Last major update issued on April 21, 2012 at 05:55 UTC.
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[Solar wind and electron fluence charts (updated daily)
[Solar cycles 21-24 (last update April 1, 2012)]
[Solar cycles 1-20]
[Graphical comparison of cycles 21, 22, 23 and 24 (last update April 1, 2012)]
[Graphical comparison of cycles 10, 12, 13, 14, 16 and 24 (last update April 1, 2012)]
[Historical solar and geomagnetic data charts 1954-2006 (last update April 5, 2007)]
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[POES auroral activity level since October
2009 - updated April 18, 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]
The geomagnetic field was quiet to active on April 20. Solar wind speed at SOHO ranged between 299 and 364 km/s. A weak disturbance arrived at ACE near 03h UTC and may have been associated with a CME observed on April 16.
Solar flux measured at 20h UTC on 2.8 GHz was 141.7 (increasing 39.0 over the last solar rotation). The Potsdam WDC planetary A index was 10 (STAR Ap - based on the mean of three hour interval ap indices: 9.8). Three hour interval K indices: 14422111 (planetary), 13322311 (Boulder).
The background x-ray flux is at the class B6 level.
At midnight UTC the visible solar disk had 11 spotted active regions (in 2K resolution SDO images).
Region 11459 [S16E02] has many small spots and is becoming
magnetically more complex. The region has minor polarity intermixing and could
produce C and minor M class flares.
Region 11460 [N15W13] added penumbral area and has minor polarity intermixing. M flares are possible.
Region 11461 [N12E26] lost penumbral area and was quiet.
Region 11462 [S25W46] has two large penumbrae with little significant magnetic complexity.
Region 11463 [S27W67] decayed further and was quiet.
Region 11464 [N23E02] decayed slowly and quietly.
New region 11465 [S17E41] emerged in the southeast quadrant on April 19 and developed very quickly on April 20 when it was numbered by SWPC. M flares are possible. The region was the source of most of the day's low level C flares.
Spotted active regions not numbered by NOAA/SWPC:
S1598 [N11E27] added a few spots and was quiet.
S1599 [S26W06] reemerged with several spots.
New region S1604 [N10E66] emerged near the northeast limb.
New region S1605 [S11E06] emerged to the north of AR 11459.
April 19-20: No obviously Earth directed CMEs were observed in LASCO and
April 18: A small CME associated with a C8 event in region 11463 could have had an Earth directed component.
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 (CH514) in the northern hemisphere will likely rotate into an Earth facing position on April 21.
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.
Long distance low and medium frequency (below 2 MHz) propagation along paths north of due west over high and upper middle latitudes is poor to fair. Propagation on long distance northeast-southwest paths is poor.
The geomagnetic field is expected to be quiet to active on April 21-22 due to CME effects and quiet to unsettled on April 23.
|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: 0-20% probability, Yellow: 20-60% probability, Red: 60-100% probability.
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.
|Active region||Date numbered
|Spot count||Location at midnight||Area||Classification||SDO / HMI 4K continuum
image with magnetic polarity overlay
|Total spot count:||92||180||78|
|Sunspot number:||162||290||178||(total spot count + 10 * number of spotted regions)|
|Weighted penumbral SN:||127||218||116||(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):||97||102||98||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|
|Month||Average measured solar flux||International sunspot number (SIDC)||Smoothed sunspot number||Average ap
|2008.07||65.7 (SF minimum)||0.5||2.8 (-0.4)|
|2011.10||137.3||88.0||(60.1 projected, +0.6)||8.28|
|2011.11||153.5||96.7||(61.6 projected, +1.5)||5.55|
|2011.12||141.3||73.0||(64.3 projected, +2.7)||3.78|
|2012.01||132.5||58.3||(67.8 projected, +3.5)||7.15|
|2012.02||106.5||33.1||(71.8 projected, +4.0)||8.81|
|2012.03||114.7||64.2||(73.9 projected, +2.1)||16.08|
|2012.04||105.1 (1)||41.4 (2A) / 62.1 (2B)||(74.9 projected, +1.0)||(11.56)|
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 SIDC international sunspot number is typically 30-50% lower. 2B) Month average to date.
3) Running average based on the quicklook Potsdam WDC ap indices. Values in red are based on the definitive international Potsdam WDC 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.