Solar Terrestrial Activity Report

Activity chart

Last major update issued on October 2, 2022 at 08:35 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 (September 1, 2022)
Solar cycle Solar cycles 23-25 (October 1, 2022) Historical solar and geomagnetic data charts 1954-2006 (April 5, 2007)
  Cycle 24-25 progress (October 1, 2022) 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 (October 1, 2022) 3rd SSN Workshop, Tucson, 2013
  Comparison of cycles 12-14, 16, 24-25 (October 1, 2022) 4th SSN Workshop, Locarno, 2014
  Solar polar fields vs. solar cycles (August 21, 2022) 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 very quiet on October 1. Solar wind speed at SOHO ranged between 370 and 484 km/sec. The high latitude magnetometer at Andenes recorded quiet to unsettled levels.

Solar flux density measured at 20h UT on 2.8 GHz was 147.9 - increasing 19.6 over the previous solar rotation. (Centered 1 year average SF at 1 AU - 183 days ago: 114.07). The Potsdam WDC planetary A index was 2 (STAR Ap - based on the mean of three hour interval ap indices: 2.0). Three hour interval K indices: 00000111 (planetary), 00001221 (Boulder), 00000133 (Andenes).

The background x-ray flux is at the class C2 level (GOES 16).

At the time of counting spots (see image time), spots were observed in 11 active regions using 2K resolution (SN: 240) and in 10 active regions using 1K resolution (SN: 165) SDO/HMI images.

Region 13107 [S24W66] decayed slowly losing all mature penumbra.
Region 13110 [N17W37] developed polarity intermixing when new flux emerged to the northeast of the largest spot with negative polarity flux inside a large area of positive polarity. This cused the region to become unstable and a major flare occurred at 20:10 UT. The region was the source of an M8.7 flare at 02:21 UT on October 2.
Region 13111 [N27E19] gained a few spots and was mostly quiet.
Region 13112 [N19E64] was quiet and stable. Note that SWPC include these spots in AR S7901. If that interpretation was correct the region would extend more than 20 degrees longitudinally.
Region 13113 [N16W27] developed slowly and was mostly quiet.
New region 13114 [S33E24] emerged early on September 30 and was numbered by SWPC the next day. The region appeared to be in slow decay late in the day.

Spotted regions not observed (or interpreted differently) by SWPC:
S7897 [N31E00] was quiet and stable.
S7901 [N22E75] has magnetically a very complex layout with multiple magnetic delta structures. Although the region was significantly less active on October 1 than on the previous day, a major flare is possible. C1 flares: C1.9 @ 10:29, C1.9 @ 14:26 UT
S7902 [N28E70] was quiet and stable.
New region S7904 [S19E31] emerged with tiny spots.
New region S7905 [N30E79] rotated into view with tiny spots.

A filament eruption near AR 13113 peaked near 13:00 UT and was associated with a partial halo CME.

C2+ flares:

Magnitude Peak time (UT) Location Source Recorded by Comment
C2.3 01:24 N21E82 S7901 GOES16  
C2.9 02:18   S7901 GOES16  
C2.6 04:01   S7901 GOES16  
C3.8 04:17   S7901 GOES16  
C6.4 04:58   13107 GOES16  
C6.6 05:02   S7901 GOES16  
C2.3 06:30   S7901 GOES16  
C2.2 07:11   S7901 GOES16 incorrectly attributed to AR 13107 by SWPC
C3.8 08:31   S7901 GOES16  
C2.8 12:06   13110 GOES16  
C3.2 12:39   S7901 GOES16  
C3.5 13:00   S7901 GOES16 attributed to AR 13113 by SWPC
C2.1 15:53   S7901 GOES16  
C2.3 16:54   S7901 GOES16  
C3.4 17:41   S7901 GOES16  
C4.3 18:04 N30E22 13111 GOES16  
C2.4 18:27   S7901 GOES16 incorrectly attributed to AR 13110 by SWPC
C3.6 19:02   13110 GOES16  
M5.8/1B 20:10 N18W36 13110 GOES16  
C2.3 22:02   13110 GOES16  

Coronal mass ejections (CMEs)

September 29-30: No obviously Earth directed CMEs were observed.
October 1: A filament eruption near AR 13113 peaked near 13h UT and was associated with a partial halo CME. This CME could reach Earth on October 4.

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]

Recurrent coronal holes (CH1103/CH1104) were Earth facing on September 27 - October 1.

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

Quiet to active conditions are likely on October 2-4 due to effects from CH1104.

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
13105 2022.09.19
2022.09.19
      S17W84        

location: S18W81

13107 2022.09.20
2022.09.21
6 8 4 S25W68 0030 CRI CRO

location: S24W66

13110 2022.09.22
2022.09.23
5 13 9 N17W38 0160 CSO DSI

location: N17W37

13111 2022.09.26
2022.09.27
3 20 5 N28E18 0090 HSX CSO

location: N27E19

S7893 2022.09.28       S15W22          
S7894 2022.09.29       N12E02            
13113 2022.09.29
2022.09.30
8 25 16 N16W29 0100 DAO DAI beta-gamma

area: 0180

S7897 2022.09.29   4   N31E00 0004   BXO  
13114 2022.09.30
2022.10.01
3 12 6 S33E26 0030 CAO CRI  
13112 2022.09.30
2022.09.30
15 9 5 N22E69 0560 EKI CAO area: 0180

location: N19E64

SWPC includes AR S7901 in this region

S7900 2022.09.30       S26W24          
S7901 2022.09.30   30 16 N22E75 0700   FKC beta-gamma-delta
S7902 2022.09.30   1 1 N28E70 0004   AXX  
S7903 2022.09.30       S12E22          
S7904 2022.10.01   4 1 S19E31 0010   BXO    
S7905 2022.10.01   4 2 N30E79 0007   BXO    
Total spot count: 40 130 65  
Sunspot number: 100 240 165  (total spot count + 10 * number of spotted regions)
Weighted SN: 73 166 101  (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): 110 132 132  

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
2021.03 76.0 75.2 17.2 21.7 (+2.7) 10.17
2021.04 75.9 76.4 24.5 24.8 (+3.1) 8.40
2021.05 75.3 77.1 21.2 25.8 (+1.0) 6.50
2021.06 79.4 81.8 25.0 27.6 (+1.8) 5.52
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 64.8 (+4.7) 10.46
2022.03 117.0 115.8 78.6 68.9 (+4.1) 10.20
2022.04 130.8 131.7 84.1 (74.2 projected, +5.3) 11.79
2022.05 133.8 136.8 96.5 (80.6 projected, +6.4) 7.48
2022.06 116.1 119.8 70.5 (86.5 projected, +5.9) 8.20
2022.07 125.4 129.5 91.4 (93.7 projected, +7.2) 9.51
2022.08 114.2 117.1 75.4 (100.2 projected, +6.5) 10.92
2022.09 135.1 136.5 96.3 (105.2 projected, +5.0) 12.2
2022.10 147.9 (1)   3.2 (2A) / 100 (2B) / 110.2 (2C) (108.3 projected, +3.1) (2.0)
2022.11       (111.2 projected, +2.9)  
2022.12       (115.9 projected, +4.7)  
2023.01       (122.0 projected, +6.1)  
2023.02       (127.0 projected, +5.0)  
2023.03       (130.0 projected, +3.0)  
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.