Solar Terrestrial Activity Report

Activity chart

Last major update issued on March 9, 2014 at 07:45 UTC.

[Solar and geomagnetic data - last month (updated daily)]
[Solar wind and electron fluence charts (updated daily)]
[Solar cycles 23-24 (last update March 1, 2014)] [Cycle 24 progress (last update March 1, 2014) ]
[Solar cycles 1-20]
[Graphical comparison of cycles 21, 22, 23 and 24 (last update March 1, 2014)]
[Graphical comparison of cycles 10, 12, 13, 14, 16 and 24 (last update March 1, 2014)]
[Historical solar and geomagnetic data charts 1954-2006 (last update April 5, 2007)]
[Archived reports since January 2003 (last update March 1, 2014)]

[POES auroral activity level since October 2009 - updated January 26, 2013]
[Solar polar fields vs solar cycles - updated February 23, 2014]
[Presentation 3rd SSN Workshop, Tucson, 2013 (pdf)]

Recent activity

The geomagnetic field was very quiet on March 8. Solar wind speed at SOHO ranged between 335 and 406 km/s.

Solar flux at 20h UTC on 2.8 GHz was 141.6 (decreasing 27.4 over the last solar rotation). The 90 day 10.7 flux at 1 AU was 154.5. The Potsdam WDC planetary A index was 3 (STAR Ap - based on the mean of three hour interval ap indices: 2.6). Three hour interval K indices: 10110001 (planetary), 10122211 (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 12 active regions in 2K resolution (SN: 247) and 10 active regions in 1K resolution (SN: 173) SDO images on the visible solar disk.

Region 11990 [S12W80] decayed slowly and quietly as it rotated to the southwest limb.
Region 11991 [S26W57] was mostly quiet and decayed quickly with only small trailing polarity spots remaining.
Region 11996 [N14W23] has polarity intermixing and could produce occasional C class flares.
Region 11998 [S10E28] was quiet and stable.
Region 11999 [S16W18] decayed and could soon become spotless.
Region 12000 [S11E14] decayed slowly and quietly.
Region 12001 [N19W65] gained spots and was quiet.
New region 12002 [S18E65] rotated into view on March 7 and was numbered by SWPC the next day. The region developed but has only small spots.
C5+ flare: M1.4 at 23:47 UTC.

Spotted regions not numbered (or interpreted differently) by SWPC:
S3197 [N09W07] was quiet and stable.
New region S3202 [N26W07] emerged and has umbra on one spot.
New region S3203 [N01W22] emerged with a penumbra spot.
New region S3204 [S01E43] emerged with a penumbra spot and has the polarity layout of a northern hemisphere group.

Coronal mass ejections (CMEs)

March 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 northern hemisphere coronal hole (CH606) may have been in an Earth facing position on March 5-6, the coronal hole could be too far to the north to become geoeffective. A small southern hemisphere coronal hole (CH607) will likely rotate into an Earth facing position on March 9.

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

Forecast

The geomagnetic field is expected to be quiet on March 9-11. On March 12-13 there is a chance of a few unsettled intervals due to effects from CH607.

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: 0-20% probability, Yellow: 20-60% probability, Red: 60-100% 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
11990 2014.02.24 2 2 1 S12W82 0110 HSX HSX

area: 0170

location: S12W80

11991 2014.02.25
2014.02.26
5 5 3 S26W61 0040 CAO HRX

location: S26W57

area: 0025

11993 2014.02.25
2014.02.26
      N17W75         plage
11995 2014.02.28 2     S16W89 0030 CAO     rotated out of view
S3173 2014.02.28       N15W58           plage
11996 2014.03.01
2014.03.02
16 39 21 N15W23 0080 DAI DRI

beta-gamma

location: N14W23

area: 0120

S3176 2014.03.02       N09W07           plage
S3177 2014.03.02       N21W55           plage
S3182 2014.03.02       S12W37           plage
S3185 2014.03.03       N14W50           plage
S3186 2014.03.03       N08W38           plage
11999 2014.03.04
2014.03.05
2 3 2 S16W19 0010 BXO BXO  
11998 2014.03.04
2014.03.05
5 27 17 S09E27 0080 CAO CAO location: S10E28

area: 0150

S3190 2014.03.04       S06W14           plage
S3191 2014.03.04       S24W30           plage
12000 2014.03.05
2014.03.06
7 13 8 S11E13 0040 CAO CRI area: 0070
S3194 2014.03.05       N16E01           plage
12001 2014.03.05
2014.03.06
4 14 8 N19W65 0050 CAO CRI beta-gamma
S3196 2014.03.07       N10E05         plage
S3197 2014.03.07   4 2 N09W07 0018   AXX  
S3198 2014.03.07       S20W27         plage
S3199 2014.03.07       S27E05         plage
12002 2014.03.07
2014.03.08
5 16 9 S19E64 0050 CAO DRI beta-gamma

area: 0090

S3202 2014.03.08   2 2 N26W07 0010   CRO    
S3203 2014.03.08   1   N01W22 0002   AXX    
S3204 2014.03.08   1   S01E43 0003   AXX    
Total spot count: 48 127 73  
Sunspot number: 138 247 173  (total spot count + 10 * number of spotted regions)
Weighted SN: 88 155 101  (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): 83 86 95 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
2012.11 121.3 118.3 61.8 59.7 (+1.1) 7.08
2012.12 108.6 105.0 40.8 59.6 (-0.1) 3.44
2013.01 127.1 123.1 62.9 58.7 (-0.9) 4.69
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 (72.8 projected, +3.8) 5.23
2013.10  132.1 131.2 85.6 (73.8 projected, +1.0) 7.71
2013.11  148.3 145.1 77.6 (72.7 projected, -1.1) 5.68
2013.12 147.7 143.1 90.3 (71.6 projected, -1.1) 4.68
2014.01 157.4 152.4 82.0 (71.6 projected, 0.0) 5.44
2014.02 170.3
(cycle peak)
166.3 102.8 (cycle peak) (70.9 projected, -0.7) 10.70
2014.03 154.1 (1)   43.5 (2A) / 168.4 (2B) / 123.2 (2C) (71.0 projected, +0.1) (4.2)

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.