Solar Terrestrial Activity Report

Activity chart

Last major update issued on April 17, 2023 at 06:55 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 (April 1, 2023)
Solar cycle Solar cycles 23-25 (April 1, 2023) Historical solar and geomagnetic data charts 1954-2006 (April 5, 2007)
  Cycle 24-25 progress (April 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 (April 1, 2023) 3rd SSN Workshop, Tucson, 2013
  Comparison of cycles 12-14, 16, 24-25 (April 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 on April 16. Solar wind speed at SOHO ranged between 331 and 433 km/sec. The high latitude magnetometer at Andenes recorded quiet levels.

Solar flux density measured at 20h UT on 2.8 GHz was 177.8 - increasing 21.7 over the previous solar rotation. (Centered 1 year average SF at 1 AU - 183 days ago: 139.85. In comparison SC24 peaked on June 28, 2014 at 145.50). The Potsdam WDC planetary A index was 4 (STAR Ap - based on the mean of three hour interval ap indices: 4.5). Three hour interval K indices: 11211001 (planetary), 11321212 (Boulder), 21212122 (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 13 active regions using 2K resolution (SN: 381) and in 12 active regions using 1K resolution (SN: 257) SDO/HMI images.

Region 13272 [S22W51] developed slowly and quietly.
Region 13273 [N08W70] decayed slowly and quietly.
Region 13275 [N19W15] decayed slowly and quietly.
Region 13276 [S22W05] developed slowly and quietly.
Region 13279 [S20E13] decayed slowly and quietly.
Region 13280 [S07W73] decayed slowly and was mostly quiet.
Region 13281 [S23E28] decayed slowly and was mostly quiet.
Region 13282 [N11E25] decayed slowly after noon and was mostly quiet. The region has weak polarity intermixing and an M class flare is possible.
New region 13283 [S22E47] rotated into view on April 13 and continued to develop on April 16 when the region received its NOAA number.

Spotted regions not observed (or interpreted differently) by SWPC:
S8463 [N21E32] reemerged with tiny spots.
S8464 [S14W01] reemerged with tiny spots.
S8467 [N08E00] decayed slowly and quietly.
S8468 [N39E13] decayed slowly and quietly.

C2+ flares:

Magnitude Peak time (UT) Location Source Recorded by Comment
C3.4 00:44   13280 GOES16 simultaneous flares in ARs 13282 and 13281
C2.8 01:41 behind NE limb   GOES16  
C2.8 01:59   13281 GOES16  
C2.2 02:26   13281 GOES16  
C3.3 03:39   13281 GOES16  
C2.4 05:33   13280 GOES16  
C4.0 07:08   13280 GOES16  
C3.7 07:34 behind NE limb   GOES16  
C2.0 09:37   13282 GOES16 attributed to AR 13280 by SWPC
C2.5 11:14   13283 GOES16  
C2.2 12:25   13282 GOES16  
C9.0 17:44 behind NE limb   GOES16  
C3.7 19:53 S06W69 13280 GOES16  
C2.6 20:46   13280 GOES16  
C2.4 21:55   13283 GOES16  
C2.3 00:00   13280 GOES16  

Coronal mass ejections (CMEs)

April 14, 16: No obviously Earth directed CMEs were observed.
April 15: An extensive filament eruption in the northwest quadrant was observed beginning in SDO/AIA imagery at 22:47 UT. A relatively faint partial halo CME was observed early on April 16  and could reach Earth on April 19 or 20 and cause unsettled to minor storm conditions.

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 holes 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 fair. Propagation on long distance northeast-southwest paths is poor.

Forecast

Quiet conditions are likely on April 15-17.

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
13272 2023.04.05
2023.04.06
6 29 14 S22W55 0030 CRO DRI

location: S22W51

13274 2023.04.08
2023.04.10
      S07W86           location: S07W82
13278 2023.04.08
2023.04.12
      N12W85            
13273 2023.04.09
2023.04.09
1 3 2 N08W69 0010 AXX CRO

location: N08W70

13275 2023.04.09
2023.04.10
1 6 2 N19W17 0020 HAX CRO

location: N19W15

S8445 2023.04.09       N22W47            
S8447 2023.04.09       S09W58            
13276 2023.04.10
2023.04.10
5 16 9 S23W06 0020 BXI DRI location: S22W05

area: 0035

13277 2023.04.10
2023.04.11
      N10W45          
13279 2023.04.10
2023.04.12
10 48 26 S20E11 0180 DSI FSO

location: S20E13

S8455 2023.04.10       N24W33            
S8456 2023.04.10       S09W41            
S8459 2023.04.11       N09W33            
13280 2023.04.11
2023.04.13
8 20 10 S07W71 0200 CSI DKO beta-gamma

location: S07W73

area: 0330

13281 2023.04.12
2023.04.13
12 42 23 S24E32 0300 EKI EAI

location: S23E28

area: 0370

13282 2023.04.13
2023.04.13
17 48 23 N11E24 0530 EKI EKI

area: 0700

location: N11E25

S8463 2023.04.13   2 1 N21E32 0003   BXO    
S8464 2023.04.13   4 3 S14W01 0008   BXO    
13283 2023.04.13
2023.04.16
5 23 9 S22E48 0050 CRI DRI beta-gamma
S8466 2023.04.13       S19E45            
S8467 2023.04.14   5 2 N08E00 0010   BXO  
S8468 2023.04.14   5 3 N39E01 0012   CRO  
S8469 2023.04.15       S15W34          
Total spot count: 65 251 127  
Sunspot number: 155 381 257  (total spot count + 10 * number of spotted regions)
Weighted SN: 106 299 175  (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): 171 210 206  

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 (99.0 projected, +2.6) 11.16
2022.11 123.4 120.7 80.5 (102.0 projected, +3.0) 9.33
2022.12 147.9 143.4 112.8 (106.8 projected, +4.8) 10.99
2023.01 182.4 176.6 143.6 (112.9 projected, +6.1) 8.73
2023.02 167.2 163.2 110.9 (117.9 projected, +5.0) 14.48
(current
SC25 peak)
2023.03 157.2 155.6 122.6 (121.0 projected, +3.1) 14.42
2023.04 145.6 (1)   43.4 (2A) / 81.3 (2B) / 138.8 (2C) (126.4 projected, +5.4) (8.1)
2023.05       (132.1 projected, +5.7)  
2023.06       (135.2 projected, +3.1)  
2023.07       (134.7 projected, -0.5)  
2023.08       (135.7 projected, +1.0)  
2023.09       (139.2 projected, +3.5)  
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.