Solar Terrestrial Activity Report

Activity chart

Last major update issued on March 28, 2023 at 07:40 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 (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 very quiet on March 27. Solar wind speed at SOHO ranged between 358 and 549 km/sec. The high latitude magnetometer at Andenes recorded quiet to unsettled levels.

Solar flux density measured at 20h UT on 2.8 GHz was 158.2 - decreasing 2.7 over the previous solar rotation. (Centered 1 year average SF at 1 AU - 183 days ago: 138.62). 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: 00000011 (planetary), 10001221 (Boulder), 10000013 (Andenes).

The background x-ray flux is at the class C1 level (GOES 16).

At the time of counting spots (see image time), spots were observed in 17 active regions using 2K resolution (SN: 325) and in 15 active regions using 1K resolution (SN: 218) SDO/HMI images.

Region 13256 [S21W50] developed as new flux emerged in the trailing spot section. A split into 2 regions is being considered. C1 flares: C1.6 @ 00:03, C1.2 @ 02:42, C1.3 @ 05:21, C1.9 @ 05:43, C1.6 @ 08:10, C1.6 @ 09:39, C1.4 @ 16:12 UT
Region 13257 [S27W33] decayed slowly and quietly.
Region 13259 [S16W38] decayed slowly and quietly.
Region 13260 [N23W32] was quiet and stable.
Region 13262 [S18E06] was mostly quiet and stable. C1 flares: C1.4 @ 01:42 UT
Region 13263 [N18W41] decayed slowly and was mostly quiet.
Region 13264 [N15E33] decayed slowly and quietly.
Region 13265 [N20W15] was quiet and stable.

Spotted regions not observed (or interpreted differently) by SWPC:
S8389 [N24W70] decayed slowly and was quiet.
S8392 [S23W11] was quiet and stable.
S8398 [N23E10] was quiet and stable.
S8399 [N15W12] decayed slowly and quietly.
S8400 [N09E69] was quiet and stable.
New region S8402 [S26W78] emerged before noon and was quiet.
New region S8405 [S06E03] emerged with tiny spots.
New region S8406 [S17E73] rotated into view with tiny spots.
New region S8407 [S19E24] was observed with tiny spots in an old plage area.

C2+ flares:

Magnitude Peak time (UT) Location Source Recorded by Comment
C4.6 06:36 S22W33 13256 GOES16  
C2.6 07:37 S20W37 13256 GOES16  
C2.7 10:55 S21W36 13256 GOES16  
C2.9 19:05 N24W69 S8389 GOES16  
C3.5/1N 20:39 S21W44 13256 GOES16  
C3.6 20:46   13256 GOES16  
C3.0 21:09 southwest limb S8401 GOES16 attributed to AR 13256 by SWPC

Coronal mass ejections (CMEs)

March 25-27: 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 (CH1138) will be Earth facing on March 27-28.

Propagation

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

Forecast

Quiet conditions are expected for March 28-29. Quiet to minor storm is likely on March 30-31 due to effects from CH1138.

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
11 26 16 S21W59 0250 EHO FHI beta-gamma

area: 0450

location: S21W50

13257 2023.03.18
2023.03.18
3 11 5 S28W34 0050 HAX CAO

location: S27W33

area: 0100

13259 2023.03.18
2023.03.19
1 7 3 S17W32 0010 AXX BXO location: S16W38
13258 2023.03.18 1     N24W69 0020 HSX      

spotless

location: N18W72

SWPC counts the spots of AR S8389

13260 2023.03.18
2023.03.19
2 9 2 N22W32 0070 HAX CAO area: 0200

location: N23W32

S8377 2023.03.19       N24W53            
13265 2023.03.20
2023.03.26
7 16 10 N20W15 0090 DAO DAO area: 0130
13262 2023.03.21
2023.03.22
3 7 2 S20E06 0060 HSX CSO area: 0170

location: S18E06

13263 2023.03.22
2023.03.24
9 33 18 N18W40 0090 DAI DRI area: 0130

location: N18W41

S8388 2023.03.22       S21E19            
S8389 2023.03.23   3 1 N24W70 0080   CAO  
13264 2023.03.23
2023.03.24
1 7 1 N15E32 0010 HSX CSO location: N15E33

area: 0100

S8391 2023.03.23       S12E02            
S8392 2023.03.23   8   S23W11 0012   BXO  
S8393 2023.03.23       N39W40            
S8397 2023.03.24       N07W54            
S8398 2023.03.25   8 3 N23E10 0015   BXO  
S8399 2023.03.26   5 2 N15W12 0010   BXO  
S8400 2023.03.26   4 1 N09E69 0010   BXO  
S8402 2023.03.27   3 2 S26W78 0007   BXO    
S8405 2023.03.27   2   S06W03 0004   BXO    
S8406 2023.03.27   2 1 S17E73 0010   BXO    
S8407 2023.03.27   4 1 S19E24 0010   BXO    
Total spot count: 38 155 68  
Sunspot number: 128 325 218  (total spot count + 10 * number of spotted regions)
Weighted SN: 83 198 111  (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): 141 179 174  

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)   96.0 (2A) / 110.2 (2B) / 137.1 (2C) (122.0 projected, +3.1) (14.9)
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.