Last major update issued on April 14, 2014 at 05:45 UTC.
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The geomagnetic field was quiet to unsettled on April 13. Solar wind speed at SOHO ranged between 324 and 410 km/s.
Solar flux at 20h UTC on 2.8 GHz was 137.1 (increasing 0.7 over the last solar rotation). The 90 day 10.7 flux at 1 AU was 150.6. The Potsdam WDC planetary A index was 12 (STAR Ap - based on the mean of three hour interval ap indices: 11.6). Three hour interval K indices: 33331232 (planetary), 33332232 (Boulder).
The background x-ray flux is at the class B5 level.
At the time of counting spots (see image time), spots were observed in 12 active regions in 2K resolution (SN: 248) and 7 active regions in 1K resolution (SN: 130) SDO images on the visible solar disk.
Region 12032 [N11W02] decayed slowly and quietly.
Region 12033 [N11E09] was quiet and stable.
Region 12034 [N04E27] was quiet and stable.
Region 12035 [S17E50] gained spots and penumbral area. A minor M class flare is possible.
New region 12036 [S18E26] emerged on April 12 and developed further on April 13. C and M class flaring is possible. The region was the source of a C7.5 flare at 04:38 UTC. This flare was superimposed on a long duration C4 event from a region at the southeast limb.
New region 12037 [S09E30] emerged on April 12 and developed on April 13. C flares are possible.
Spotted regions not numbered (or interpreted differently) by SWPC:
S3309 [S25W33] was quiet and stable.
S3311 [S10W14] reemerged with penumbra spots.
New region S3317 [S09E76] rotated into view with penumbra spots.
New region S3318 [N15E49] was observed with a penumbra spot.
New region S3319 [N25W14] emerged with penumbra spots.
New region S3320 [N16W09] emerged with a penumbra spot.
April 11-13: No obviously Earth directed CMEs were observed in LASCO and STEREO imagery.
Coronal hole history (since October
Compare today's report to the situation one solar rotation ago: 28 days ago 27 days ago 26 days ago
No obvious coronal holes are currently in or near Earth facing positions.
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 to good.
The geomagnetic field is expected to be quiet on April 14-16.
|Coronal holes (1)||Coronal mass ejection (2)||M and X class flares (3)|
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.
|Active region||Date numbered
|Spot count||Location at midnight||Area||Classification||SDO / HMI 4K continuum
image with magnetic polarity overlay
|Total spot count:||35||128||60|
|Sunspot number:||95||248||130||(total spot count + 10 * number of spotted regions)|
|Weighted SN:||63||156||88||(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):||57||87||72||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 ap
|2013.10||132.1||131.2||85.6||(74.9 projected, +1.8)||7.71|
|2013.11||148.3||145.1||77.6||(74.9 projected, -0.0)||5.68|
|2013.12||147.7||143.1||90.3||(74.4 projected, -0.5)||4.68|
|2014.01||157.4||152.4||82.0||(74.3 projected, -0.1)||5.44|
|166.3||102.8 (cycle peak)||(73.7 projected, -0.6)||10.70|
|2014.03||149.9||148.5||92.2||(73.8 projected, +0.1)||4.88|
|2014.04||142.4 (1)||49.0 (2A) / 113.1 (2B) / 103.7 (2C)||(73.0 projected, -0.8)||(7.2)|
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.