Solar Terrestrial Activity Report

Activity chart

Last major update issued on May 6, 2015 at 05:05 UT

Charts (* = updated daily) Data and archive
  Solar wind (*) Solar and geomagnetic data - last month (*)
  Electron fluence (*) Archived daily reports and monthly data from 2003.01 (May 1, 2015)
Solar cycle Solar cycles 23-24 (May 1, 2015) Historical solar and geomagnetic data charts 1954-2006 (April 5, 2007)
  Cycle 24 progress (May 1, 2015) Noon SDO sunspot count 1K Reference: 4K (large file) (*)
  Solar cycles 1-20 POES auroral activity level October 2009 - December 2012
  Comparison of cycles 21, 22, 23 and 24 (May 1, 2015) 3rd SSN Workshop, Tucson, 2013
  Comparison of cycles 10, 12, 13, 14, 16 and 24 (May 1, 2015) 4th SSN Workshop, Locarno, 2014
  Solar polar fields vs solar cycles (April 10, 2015)  

Recent activity

The geomagnetic field was quiet on May 5. Solar wind speed at SOHO ranged between 344 and 426 km/s. A solar wind shock was observed at SOHO at 00:50 UT on May 6, the arrival of the CME observed on May 2/3.

Solar flux at 20h UTC on 2.8 GHz was 127.8 (increasing 21.8 over the last solar rotation). The 90 day 10.7 flux at 1 AU was 125.4. The Potsdam WDC planetary A index was 5 (STAR Ap - based on the mean of three hour interval ap indices: 4.9). Three hour interval K indices: 11122112 (planetary), *****214 (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 11 active regions using 2K resolution (SN: 249) and 7 active regions using 1K resolution (SN: 148) SDO images on the visible solar disk.

Region 12335 [S16E10] still has a weak magnetic delta centrally and could produce a minor M class flare.
Region 12336 [N13W14] decayed slowly and quietly.
Region 12337 [S17E29] was quiet and stable.
Region 12338 [N04E30] developed further and could produce C flares.
New region 12339 [N12E75] rotated fully into view revealing a complex and compact region with major flare potential.

Spotted regions not numbered (or interpreted differently) by SWPC:
S4426 [S12W18] decayed slowly and quietly.
S4439 [N12E49] decayed slowly and quietly.
S4442 [S28E22] was quiet and stable.
New region S4444 [S02E48] emerged with a penumbra spot.
New region S4445 [S04E22] emerged with a penumbra spot.
New region S4446 [S05W67] emerged with a penumbra spot.

C2+ flares:

Magnitude Peak time (UTC) Location AR Recorded by Comment
C2.1 02:33 S18E25 12335 GOES15  
C2.5 03:03   12339 GOES15  
C5.1 04:03 N09E77 12339 GOES15 attributed to AR 12338 by SWPC
C2.6 04:47   12339 GOES15  
C2.6 05:02   12339 GOES15  
C2.6 07:11 S18E21 12335 GOES15  
C4.3 08:02   12339 GOES15  
C3.7 08:37   12339 GOES15  
C2.9 08:58   12339 SDO/EVE  
C3.7 09:20   12339 GOES15  
M1.9 09:47   12339 GOES15  
M1.0 09:59   12339 SDO/EVE  
C6.6 11:29   12335 GOES15  
C3.6 11:58   12335 GOES15  
C2.5 13:24   12335 SDO/EVE  
M1.2/1N 13:53 N15E75 12339 GOES15  
M1.3 14:25   12335 GOES15  
C2.7 15:20   12335 SDO/EVE  
C3.0 15:42   12335 SDO/EVE  
C2.5 17:07   12335 SDO/EVE C1.9/2N @ GOES15
M2.6 17:24   12335 GOES15  
C3.8 17:58   12339 SDO/EVE  
C2.2 20:54   12335 SDO/EVE  
C2.5 21:43   12339 GOES15  
X2.7 22:11   12339 GOES15 CME

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

Coronal mass ejections (CMEs)

May 3-5: 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 trans equatorial coronal hole (CH666) was in a potentially geoeffective position on May 2. CH666 has decayed and may not be capable of creating a geomagnetic disturbance. A recurrent extension (CH667) of the southern polar coronal hole could rotate across the central meridian on May 8-9.

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 unsettled to active with a chance of minor storm intervals on May 6 due to CME effects. Quiet to unsettled is likely on May 7-8.

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 overlays
Comment
SWPC Magnetic
(SDO)
SWPC STAR Current Previous
2K 1K
12334 2015.04.27
2015.04.30
      S20W59            
S4421 2015.04.27       S10W57            
12335 2015.04.30 25 53 34 S16E11 0280 EKC EAC beta-gamma-delta

area: 0450

S4426 2015.04.30   5 2 S12W18 0010   BXO  
S4428 2015.04.30       N13W42            
S4429 2015.05.01       S27W16          
S4432 2015.05.02       S10W48          
12338 2015.05.02
2015.05.03
7 17 9 N03E29 0070 DSO DAO area: 0160
12336 2015.05.02
2015.05.03
10 19 9 N13W14 0040 DSO DRI  
12337 2015.05.02
2015.05.03
2 11 6 S17E28 0010 BXO CRI area: 0020
S4437 2015.05.02       N10W42            
S4438 2015.05.03       N05E40            
S4439 2015.05.03   2 1 N12E49 0004   BXO  
12339 2015.05.03
2015.05.04
5 27 17 N12E70 0250 EKC EKC area: 0700

location: N12E75

S4441 2015.05.04       N13E22          
S4442 2015.05.04   1   S27E23 0002   AXX  
S4443 2015.05.04       S03W43          
S4444 2015.05.05   2   S02E48 0003   BXO    
S4445 2015.05.05   1   S04E22 0003   AXX    
S4446 2015.05.05   1   S05W67 0003   AXX    
Total spot count: 49 139 78  
Sunspot number: 99 249 148  (total spot count + 10 * number of spotted regions)
Weighted SN: 79 165 104  (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): 59 87 81 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
2013.12 147.7 143.1 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) (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 78.5 (-1.2) 4.50
2014.08 124.7 127.9 74.7 75.5 (-3.0) 7.71
2014.09 146.6 148.1 87.6 70.8 (-4.7) 9.78
2014.10 153.4 152.9 60.6 67.3 (-3.5) 8.96
2014.11 154.8 151.4 70.1 (64.9 projected, -2.4) 9.33
2014.12 158.7 153.8 78.0 (62.6 projected, -2.3) 11.24
2015.01 141.9 137.3 67.0 (60.4 projected, -2.2) 9.46
2015.02 129.1 126.0 44.8 (58.7 projected, -1.7) 9.92
2015.03 125.9 124.6 38.4 (56.3 projected, -2.4) 16.14
2015.04 128.8 129.7 54.4 (53.7 projected, -2.6) 10.3
2015.05 (113.6)    9.3 (2A) / 57.8 (2B) / 79.0 (2C) (51.5 projected, -2.2) (5.5)

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.