Solar Terrestrial Activity Report

Activity chart

Last major update issued on March 9, 2023 at 04:45 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 unsettled on March 8. Solar wind speed at SOHO ranged between 376 and 460 km/sec. The high latitude magnetometer at Andenes recorded quiet to minor storm levels.

Solar flux density measured at 20h UT on 2.8 GHz was 181.9 - decreasing 32.7 over the previous solar rotation. (Centered 1 year average SF at 1 AU - 183 days ago: 136.56). The Potsdam WDC planetary A index was 7 (STAR Ap - based on the mean of three hour interval ap indices: 7.4). Three hour interval K indices: 12221133 (planetary), 12222332 (Boulder), 12321355 (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 16 active regions using 2K resolution (SN: 330) and in 14 active regions using 1K resolution (SN: 236) SDO/HMI images.

Region 13238 [N08W55] decayed slowly and quietly.
Region 13239 [N33W33] was quiet and stable.
Region 13240 [S22W25] decayed slowly and quietly.
Region 13241 [N28W19] was quiet and stable.
Region 13242 [N10W17] lost the magnetic delta. Minor polarity intermixing still exists and another M class flare is possible.
Region 13244 [S22W82] decayed slowly and was mostly quiet. C1 flares: C1.9 @ 01:15, C1.8 @ 02:47, C1.5 @ 05:46 UT
Region 13245 [S22E10] gained spots and area. M class flaring is likely. C1 flares: C1.7 @ 02:08, C1.4 @ 06:59, C1.7 @ 08:58 UT
Region 13246 [N24E27] decayed slowly and quietly.
Region 13247 [S22E43] developed slowly and was mostly quiet. The easternmost spots may be another group. C1 flare: C1.7 @ 23:26 UT
Region 13248 [N15W73] was mostly quiet and stable. C1 flares: C1.7 @ 05:25 UT
Region 13249 [S12E63] was quiet and stable.

Spotted regions not observed (or interpreted differently) by SWPC:
S8341 [S04W22] was quiet and stable.
New region S8347 [N12W56] emerged before noon to the north of AR 13238.
New region S8348 [N22E70] rotated into view with small spots. C1 flares: C1.7 @ 12:25 UT
New region S8349 [S13E82] rotated into view with a mature spot.
New region S8350 [N13E23] emerged with tiny spots.

C2+ flares:

Magnitude Peak time (UT) Location Source Recorded by Comment
C2.1 09:09   13245 GOES16  
M1.1 10:12   13242 GOES16 LDE
C3.3 13:41   13242 GOES16  
C2.0 16:35   S8348 GOES16  
C3.7 19:44   13242 GOES16 incorrectly attributed to AR 13245 by SWPC
M1.3/1N 22:44 S24E14 13245 GOES16  

Coronal mass ejections (CMEs)

March 7-9: No obviously Earth directed CMEs were observed.
March 6: A faint full halo CME was observed after the major M5.8 flare in AR 13243 early in the day. While the main ejecta will not reach Earth, there is a chance of weak effects reaching Earth before noon on March 9.

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 hole are currently in or near Earth facing positions.

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

Quiet to unsettled conditions are likely on March 9-11 with a chance of active intervals should a component of the February 6 CME reach Earth.

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
13244 2023.02.25
2023.03.03
3 2 2 S22W88 0030 CRO HRX

location: S22W82

13238 2023.02.26
2023.02.27
1 2 2 N09W58 0030 CRO AXX location: N08W55

SWPC mismatch spot count and classification

13239 2023.02.27
2023.02.28
1 1 1 N33W37 0140 HSX HSX location: N33W33
13241 2023.02.28
2023.03.01
1 11 6 N29W22 0070 HSX CSO

location: N28W19

13240 2023.02.28
2023.03.01
  9   S09W49 0015   BXO

location: S22W25

SWPC on March 6 moved the location to near AR S8327

13242 2023.03.01
2023.03.02
18 57 32 N10W15 0245 ESI ESI beta-gamma

location: N10W17

S8326 2023.03.02       S20W54            
S8327 2023.03.02       S09W51          
13245 2023.03.02
2023.03.03
11 40 31 S23E07 0440 DHI DKC

beta-gamma

area: 0500

location: S22E10

S8330 2023.03.03       S17W01            
S8331 2023.03.03       S30W37            
S8333 2023.03.04       N28W59            
13246 2023.03.04
2023.03.05
1 5 2 N23E28 0050 HAX CSO location: N24E27

area: 0090

S8335 2023.03.04       N22W15            
S8336 2023.03.04       S08W07            
13247 2023.03.05
2023.03.06
3 22 9 S24E41 0100 CAO DSI location: S22E43
13248 2023.03.05
2023.03.06
6 9 5 N15W72 0030 CRO DRO location: N15W73
S8340 2023.03.05       N28W44            
S8341 2023.03.05   1 1 S04W22 0003   AXX  
S8343 2023.03.06       S12E09            
13249 2023.03.07
2023.03.07
1 1 1 S12E61 0150 HSX HSX location: S12E63
S8346 2023.03.07       N26E45          
S8347 2023.03.08   4 1 N12W56 0012   CRO    
S8348 2023.03.08   3 2 N22E70 0020   BXO    
S8349 2023.03.08   1 1 S13E82 0100   HSX    
S8350 2023.03.08   2   N13E23 0002   BXO    
Total spot count: 46 170 96  
Sunspot number: 146 330 236  (total spot count + 10 * number of spotted regions)
Weighted SN: 95 224 150  (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): 161 182 190  

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
2023.03 177.3 (1)   35.3 (2A) / 136.9 (2B) / 159.7 (2C) (122.0 projected, +3.1) (13.5)
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.