Last major update issued on March 8, 2015 at 05:20 UT.
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The geomagnetic field was unsettled to active on March 7. Solar wind speed at SOHO ranged between 452 and 563 km/s under the influence of a high speed stream from CH657.
Solar flux at 20h UTC on 2.8 GHz was 137.8 (decreasing 15.0 over the last solar rotation). The 90 day 10.7 flux at 1 AU was 138.1. The Potsdam WDC planetary A index was 21 (STAR Ap - based on the mean of three hour interval ap indices: 21.4). Three hour interval K indices: 44433434 (planetary), 34333422 (Boulder).
The background x-ray flux is at the class C1 level.
At the time of counting spots (see image time), spots were observed in 7 active regions using 2K resolution (SN: 119) and 5 active regions using 1K resolution (SN: 72) SDO images on the visible solar disk.
Region 12296 [S11E12] decayed slowly and quietly.
Region 12297 [S16E68] is a complex region with a small magnetic delta in an intermediate northern penumbra. Further major flares are possible.
Spotted regions not numbered (or interpreted
differently) by SWPC:
S4256 [S13W33] was quiet and stable.
S4262 [N17W02] reemerged with penumbra spots.
S4263 [S22W70] decayed slowly and quietly.
S4270 [S26E19] was quiet and stable.
New region S4271 [S01W02] was observed with a penumbra spot.
C2+ flares (GOES):
|Magnitude||Peak time (UTC)||Location||AR||Comment|
|C3.6||14:41||12297||see SDO/EVE/ESP plot, XRS-B proxy|
March 5: No obviously Earth directed CMEs were observed in LASCO
March 6: A partial halo CME was observed after the M3 event in AR 12297.
March 7: A fast partial halo CME was associated with the M9 event in AR 12297.
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 (CH657) was in an Earth facing position on March 3-5. Another recurrent coronal hole (CH658) will likely rotate across the central meridian on March 9.
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.
The geomagnetic field is expected to be quiet to unsettled with occasional active intervals on March 8-10 due to effects from CH657. While the core of the CME observed on March 7 will not reach Earth, there is a chance that weak extensions of the CME could cause unsettled and active intervals on March 10-11.
|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.
(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
|Spot count||Location at midnight||Area||Classification||SDO / HMI 4K continuum
image with magnetic polarity overlay
|Total spot count:||10||49||22|
|Sunspot number:||20||119||72||(total spot count + 10 * number of spotted regions)|
|Weighted SN:||15||59||32||(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):||12||42||40||k * (sunspot number). k = 0.6 for SWPC, k = 0.35 for MSN 2K, k = 0.55 for MSN 1K (MSN=Magnetic Sunspot Number)|
|Month||Average solar flux||International sunspot number
|Smoothed sunspot number||Average
|166.3||102.3 (cycle peak)||78.4 (+1.1)||10.70|
(likely solar max)
|2014.09||146.6||148.1||87.6||(71.6 projected, -4.0)||9.78|
|2014.10||153.4||152.9||60.6||(69.2 projected, -2.4)||8.96|
|2014.11||154.8||151.4||70.1||(67.4 projected, -1.8)||9.33|
|2014.12||158.7||153.8||78.0||(66.3 projected, -1.1)||11.24|
|2015.01||141.9||137.3||67.0||(65.1 projected, -1.2)||9.46|
|2015.02||129.1||126.0||44.8||(63.6 projected, -1.5)||9.92|
|2015.03||(128.4)||9.7 (2A) / 42.9 (2B) / 59.1 (2C)||(61.6 projected, -2.0)||(15.2)|
1) Running average based on the daily 20:00 UTC observed solar flux value at
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.