Solar Terrestrial Activity Report

Activity chart

Last major update issued on May 6, 2022 at 11:40 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 (May 1, 2022)
Solar cycle Solar cycles 23-25 (May 1, 2022) Historical solar and geomagnetic data charts 1954-2006 (April 5, 2007)
  Cycle 24-25 progress (May 1, 2022) Noon SDO sunspot count 1K image / 4K (*)
  Solar cycles 1-24 (June 1, 2020) POES auroral activity level October 2009 - December 2012]
  Comparison of cycles 21-25 (May 1, 2022) 3rd SSN Workshop, Tucson, 2013
  Comparison of cycles 12-14, 16, 24-25 (May 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 May 5. The high latitude magnetometer at Andenes recorded quiet to active levels.

Solar flux density measured at 20h UT on 2.8 GHz was 119.9 - increasing 11.0 over the previous solar rotation. (Centered 1 year average SF at 1 AU - 183 days ago: 95.30). 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: 11100111 (planetary), 11111211 (Boulder), 42212122 (Andenes).

The background x-ray flux is at the class B8 level (GOES 16).

At the time of counting spots (see image time), spots were observed in 11 active regions using 2K resolution (SN: 198) and in 6 active regions using 1K resolution (SN: 106) SDO/HMI images.

Region 12998 [S20W79] was quiet and stable. Note that SWPC assigned a new number (12999) to the region due to the faulty initial location of AR 12998. For data consistency the original number is used in this report.
Region 13001 [S31W39] was quiet and stable.
Region 13004 [S14W30] developed further in the leading penumbra, however, some decay was observed in the trailing spot section. There is still an elongated magnetic delta in the southeastern part of the largest penumbra, positive polarity umbrae and penumbra are sandwiched between negative polarity areas. A major flare is possible. C1 flares: C1.7 @ 00:15, C1.9 @ 06:46, C1.7 @ 10:00, C1.8 @ 13:04, C1.4 @ 16:12, C1.4 @ 18:04, C1.7 @ 19:09, C1.7 @ 23:37 UT
Region 13006 [S30E56] developed slowly and became less active. The main penumbra contains opposite polarity umbrae and this delta is likely the cause of most flares from this region. Another major flare is possible. C1 flares: C1.8 @ 07:46, C1.3 @ 18:32 UT

Spotted regions not observed (or interpreted differently) by SWPC:
S7518 [S09W61] reemerged with a tiny spot.
S7542
[S15W18] was quiet and stable.
New region S7545 [S21W07] emerged with a tiny spot.
New region S7546 [S25E18] was observed with tiny spots.
New region S7547 [S19W62] emerged with a tiny spot.
New region S7548 [S18E33] emerged with a tiny spot.
New region S7549 [N25E01] emerged with tiny spots.

C2+ flares:

Magnitude Peak time (UT) Location Source Recorded by Comment
C4.0 01:38 S16W17 13004 GOES16  
C3.8 03:03   13004 GOES16  
C2.9 03:22 S18W19 13004 GOES16  
C2.9 04:24   13004 GOES16  
C5.7 04:49   13004 GOES16 weak type IV radio sweep
C2.1 06:21   13004 GOES16  
C3.8 07:20   13004 GOES16  
C2.6 08:35   13004 GOES16  
C4.1 09:03   13004 GOES16  
C6.5 11:19   13006 GOES16  
C8.7 11:55   13004 GOES16  
M2.2 13:16   13004 GOES16  
C6.8 13:37   13004 GOES16  
M2.7 14:10   13006 GOES16  
C3.4 15:39   13004 GOES16  
C2.4 22:20   13004 GOES16  
C2.6 23:03 S16W27 13004 GOES16  
C3.9 23:59 S16W29 13004 GOES16  

Coronal mass ejections (CMEs)

May 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]

No obvious coronal holes are currently in or near Earth facing locations.

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

Forecast

Quiet conditions are likely on May 5-7.

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
12998 2022.04.23
2022.04.23
  1 1   0110   HSX

location: S20W79

12999 2022.04.25 1     S21W80 0070 HSX       SWPC renumber of AR 12998
S7518 2022.04.25   1   S09W61 0003   AXX    
13000 2022.04.25
2022.04.26
      S17W51           location: S18W46
13001 2022.04.25
2022.04.26
1 5 2 S32W40 0090 HSX CSO location: S31W39

area: 0120

13002 2022.04.26
2022.04.28
      N13W73            
S7525 2022.04.26       N31W38            
S7526 2022.04.26       S17W57            
13004 2022.04.27
2022.05.02
26 56 32 S16W29 0500 DKC DKC beta-gamma-delta

area: 0650

location: S14W30

13003 2022.04.28
2022.04.29
3     S24W27 0010 BXO      

 

S7534 2022.04.30       N18W50            
13005 2022.05.01
2022.05.02
      N20W36          
S7537 2022.05.02       S17W08            
S7538 2022.05.02       S19E02            
13006 2022.05.02
2022.05.04
4 24 9 S27E50 0050 CAO EAO beta-gamma-delta

location: S30E56

S7540 2022.05.02       S13E43            
S7541 2022.05.04       S23W25         wrongly numbered, this is AR 13003
S7542 2022.05.04   3 1 S15W18 0010   CRO  
S7543 2022.05.04       N32W22          
S7544 2022.05.04       S30W52          
S7545 2022.05.05   1 1 S21W07 0004   AXX    
S7546 2022.05.05   3   S25E18 0006   AXX    
S7547 2022.05.05   1   S19W62 0001   AXX    
S7548 2022.05.05   1   S18E33 0001   AXX    
S7549 2022.05.05   2   N25E01 0002   BXO    
Total spot count: 35 98 46  
Sunspot number: 85 208 106  (total spot count + 10 * number of spotted regions)
Weighted SN: 60 126 74  (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): 94 112 85  

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
 

2020.10

74.6 74.2 14.6 11.9 (+1.4) 6.13
2020.11 89.9 88.0 34.5 13.6 (+1.7) 4.77
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 (50.0 projected, +5.0) 9.83
2021.12 103.0 99.8 67.5 (55.8 projected, +5.8) 6.40
2022.01 103.8 100.5 54.0 (60.3 projected, +4.5) 8.92
2022.02 109.1 106.5 59.7 (65.2 projected, +4.9) 10.46
2022.03 117.0 115.8 78.5 (70.7 projected, +5.5) 10.20
2022.04 130.8 131.7 84.1 (75.9 projected, +5.2) 12.0
2022.05 117.1 (1)   9.9 (2A) / 61.4 (2B) / 88.7 (2C) (82.3 projected, +6.4) (5.4)
2022.06       (88.2 projected, +5.9)  
2022.07       (95.4 projected, +7.2)  
2022.08       (102.1 projected, +6.7)  
2022.09       (107.1 projected, +5.0)  
2022.10       (110.3 projected, +3.2)  

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.