Solar Terrestrial Activity Report

Activity chart

Last major update issued on May 9, 2014 at 05:40 UTC.

[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]
[Presentation 3rd SSN Workshop, Tucson, 2013 (pdf)]

Recent activity

The geomagnetic field was quiet to active on May 8. Solar wind speed at SOHO ranged between 328 and 403 km/s.

Solar flux at 20h UTC on 2.8 GHz was 148.1 (increasing 10.5 over the last solar rotation). The 90 day 10.7 flux at 1 AU was 149.4. The Potsdam WDC planetary A index was 18 (STAR Ap - based on the mean of three hour interval ap indices: 18.0). Three hour interval K indices: 23342334 (planetary), 24343433 (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 19 active regions in 2K resolution (SN: 308) and 17 active regions in 1K resolution (SN: 229) SDO images on the visible solar disk.

Region 12049 [S08W77] developed slowly and was quiet.
Region 12050 [N12W71] decayed slowly and quietly.
Region 12052 [S12W31] decayed losing all umbrae.
Region 12053 [N09W15] decayed slowly and quietly.
Region 12054 [S12E12] decayed slowly and quietly.
Region 12055 [N12E30] gained a few spots and was quiet. An M class flare is possible.
Region 12056 [N05E45] still has a magnetic delta structure in the trailing penumbra another major flare is possible.
Region 12057 [N15E53] was quiet and stable.
New region 12058 [S12E68] rotated into view on May 7 and was numbered by SWPC the next day.

Spotted regions not numbered (or interpreted differently) by SWPC:
S3386 [S19W28] was quiet and stable.
S3393 [S12W68] was quiet and stable.
S3394 [S16W03] was quiet and stable.
S3398 [S26W10] reemerged with a penumbra spot.
S3401 [N03E56] was quiet and stable.
New region S3404 [N13E19] emerged with penumbra spots.
New region S3405 [N09E50] emerged with a few spots.
New region S3406 [N00E47] was split off from AR 12056.
New region S3407 [S17E79] rotated into view.
New region S3408 [S33E07] emerged with penumbra spots.

C2+ Flares (SDO/EVE):

Magnitude Time (UTC) Location AR
C2.7 01:39 N03E60 12056
C2.9 09:53 S15E90  
M7.7 10:05 N06E55 12056

Coronal mass ejections (CMEs)

May 6-8: 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 southern hemisphere coronal hole (CH616) was in an Earth facing position on May 7.

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 poor. Propagation on long distance northeast-southwest paths is fair.

Forecast

The geomagnetic field is expected to be quiet to unsettled on May 9-10 and quiet on May 11.

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
12049 2014.04.26
2014.04.27
6 4 4 S08W76 0200 CSO DAO

area: 0300

12050 2014.04.27 1 1   N12W74 0010 AXX AXX location: N12W71

area: 0002

12052 2014.05.01
2014.05.02
2 6 3 S12W32 0010 BXO BXO area: 0022
S3379 2014.05.01       S06W21           plage
S3380 2014.05.02       N10W18           plage
S3382 2014.05.02       S14W48           plage
12053 2014.05.03 3 9 5 N10W16 0030 CAO CRO

location: N09W15

12054 2014.05.03
2014.05.04
1 13 2 S12E11 0020 HRX CRO  
S3385 2014.05.03       N10E06           plage
S3386 2014.05.03   3 2 S19W28 0012   BXO  
12055 2014.05.04
2014.05.05
4 21 11 N12E32 0450 DHO EKO area: 0790

location: N12E30

S3389 2014.05.04       S32W14           plage
12056 2014.05.05
2014.05.06
15 34 15 N04E44 0350 EKI EKC beta-gamma-delta

location: N05E45

area: 0560

S3393 2014.05.05   1 1 S12W68 0006   AXX  
S3394 2014.05.05   2 2 S16W03 0008   BXO  
S3395 2014.05.05       S12E03           plage
12057 2014.05.06
2014.05.07
1 1 1 N15E53 0070 HSX HAX area: 0170
S3397 2014.05.06       S15E51           plage
S3398 2014.05.06   1 1 S26W10 0003        
S3399 2014.05.06       S02W58           plage
S3400 2014.05.06       S24W46           plage
S3401 2014.05.07   2 1 N03E56 0005   AXX  
12058 2014.05.07
2014.05.08
1 3 1 S12E69 0050 HAX HAX area: 0100
S3403 2014.05.07       N14E06         plage
S3404 2014.05.08   7 5 N13E19 0018   AXX    
S3405 2014.05.08   4 3 N09E50 0020   CRO    
S3406 2014.05.08   2 1 N00E47 0050   HAX    
S3407 2014.05.08   2 1 S17E79 0060   HAX    
S3408 2014.05.08   2   S33E07 0003   AXX    
Total spot count: 34 118 59  
Sunspot number: 124 308 229  (total spot count + 10 * number of spotted regions)
Weighted SN: 77 172 113  (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): 74 108 126 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
2014.05 136.4 (1)   30.5 (2A) / 118.3 (2B) / 95.4 (2C) (74.4 projected, -2.6) (6.9)

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.