote possibility that we'll see activity in August approaching the most active months of solar cycle 23. With at least 4 consecutive months of high sunspot counts the projected peak for the smoothed ISN (365 days smoothing) has increased significantly to above 160. The month of the peak is currently likely to occur sometime between July and November 2024.
--------------------------------------------------------------------------------------
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.
