Solar Terrestrial Activity Report

Activity chart

Last major update issued on April 15, 2015 at 04:25 UT

[Solar and geomagnetic data - last month (updated daily)]
[Solar wind and electron fluence charts (updated daily)]
[Solar cycles 23-24 (last update April 1, 2015)] [Cycle 24 progress (last update April 1, 2015) ]
[Solar cycles 1-20]
[Graphical comparison of cycles 21, 22, 23 and 24 (last update April 1, 2015)]
[Graphical comparison of cycles 10, 12, 13, 14, 16 and 24 (last update April 1, 2015)]
[Historical solar and geomagnetic data charts 1954-2006 (last update April 5, 2007)]
[Archived reports since January 2003 (last update April 1, 2015)]

[Noon SDO sunspot count 1K Reference: 4K (large file) (updated daily)]

[POES auroral activity level October 2009 - December 2012]
[Solar polar fields vs solar cycles - updated April 10, 2015]
[Presentations: 3rd SSN Workshop, Tucson, 2013 (pdf) / 4th SSN Workshop, Locarno, 2014]

Recent activity

The geomagnetic field was quiet to active on April 14. Solar wind speed at SOHO ranged between 272 and 421 km/s. A disturbance associated with a co-rotating interaction region and an extension of the southern polar coronal hole, began after noon.

Solar flux at 20h UTC on 2.8 GHz was 146.8 (increasing 32.0 over the last solar rotation). The 90 day 10.7 flux at 1 AU was 126.2. The Potsdam WDC planetary A index was 12 (STAR Ap - based on the mean of three hour interval ap indices: 11.5). Three hour interval K indices: 01113434 (planetary), 01123533 (Boulder).

The background x-ray flux is at the class B7 level.

At the time of counting spots (see image time), spots were observed in 12 active regions using 2K resolution (SN: 229) and 10 active regions using 1K resolution (SN: 151) SDO images on the visible solar disk.

Region 12321 [N12E29] was mostly quiet and stable.
Region 12322 [N15E02] decayed slowly and quietly.
Region 12323 [S17W72] decayed slowly and quietly.
New region 12324 [N19E61] rotated into view early on April 13 and was numbered the next day by SWPC.
New region 12325 [N04E69] rotated into view on April 13.

Spotted regions not numbered (or interpreted differently) by SWPC:
S4367 [N08E37] was quiet and has polarity intermixing.
S4368 [N16E37] decayed slowly and was quiet.
S4369 [S03W27] decayed slowly and was quiet.
S4374 [N18E20] decayed slowly and quietly.
S4376 [N12W38] decayed slowly and quietly.
New region S4377 [N12E05] emerged just south of AR 12322.
New region S4378 [N26W11] emerged with a penumbra spot.

C2+ flares:

Magnitude Peak time (UTC) Location AR Recorded by Comment
C2.9 (LDE) 15:50 east limb   SDO/EVE filament eruption, CME

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

Coronal mass ejections (CMEs)

April 12-14: 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]

An extension (CH663) of the southern polar coronal hole could be associated with a co-rotating interaction region. The extension rotated across the central meridian on April 11-12.

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 to fair.

Forecast

The geomagnetic field is expected to be quiet to active on April 15 and quiet to unsettled on April 16-17.

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
12320 2015.04.02
2015.04.04
3     S14W92 0070 DAO    

rotated out of view

12318 2015.04.03       N08W80           location: N07W62
12323 2015.04.06
2015.04.11
5 4 2 S16W76 0060 BXO CAO  
S4358 2015.04.07       S17W11            
S4359 2015.04.07       N11W28            
S4360 2015.04.08       S10W53            
S4361 2015.04.09       S22W34            
S4362 2015.04.10       S04W10          
12322 2015.04.10
2015.04.11
3 10 4 N14W02 0020 BXO CRO

location: N15E02

S4364 2015.04.10       N10E07            
12321 2015.04.10
2015.04.11
14 39 18 N13E26 0620 EKC DAI beta-gamma

area: 0510

location: N12E29

S4367 2015.04.11   13 8 N08E37 0240   DAO  
S4368 2015.04.11   14 4 N16E37 0050   CAO  
S4369 2015.04.12   2 1 S03W27 0006   BXO  
S4370 2015.04.12       S19W40            
12324 2015.04.13
2015.04.14
11 14 8 N19E59 0390 DKI CKO area: 0550
S4372 2015.04.13       S18E27          
12325 2015.04.13
2015.04.14
1 5 3 N04E67 0130 HSX CKO area: 0300
S4374 2015.04.13   1 1 N18E20 0005   AXX  
S4375 2015.04.13       N10E22          
S4376 2015.04.13   2   N12W38 0003   BXO  
S4377 2015.04.14   4 2 N12E05 0015   BXO    
S4378 2015.04.14   1   N26W11 0002   AXX    
Total spot count: 37 109 51  
Sunspot number: 97 219 151  (total spot count + 10 * number of spotted regions)
Weighted SN: 67 152 94  (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): 58 77 83 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
2013.11  148.3 145.1 77.6 75.4 (+0.4) 5.68
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)
(likely 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 78.6 (-1.1) 4.50
2014.08 124.7 127.9 74.7 75.6 (-3.0) 7.71
2014.09 146.6 148.1 87.6 70.9 (-4.7) 9.78
2014.10 153.4 152.9 60.6 (67.3 projected, -3.6) 8.96
2014.11 154.8 151.4 70.1 (64.7 projected, -2.6) 9.33
2014.12 158.7 153.8 78.0 (62.4 projected, -2.3) 11.24
2015.01 141.9 137.3 67.0 (60.2 projected, -2.2) 9.46
2015.02 129.1 126.0 44.8 (58.4 projected, -1.8) 9.92
2015.03 125.9 124.6 38.4 (56.1 projected, -2.3) 16.14
2015.04 (122.5)   26.5 (2A) / 56.7 (2B) / 69.8 (2C) (53.4 projected, -2.7) (9.2)

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.