The geomagnetic field was quiet to briefly unsettled on August 5. Solar wind speed at SOHO ranged between 371 and 435 km/sec. The high latitude magnetometer at Andenes recorded quiet to major storm levels. A brief disturbance was observed started just after midnight early on August 6.
Solar flux density measured at 20h UT on 2.8 GHz was 112.2 - decreasing 24.7 over the previous solar rotation. (Centered 1 year average SF at 1 AU - 183 days ago: 107.17). The Potsdam WDC planetary A index was 5 (STAR Ap - based on the mean of three hour interval ap indices: 5.1). Three hour interval K indices: 32001102 (planetary), 32001312 (Boulder), 64012204 (Andenes).
The background x-ray flux is at the class B4 level (GOES 16).
At the time of counting spots (see image time), spots were observed in 10 active regions using 2K resolution (SN: 187) and in 7 active regions using 1K resolution (SN: 107) SDO/HMI images.
Region 13068 [S16W56] developed in the leading
spot section and produced a few C flares incuding a C4 flare at 06:44 UT
with an associated moderate type II radio sweep. LASCO imagery had only
scant coverage of the hours afterwards and it is uncertain if there was a
CME. C1 flares: C1.1 @ 00:50, C1.0 @ 10:00 UT
Region 13070 [N15W03] was quiet and stable.
Region 13071 [S18E32] was quiet and stable.
Region 13072 [S23W41] decayed early in the day, then developed after
noon.
New region 13073 [S34W42] emerged on August 3 and was numbered 2 days
later by SWPC.
New region 13074 [S16E68] rotated into view on August 4 and was
numbered by SWPC the following day.
Spotted regions not observed (or interpreted
differently) by SWPC:
New region
S7748 [N20E81] rotated into view at the northeast limb.
New region S7749 [S32E03] emerged with a tiny
spot.
New region S7750 [N15E19] was observed with
tiny spots in an old plage area.
New region S7751 [S16W30] emerged with a tiny spot.
A large filament eruption began at about 01:10 UT on August 6 at a high latitude in the southeast quadrant. A CME was observed afterwards, but it is not likely to have a potentially geoeffective component.
C2+ flares:
Magnitude | Peak time (UT) | Location | Source | Recorded by | Comment |
C5.5 | 06:07 | S34W33 | 13073 | GOES16 | |
C4.9 | 06:43 | S13W41 | 13067 | GOES16 | moderate type II radio sweep |
August 3-5: No obviously Earth directed CMEs were observed in available LASCO imagery.
[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 hemisphere coronal hole (CH1092) will be Earth facing on August 5-6.
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 to fair.
Quiet conditions are expected for August 6-7. Quiet to minor storm conditions are possible on August 8-9 due to effects from CH1092.
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 midnigh4t | Area | Classification | SDO / HMI 4K continuum image with magnetic polarity overlays |
Comment | ||||
---|---|---|---|---|---|---|---|---|---|---|---|
SWPC/ USAF |
Magnetic (SDO) |
SWPC | STAR | Current | Previous | ||||||
2K | 1K | ||||||||||
13067 | 2022.07.25 2022.07.26 |
N21W70 | location: N19W66 | ||||||||
13068 | 2022.07.27 2022.07.28 |
7 | 14 | 8 | S15W52 | 0210 | DSO | DAI |
location: S16W56 |
||
13070 | 2022.07.31 2022.08.01 |
3 | 1 | N15W06 | 0007 | BXO | location: N15W03 | ||||
13071 | 2022.08.01 2022.08.03 |
2 | 7 | 2 | S19E30 | 0120 | HSX | CSO | |||
S7742 | 2022.08.01 | N17W47 | |||||||||
S7743 | 2022.08.01 | N21W29 | |||||||||
13072 | 2022.08.03 2022.08.04 |
6 | 28 | 12 | S23W40 | 0020 | BXO | DRI | area: 0090 | ||
13073 | 2022.08.03 2022.08.05 |
3 | 15 | 8 | S35W45 | 0040 | CAO | DAI | area: 0090 | ||
S7746 | 2022.08.03 | S22E07 | |||||||||
13074 | 2022.08.04 2022.08.05 |
1 | 4 | 3 | S18E68 | 0120 | HSX | CSO |
was AR S7747 area: 0180 |
||
S7748 | 2022.08.05 | 1 | N20E81 | 0005 | AXX | ||||||
S7749 | 2022.08.05 | 1 | S32E03 | 0001 | AXX | ||||||
S7750 | 2022.08.05 | 13 | 3 | N15E19 | 0020 | BXO | |||||
S7751 | 2022.08.05 | 1 | S16W30 | 0001 | AXX | ||||||
Total spot count: | 19 | 87 | 37 | ||||||||
Sunspot number: | 69 | 187 | 107 | (total spot count + 10 * number of spotted regions) | |||||||
Weighted SN: | 39 | 110 | 70 | (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): | 76 | 103 | 86 |
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 |
2021.01 | 76.0 | 73.6 | 10.4 | 17.3 (+2.0) | 4.39 |
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 | (65.8 projected, +5.7) | 10.46 |
2022.03 | 117.0 | 115.8 | 78.6 | (70.8 projected, +5.0) | 10.20 |
2022.04 | 130.8 | 131.7 | 84.1 | (75.9 projected, +5.1) | 11.79 |
2022.05 | 133.8 | 136.8 | 96.5 | (82.4 projected, +6.5) | 7.48 |
2022.06 | 116.1 | 119.8 | 70.5 | (88.3 projected, +5.9) | 8.20 |
2022.07 | 125.4 | 129.5 | 91.4 | (95.5 projected, +7.2) | 9.51 |
2022.08 | 102.8 (1) | 6.9 (2A) / 43.0 (2B) / 100.9 (2C) | (102.0 projected, +6.5) | (6.5) | |
2022.09 | (106.9 projected, +4.9) | ||||
2022.10 | (110.1 projected, +3.2) | ||||
2022.11 | (112.9 projected, +2.8) | ||||
2022.12 | (117.7 projected, +4.8) | ||||
2023.01 | (123.7 projected, +6.0) | ||||
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.