Solar Terrestrial Activity Report

Activity chart

Last major update issued on March 11, 2012 at 06:30 UTC.

[Solar and geomagnetic data - last month (updated daily)]
[Solar wind and electron fluence charts (updated daily)
[Solar cycles 21-24 (last update March 2, 2012)]
[Solar cycles 1-20]
[Graphical comparison of cycles 21, 22, 23 and 24 (last update March 2, 2012)]
[Graphical comparison of cycles 10, 12, 13, 14, 16 and 24 (last update March 2, 2012)]
[Historical solar and geomagnetic data charts 1954-2006 (last update April 5, 2007)]
[Archived reports since January 2003 (last update March 1, 2012)]

[POES auroral activity level since October 2009 - updated March 5, 2012]
Annotated geomagnetic activity charts - Carrington rotation 2118 [December 2011 - January 2012] - 2119 [January-February 2012]
[Solar polar fields vs solar cycles - updated June 27, 2011]

Recent activity

The geomagnetic field was quiet to active on March 10. Solar wind speed at SOHO ranged between 450 and 620 km/s under the decreasing influence of a CME.

Solar flux measured at 17h UTC on 2.8 GHz was 140.6 (increasing 30.2 over the last solar rotation, the observation at 20h UTC was flare enhanced). The planetary A index was 18 (STAR Ap - based on the mean of three hour interval ap indices: 17.9). Three hour interval K indices: 44332342 (planetary), 55333332 (Boulder).

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

At midnight UTC the visible solar disk had 9 spotted active regions (in 2K resolution SDO images).

Region 11428 [S16W45] decayed quickly and lost all penumbra on the trailing spots. Flare: C1.9 at 07:02 UTC
Region 11429 [N18W23] decayed in the central and trailing spot sections, however, the leading positive and negative polarity spots merged again forming a significant magnetic delta structure. Further major flares are possible. Flares: C3.5 at 02:39, C1.9 at 07:46, major M8.4 long duration event peaking at 17:44 UTC. The latter event may have been triggered by an event in region 11430. An impressive and fast CME was observed.
Region 11430 [N20W41] decayed slowly. Flare: C8.0 long duration event peaking at 15:52 UTC. A small CME was observed after this event.
Region 11432 [N15E54] decayed a little as the magnetic delta structure disappeared. Flares: C3.8 at 01:19, C1.2 at 13:26 UTC.

Spotted regions not reported by NOAA/SWPC:
[S1505] reemerged on March 9. Location at midnight: S25W56
[S1512] reemerged on March 10. Location at midnight: S23W04
[S1517] emerged in the southeast quadrant on March 9. Location at midnight: S23E10
[S1522] emerged near the southeast limb on March 10. Location at midnight: S22E70
[S1523] rotated into view at the northeast limb on March 10. Location at midnight: N11E77

Coronal mass ejections (CMEs)

March 8: No obviously Earth directed CMEs were observed in LASCO and STEREO imagery.
March 9: The M6 event in region 11429 produced a full halo CME. This CME could reach Earth before noon on March 11.
March 10: The M8 event in region 11429 was associated with an inpressive halo CME which is likely to reach Earth early on March 12.

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 large recurrent trans equatorial coronal hole (CH507) will likely rotate in an Earth facing position on March 13-14.

The above coronal hole map is based on a method where coronal holes are detected automatically. While the method may need some fine tuning, it has significant advantages over detecting coronal holes manually. The main improvement is the ability to detect coronal holes at and just beyond the solar limbs. Early results using this method for SDO images over a span of several weeks indicate a good match between coronal holes observed over the visible disk and their extent and position at the east and west limbs. Note that the polar coronal holes are easily detected using this method, the extent and intensity of both CHs are consistent with other data sources.

Propagation

Long distance low and medium frequency (below 2 MHz) propagation along paths north of due west over high and upper middle latitudes is very poor. Propagation on long distance northeast-southwest paths is poor to fair.

Forecast

The geomagnetic field is expected to be quiet to major storm on March 11 due to CME effects. Unsettled to severe storm is likely on March 12 due to another CME. On March 13 quiet to minor storm conditions is likely.

Coronal holes (1) Coronal mass ejections (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 higher resolution image) Compare to the previous day's image

When available the active region map has a coronal hole polarity overlay where red (pink) is negative and blue (blue-green) 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 STAR SDO SWPC STAR Current Previous
2K 1K
S1505 2012.03.02   2   S25W56 0000   BXO  
11428 2012.03.02
2012.03.03
14 12 8 S17W46 0060 CRO CAO

 

11429 2012.03.02
2012.03.03
22 60 22 N18W26 0880 EKC EKC beta-gamma-delta

location: N18W23

reversed polarities

11430 2012.03.04 9 19 8 N21W42 0100 CAO CAI  
S1512 2012.03.05   2   S23W04 0000   AXX    
S1514 2012.03.07       N12W02           plage
11432 2012.03.08
2012.03.09
4 10 5 N15E52 0080 HSX DAO  
S1516 2012.03.08       N27W19           plage
S1517 2012.03.09   2   S23E10 0000   AXX  
S1520 2012.03.09       N27E09         plage
S1521 2012.03.09       S32W42         plage
S1522 2012.03.10   3 2 S22E70 0050   DRO    
S1523 2012.03.10   2 2 N11E77 0060   CSO    
Total spot count: 49 112 47  
Sunspot number: 89 202 107  (total spot count + 10 * number of spotted regions)
Weighted penumbral SN: 72 145 80  (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): 53 71 59 k * (sunspot number). k = 0.6 for SWPC, k = 0.35 (changed from 0.45 on March 1, 2011) for STAR SDO 2K, k = 0.55 for STAR SDO 1K

Monthly solar cycle data

Month Average measured solar flux International sunspot number (SIDC) Smoothed sunspot number Average ap
(3)
2008.07 65.7 (SF minimum) 0.5 2.8 (-0.4)  
2008.12 69.2 0.8 1.7 (-)
sunspot minimum
3.25
2010.12 84.2 14.4 28.8 (+2.3) 3.41 / 4.35
2011.01 83.6 19.1 31.0 (+2.2) 4.32 / 5.51
2011.02 94.6 29.4 33.4 (+2.4) 5.41 / 6.44
2011.03 115.0 56.2 36.9 (+3.5) 7.79 / 8.18
2011.04 112.6 54.4 41.8 (+4.9) 9.71 / 8.83
2011.05 95.8 41.6 47.6 (+5.8) 9.18 / 8.94
2011.06 95.8 37.0 53.2 (+5.6) 8.96 / 8.06
2011.07 94.2 43.9 57.2 (+4.0) 9.14 / 8.16
2011.08 101.7 50.6 59.0 (+1.8) 8.16 / 7.26
2011.09 133.8 78.0 (59.2 projected, +0.2) 12.80 / 12.27
2011.10 137.3 88.0 (59.4 projected, +0.2) 7.52 / 8.28
2011.11 153.5 96.7 (60.8 projected, +1.4) 4.58 / 5.55
2011.12 141.3 73.0 (63.6 projected, +2.8) 3.32
2012.01 132.5 58.3 (67.1 projected, +3.5) 6.59
2012.02 106.5 33.1 (71.0 projected, +3.9) 8.09
2012.03 127.4 (1) 24.4 (2A) / 75.7 (2B) (73.2 projected, +2.2) (26.91)

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 SIDC international sunspot number is typically 30-50% lower. 2B) Month average to date.
3) Running average based on the preliminary daily SWPC ap indices. Values in red are based on the official NGDC ap indices.

This report has been prepared by Jan Alvestad. It is based on 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.