Solar Terrestrial Activity Report

Activity chart

Last major update issued on April 23, 2015 at 06:30 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 unsettled on April 22. Solar wind speed at SOHO ranged between 457 and 560 km/s.

Solar flux at 20h UTC on 2.8 GHz was 150.3 (increasing 14.2 over the last solar rotation). The 90 day 10.7 flux at 1 AU was 129.0. The Potsdam WDC planetary A index was 8 (STAR Ap - based on the mean of three hour interval ap indices: 8.4). Three hour interval K indices: 22322122 (planetary), 22433323 (Boulder).

The background x-ray flux is at the class B9 level.

At the time of counting spots (see image time), spots were observed in 19 active regions using 2K resolution (SN: 345) and 16 active regions using 1K resolution (SN: 235) SDO images on the visible solar disk.

Region 12321 [N11W73] was quiet and stable.
Region 12324 [N18W46] decayed slowly producing a few low level C flares.
Region 12325 [N05W38] was mostly quiet and stable. Minor polarity intermixing was observed.
Region 12327 [S09E04] was quiet and stable.
Region 12330 [N15E08] was quiet and stable.
Region 12331 [S10W05] developed slowly and was mostly quiet.
Region 12332 [S14W30] decayed slowly and quietly.
New region 12333 [N20E65] rotated into view on April 21 and was numbered by SWPC the next day.

Spotted regions not numbered (or interpreted differently) by SWPC:
S4367 [N08W71] decayed slowly and quietly.
S4383 [S10W15] was quiet and stable.
S4389 [S22E10] was quiet and stable.
S4398 [N10W12] developed slowly and quietly.
S4400 [N08E19] was quiet and stable.
S4404 [N08E52] was quiet and stable.
S4406 [S11W39] decayed slowly and quietly.
New region S4407 [N18E40] was observed with penumbra spots.
New region S4408 [N20W67] emerged quickly with several spots. C flares are possible.
New region S4409 [S03E42] was observed with a penumbra spot.
New region S4410 [N23E13] emerged with penumbra spots.

C2+ flares:

Magnitude Peak time (UTC) Location AR Recorded by Comment
C2.3 01:15   S4392 GOES15 attributed to AR 12325 by SWPC
C3.7/1N 01:44 N23W32 12324 GOES15  
C4.6 02:07   S4392 GOES15 attributed to AR 12325 by SWPC
C5.5 02:18   S4392 SDO/EVE, Learmonth  
C2.8 03:05   S4392 GOES15 attributed to AR 12333 by SWPC
C4.0 03:20   S4392 SDO/EVE  
C4.1 03:25 N22W35 12324 GOES15  
C2.8 04:51   12324 SDO/EVE  
C2.3 06:11   S4392 GOES15  
C2.3 07:11 S10E17 12327 GOES15  
C3.8 08:06 N21W37 12324 GOES15  
M1.1 08:44 N10W90 S4392 GOES15 attributed to AR 12332 by SWPC
C6.8 09:18   12324 SDO/EVE, San Vito  

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

Coronal mass ejections (CMEs)

April 20-22: 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 southern hemisphere coronal hole (CH665) will likely rotate into an Earth facing position on April 26-27.

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 unsettled on April 23-25.

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
12321 2015.04.10
2015.04.11
1 1   N07W73 0030 HSX AXX area: 0002

location: N13W73

SWPC data is for AR S4367

S4367 2015.04.11   1 1 N08W71 0020   HRX  
12326 2015.04.11
2015.04.16
      N15W69          
12324 2015.04.13
2015.04.14
14 19 12 N19W47 0165 CAI CAI  
12325 2015.04.13
2015.04.14
7 21 11 N06W39 0205 CAO DKO area: 0360

location: N05W38

S4383 2015.04.16   13 2 S10W15 0025   BXO  
12327 2015.04.16
2015.04.17
3 16 9 S10E03 0090 HSX CSI area: 0170
S4389 2015.04.17   3 2  S22E10 0010   BXO  
12331 2015.04.17
2015.04.21
15 26 14  S10W04 0040 DAC DAI area: 0180
12329 2015.04.17
2015.04.19
8      S08W93 0050 CRO     rotated out of view
12332 2015.04.18
2015.04.21
5 4 2  S13W31 0020 CRO DRO area: 0030
12330 2015.04.19
2015.04.20
  4 2  N15E04 0010   AXX  
S4398 2015.04.19   11 5  N10W12 0030   CRO  
S4400 2015.04.20   6 3  N08E19 0015   BXO images/AR_S4400_20150422_2345.png images/AR_S4400_20150421_2345.png  
S4404 2015.04.21   4 2  N08E52 0010   BXO  
12333 2015.04.21
2015.04.22
1 4 1  N19E62 0030 HRX HAX area: 0060

location: N20E65

S4406 2015.04.21   2    S11W39 0006   BXO  
S4407 2015.04.22   3 2  N18E40 0010   BXO    
S4408 2015.04.22   14 6  N20W67 0100   DAI   beta-gamma
S4409 2015.04.22   1 1  S03E42 0003   AXX    
S4410 2015.04.22   2    N23E13 0005   BXO    
Total spot count: 54 155 75  
Sunspot number: 134 345 235  (total spot count + 10 * number of spotted regions)
Weighted SN: 88 199 119  (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): 80 121 129 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 (132.9)   57.5 (2A) / 78.4 (2B) / 85.3 (2C) (53.4 projected, -2.7) (12.1)

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.