Solar Terrestrial Activity Report

Activity chart

Partial update issued on May 21, 2014 at 06:00 UTC. The active region section was updated at 11:10 UTC. Updates May 18-23 will be irregular and possibly incomplete.

[Solar and geomagnetic data - last month (updated daily)]
[Solar wind and electron fluence charts (updated daily)]
[Solar cycles 23-24 (last update May 1, 2014)] [Cycle 24 progress (last update May 1, 2014) ]
[Solar cycles 1-20]
[Graphical comparison of cycles 21, 22, 23 and 24 (last update May 1, 2014)]
[Graphical comparison of cycles 10, 12, 13, 14, 16 and 24 (last update May 1, 2014)]
[Historical solar and geomagnetic data charts 1954-2006 (last update April 5, 2007)]
[Archived reports since January 2003 (last update May 1, 2014)]

[POES auroral activity level October 2009 - December 2012]
[Solar polar fields vs solar cycles - updated April 17, 2014]
[Presentations: 3rd SSN Workshop, Tucson, 2013 (pdf) / 4th SSN Workshop, Locarno, 2014]

Recent activity

The geomagnetic field was quiet on May 20. Solar wind speed at SOHO ranged between 328 and 358 km/s.

Solar flux at 20h UTC on 2.8 GHz was 117.2 (decreasing 18.9 over the last solar rotation). The 90 day 10.7 flux at 1 AU was 148.1. The Potsdam WDC planetary A index was 3 (STAR Ap - based on the mean of three hour interval ap indices: 2.9). Three hour interval K indices: 11111100 (planetary), 11122211 (Boulder).

The background x-ray flux is at the class B4 level.

At the time of counting spots (see image time), spots were observed in 14 active regions in 2K resolution (SN: 192) and 10 active regions in 1K resolution (SN: 126) SDO images on the visible solar disk.

Region 12061 [S23W47] was quiet and stable.
Region 12063 [N10W38] decayed slowly and quietly.
Region 12065 [S18W02] decayed slowly and quietly and lost the trailing spot section when AR 12072 emerged.
Region 12066 [S17W53] was quiet and stable.
Region 12068 [S16W14] was quiet and stable.
Region 12069 [S18E27] developed slowly and quietly.
Region 12070 [S17W75] decayed slowly and quietly.
Region 12071 [S12E64] developed slowly and was mostly quiet.
New region 12072 [S18E08] emerged in what used to be the trailing spot section of AR 12065.

Spotted regions not numbered (or interpreted differently) by SWPC:
S3444 [S26E38] was quiet and stable.
S3446 [N02W08] reemerged with a penumbra spot.
New region S3455 [S11E77] rotated into view.
New region S3456 [N25W80] emerged with a penumbra spot.
New region S3457 [N20W17] emerged with a penumbra spot.

C2+ Flares (SDO/EVE):

Magnitude Time (UTC) Location AR

Coronal mass ejections (CMEs)

May 18-20: No obviously Earth directed CMEs were observed in LASCO and STEREO 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

A small trans equatorial coronal hole (CH618) will rotate into an Earth facing position on May 21.

Coronal hole map

Propagation

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

Forecast

The geomagnetic field is expected to be quiet on May 21-23. On May 24 there is a slight chance of unsettled intervals should a stream from CH618 reach Earth.

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 overlay
Comment
SWPC Magnetic
(SDO)
SWPC STAR Current Previous
2K 1K
12060 2014.05.08
2014.05.11
2     S13W89   HAX    

rotated out of view

12061 2014.05.10
2014.05.11
1 2 2 S25W49 0050 HSX CSO area: 0150
S3417 2014.05.11       S23W58           plage
S3418 2014.05.11       N22W43           plage
S3422 2014.05.13       S23W16           plage
S3423 2014.05.13       S09W45           plage
12063 2014.05.13
2014.05.14
2 2 2 N09W38 0010 AXX HRX

 

12064 2014.05.13
2014.05.14
      N09W54           plage
12066 2014.05.13
2014.05.16
5 9 3 S17W53 0040 DAO DAO  
12065 2014.05.14
2014.05.15
2 4 2 S20E01 0010 BXO AXX location: S18W03
S3433 2014.05.15       N18W55           plage
S3436 2014.05.15       N08W17           plage
S3437 2014.05.15       N25E03           plage
12068 2014.05.16
2014.05.17
3 2 2 S15W16 0010 BXO BXO location: S16W14
S3440 2014.05.16       S12W39           plage
S3441 2014.05.16       N27W50           plage
S3443 2014.05.16       N10W34           plage
S3444 2014.05.17   1   S25E34 0003   AXX  
12069 2014.05.17
2014.05.18
1 6 3 S18E27 0000 AXX CRO  
S3446 2014.05.17   1   N02W08          
S3448 2014.05.17       S35W11         plage
S3449 2014.05.18       N26W00         plage
12070 2014.05.18
2014.05.19
4 2   S18W76 0010 BXO BXO  
S3452 2014.05.18       N17W35            
12071 2014.05.19 4 12 5 S12E64 0030 CRO DAO area: 0180
12072 2014.05.20 2 8 5 S20E07 0010 AXX DRO   area: 0045
S3455 2014.05.20   1 1 S11E77 0090   HSX    
S3456 2014.05.20   1   N25W80 0002   AXX    
S3457 2014.05.20   1 1 N20W17 0003   AXX    
Total spot count: 26 52 26  
Sunspot number: 126 192 126  (total spot count + 10 * number of spotted regions)
Weighted SN: 44 86 60  (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): 76 67 69 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
2013.02 104.3 101.8 38.0 58.4 (-0.3) 6.11
2013.03 111.3 110.2 57.9 57.5 (-0.9) 10.56
2013.04 124.8 125.9 72.4 57.9 (+0.4) 5.40
2013.05 131.4 134.3 78.7 59.9 (+2.0) 9.73
2013.06 110.1 113.7 52.5 62.6 (+2.7) 12.60
2013.07 115.5 119.3 57.0 65.5 (+2.9) 9.47
2013.08 114.6 118.3 66.0 69.0 (+3.5) 8.27
2013.09 102.6 103.7 36.9 73.1 (+4.1) 5.23
2013.10  132.1 131.2 85.6 75.0 (+1.9) 7.71
2013.11  148.3 145.1 77.6 (75.6 projected, +0.6) 5.68
2013.12 147.7 143.1 90.3 (76.6 projected, +1.0) 4.68
2014.01 157.4 152.4 82.0 (77.6 projected, +1.0) 5.44
2014.02 170.3
(cycle peak)
166.3 102.8 (cycle peak) (77.4 projected, -0.2) 10.70
2014.03 149.9 148.5 92.2 (77.9 projected, +0.5) 4.88
2014.04 143.9 144.8 84.7 (77.0 projected, -0.9) 7.88
2014.05 141.9 (1)   84.7 (2A) / 131.3 (2B) / 98.7 (2C) (74.4 projected, -2.6) (5.7)

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.