Solar Terrestrial Activity Report

Activity chart

Last major update issued on August 26, 2022 at 10:00 UT.

Charts (* = updated daily) Data and archive
  Solar wind (*) Solar and geomagnetic data - last month (*)
  Electron fluence (*) Archived daily reports and monthly data since 2003.01 (August 7, 2022)
Solar cycle Solar cycles 23-25 (August 1, 2022) Historical solar and geomagnetic data charts 1954-2006 (April 5, 2007)
  Cycle 24-25 progress (August 1, 2022) Noon SDO sunspot count 1K image / 4K (*)
  Solar cycles 1-24 (July 1, 2020) POES auroral activity level [October 2009 - December 2012]
  Comparison of cycles 21-25 (August 1, 2022) 3rd SSN Workshop, Tucson, 2013
  Comparison of cycles 12-14, 16, 24-25 (August 1, 2022) 4th SSN Workshop, Locarno, 2014
  Solar polar fields vs. solar cycles (August 21, 2022) Cycle 25 spots (final update December 25, 2019)
  Solar cycles 24-25 transition using 365d smoothing Research: Solar Cycle 25 Started on November 17, 2019 with 365 Days Smoothing

Recent activity

The geomagnetic field was quiet on August 25. Solar wind speed at SOHO ranged between 346 and 469 km/sec. The high latitude magnetometer at Andenes recorded quiet levels.

Solar flux density measured at 20h UT on 2.8 GHz was 117.8 - increasing 24.8 over the previous solar rotation. (Centered 1 year average SF at 1 AU - 183 days ago: 109.34). The Potsdam WDC planetary A index was 3 (STAR Ap - based on the mean of three hour interval ap indices: 3.4). Three hour interval K indices: 10111002 (planetary), 10111112 (Boulder), 20022002 (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 11 active regions using 2K resolution (SN: 216) and in 10 active regions using 1K resolution (SN: 152) SDO/HMI images.

Region 13085 [N30W37] decayed slowly and quietly.
Region 13086 [S23E14] matured and was quiet.
Region 13087 [S14E39] was quiet and stable.
New region 13088 [S28W46] emerged on August 24 and continued to develop rapidly on August 25 when the group was numbered by SWPC. The region is currently not very complex magnetically, however, the rapid development spurred one M and multiple C flares. A major flare is possible. C1 flares: C1.8 @ 09:36, C1.4 @ 11:52, C1.7 @ 13:56, C1.5 @ 14:26, C1.9 @ 17:21 UT
New region 13089 [S22E58] emerged on August 24 and developed quickly on August 25 as the region was assigned its NOAA number. The region had a magnetic delta at its center during most of the day, however, this disappeared. Significant polarity intermixing is still present and further M class flares are possible. Early on August 26 the magnetic delta is back. C1 flares: C1.0 @ 02:33, C1.3 @ 04:04, C1.4 @ 07:04, C1.2 @ 09:28, C1.4 @ 12:09, C1.7 @ 15:16, C1.5 @ 17:41, C1.4 @ 21:15 UT
New region 13090 [N16E62] rotated into view on August 23 and was numbered 2 days later by SWPC as the region began to decay. The easternmost spot could be a separate region.

Spotted regions not observed (or interpreted differently) by SWPC:
S7803 [N20E15] was quiet and stable.
New region S7811 [N13E13] emerged with tiny spots.
New region S7812 [N35W37] emerged with a tiny spot to the north of AR 13085.
New region S7813 [N03E01] emerged with tiny spots.
New region S7814 [N34E20] emerged with tiny spots.

C2+ flares:

Magnitude Peak time (UT) Location Source Recorded by Comment
C2.0 06:08 S22E70 13089 GOES16  
C3.6 10:01   13089 GOES16  
C2.0 11:19 S23E68 13089 GOES16  
C2.4 15:48   13089 GOES16  
C2.1 16:01   13089 GOES16  
C3.2 16:40   13089 GOES16  
C7.3/1N 17:58   13089 GOES16  
C7.2 18:58   13088 GOES16  
C8.0 19:09   13089 GOES16  
M1.8/1N 19:51   13088 GOES16 simultaneous flare in AR 13089
C2.2 22:03 S28W42 13088 GOES16  
C2.0 22:34   13089 GOES16  
C9.1 23:19   13088 GOES16  
M1.0 23:27   13089 GOES16  

Coronal mass ejections (CMEs)

August 23-24: No obvious Earth directed CMEs were observed.
August 25: A partial halo CME was observed after 05 UT in LASCO C3 imagery. The distribution of material indicates a northern hemisphere source, however, with the lack of obvious CMEs on the frontside, the source was likely backsided.

Coronal holes

[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 southern hemisphere coronal hole (CH1096) will be rotating across the central meridian on August 25-27.

Propagation

Long distance low and medium frequency (below 2 MHz) propagation along paths north of due west over upper middle and high latitudes is fair to good. Propagation on long distance northeast-southwest paths is poor.

Forecast

Quiet conditions are likely on August 26-27 becoming quiet to active on August 28-29 due to effects from CH1096.

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.

Active solar regions


(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
13084 2022.08.14       S07W78           location: S10W74
13082 2022.08.15
2022.08.16
      N29W65           location: N27W67
S7786 2022.08.16       S17W41            
S7788 2022.08.16       S16W44            
S7792 2022.08.18       N30W38            
13085 2022.08.20
2022.08.21
10 15 6 N32W35 0280 DKO ESO

location: N30W37

13086 2022.08.21
2022.08.23
3 17 10 S24E14 0120 DSO DAO location: S23E14

area: 0080

S7803 2022.08.21   3 1 N20E15 0005   AXX  
S7804 2022.08.21       N28W03            
S7806 2022.08.22       N08W01            
13087 2022.08.22
2022.08.23
1 4 1 S16E38 0040 HAX HAX location: S14E39
13090 2022.08.23
2022.08.25
1 4 2 N14E60 0010 AXX BXO  
13088 2022.08.24
2022.08.25
10 28 14 S26W45 0240 DAI DKC location: S28W46

area: 0500

13089 2022.08.24 9 24 14 S24E56 0150 DSI DAI beta-gamma-delta

location: S22E58

S7811 2022.08.25   6 2 N13E13 0012   CRO    
S7812 2022.08.25   1 1 N35W37 0004   AXX    
S7813 2022.08.25   2   N03E01 0003   BXO    
S7814 2022.08.25   2 1 N34E20 0007   CRO    
Total spot count: 34 106 52  
Sunspot number: 94 216 152  (total spot count + 10 * number of spotted regions)
Weighted SN: 64 142 88  (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): 103 119 122  

Monthly solar cycle data

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
2022.08 111.7 (1)   55.6 (2A) / 69.0 (2B) / 88.6 (2C) (102.0 projected, +6.5) (11.2)
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.

Solar cycles 24-25

Smoothed SF and sunspot numbers

 

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.