Last major update issued on May 31, 2014 at 05:30 UTC.
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The geomagnetic field was quiet to active on May 30. Solar wind speed at SOHO ranged between 297 and 356 km/s. A weak disturbance began after 10h UT.
Solar flux at 20h UTC on 2.8 GHz was 101.6 (decreasing 31.0 over the last solar rotation). The 90 day 10.7 flux at 1 AU was 142.2. The Potsdam WDC planetary A index was 8 (STAR Ap - based on the mean of three hour interval ap indices: 8.0). Three hour interval K indices: 01122241 (planetary), 12322332 (Boulder).
The background x-ray flux is at the class B2 level.
At the time of counting spots (see image time), spots were observed in 8 active regions using 2K resolution (SN: 117) and 6 active regions using 1K resolution (SN: 77) SDO images on the visible solar disk.
Region 12073 [S11W50] decayed slowly and quietly.
Region 12075 [S08W13] decayed as the single penumbra fragmented into several penumbrae.
Region 12076 [S18W43] decayed slowly and quietly.
New region 12077 [S04E76] rotated into view.
Spotted regions not numbered (or interpreted differently) by SWPC:
S3477 [N19W03] was quiet and stable.
S3483 [S15E16] decayed slowly and quietly.
S3486 [S17W52] decayed slowly and quietly.
New region S3490 [S17E44] emerged with penumbra spots.
May 28-30: 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
A coronal hole (CH620) in the southern hemisphere could rotate into an Earth facing position on May 31 - June 1.
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 poor.
The geomagnetic field is expected to be mostly quiet on May 31 - June 2. On June 3-4 quiet to unsettled conditions are possible due to effects from CH620.
|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:||16||34||17|
|Sunspot number:||56||114||77||(total spot count + 10 * number of spotted regions)|
|Weighted SN:||29||50||33||(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):||34||40||42||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
|2013.11||148.3||145.1||77.6||(75.6 projected, +0.6)||5.68|
|2013.12||147.7||143.1||90.3||(76.6 projected, +1.0)||4.68|
|2014.01||157.4||152.4||82.0||(77.6 projected, +1.0)||5.44|
|166.3||102.8 (cycle peak)||(77.4 projected, -0.2)||10.70|
|2014.03||149.9||148.5||92.2||(77.9 projected, +0.5)||4.88|
|2014.04||143.9||144.8||84.7||(77.0 projected, -0.9)||7.88|
|2014.05||130.5 (1)||114.8 (2A) / 118.6 (2B) / 94.6 (2C)||(74.4 projected, -2.6)||(5.8)|
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.