Solar Terrestrial Activity Report

Activity chart

Last major update issued on July 22, 2023 at 08:05 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 (July 6, 2023)
Solar cycle Solar cycles 23-25 (July 1, 2023) Historical solar and geomagnetic data charts 1954-2006 (April 5, 2007)
  Cycle 24-25 progress (July 1, 2023) 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 (July 1, 2023) 3rd SSN Workshop, Tucson, 2013
  Comparison of cycles 12-14, 16, 24-25 (July 1, 2023) 4th SSN Workshop, Locarno, 2014
  Solar polar fields vs. solar cycles (July 10, 2023) 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 to active on July 21 due to CME influences. Solar wind speed at SOHO ranged between 361 and 423 km/sec. The high latitude magnetometer at Andenes recorded quiet to major storm levels. A solar wind shock was observed at ACE at 16:08 UT, the likely arrival of the July 17 CME. A transient was observed arriving at DSCOVR at 19:24 UT, probably related to a CME observed on July 18.

Solar flux density measured at 20h UT on 2.8 GHz was 172.8 - increasing 12.0 over the previous solar rotation. (Centered 1 year average SF at 1 AU - 183 days ago: 147.98. In comparison SC24 peaked on June 28, 2014 at 145.50). The Potsdam WDC planetary A index was 12 (STAR Ap - based on the mean of three hour interval ap indices: 11.8). Three hour interval K indices: 33211224 (planetary), 34222334 (Boulder), 45122326 (Andenes).

The background x-ray flux was 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: 257) and in 8 active regions using 1K resolution (SN: 154) SDO/HMI images.

Region 13372 [N22W52] decayed slowly and produced a few low level C flares. The region was the source of an M3.1 flare at 03:36 UT on July 22. C1 flares: C1.4 @ 04:20, C1.8 @ 23:21 UT
Region 13373 [N07W25] decayed slowly in the intermediate spot section. The region was the source of an M1.0 flare at 04:16 on July 22. C1.4 flares: C1.4 @ 04:41, C1.4 @ 08:14, C1.7 @ 22:29, C1.7 @ 22:52  UT
Region 13376 [N22W11] was quiet and stable.
Region 13377 [S09E20] was quiet and stable.
Region 13378 [S27W15] decayed slowly and was mostly quiet. C1 flares: C1.5 @ 07:40, C1.5 @ 09:52 UT
Region 13379 [N15E44] was mostly unchanged and quiet. C1 flares: C1.9 @ 05:47 UT

Spotted regions not observed (or interpreted differently) by SWPC/USAF:
S8775 [S25E18] was quiet and stable.
S8781 [N14E04] was quiet and stable.
S8784 [S43E51] was quiet and stable.
New region S8786 [N10E18] emerged with a tiny spot.
New region S8787 [N07W64] emerged with a tiny spot.

A C1.4 flare at 20:13 UT had its origin behind the southeast limb.

C2+ flares:

Magnitude Peak time (UT) Location Source Recorded by Comment
C2.2 00:30   13373 GOES16  
C2.1 10:54 N05W19 13373 GOES16  

Coronal mass ejections (CMEs)

July 19-21: No obviously Earth directed CMEs were observed.
July 22: A CME was associated with an M1.0 flare in AR 13373 early in the day. It is not yet certain if this CME has any Earth directed components.

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 (CH1161) was in an Earth facing position on July 18.

Propagation

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.

Forecast

The geomagnetic field is expected to be quiet to unsettled on July 22 due to CME effects. Weak effects from CH1161 are possible on April 23. Quiet conditions are likely on July 24.

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
13371 2023.07.10
2023.07.11
      S15W67          

location: S15W62

13372 2023.07.11
2023.07.11
9 20 14 N23W51 0340 EKO FKO

area: 0520

location: N22W52

13373 2023.07.13
2023.07.14
22 43 26 N08W30 0550 EKC FKC beta-delta

area: 0720

location: N07W25

13374 2023.07.13
2023.07.14
      S08W26          
S8765 2023.07.13       S00W55            
S8771 2023.07.15       S32W18            
13376 2023.07.15
2023.07.17
9 17 5 N25W11 0100 CSO CSO

area: 0180

location: N22W11

13377 2023.07.17
2023.07.17
5 11 6 S09E20 0210 DSO DHO

area: 0570

S8775 2023.07.17   11   S25E18 0015   BXO  
S8777 2023.07.17       S19W24            
13378 2023.07.18
2023.07.19
8 18 10 S26W14 0030 CRO CSO area: 0090
13379 2023.07.18
2023.07.19
8 14 10 N16E48 0270 FHO FHI area: 0530

location: N15E44

S8780 2023.07.18       N19E46           included in AR 13379
S8781 2023.07.18   9 2 N14E04 0020   BXO  
S8782 2023.07.19       N12E07            
S8783 2023.07.19       S25W38            
S8784 2023.07.20   2 1 S43E51 0010   CRO  
S8785 2023.07.20       S18W43          
S8786 2023.07.21   1   N10E18 0002   AXX    
S8787 2023.07.21   1   N07W64 0001   AXX    
Total spot count: 61 147 74  
Sunspot number: 121 257 154  (total spot count + 10 * number of spotted regions)
Weighted SN: 104 200 127  (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): 133 141 123  

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 (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
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 64.7 (+4.6) 10.46
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 92.5 (+5.8) 10.92
2022.09 135.1 136.5 96.0 96.4 (+3.9) 12.18
2022.10 133.5 132.7 95.5 98.7 (+2.3) 11.16
2022.11 123.4 120.7 80.5 101.0 (+2.3) 9.33
2022.12 147.9 143.4 112.8 106.6 (+5.6) 10.99
2023.01 182.4 176.6 143.6 (113.7 projected, +6.1) 8.73
2023.02 167.2 163.2 110.9 (118.5 projected, +4.8) 14.48
(current
SC25 peak)
2023.03 157.2 155.6 122.6 (121.6 projected, +3.1) 14.42
2023.04 145.4 146.4 96.4 (127.0 projected, +5.4) 13.40
2023.05 155.6 159.2 137.9 (132.7 projected, +5.7) 10.67
2023.06 161.7 166.8 163.4 (135.9 projected, +3.2) 8.95
2023.07  178.9 (1)   97.5 (2A) / 144.0 (2B) / 162.6 (2C) (135.4 projected, -0.5) (8.2)
2023.08       (136.4 projected, +1.0)  
2023.09       (139.8 projected, +3.4)  
2023.10       (141.6 projected, +1.8)  
2023.11       (144.2 projected max SC25, +2.6)  
2023.12       (143.4 projected, -0.1)  
2024.01       (140.1 projected, -3.3)  

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

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.