Solar Terrestrial Activity Report

Activity chart

Last major update issued on October 2, 2015 at 04:40 UT.

Charts (* = updated daily) Data and archive
  Solar wind (*) Solar and geomagnetic data - last month (*)
  Electron fluence (*) Archived daily reports and monthly data from 2003.01 (October 1, 2015)
Solar cycle Solar cycles 23-24 (October 1, 2015) Historical solar and geomagnetic data charts 1954-2006 (April 5, 2007)
  Cycle 24 progress (October 1, 2015) Noon SDO sunspot count 1K Reference: 4K (large file) (*)
  Solar cycles 1-24 (July 17, 2015) POES auroral activity level October 2009 - December 2012
  Comparison of cycles 21, 22, 23 and 24 (October 1, 2015) 3rd SSN Workshop, Tucson, 2013
  Comparison of cycles 12, 13, 14, 16 and 24 (October 1, 2015) 4th SSN Workshop, Locarno, 2014
  Solar polar fields vs solar cycles (September 16, 2015)  

Recent activity

The geomagnetic field was quiet to active on October 1. Solar wind speed at SOHO ranged between 273 and 430 km/s. A co-rotating interaction region associated with CH692 arrived at ACE near 11h UT while a low speed stream from CH692 itself became the dominant solar wind source after 23h UT.

Solar flux at 20h UTC on 2.8 GHz was 119.7 (increasing 29.8 over the last solar rotation, the measurement may have been flare enhanced by a C1.7 event in AR 12422 peaking at 20:00 UT). The 90 day 10.7 flux at 1 AU was 107.0. The Potsdam WDC planetary A index was 11 (STAR Ap - based on the mean of three hour interval ap indices: 11.4). Three hour interval K indices: 11113433 (planetary), 01313432 (Boulder).

The background x-ray flux is at the class C1 level.

At the time of counting spots (see image time), spots were observed in 6 active regions using 2K resolution (SN: 149) and 4 active regions using 1K resolution (SN: 87) SDO images on the visible solar disk.

Region 12420 [N11W70] decayed slowly and quietly.
Region 12422 [S20W66] decayed in the leading spot section while the central section has a complex magnetic layout. Another major flare is possible. The region was the source of an impulsive major M5.5 flare at 00:13 UT on October 2.
Region 12427 [N17W04] increased penumbral area in the leading spot section and lost area in the trailing spots.

Spotted regions not numbered (or interpreted differently) by SWPC:
S4781 [S17W03] regained a leader spot.
S4791 [N09E28] was quiet and stable.
New region S4793 [S20E16] was observed with tiny spots.

C2+ flares:

Magnitude Peak time (UTC) Location AR Recorded by Comment
C2.9 02:07 S20W64 12422 SDO/EVE  
C6.3/1F 02:15 S20W59 12422 GOES15  
C3.5 08:35 S23W65 12422 GOES13  
C7.7/1F (LDE) 09:34 S24W62 12422 GOES13  
M4.5/1F 13:10 S23W64 12422 GOES15  
C3.7 21:24 S19W65 12422 GOES15  

Flare activity (SDO/EVE/ESP XRS-B proxy)

Coronal mass ejections (CMEs)

September 29 - October 1: No obviously Earth directed CMEs were observed in available LASCO imagery. The west limb CME observed on September 30 may have had a small Earth directed component.

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 small recurrent northern hemisphere coronal hole (CH692) was in an Earth facing position on September 29. A recurrent trans equatorial coronal hole (CH694) will likely rotate into an Earth facing position on October 4-6.

Propagation

Long distance low and medium frequency (below 2 MHz) propagation along paths north of due west over upper middle latitudes is poor. Propagation on long distance northeast-southwest paths is poor to fair.

Forecast

The geomagnetic field is expected to be quiet to unsettled with a chance of active intervals on October 2 due to effects from CH692 and quiet on October 3-6. There is a minor chance a component of the CME observed on September 30 could reach Earth on October 3 and cause unsettled to active conditions. Quiet to minor storm conditions are possible on October 7-9 due to effects from CH694.

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) 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 numbered solar regions according to the Solar Region Summary provided by NOAA/SWPC. 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.

Active region Date numbered
detected
Spot count Location at midnight Area Classification SDO / HMI 4K continuum
image with magnetic polarity overlays
Comment
SWPC Magnetic
(SDO)
SWPC STAR Current Previous
2K 1K
12420 2015.09.19
2015.09.20
3 3 3 N10W70 0020 CRO ERO

 

12422 2015.09.22 18 32 20 S17W69 0750 FKC FKC beta-gamma-delta

location: S20W66

12425 2015.09.23
2015.09.25
      S05W87            
12426 2015.09.24
2015.09.25
      N16W34          
S4781 2015.09.26   2   S17W03 0003   BXO images/AR_S4781_20151001_2345.png  
12427 2015.09.27 22 48 23 N18W04 0180 DSO DAI

beta-gamma

area: 0300

S4786 2015.09.27       S10W71            
S4787 2015.09.28       S18W48            
S4791 2015.09.30   2   N09E28 0003   AXX  
S4792 2015.09.30       N16E44          
S4793 2015.10.01   2 1 S17W03 0004   AXX    
Total spot count: 43 89 47  
Sunspot number: 73 149 87  (total spot count + 10 * number of spotted regions)
Weighted SN: 61 107 65  (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): 80 82 74 k * (sunspot number)
As of July 1, 2015: k = 1.1 for SWPC, k = 0.55 for MSN 2K, k = 0.85 for MSN 1K (MSN=Magnetic Sunspot Number)

Monthly solar cycle data

Month Average solar flux International sunspot number
(WDC-SILSO) (4)
Smoothed sunspot number (4) Average ap
(3)
Measured 1 AU
2014.02 170.3
(cycle peak)
166.3 146.1 (cycle peak) 110.5 (+1.2) 10.70
2014.04 143.9 144.8 112.5 116.4 (+2.1) (solar max) 7.88
2014.05 129.7 132.9 112.5 115.0 (-1.4) 5.75
2014.06 122.0 125.8 102.9 114.1 (-0.9) 6.72
2014.07 137.4 141.8 100.2 112.6 (-1.5) 4.50
2014.08 124.7 127.9 106.9 108.3 (-4.3) 7.71
2014.09 146.6 148.1 130.0 101.9 (-6.4) 9.78
2014.10 153.4 152.9 90.0 97.3 (-4.6) 8.96
2014.11 154.8 151.4 103.6 94.7 (-2.6) 9.33
2014.12 158.7 153.8 112.9 92.2 (-2.5) 11.24
2015.01 141.9 137.3 93.0 89.3 (-2.9) 9.46
2015.02 129.1 126.0 66.7 86.1 (-3.2) 9.92
2015.03 125.9 124.6 54.5 82.2 (-3.9) 16.14
2015.04 128.8 129.7 75.3 (78.7 projected, -3.5) 10.73
2015.05 120.0 122.6 88.8 (75.9 projected, -2.8) 8.29
2015.06 122.3 126.1 66.5 (72.2 projected, -3.7) 13.15
2015.07 107.0 110.8 66.4 (68.5 projected, -3.7) 8.83
2015.08 105.4 108.0 64.6 (67.3 projected, -1.2) 14.58
2015.09 101.7 102.7 78.1 (67.6 projected, +0.3) 15.7
2015.10 (119.7)   2.4 (2A) / 73 (2B) / 83.5 (2C) (66.7 projected, -0.9) (11.4)

1) Running average based on the daily 20:00 UTC observed solar flux value at 2800 MHz.
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) Updated to new data set from WDC-SILSO on July 1, 2015

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.