Solar Terrestrial Activity Report

Activity chart

Last major update issued on February 18, 2024 at 09:10 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, 2024)
Solar cycle Solar cycles 23-25 (February 1, 2024) Historical solar and geomagnetic data charts 1954-2006 (April 5, 2007)
  Cycle 24-25 progress (February 1, 2024) 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, 2024) 3rd SSN Workshop, Tucson, 2013
  Comparison of cycles 12-14, 16, 24-25 (February 1, 2024) 4th SSN Workshop, Locarno, 2014
  Solar polar fields vs. solar cycles (January  3, 2024) 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
Calculating the Strength of Solar Cycle 25 Using 365-day Smoothing

Recent activity

The geomagnetic field was quiet on February 17. Solar wind speed at SOHO ranged between 311 and 380 km/sec. The high latitude magnetometer at Andenes recorded quiet to active levels. The above 10 MeV proton flux was at 1.4 pfu at the end of the day.

Solar flux density measured at 20h UT on 2.8 GHz was 169.9 - decreasing 8.6 over the previous solar rotation. (Centered 1 year average SF at 1 AU - 183 days ago: 157.20. In comparison SC24 peaked on June 28, 2014 at 145.50. Current SC25 peak: 158.71 on June 27, 2023). The Potsdam WDC planetary A index was 4 (STAR Ap - based on the mean of three hour interval ap indices: 3.6). Three hour interval K indices: 11021012 (planetary), 11012212 (Boulder), 11001034 (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 11 active regions using 2K resolution (SN: 214) and in 10 active regions using 1K resolution (SN: 150) SDO/HMI images.

Region 13581 [S21W45] decayed slowly and quietly.
Region 13582 [N04W83] decayed slowly and quietly.
Region 13583 [N09W57] developed further in the leading spot section and could produce minor M class flares.
Region 13584 [S14W21] developed gaining many small and tiny spots.
Region 13585 [N14E07] was quiet and stable.
Region 13586 [N27E33] was mostly quiet and stable.
Region 13587 [S21E10] decayed slowly and quietly.
Region 13588 [S02E09] was quiet and stable.

Spotted regions not observed (or interpreted differently) by SWPC/USAF:
S9428 [S12E05] was quiet and stable.
New region S9432 [S21E42] emerged with tiny spots before noon, then decayed slowly.
New region S9433 [S11E19] emerged with tiny spots before noon with slow decay observed after noon.

AR 13576 produced a few C1 flares while at the southwest limb: C1.8 @ 02:07, C1.8 @ 02:29 UT

C2+ flares:

Magnitude Peak time (UT) Location Source Recorded by Comment
C2.2 00:49   13583 GOES16  
C2.3 03:23   13576 GOES16  
C5.2 05:59   13583 GOES16 LDE
C2.0 07:54   13576 GOES16  
C5.5 10:35 N07W49 13583 GOES16  
C2.9 12:36 behind northeast limb   GOES16 simultaneous flare in AR 13583
C7.4 18:20   13576 GOES16  
C7.9 18:34   13584 GOES16  
C3.9 20:08 behind northeast limb   GOES16  
C3.1 21:04 behind northeast limb   GOES16  
C3.7 22:40 behind northeast limb   GOES16 LDE

Coronal mass ejections (CMEs)

February 15-17: 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]

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

Forecast

The geomagnetic field is expected to be quiet to unsettled February 17-19.

