Solar Terrestrial Activity Report

Activity chart

Last major update issued on March 1, 2023 at 07:15 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 (February 4, 2023)
Solar cycle Solar cycles 23-25 (March 1, 2023) Historical solar and geomagnetic data charts 1954-2006 (April 5, 2007)
  Cycle 24-25 progress (March 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 (March 1, 2023) 3rd SSN Workshop, Tucson, 2013
  Comparison of cycles 12-14, 16, 24-25 (March 1, 2023) 4th SSN Workshop, Locarno, 2014
  Solar polar fields vs. solar cycles (January 21, 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 at quiet to major storm levels on February 28 due to CME effects. Solar wind speed at SOHO ranged between 561 and 826 km/sec. The high latitude magnetometer at Andenes recorded quiet to major storm levels.

Solar flux density measured at 20h UT on 2.8 GHz was 160.9 - increasing 27.4 over the previous solar rotation. (Centered 1 year average SF at 1 AU - 183 days ago: 135.17). The Potsdam WDC planetary A index was 27 (STAR Ap - based on the mean of three hour interval ap indices: 26.6). Three hour interval K indices: 65332144 (planetary), ******** (Boulder), 56332256 (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: 214) and in 8 active regions using 1K resolution (SN: 125) SDO/HMI images.

Region 13230 [S22W58] decayed slowly and was mostly quiet.
Region 13234 [N23W38] is still a complex region with multiple magnetic deltas. Some decay was observed in the easternmost spot section. Another major flare is possible.
Region 13236 [S27W44] decayed further and was quiet.
Region 13238 [N09E51] was quiet and stable.
New region 13239 [N32E69] rotated into view on February 27 and was numbered the next day by SWPC. C1 flare: C1.6 @ 12:05 UT

Spotted regions not observed (or interpreted differently) by SWPC:
S8310 [S26E05] was quiet and stable.
S8311 [S20E21] was quiet and stable.
S8316 [N19W05] was quiet and stable.
New region S8319 [N28E85] rotated partly into view and might be capable of M class flaring.
New region S8320 [S15E67] emerged with a tiny spot. This region has produced several flares early on March 1.
New region S8321 [N41E29] emerged with a tiny spot at a high latitude location.

C2+ flares:

Magnitude Peak time (UT) Location Source Recorded by Comment
C2.2 00:25   13230 GOES16  
C2.4 04:12   13230 GOES16  
C2.4 05:06   S8319 GOES18  
C2.4 05:33   13234 GOES16  
C2.5 06:28   13234 GOES16  
C3.3 06:59   13234 GOES18  
C2.0 08:44   13234 GOES16  
C2.0 14:16   13234 GOES16  
C2.1 14:40   13235 GOES16  
C5.8 16:22 N26W31 13234 GOES16  
M8.6 17:50   13234 GOES16  
C2.4 20:55   13234 GOES16  
C4.3 22:34   13234 GOES16  
C2.8 23:35   13234 GOES16  

Coronal mass ejections (CMEs)

February 26-28: 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]

A recurrent trans equatorial coronal hole (CH1132) was Earth facing on February 24-25. Due to the strong solar storms overtaking the associated high speed stream, it will not be possible to observe any disturbance during this solar rotation.
A trans equatorial coronal hole (CH1133) will likely rotate across the central meridian on March 1-2.

Propagation

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

Forecast

Quiet to active conditions are likely on March 1 due to lingering CME effects. March 2-3 could see quiet to unsettled conditions. Effects from CH1133 could cause unsettled to minor storm conditions on March 4-5.

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
13229 2023.02.16
2023.02.16
      N26W88          
13230 2023.02.17
2023.02.18
2 7 2 S23W58 0010 AXX BXO location: S22W58
13234 2023.02.20
2023.02.20
25 51 26 N25W36 0860 FKC EKC beta-gamma-delta

location: N23W38

S8301 2023.02.21       S12W41            
13235 2023.02.22
2023.02.23
      N19W59          
13236 2023.02.23
2023.02.23
9 22 9 S27W44 0080 CSO CRO area: 0060
13237 2023.02.23
2023.02.24
2     S08W25 0000 AXX    

real location: S13W30

SWPC observers were confused by the spots of AR S8315 on February 27 and changed the location to that group

S8306 2023.02.23       N12W17            
S8307 2023.02.24       N13W47            
S8308 2023.02.24       S22W19          
S8309 2023.02.25       N13W15            
S8310 2023.02.25   3   S26E05 0004   BXO  
S8311 2023.02.25   9 2 S20E21 0020   BXO  
S8313 2023.02.25       N18W04            
13238 2023.02.26
2023.02.27
1 5 3 N09E50 0070 HSX CSO location: N09E51

area: 0150

S8315 2023.02.26       S08W25          
S8316 2023.02.27   2   N18W05 0003   BXO  
13239 2023.02.27
2023.02.28
1 2 1 N30E69 0090 HSX HSX location: N32E69

area: 0160

S8318 2023.02.27       S29E23          
S8319 2023.02.28   1 1 N28E85 0100   HSX    
S8320 2023.02.28   1 1 S15E67 0005   AXX    
S8321 2023.02.28   1   N41E29 0002   AXX    
Total spot count: 40 104 45  
Sunspot number: 100 214 125  (total spot count + 10 * number of spotted regions)
Weighted SN: 65 132 73  (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): 110 118 100  

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
2021.08 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 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 77.2 (+4.2) 7.48
2022.06 116.1 119.8 70.3 80.9 (+3.7) 8.20
2022.07 125.4 129.5 91.4 86.5 (+5.6) 9.51
2022.08 114.2 117.1 74.6 92.3 (+5.8) 10.92
2022.09 135.1 136.5 96.0 (97.0 projected, +4.7) 12.18
2022.10 133.5 132.7 95.4 (100.2 projected, +3.2) 11.16
2022.11 123.4 120.7 77.6 (103.0 projected, +2.8) 9.33
2022.12 147.9 143.4 113.1 (107.8 projected, +4.8) 10.99
2023.01 182.4 176.6 143.6 (113.8 projected, +6.0) 8.73
2023.02 167.2 163.2 110.9 (118.9 projected, +5.1) 14.6
2023.03 (1)   (2A/2B) / 150.0 (2C) (122.0 projected, +3.1) ()
2023.04       (127.4 projected, +5.4)  
2023.05       (133.2 projected, +5.8)  
2023.06       (136.4 projected, +3.2)  
2023.07       (135.9 projected, -0.5)  
2023.08       (136.9 projected, +1.0)  
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.