Solar Terrestrial Activity Report

Activity chart

Last major update issued on December 18, 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 (December 3, 2015)
Solar cycle Solar cycles 23-24 (December 1, 2015) Historical solar and geomagnetic data charts 1954-2006 (April 5, 2007)
  Cycle 24 progress (December 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 (December 1, 2015) 3rd SSN Workshop, Tucson, 2013
  Comparison of cycles 12, 13, 14, 16 and 24 (December 1, 2015) 4th SSN Workshop, Locarno, 2014
  Solar polar fields vs. solar cycles (November 16, 2015)  

Recent activity

The geomagnetic field was quiet to unsettled on December 17. Solar wind speed at SOHO ranged between 375 and 475 km/s.

Solar flux at 20h UTC on 2.8 GHz was 117.8 (increasing 6.8 over the last solar rotation). The 90 day 10.7 flux at 1 AU was 106.6. The Potsdam WDC planetary A index was 5 (STAR Ap - based on the mean of three hour interval ap indices: 5.4). Three hour interval K indices: 11011232 (planetary), 11022332 (Boulder).

The background x-ray flux is at the class B3 level.

At the time of counting spots (see image time), spots were observed in 9 active regions using 2K resolution (SN: 166) and 3 active regions using 1K resolution (SN: 52) SDO images on the visible solar disk.

Region 12465 [S04W69] reemerged with tiny spots.
Region 12468 [S15W26] decayed slowly and quietly.
Region 12469 [N18E01] gained a few spots and was quiet.
Region 12470 [N13E16] was mostly quiet and stable.
Region 12471 [S21E06] was quiet and stable.

Spotted regions not numbered (or interpreted differently) by SWPC:
S4956 [N12W28] was quiet and stable.
S4964 [N25W44] reemerged with a tiny spot.
S4968 [N22E52] was quiet and stable.
S4969 [S16E60] gained a few tiny spots.

C2+ flares:

Magnitude Peak time (UTC) Location AR Recorded by Comment
           

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

Coronal mass ejections (CMEs)

December 15, 17: No obviously Earth directed CMEs were observed in available LASCO imagery.
December 16: Two likely Earth directed CMEs were observed during the day. The first was observed after the C6 LDE in AR 12468 while the second was caused by an extensive filament eruption from near the equator stretching to the southern polar crown filament.

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

Forecast

The geomagnetic field is expected to be quiet for most or all of December 18. The CMEs observed on December 16 will likely reach Earth on December 19 (maybe as early as late on December 18) and could cause unsettled to minor storm conditions with a chance of major storming.

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.
As of December 12, 2015, the active region maps are based on image products from semi-automated sunspot counting at 4K resolution.

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
12465 2015.12.06
2015.12.07
  2   S06W74 0004   BXO   location: S04W69
12468 2015.12.09
2015.12.10
3 11 2 S17W27 0020 CRO CRO

location: S15W26

S4956 2015.12.11   6   N12W28 0010   BXO images/AR_S4956_20151216_2345.png  
12469 2015.12.11
2015.12.12
2 16 3 N18W01 0020 HAX CRO

area: 0040

12470 2015.12.12 17 32 17 N15E18 0610 EKO FHI

area: 0830

location: N13E16

S4964 2015.12.12   1   N25W44 0003   AXX    
S4965 2015.12.12       S24W44            
12471 2015.12.14   3   S21E02 0007   AXX location: S21E06
S4968 2015.12.15   2   N22E52 0002   AXX  
S4969 2015.12.16   3   S16E60 0008   AXX  
S4970 2015.12.16       S26E31          
Total spot count: 22 76 22  
Sunspot number: 52 166 52  (total spot count + 10 * number of spotted regions)
Weighted SN: 40 92 38  (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): 57 91 44 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
2014.10 153.4 152.9 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 78.9 (-3.3) 10.73
2015.05 120.0 122.6 88.8 76.0 (-2.9) 8.29
2015.06 122.3 126.1 66.5 (72.1 projected, -3.9) 13.15
2015.07 107.0 110.8 66.4 (68.4 projected, -3.7) 8.83
2015.08 105.4 108.0 64.6 (67.2 projected, -1.2) 14.58
2015.09 101.7 102.7 78.1 (67.4 projected, +0.2) 15.78
2015.10 104.1 103.3 61.7 (66.5 projected, -0.9) 14.02
2015.11 109.3 106.9 63.2 (64.5 projected, -2.0) 12.09
2015.12 (109.3)   31.0 (2A) / 56.5 (2B) / 71.8 (2C) (62.7 projected, -1.8) (11.3)

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.