Coronal holes (1) Coronal mass ejections (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
13581 2024.02.07
2024.02.08
1 3 1 S21W46 0030 HSX HSX location: S21W45

area: 0050

13582 2024.02.08
2024.02.10
2 2 1 N06W78 0030 CRO AXX

area: 0005

location: N04W83

13583 2024.02.08
2024.02.10
11 34 19 N09W53 0270 FKI FKI

beta-gamma

area: 0410

location: N09W57

 
13584 2024.02.09
2024.02.10
6 28 14 S14W21 0020 CRO DRI area: 0060
S9415 2024.02.10       N14W53            
S9417 2024.02.10       N26W52            
S9418 2024.02.11       N10W74          
13585 2024.02.12
2024.02.13
  8 2 N13E05 0015   BXO location: N14E07
S9421 2024.02.12       N27W27          
S9422 2024.02.12       S03W51            
13587 2024.02.13
2024.02.15
6 9 6 S21E10 0010 BXO DRO area: 0030
13586 2024.02.13
2024.02.15
1 5 2 N27E33 0150 HSX CSO

area: 0190

13588 2024.02.14
2024.02.15
  2   S03W00 0002   BXO location: S02E05
13589 2024.02.15
2024.02.15
3     S07W78 0010 BXO      
S9427 2024.02.15       N26W80          
S9428 2024.02.15   7 1 S12E05 0020   BXO  
S9431 2024.02.16       S28W11          
S9432 2024.02.17   1 1 S21E42 0003   AXX    
S9433 2024.02.17   5 3 S11E19 0010   BXO    
Total spot count: 30 104 50  
Sunspot number: 100 214 150  (total spot count + 10 * number of spotted regions)
Weighted SN: 56 130 76  (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): 110 118 120  

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
2022.07 125.4 129.5 91.4 86.7 (+5.6) 9.51
2022.08 114.2 117.1 74.6 92.6 (+5.9) 10.92
2022.09 135.1 136.5 96.0 96.5 (+3.9) 12.18
2022.10 133.5 132.7 95.5 98.9 (+2.4) 11.16
2022.11 123.4 120.7 80.5 101.2 (+2.3) 9.33
2022.12 147.9 143.4 112.8 106.7 (+5.5) 10.99
2023.01 182.4 176.6 144.4 113.3 (+6.6) 8.73
2023.02 167.2 163.2 111.3 117.8 (+3.5) 14.48
(current
SC25 peak)
2023.03 157.2 155.6 123.3 121.1 (+3.3) 14.42
2023.04 145.4 146.4 97.6 122.9 (+1.8) 13.40
2023.05 155.6 159.2 137.4 124.1 (+1.2) 10.67
2023.06 161.7 166.8 160.5 125.2 (+1.1)
(SC25 solar max candidate)
8.95
2023.07  176.4 182.2 160.0 124.3 (-0.9) 8.15
2023.08  153.7 157.6 114.8 (123.4 projected, -0.9) 7.19
2023.09  154.4 156.0 134.2 (123.1 projected, -0.3) 14.26
2023.10  142.8 141.9 99.4 (123.9 projected, +0.8) 8.16
2023.11 153.5 150.2 105.4 (123.9 projected, +0.0) 12.20
2023.12 151.1 146.4 114.2 (120.5 projected, -3.4) 9.60
2024.01 164.6 159.3 123.0 (117.1 projected, -3.3) 5.46
2024.02 176.1 (1)   79.2 (2A) / 135.1 (2B) / 152.5 (2C) (116.3 projected, -0.8) (5.1)
2024.03       (115.8 projected, -0.5)  
2024.04       (115.7 projected, -0.1)  
2024.05       (117.0 projected, +1.3)  
2024.06       (116.2 projected, -0.8)  
2024.07       (114.5 projected, -1.7)  
2024.08       (113.1 projected, -1.4)  

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: WDC-SILSO, Royal Observatory Of Belgium, Brussels

Solar cycles 24-25

Smoothed SF and sunspot numbers

Update on the progress of solar cycle 25 as of February 11, 2024

The relatively high solar activity during the first weeks of 2024 has changed the outlook regarding solar max. The first peak in June 2023 currently has a less than 10% probability of being the actual solar max. The next candidate month is October 2023 (October 8-11 if zooming in on a specific date). The likelihood of October 2023 surpassing June 2023 is at least 50%. It is still likely that solar max will be sometime between October 2023 and March 2025.

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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.