Solar Terrestrial Activity Report

Activity chart

Last major update issued on March 25, 2023 at 13:20 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 (March 3, 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 quiet to very severe storm on March 24 due to CME effects (before 17h) and a high speed stream from CH1136 (after 17h UT). Solar wind speed at SOHO ranged between 377 and 524 km/sec. The high latitude magnetometer at Andenes recorded quiet to severe storm levels.

Solar flux density measured at 20h UT on 2.8 GHz was 157.4 - increasing 5.0 over the previous solar rotation. (Centered 1 year average SF at 1 AU - 183 days ago: 138.30). The Potsdam WDC planetary A index was 70 (STAR Ap - based on the mean of three hour interval ap indices: 69.6). Three hour interval K indices: 78642354 (planetary), 68753342 (Boulder), 77544565 (Andenes).

The background x-ray flux is at the class B7 level (GOES 16).

At the time of counting spots (see image time), spots were observed in 19 active regions using 2K resolution (SN: 406) and in 14 active regions using 1K resolution (SN: 247) SDO/HMI images.

Region 13256 [S22W12] gained many spots in the trailing spot section and appears to be developing a magnetic delta there. M class flaring is possible. C1 flares: C1.7 @ 06:07, C1.0 @ 11:31, C1.7 @ 12:20 UT
Region 13257 [S27E04] gained small trailing spots and was quiet.
Region 13258 [N18W33] reemerged with a tiny spot. (meanwhile SWPC is including the spots of AR S8389 in AR 13258)
Region 13259 [S15E01] gained spots and still has weak polarity intermixing.
Region 13260 [N23E07] was mostly quiet and stable. C1 flares: C1.7 @ 22:07 UT
Region 13262 [S18E44] was mostly quiet and stable. C1 flares: C1.3 @ 12:14 UT
New region 13264 [N15E71] rotated into view on March 23 with SWPC numbering the region the next day.

Spotted regions not observed (or interpreted differently) by SWPC:
S8370 [N25W41] was quiet and stable.
S8377 [N27W13] reemerged with tiny spots.
S8383 [N21E22] was quiet and stable.
S8387 [N17W01] developed further and could produce C flares. C1 flares: C1.1 @ 16:50, C1.1 @ 17:32, C1.0 @ 18:27 UT
S8388 [S21E54] was quiet and stable.
S8389 [N24W29] developed further.
S8391 [S11E39] was quiet and stable.
S8392 [S28E25] was quiet and stable.
New region S8394 [N22E00] emerged to the north of AR S8387 with tiny spots.
New region S8395 [N12W42] emerged with a tiny spot.
New region S8396 [S24W23] emerged with tiny spots.
New region S8397 [N07W15] emerged with a tiny spot.

C2+ flares:

Magnitude Peak time (UT) Location Source Recorded by Comment
C2.2 13:40 S21E00 13256 GOES16  

Coronal mass ejections (CMEs)

March 22-24: 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 large southern hemisphere coronal hole (CH1136) was Earth facing on March 20-22. A trans equatorial coronal hole (CH1137) began to rotate across the central meridian on March 23 and then collapsed. A recurrent trans equatorial coronal hole (CH1138) will likely become Earth facing on March 28.

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 25-26 due to coronal hole effects. Quiet is expected for March 27-28.

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
13256 2023.03.16
2023.03.17
15 59 35 S23W18 0240 EAO FHI area: 0620

location: S22W12

S8370 2023.03.17   4   N25W41 0005   BXO  
13257 2023.03.18
2023.03.18
2 21 7 S27E01 0180 HSX CSO

area: 0310

location: S27E04

13259 2023.03.18
2023.03.19
8 32 17 S21W05 0020 CRO DRI location: S15E01

SWPC location is far off

location: 0090

13258 2023.03.18 5 1   N18W37 0020 CRO AXX  

location: N18W33

area: 0002

SWPC includes AR S8389 spots

13260 2023.03.18
2023.03.19
5 13 7 N20E04 0180 CSO DAO area: 0240

location: N23E07

S8376 2023.03.18       S43W32            
S8377 2023.03.19   4 1 N24W14 0007   BXO    
S8378 2023.03.20       N06W35            
S8380 2023.03.20       S29W36            
S8381 2023.03.20       S42W14            
S8383 2023.03.20   11 3 N21E22 0020   BXO  
S8384 2023.03.20       S11W58            
13262 2023.03.21
2023.03.22
2 6 3 S19E43 0130 HAX CSO area: 0190

location: S18E44

S8386 2023.03.21       N19W23            
S8387 2023.03.22   35 19 N17W01 0150   DAI  
S8388 2023.03.22   1 1 S21E54 0005   HRX  
S8389 2023.03.23   14 7 N24W29 0100   DAO  
13264 2023.03.23
2023.03.24
1 1 1 N16E70 0030 HSX HSX location: N15E71

area: 0110

S8391 2023.03.23   3 1 S11E39 0005   BXO  
S8392 2023.03.23   1   S28E25 0002   AXX  
S8393 2023.03.23       N39W01          
S8394 2023.03.24   5 2 N22E00 0012   BXO    
S8395 2023.03.24   1   N12W42 0003   AXX    
S8396 2023.03.24   3 3 S24W23 0008   BXO    
S8397 2023.03.24   1   N07W15 0002   AXX    
Total spot count: 38 216 107  
Sunspot number: 108 406 247  (total spot count + 10 * number of spotted regions)
Weighted SN: 69 262 153  (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): 119 223 198  

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) 14.48
(current
SC25 peak)
2023.03 159.2 (1)   83.3 (2A) / 107.6 (2B) / 136.2 (2C) (122.0 projected, +3.1) (16.0)
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.