Solar Terrestrial Activity Report

Activity chart

Last major update issued on May 15, 2023 at 05:50 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, 2023)
Solar cycle Solar cycles 23-25 (May 1, 2023) Historical solar and geomagnetic data charts 1954-2006 (April 5, 2007)
  Cycle 24-25 progress (May 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 (May 1, 2023) 3rd SSN Workshop, Tucson, 2013
  Comparison of cycles 12-14, 16, 24-25 (May 1, 2023) 4th SSN Workshop, Locarno, 2014
  Solar polar fields vs. solar cycles (April 5, 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 unsettled on May 14 under the influence of weak effects from CH1146/CH1147. Solar wind speed at SOHO ranged between 399 and 532 km/sec. The high latitude magnetometer at Andenes recorded quiet to active levels.

Solar flux density measured at 20h UT on 2.8 GHz was 139.7 - decreasing 26.9 over the previous solar rotation. (Centered 1 year average SF at 1 AU - 183 days ago: 141.06. In comparison SC24 peaked on June 28, 2014 at 145.50). The Potsdam WDC planetary A index was 7 (STAR Ap - based on the mean of three hour interval ap indices: 7.3). Three hour interval K indices: 12112332 (planetary), 12112432 (Boulder), 22113443 (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 15 active regions using 2K resolution (SN: 280) and in 13 active regions using 1K resolution (SN: 197) SDO/HMI images.

Region 13297 [N09W84] decayed slowly and was mostly quiet.
Region 13301 [N13E03] decayed slowly and quietly.
Region 13302 [N18E09] was quiet and stable.
Region 13303 [S12W09] decayed slowly and quietly.
Region 13304 [N21W20] decayed slowly and quietly.
Region 13305 [N09E11] developed initially, then decayed slowly.
New region 13306 [S19W34] first emerged on May 10, then decayed. New flux emerged on May 13 and the region developed further as it was numbered by SWPC. The region has minor polarity intermixing. C1 flares: C1.2 @ 19:45, C1.6 @ 21:11 UT

Spotted regions not observed (or interpreted differently) by SWPC:
S8549 [S22W03] was quiet and stable.
S8556 [N13W33] decayed slowly and quietly.
New region S8559 [N27W24] emerged with tiny spots.
New region S8560 [S28E29] emerged with tiny spots.
New region S8561 [N11E27] emerged early in the day, then decayed slowly.
New region S8563 [S09E48] emerged with a few spots.
New region S8564 [S22W20] emerged with tiny spots.
New region S8565 [S22E35] emerged with tiny spots.

AR 13296 produced a C1.4 flare at 11:50 and a C1.1 flare at 15:09 UT from behind the northwest limb.
A C1.8 flare, likely from a source near the southeast limb, was recorded at 21:21 UT.
Other C1 flares noted (awaiting source confirmation if SDO/AIA images become available): C1.1 @ 01:52, C1.4 @ 02:54, C1.6 @ 06:39 UT

C2+ flares:

Magnitude Peak time (UT) Location Source Recorded by Comment
C3.5 04:06     GOES16  
C2.9 04:30     GOES16  
C3.6 04:44 N08E28 13305 GOES16  
C2.2 05:33     GOES16  
C7.0 09:17   13296 GOES16  
C2.2 22:35   13306 GOES16  
C2.3 22:51   13306 GOES16  

Coronal mass ejections (CMEs)

May 12-14: No obviously Earth directed CMEs were observed.

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]

An elongated northern hemisphere coronal hole (CH1146) was Earth facing on May 8-11. A southern hemisphere coronal hole (CH1147) rotated across the central meridian on May 11. A recurrent trans equatorial coronal hole (CH1148) will likely become Earth facing on May 16-17.

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.

Forecast

Mostly quiet geomagnetic conditions are expected on May 15-18. On May 19-20 effects from CH1148 could cause quiet to minor storm conditions.

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
13294 2023.05.01
2023.05.02
1     S07W87 0010 AXX     rotated out of view
13297 2023.05.02
2023.05.02
2 2 1 N09W83 0040 CAO HSX

location: N09W84

area: 0180

13299 2023.05.03
2023.05.04
      S08W67          

location: S07W65

S8529 2023.05.04       S26W48            
13300 2023.05.06
2023.05.09
      N09W67        

 

13303 2023.05.07
2023.05.09
  8 1 S10W13 0010   AXX location: S12W09
13301 2023.05.08
2023.05.09
4 8 6 N14W00 0120 HAX HAX

location: N13E03

S8543 2023.05.08       N25W47            
13304 2023.05.08
2023.05.11
8 13 7 N22W19 0030 CRO DRO location: N21W20
13302 2023.05.08
2023.05.09
5 17 7 N19E05 0070 CSO DSO area: 0130

location: N18E09

S8549 2023.05.09   11 3 S22W03 0020   BXO  
S8551 2023.05.10       N13W19          
13306 2023.05.10
2023.05.14
5 17 9 S18W36 0040 CAO DRI location: S19W34

area: 0060

S8553 2023.05.10       N26W36            
13305 2023.05.12 14 37 24 N10E11 0070 DAI DAI

location: N09E11

area: 0200

S8555 2023.05.12       S23W19            
S8556 2023.05.12   1   N13W33 0001   AXX  
S8557 2023.05.13       N25W23          
S8558 2023.05.13       S37E32          
S8559 2023.05.14   4 3 N27W24 0015   BXO    
S8560 2023.05.14   3   S28E24 0007   BXO    
S8561 2023.05.14   1 1 N11E29 0003   AXX    
S8563 2023.05.14   4 3 S09E48 0020   CRO    
S8564 2023.05.14   2 1 S22W20 0005   BXO    
S8565 2023.05.14   2 1 S22E35 0006   BXO    
Total spot count: 39 130 67  
Sunspot number: 109 280 197  (total spot count + 10 * number of spotted regions)
Weighted SN: 67 159 96  (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): 120 154 158  

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
2021.09 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 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 (100.4 projected, +1.7) 9.33
2022.12 147.9 143.4 112.8 (104.1 projected, +3.7) 10.99
2023.01 182.4 176.6 143.6 (110.1 projected, +6.0) 8.73
2023.02 167.2 163.2 110.9 (115.2 projected, +5.1) 14.48
(current
SC25 peak)
2023.03 157.2 155.6 122.6 (118.3 projected, +3.1) 14.42
2023.04 145.4 146.4 96.4 (123.7 projected, +5.4) 13.40
2023.05 157.5 (1)   55.2 (2A) / 122.3 (2B) / 153.7 (2C) (129.3 projected, +5.6) (11.9)
2023.06       (132.5 projected, +3.2)  
2023.07       (132.0 projected, -0.5)  
2023.08       (133.0 projected, +1.0)  
2023.09       (136.4 projected, +3.4)  
2023.10       (138.3 projected, +1.9)  
2023.11       (141.4 projected, +3.1)  
2023.12       (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.