Solar Terrestrial Activity Report

Activity chart

Last major update issued on May 10, 2015 at 05:25 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 to unsettled on May 9. Solar wind speed at SOHO ranged between 345 and 539 km/s.

Solar flux at 20h UTC on 2.8 GHz was 154.5 (increasing 20.6 over the last solar rotation). The 90 day 10.7 flux at 1 AU was 125.6. The Potsdam WDC planetary A index was 7 (STAR Ap - based on the mean of three hour interval ap indices: 7.4). Three hour interval K indices: 10031333 (planetary), 11022333 (Boulder).

The background x-ray flux is at the class B6 level.

At the time of counting spots (see image time), spots were observed in 10 active regions using 2K resolution (SN: 227) and 9 active regions using 1K resolution (SN: 164) SDO images on the visible solar disk.

Region 12335 [S15W44] decayed further and was quiet.
Region 12337 [S17W23] developed slowly and quietly.
Region 12338 [N04W21] decayed slowly and quietly.
Region 12339 [N11E20] displayed signs of decay and became magnetically less complex. The region has polarity intermixing and could produce C and M class flares.
Region 12340 [S08E39] has minor polarity intermixing and was quiet.
Region 12341 [S20E48] was quiet and stable.
New region 12342 [N18E63] rotated into view on May 8 and was numbered by SWPC the next day.

Spotted regions not numbered (or interpreted differently) by SWPC:
S4450 [N15E36] was quiet and stable.
New region S4453 [N08E53] emerged with a few penumbra spots.
New region S4454 [S08E07]emerged with penumbra spots.

C2+ flares:

Magnitude Peak time (UTC) Location AR Recorded by Comment
C7.4 (LDE) 01:34 N14E77 12342 GOES15 CME
SDO/EVE: C9.6 @ 01:40. Flare location @ AIA335: N17E79
C3.0 08:13 N14E35 12339 GOES15  

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

Coronal mass ejections (CMEs)

May 7-9: No obviously Earth directed CMEs were observed.

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 extension (CH667) of the southern polar coronal hole rotated across the central meridian on May 8-9 and may be associated with a co-rotating interaction region.

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 quiet to unsettled on May 10. On May 11-12 effects from CH667 and a co-rotating interaction region could cause unsettled to minor storm conditions.

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
12335 2015.04.30 8 12 6 S16W42 0040 CAO CRO  
12338 2015.05.02
2015.05.03
4 3   N05W24 0020 CRO AXX  
12336 2015.05.02
2015.05.03
      N13W71            
12337 2015.05.02
2015.05.03
4 13 6 S17W23 0020 CRO DRO area: 0050
S4438 2015.05.03       N05W12            
S4439 2015.05.03       N12W05            
12339 2015.05.03
2015.05.04
40 67 43 N12E24 0840 FKC FKC beta-gamma

area: 1140

location: N11E20

S4441 2015.05.04       N13W30            
S4442 2015.05.04       S29W31          
S4444 2015.05.05       S03W05            
S4445 2015.05.05       S04W30            
12340 2015.05.06
2015.05.07
5 8 5 S09E38 0040 CAO CAO

 

12341 2015.05.06
2015.05.07
1 2 1 S20E47 0070 HSX HSX area: 0130
S4449 2015.05.06       N26W24          
S4450 2015.05.07   11 7 N15E36 0030   BXO  
S4451 2015.05.07       S17W08            
12342 2015.05.08
2015.05.09
4 5 4 N18E63 0030 CRO DRO  
S4453 2015.05.09   3 1 N08E53 0010   BXO    
S4454 2015.05.09   3 1 S08E07 0010   BXO    
Total spot count: 66 127 74  
Sunspot number: 136 227 164  (total spot count + 10 * number of spotted regions)
Weighted SN: 100 156 103  (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): 82 79 90 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) 10.3
2015.05 (128.3)    25.8 (2A) / 88.9 (2B) / 82.7 (2C) (51.5 projected, -2.2) (7.3)

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). 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.