Solar Terrestrial Activity Report

Activity chart

Last major update issued on July 6, 2022 at 10:25 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, 2022)
Solar cycle Solar cycles 23-25 (July 1, 2022) Historical solar and geomagnetic data charts 1954-2006 (April 5, 2007)
  Cycle 24-25 progress (July 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 (July 1, 2022) 3rd SSN Workshop, Tucson, 2013
  Comparison of cycles 12-14, 16, 24-25 (July 1, 2022) 4th SSN Workshop, Locarno, 2014
  Solar polar fields vs. solar cycles (April 10, 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 very quiet on July 5. Solar wind speed at SOHO ranged between 339 and 407 km/sec. The high latitude magnetometer at Andenes recorded quiet levels.

Solar flux density measured at 20h UT on 2.8 GHz was 109.4 - increasing 9.5 over the previous solar rotation. (Centered 1 year average SF at 1 AU - 183 days ago: 103.00). The Potsdam WDC planetary A index was 2 (STAR Ap - based on the mean of three hour interval ap indices: 2.4). Three hour interval K indices: 00000111 (planetary), 33122212 (Boulder), 21000111 (Andenes).

The background x-ray flux is at the class B5 level (GOES 16).

At the time of counting spots (see image time), spots were observed in 14 active regions using 2K resolution (SN: 222) and in 9 active regions using 1K resolution (SN: 126) SDO/HMI images.

Region 13046 [N17E09] was quiet and stable.
Region 13047 [S19W31] decayed slowly and produced the largest C flare of the day.
Region 13049 [S13E26] decayed slowly and quietly.
Region 13050 [N18E18] decayed slowly and was somewhat unstable producing a few small C flares. C1 flares: C1.6 @ 09:11 UT
Region 13051 [N28E16] was quiet and stable.
New region 13052 [N15E54] emerged on July 4 and was numbered by SWPC the next day. C1 flares: C1.1 @ 11:37 UT
New region 13053 [N14E72] rotated into view on July 4 and displayed several trailing spots the next day and was numbered by SWPC. C1 flares: C1.5 @ 01:17, C1.3 @ 02:13, C1.5 @ 02:35, C1.2 @ 03:05, C1.1 @ 08:06, C1.3 @ 09:02, C1.1 @ 10:09, C1.2 @ 10:57 UT

Spotted regions not observed (or interpreted differently) by SWPC:
S7678 [S15W04] was quiet and stable.
New region S7681 [S30W00] emerged before noon. While the initial spot disappeared, another one emerged.
New region S7682 [N21W13] emerged with several spots.
New region S7683 [N18W25] emerged with tiny spots.
New region S7684 [N41W20] was observed with a tiny spot in an old plage area.
New region S7685 [S13E67] rotated into view with a single, tiny spot.
New region S7686 [S18E14] was observed with tiny spots in an old plage area.

C2+ flares:

Magnitude Peak time (UT) Location Source Recorded by Comment
C5.8 03:47 N14E85 13053 GOES16  
C9.8 04:07   13047 GOES16 weak type II radio sweep
C2.4 12:05 N17E64 13052 GOES16  
C7.5/1F 12:38 N14E80 13053 GOES16  

Coronal mass ejections (CMEs)

July 3-5: No obviously Earth directed CMEs were observed in available LASCO imagery.

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 large northern hemisphere coronal hole (CH1086) was in an Earth facing position on July 2-4.

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 to fair. Propagation on long distance northeast-southwest paths is poor.

Forecast

Quiet to active conditions are likely on July 6-7 due to effects from CH1086 becoming quiet to unsettled on July 8.

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
13044 2022.06.27
2022.06.28
      S21W83           location: S19W79
13043 2022.06.27
2022.06.28
      S15W71           location: S14W67
13045 2022.06.28
2022.06.30
4     S20W33 0001 AXX     location: S10W37

spotless

SWPC has counted spots in AR 13047 twice and moved AR 13045 to the same position

S7664 2022.06.29       S27W54            
13046 2022.06.30
2022.07.01
1 4 3 N18E09 0070 HSX CSO area: 0110

location: N17E09

13047 2022.06.30
2022.07.02
6 11 4 S20W35 0010 BXO BXO  
13048 2022.07.01
2022.07.02
      S08W05            
13049 2022.07.01
2022.07.03
1 3   S12E21 0010 AXX BXO location: S13E26

area: 0007

S7670 2022.07.01       N16W47            
S7671 2022.07.01       S32W17            
13051 2022.07.02
2022.07.04
3 12 6 N28E16 0030 CRO CRO area: 0060
13050 2022.07.02
2022.07.04
  4   N18E16 0006   BXO  
S7674 2022.07.02       S23W24            
13052 2022.07.04
2022.07.05
6 18 8 N15E56 0030 CRO DRI area: 0050
S7678 2022.07.04   3 2 S15W04 0012   CRO  
13053 2022.07.04
2022.07.05
1 12 7 N14E72 0180 HSX EHO area: 0470
S7680 2022.07.04       S32E09          
S7681 2022.07.05   1 1 S30W00 0003   AXX    
S7682 2022.07.05   7 4 N21W13 0040   DRO    
S7683 2022.07.05   2 1 N18W25 0005   BXO    
S7684 2022.07.05   1   N41W20 0001   AXX    
S7685 2022.07.05   1   S13E67 0002   AXX    
S7686 2022.07.05   3   S18E14 0005   BXO  

 

Total spot count: 22 82 36  
Sunspot number: 92 222 126  (total spot count + 10 * number of spotted regions)
Weighted SN: 38 109 63  (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): 101 122 101  

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
2020.12 86.9 84.2 23.1 15.3 (+1.7) 4.72
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 31.3 (+3.7) 5.51
2021.08 77.7 79.7 22.0 35.3 (+4.0) 6.19
2021.09 87.0 88.2 51.3 40.0 (+4.7) 6.33
2021.10 88.9 88.3 37.4 45.0 (+5.0) 7.38
2021.11 86.2 84.4 34.8 50.6 (+5.6) 9.83
2021.12 103.0 99.8 67.5 55.7 (+5.1) 6.40
2022.01 103.8 100.5 54.0 (59.5 projected, +3.8) 8.92
2022.02 109.1 106.5 59.7 (65.1 projected, +5.6) 10.46
2022.03 117.0 115.8 78.5 (70.5 projected, +5.4) 10.20
2022.04 130.8 131.7 84.1 (75.7 projected, +5.2) 11.79
2022.05 133.8 136.8 96.5 (82.2 projected, +6.5) 7.48
2022.06 116.1 119.8 70.6 (88.1 projected, +5.9) 8.4
2022.07 102.8 (1)   10.0 (2A) / 61.8 (2B) / 99.1 (2C) (95.3 projected, +7.2) (9.9)
2022.08       (101.9 projected, +6.6)  
2022.09       (106.9 projected, +5.0)  
2022.10       (110.1 projected, +3.2)  
2022.11       (112.9 projected, +2.8)  
2022.12       (117.7 projected, +4.8)  
2023.11       (141.4 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.