Solar Terrestrial Activity Report

Activity chart

Last major update issued on February 18, 2023 at 06:00 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 (February 1, 2023) Historical solar and geomagnetic data charts 1954-2006 (April 5, 2007)
  Cycle 24-25 progress (February 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 (February 1, 2023) 3rd SSN Workshop, Tucson, 2013
  Comparison of cycles 12-14, 16, 24-25 (February 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 February 17. Solar wind speed at SOHO ranged between 401 and 590 km/sec. The high latitude magnetometer at Andenes recorded quiet to unsettled levels.

Solar flux density measured at 18h UT on 2.8 GHz was 165.1 - decreasing 43.6 over the previous solar rotation. Solar flux at 20h UT was strongly flare enhanced and therefore replaced by the only measurement of the day not affected by the X2 flare. (Centered 1 year average SF at 1 AU - 183 days ago: 133.29). The Potsdam WDC planetary A index was 6 (STAR Ap - based on the mean of three hour interval ap indices: 6.0). Three hour interval K indices: 23211110 (planetary), ******** (Boulder), 23211020 (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 14 active regions using 2K resolution (SN: 235) and in 13 active regions using 1K resolution (SN: 180) SDO/HMI images.

Region 13216 [N23W71] was quiet and stable.
Region 13217 [S12W44] was quiet and stable.
Region 13219 [S08W50] decayed slowly and quietly.
Region 13220 [S13W27] was quiet and stable.
Region 13221 [N13W30] reemerged with tiny spots.
Region 13224 [N21W29] was quiet and stable.
Region 13225 [S21W56] developed as new flux emerged.
Region 13226 [N10W20] decayed slowly in the trailing spot section and was mostly quiet. An M class flare is possible.
Region 13229 [N26E60] was mostly unchanged and produced several C flares and a major X2 flare. Further major flares are possible. C1 flares: C1.3 @ 04:25, C1.9 @ 07:33 UT

Spotted regions not observed (or interpreted differently) by SWPC:
S8279 [N21W11] was quiet and stable.
S8283 [N12W01] was quiet and stable.
New region S8286 [S10E57] emerged with tiny spots.
New region S8287 [S23E82] rotated into view with a mature spot.
New region S8288 [N20E18] emerged with tiny spots.

C2+ flares:

Magnitude Peak time (UT) Location Source Recorded by Comment
C3.8 01:35   13229 GOES16  
C2.2 09:38 N25E69 13229 GOES16  
C2.1 10:33     GOES16  
C2.0 10:50   13229 GOES16  
C2.0 11:48 N08W08 13226 GOES16  
C2.0 12:48   13229 GOES16  
X2.2/2B 20:16 N25E64 13229 GOES16 LDE. Fast full halo CME. Strong type II radio sweep

Coronal mass ejections (CMEs)

February 15: A filament eruption occurred between ARs 13220 and 13226 starting at 01:07 UT in SDO/AIA imagery. A partial halo CME was observed afterwards. This CME could reach Earth between noon on February 17 and noon on February 18.
February 16: A partial halo CME was observed after the C9 flare in AR13216. A glancing blow is possible on February 19-20.
February 17: The X2.2/2B flare in AR 13229 at 20:16 UT was associated with a very fast and wide full halo CME. The CME could impact Earth on February 19 and cause active to severe 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]

A northern hemisphere coronal hole (CH1130) was Earth facing on February 14. A southern hemisphere coronal hole (CH1131) rotated the central meridian on February 17.

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 minor storm conditions are likely on February 18 due to CME effects. Quiet to severe storm is expected on February 19-20 due to the February 17 CME.

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
13216 2023.02.05
2023.02.06
1 1 1 N23W72 0110 HSX HSX  
13218 2023.02.07
2023.02.08
      N11W66          

location: N14W60

13217 2023.02.07
2023.02.08
3 1 1 S11W47 0150 CSO HHX

location: S12W44

area: 0300

13219 2023.02.08
2023.02.09
  4 1 S06W55 0010   CRO location: S08W50
S8259 2023.02.08       N18W44            
13220 2023.02.09
2023.02.09
1 7 4 S14W29 0140 HSX CSO area: 0240

location: S13W27

13221 2023.02.09
2023.02.09
  4   N19W33 0005   BXO  

location: N13W30

S8264 2023.02.09       S13W34            
13223 2023.02.10
2023.02.11
      N17W55         location: N13W48
13224 2023.02.11
2023.02.11
  7 1 N22W34 0010   BXO

location: N21W29

13225 2023.02.11
2023.02.12
3 13 6 S21W59 0070 DAO DAO

location: S21W56

13228 2023.02.11
2023.02.13
      S24W42            
S8273 2023.02.11       N27W19            
S8274 2023.02.11       N22W11            
13226 2023.02.12
2023.02.13
12 38 23 N10W19 0390 EHI EKO

area: 0470

13227 2023.02.12
2023.02.13
      S03W15         location: S03W12
S8279 2023.02.13   9 2 N21W11 0015   BXO  
S8280 2023.02.15       S35W04            
S8281 2023.02.15       S11W09            
S8283 2023.02.15   4 1 N12W01 0008   BXO  
13229 2023.02.16
2023.02.16
6 12 7 N25E58 0400 DKO DKO location: N26E60
S8286 2023.02.17   2 1 S10E57 0008   CRO    
S8287 2023.02.17   1 1 S23E82 0190   HSX    
S8288 2023.02.17   2 1 N20E18 0008   BXO    
Total spot count: 26 105 50  
Sunspot number: 86 245 180  (total spot count + 10 * number of spotted regions)
Weighted SN: 66 161 106  (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): 95 135 144  

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 (solar max) 7.88
2017.09 91.3 92.3 43.6 18.2 (-1.3) 18.22
(cycle 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
2021.07 81.0 83.6 34.3 31.4 (+3.8) 5.51
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 (92.4 projected, +5.9) 10.92
2022.09 135.1 136.5 96.0 (97.4 projected, +5.0) 12.18
2022.10 133.5 132.7 95.4 (100.5 projected, +3.1) 11.16
2022.11 123.4 120.7 77.6 (103.4 projected, +2.9) 9.33
2022.12 147.9 143.4 113.1 (108.2 projected, +4.8) 10.99
2023.01 182.4 176.6 143.6 (114.2 projected, +6.0) 8.73
2023.02 172.2 (1)   79.3 (2A) / 130.5 (2B) / 160.8 (2C) (119.2 projected, +5.0) (11.7)
2023.03       (122.3 projected, +3.1)  
2023.04       (127.7 projected, +5.4)  
2023.05       (133.5 projected, +5.8)  
2023.06       (136.8 projected, +3.3)  
2023.07       (136.3 projected, -0.5)  
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.