Solar Terrestrial Activity Report

Activity chart

Last major update issued on April 21, 2015 at 05:00 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 20. Solar wind speed at SOHO ranged between 354 and 437 km/s. A high speed stream associated with CH664 arrived late in the day and early on April 21.

Solar flux at 20h UTC on 2.8 GHz was 149.7 (increasing 16.7 over the last solar rotation). The 90 day 10.7 flux at 1 AU was 128.2. The Potsdam WDC planetary A index was 9 (STAR Ap - based on the mean of three hour interval ap indices: 8.8). Three hour interval K indices: 33112133 (planetary), 33123203 (Boulder).

The background x-ray flux is at the class B8 level.

At the time of counting spots (see image time), spots were observed in 16 active regions using 2K resolution (SN: 324) and 14 active regions using 1K resolution (SN: 215) SDO images on the visible solar disk.

Region 12321 [N12W52] decayed quickly and was quiet.
Region 12324 [N19W18] was quiet and stable.
Region 12325 [N04W11] was mostly unchanged and quiet.
Region 12326 [N15W36] was quiet and stable.
Region 12327 [S09E30] was quiet and stable.
Region 12329 [S07W62] gained spots and was quiet.
New region 12330 [N16E32] emerged on April 19 and was numbered by SWPC the next day as the region began to decay.

Spotted regions not numbered (or interpreted differently) by SWPC:
S4367 [N08W43] decayed slowly and quietly.
S4383 [S12E12] was quiet and stable.
S4389 [S22E38] was quiet and stable.
S4390 [S10E23] reemerged with several penumbra spots.
S4392 [N11W72] developed relatively quickly as new flux emerged and became a compact region with a small magnetic delta. A minor M class flare is possible.
S4394 [S10W09] decayed slowly and quietly.
S4398 [N08E22] decayed slowly and quietly.
New region S4400 [N09E38] emerged with a penumbra spot.
New region S4401 [N20W40] emerged with a few penumbra spots.

C2+ flares:

Magnitude Peak time (UTC) Location AR Recorded by Comment
C2.4 (LDE) 21:16 NE limb   GOES15 attributed to AR 12321 by SWPC

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

Coronal mass ejections (CMEs)

April 18-20: 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 southern hemisphere coronal hole (CH664) rotated across the central meridian on April 16-18.

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 21-23 with a chance of active intervals on April 21 due to effects from CH664.

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
12322 2015.04.10
2015.04.11
3     N11W71 0030 CRO       spotless

location: N13W79

SWPC has moved AR 12322 to the location of AR S4392

12321 2015.04.10
2015.04.11
9 8 2 N10W49 0080 CSO BXO area: 0020

location: N12W52

S4367 2015.04.11   10 1 N08W43 0070   CAO  
12326 2015.04.11
2015.04.16
1 4 3 N15W41 0010 AXX BXO location: N15W36
12324 2015.04.13
2015.04.14
9 25 18 N19W18 0230 DKI CAI  
S4372 2015.04.13       S18W51            
12325 2015.04.13
2015.04.14
8 22 11 N05W09 0220 CKO DKO area: 0360

location: N04W11

S4375 2015.04.13       N10W56            
S4380 2015.04.15       S13W27          
S4381 2015.04.15       N18W36            
S4383 2015.04.16   13 6 S12E12 0035   BXO  
12327 2015.04.16
2015.04.17
4 15 4 S09E30 0110 CSO CSO  
S4385 2015.04.16       S18W45          
S4388 2015.04.17        N17W57            
S4389 2015.04.17   4 1  S22E38 0008   BXO  
S4390 2015.04.17   7 4  S10E23 0025   BXO    
12329 2015.04.17
2015.04.19
8 26 10  S08W62 0030 CRO DRI  
S4392 2015.04.17   13 9  N11W72 0170   DAC beta-gamma-delta
S4394 2015.04.18   2    S10W09 0012   AXX  
S4395 2015.04.18        S15W50            
12330 2015.04.19
2015.04.20
3 9 5  N15E32 0030 DSO BXO  
S4398 2015.04.19   1    N08E22 0003   AXX  
S4400 2015.04.20   1 1  N09E38 0003   AXX    
S4401 2015.04.20   3 2  N20W40 0008   BXO    
Total spot count: 45 164 75  
Sunspot number: 125 324 215  (total spot count + 10 * number of spotted regions)
Weighted SN: 86 197 108  (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): 75 113 118 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 (131.0)   47.9 (2A) / 71.9 (2B) / 82.8 (2C) (53.4 projected, -2.7) (11.9)

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.