Solar Terrestrial Activity Report

Activity chart

Last major update issued on January 4, 2024 at 04:15 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 (January 1, 2024)
Solar cycle Solar cycles 23-25 (January 1, 2024) Historical solar and geomagnetic data charts 1954-2006 (April 5, 2007)
  Cycle 24-25 progress (January 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 (January 1, 2024) 3rd SSN Workshop, Tucson, 2013
  Comparison of cycles 12-14, 16, 24-25 (January 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 (new)

Recent activity

The geomagnetic field was quiet to unsettled on January 3 under the influence of weak CME effects after 05 UT. Solar wind speed at SOHO ranged between 368 and 495 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 140.2 - increasing 5.6 over the previous solar rotation. (Centered 1 year average SF at 1 AU - 183 days ago: 158.41. 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 11 (STAR Ap - based on the mean of three hour interval ap indices: 10.6). Three hour interval K indices: 32122321 (planetary), 22232322 (Boulder), 42112353 (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 10 active regions using 2K resolution (SN: 192) and in 8 active regions using 1K resolution (SN: 134) SDO/HMI images.

Region 13534 [S14W33] developed slowly as new flux emerged. C1 flares: C1.2 @ 21:04, C1.4 @ 21:16 UT
Region 13536 [N05E36] regained a magnetic delta structure and produced a number of low level C flares. Early on January 4 the region produced 2 M flares, the largest being an M3.8 event at 01:55 UT. C1 flares: C1.8 @ 10:10, C1.3 @ 13:34, C1.4 @ 00:10 (on January 4) UT
Region 13537 [N17E32] decayed slowly and was mostly quiet. C1 flares: C1.8 @ 14:56 UT
New region 13538 [N20E12] emerged with several spots. C1 flares: C1.5 @ 16:56, C1.6 @ 17:17, C1.1 @ 22:53 UT

Spotted regions not observed (or interpreted differently) by SWPC/USAF:
S9273 [S12W19] decayed slowly and quietly.
S9279 [N07E45] was mostly quiet and stable. C1 flares: C1.0 @ 23:54 UT
S9288 [N21W13] decayed slowly and quietly.
New region S9290 [N12W26] emerged with tiny spots.
New region S9291 [N12E74] rotated into view with a tiny spot.
New region S9292 [N21E18] emerged to the east of AR 13538.

The most recent above 10 MeV proton flux peak was at 17.9 pfu at 00:40 UT on January 4.

An active region at the northeast limb produced a C1.2 flare at 02:59 and a C1.4 flare at 16:21 UT

C2+ flares:

Magnitude Peak time (UT) Location Source Recorded by Comment
C3.0 10:18 N05E49 13536 GOES16  
C2.7 19:58 N06E39 13536 GOES16  

Coronal mass ejections (CMEs)

January 1-3: No obviously Earth directed CME 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 positive polarity southern hemisphere coronal hole (CH1196) will be Earth facing on January 4-6. CH1196 may be too far to the south to cause a geomagnetic disturbance.

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 very poor. Propagation on long distance northeast-southwest paths is poor.

Forecast

The geomagnetic field is expected to be quiet to unsettled on January 4 due to CME effects. Quiet conditions are likely on January 5-6.

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
13534 2023.12.26
2023.12.27
2 13 6 S14W37 0010 BXO CRO

location: S14W33

area: 0030

S9269 2023.12.27       N20W48            
S9271 2023.12.29       N00W54            
S9273 2023.12.29   1 1 S12W16 0003   AXX  
S9275 2023.12.30       S02W44            
13536 2023.12.31
2023.12.31
10 28 16 N06E37 0250 EKO DAC beta-delta

location: N05E36

S9279 2023.12.31   14 9 N07E45 0050   CRO  
S9280 2023.12.31       N20W33            
S9281 2023.12.31       N08E06            
S9282 2023.12.31       S18W27            
13538 2023.12.31
2024.01.03
5 16 12 N21E11 0030 DAO CRI location: N20E12

area: 0060

S9284 2024.01.01       S01W05            
13537 2024.01.01
2024.01.02
6 9 5 N18E34 0060 CAO CAO area: 0090

location: N17E32

S9286 2024.01.01       N07W40          
S9287 2024.01.02       N20E22          
S9288 2024.01.02   1   N21W13 0002      
S9289 2024.01.02       S13W03          
S9290 2024.01.03   6 3 N12W26 0013   BXO    
S9291 2024.01.03   1   N12E74 0002   AXX    
S9292 2024.01.03   3 2 N21E18 0010   BXO    
Total spot count: 23 92 54  
Sunspot number: 63 192 134  (total spot count + 10 * number of spotted regions)
Weighted SN: 43 111 73  (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): 69 106 107  

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
2022.05 133.8 136.8 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 92.6 (+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)
2023.03 157.2 155.6 123.3 121.0 (+3.2) 14.42
2023.04 145.4 146.4 97.6 122.7 (+1.7) 13.40
2023.05 155.6 159.2 137.4 123.9 (+1.2) 10.67
2023.06 161.7 166.8 160.5 125.0 (+1.1)
(SC25 solar max candidate)
8.95
2023.07  176.4 182.2 159.1 (124.6 projected, -0.4) 8.15
2023.08  153.7 157.6 114.8 (124.1 projected, -0.5) 7.19
2023.09  154.4 156.0 133.6 (123.8 projected, -0.3) 14.26
2023.10  142.8 141.9 99.4 (124.6 projected, +0.8) 8.16
2023.11 153.5 150.2 105.4 (124.6 projected, +0.0) 12.20
2023.12 151.1 146.4 114.2 (121.2 projected, -3.4) 9.7
2024.01 139.3 (1)   5.4 (2A) / 55.3 (2B) / 132.0 (2C) (117.9 projected, -3.3) (9.1)
2024.02       (117.1 projected, -0.8)  
2024.03       (116.6 projected, -0.5)  
2024.04       (116.6 projected, +0.0)  
2024.05       (117.0 projected, -0.8)  
2024.06       (114.9 projected, -2.1)  

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 January 3, 2024

The relatively low solar activity during the last months of 2023 significantly increased the possibility that solar cycle 25 has already peaked. Whether the first peak in June 2023 will be the actual solar max will not be known for some time. Due to the relatively high solar activity early in 2023 it is unlikely there will be another solar max candidate, if at all, until at least May 2024. Both the northern and southern polar fields, as well as the averaged total field, have already reversed polarities.

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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.