Solar Terrestrial Activity Report

Activity chart

Last major update issued on March 14, 2022 at 12:25 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 (March 1, 2022)
Solar cycle Solar cycles 23-25 (March 1, 2022) Historical solar and geomagnetic data charts 1954-2006 (April 5, 2007)
  Cycle 24-25 progress (March 1, 2022) Noon SDO sunspot count 1K image / 4K (*)
  Solar cycles 1-24 (June 1, 2020) POES auroral activity level October 2009 - December 2012]
  Comparison of cycles 21-25 (March 1, 2022) 3rd SSN Workshop, Tucson, 2013
  Comparison of cycles 12-14, 16, 24-25 (March 1, 2022) 4th SSN Workshop, Locarno, 2014
  Solar polar fields vs. solar cycles (August 22, 2021) 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 major storm on March 13 under the influence of effects from the March 10 CME. The CME was observed reaching SOHO at 10:09 UT. The high latitude magnetometer at Andenes recorded quiet to severe storm levels.

Solar flux density measured at 20h UT on 2.8 GHz was 122.9 - increasing 15.6 over the previous solar rotation. (Centered 1 year average SF at 1 AU - 183 days ago: 88.09). The Potsdam WDC planetary A index was 40 (STAR Ap - based on the mean of three hour interval ap indices: 39.9). Three hour interval K indices: 21145666 (planetary), 11045556 (Boulder), 31045647 (Andenes).

The background x-ray flux is at the class B7 level (GOES 16).

At the time of counting spots (see image time), spots were observed in 7 active regions using 2K resolution (SN: 154) and in 7 active regions using 1K resolution (SN: 116) SDO/HMI images.

Region 12960 [S19W62] was quiet and stable.
Region 12965 [N23E08] developed another magnetic delta and produced an M2 flare at 08:40 UT on March 14. Further M class flaring is likely.
Region 12967 [N18E47] was quiet and stable.
New region 12968 [S20E42] was observed with spots on March 13. SWPC numbered the region 3 days later when the region was decaying.

Spotted regions not observed (or interpreted differently) by SWPC:
S7417 [S19W12] was quiet and stable.
S7423
[S25W28] was quiet and table.
S7426 [S22E45] emerged with tiny spots.

AR 12964 produced flares while at the southwest limb: C1.4 @ 06:15, C1.3 @ 19:58, C1.0 @ 20:26 UT.

C2+ flares:

Magnitude Peak time (UT) Location Source Recorded by Comment
C4.9 03:23 N30W36 12962 GOES16  
C3.9 23:41   12964 GOES16  

Coronal mass ejections (CMEs)

March 11-13: No obviously Earth directed CMEs were observed in available LASCO imagery.

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 locations.

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

The geomagnetic field is expected to be unsettled to major storm on March 14 due to CME effects and quiet to active on March 15. Quiet conditions are likely on March 16.

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
12960 2022.03.02
2022.03.03
2 3 2 S20W61 0300 CHO CHO

 

12962 2022.03.05       N27W49         location: N25W45
12965 2022.03.08 20 60 36 N24E09 0600 FKI FAC beta-gamma-delta

location: N23E08

S7411 2022.03.08       S27W37            
S7414 2022.03.09       S32W36            
S7417 2022.03.10   5 2 S19W12 0012   CRO  
S7418 2022.03.10       S16E28            
12968 2022.03.10
2022.03.13
1 3 1 S21E43 0010 AXX AXX location: S20E42
S7420 2022.03.10       S16W50            
12967 2022.03.11
2022.03.12
1 1 1 N17E46 0030 HSX HSX area: 0050

location: N18E47

S7422 2022.03.11       N30E39            
S7423 2022.03.11   4 1 S25W28 0007   BXO  
S7424 2022.03.11       S33W26            
S7425 2022.03.12       S16W05          
S7426 2022.03.12   8 3 S22E31 0015   CRO  
Total spot count: 24 84 46  
Sunspot number: 64 154 116  (total spot count + 10 * number of spotted regions)
Weighted SN: 49 110 72  (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): 70 85 93  

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
2020.08 71.6 73.4 7.5 9.5 (+0.5) 5.68
2020.09 70.7 71.4 0.7 10.5 (+1.0) 8.59
2020.10 74.6 74.2 14.6 11.9 (+1.4) 6.13
2020.11 89.9 88.0 34.5 13.6 (+1.7) 4.77
2020.12 86.9 84.2 23.1 15.3 (+1.7) 4.72
2021.01 76.0 73.6 10.4 17.3 (+2.0) 4.39
2021.02 74.3 72.4 8.2 19.0 (+1.7) 9.50
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 27.7 (+1.9) 5.52
2021.07 81.0 83.6 34.3 31.4 (+3.7) 5.51
2021.08 77.7 79.7 22.0 35.3 (+3.9) 6.19
2021.09 87.0 88.2 51.3 (39.9 projected, +4.6) 6.33
2021.10 88.9 88.3 38.1 (43.6 projected, +3.7) 7.38
2021.11 86.2 84.4 35.0 (48.2 projected, +4.6) 9.83
2021.12 103.0 99.8 67.6 (54.0 projected, +5.8) 6.40
2022.01 103.8 100.5 54.0 (57.7 projected, +3.7) 8.92
2022.02 109.1 106.5 59.7 (62.4 projected, +4.7) 10.5
2022.03 116.8 (1)   34.5 (2A) / 82.2 (2B) / 80.2 (2C) (67.9 projected, +5.5) (13.0)
2022.04       (73.0 projected, +5.1)  
2022.05       (79.4 projected, +6.4)  
2022.06       (85.3 projected, +5.9)  
2022.07       (92.6 projected, +7.3)  
2022.08       (99.2 projected, +6.6)  

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.