Solar Terrestrial Activity Report

Activity chart

Last major update issued on May 16, 2015 at 06:20 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 (May 1, 2015)
Solar cycle Solar cycles 23-24 (May 1, 2015) Historical solar and geomagnetic data charts 1954-2006 (April 5, 2007)
  Cycle 24 progress (May 1, 2015) Noon SDO sunspot count 1K Reference: 4K (large file) (*)
  Solar cycles 1-20 POES auroral activity level October 2009 - December 2012
  Comparison of cycles 21, 22, 23 and 24 (May 1, 2015) 3rd SSN Workshop, Tucson, 2013
  Comparison of cycles 10, 12, 13, 14, 16 and 24 (May 1, 2015) 4th SSN Workshop, Locarno, 2014
  Solar polar fields vs solar cycles (May 9, 2015)  

Recent activity

The geomagnetic field was quiet on May 15. Solar wind speed at SOHO ranged between 446 and 569 km/s.

Solar flux at 20h UTC on 2.8 GHz was 136.5 (decreasing 11.1 over the last solar rotation). The 90 day 10.7 flux at 1 AU was 127.6. The Potsdam WDC planetary A index was 6 (STAR Ap - based on the mean of three hour interval ap indices: 6.4). Three hour interval K indices: 22222112 (planetary), 22332312 (Boulder).

The background x-ray flux is at the class B5 level.

At the time of counting spots (see image time), spots were observed in 14 active regions using 2K resolution (SN: 243) and 13 active regions using 1K resolution (SN: 180) SDO images on the visible solar disk.

Region 12339 [N11W58] decayed slowly losing spots. There is still a chance of an M class flare.
Region 12340 [S08W37] was quiet and stable.
Region 12341 [S20W30] was quiet and stable.
Region 12342 [N17W21] was mostly unchanged and mostly quiet.
Region 12343 [N10W28] decayed slowly and quietly.
Region 12344 [S09E02] was quiet and stable
Region 12345 [N15W44] was quiet and stable.
Region 12346 [S08E14] decayed slowly and quietly.
Region 12347 [N05E16] was quiet and stable.
Region 12348 [S10E48] was quiet and stable.

Spotted regions not numbered (or interpreted differently) by SWPC:
S4459 [N10W07] was quiet and stable.
S4466 [N12E28] gained a few spots and was quiet.
S4469 [N17W08] decayed slowly and quietly.
S4471 [N19E16] was quiet and stable.

C2+ flares:

Magnitude Peak time (UTC) Location AR Recorded by Comment
C2.0 22:30 N18W15 12342 GOES15  
C2.5 23:29   12339 GOES15  

Flare activity according to SDO/EVE/ESP XRS-B proxy

Coronal mass ejections (CMEs)

May 14-15: No obviously Earth directed CMEs were observed.
May 13: A faint full halo CME was observed in LASCO C3 imagery after the C9 event in AR 12345.

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 recurrent southern hemisphere coronal hole (CH668) was in an Earth facing position on May 14-15.

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.

Forecast

The geomagnetic field is expected to be mostly quiet on May 16. Late on May 16 and on May 17 there is a chance a CME could arrive and cause unsettled to minor storm conditions. A high speed stream associated with CH668 could arrive on May 17 and cause unsettled to active conditions that day and on May 18.

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
12339 2015.05.03
2015.05.04
26 36 18 N12W59 0310 FKC FKC area: 0480
12340 2015.05.06
2015.05.07
  5 1 S08W41 0010   BXO

 

12341 2015.05.06
2015.05.07
1 4 3 S20W31 0070 HSX CSO area: 0120
12345 2015.05.07
2015.05.11
  5 2 N11W49 0012   BXO location: N15W44
12342 2015.05.08
2015.05.09
3 9 6 N17W22 0070 HSX CAO

area: 0130

12343 2015.05.09
2015.05.10
  1   N09W27 0002   AXX  
12344 2015.05.10 2 3 3 S09E02 0050 HAX CAO  
12346 2015.05.10
2015.05.11
7 17 4 S08E15 0030 CAO CRI

area: 0060

12347 2015.05.10
2015.05.11
1 6 3 N05E13 0000 AXX BXO  
S4459 2015.05.11   3 1 N10W07 0007   AXX  
S4463 2015.05.12       N07W16            
12348 2015.05.12
2015.05.14
3 4 3 S10E48 0110 HSX CSO area: 0180
S4466 2015.05.12   6 4 N12E28 0020   BXO  
S4467 2015.05.12       N23E35          
S4468 2015.05.12       N13E16            
S4469 2015.05.13   1 1 N17W08 0005   AXX  
S4470 2015.05.13       N20W28          
S4471 2015.05.14   3 1 N19E16 0008   BXO  
Total spot count: 43 103 50  
Sunspot number: 113 243 180  (total spot count + 10 * number of spotted regions)
Weighted SN: 78 136 83  (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): 68 85 99 k * (sunspot number). k = 0.6 for SWPC, k = 0.35 for MSN 2K, k = 0.55 for MSN 1K (MSN=Magnetic Sunspot Number)

Monthly solar cycle data

Month Average solar flux International sunspot number
(WDC-SILSO)
Smoothed sunspot number Average ap
(3)
Measured 1 AU
2013.12 147.7 143.1 90.3 76.0 (+0.6) 4.68
2014.01 157.4 152.4 81.8 77.3 (+1.3) 5.44
2014.02 170.3
(cycle peak)
166.3 102.3 (cycle peak) 78.4 (+1.1) 10.70
2014.03 149.9 148.5 91.9 80.8 (+2.4) 4.88
2014.04 143.9 144.8 84.7 81.9 (+1.1) (solar max) 7.88
2014.05 129.7 132.9 75.2 80.5 (-1.4) 5.75
2014.06 122.0 125.8 71.0 79.7 (-0.8) 6.72
2014.07 137.4 141.8 72.5 78.5 (-1.2) 4.50
2014.08 124.7 127.9 74.7 75.5 (-3.0) 7.71
2014.09 146.6 148.1 87.6 70.8 (-4.7) 9.78
2014.10 153.4 152.9 60.6 67.3 (-3.5) 8.96
2014.11 154.8 151.4 70.1 (64.9 projected, -2.4) 9.33
2014.12 158.7 153.8 78.0 (62.6 projected, -2.3) 11.24
2015.01 141.9 137.3 67.0 (60.4 projected, -2.2) 9.46
2015.02 129.1 126.0 44.8 (58.7 projected, -1.7) 9.92
2015.03 125.9 124.6 38.4 (56.3 projected, -2.4) 16.14
2015.04 128.8 129.7 54.4 (53.7 projected, -2.6) 10.73
2015.05 (138.6)   53.7 (2A) / 111.1 (2B) / 89.7 (2C) (51.5 projected, -2.2) (10.4)

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). The official WDC-SILSO international sunspot number is typically 30-50% lower. 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.

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 the UTC day. Comments and suggestions are always welcome.

SDO images are courtesy of NASA/SDO and the AIA, EVE, and HMI science teams.