|Charts (* = updated daily)||Data and archive|
|Solar wind (*)||Solar and geomagnetic data - last month (*)|
|Electron fluence (*)||Archived daily reports and monthly data from 2003.01 (February 1, 2016)|
|Solar cycle||Solar cycles 23-24 (February 1, 2016)||Historical solar and geomagnetic data charts 1954-2006 (April 5, 2007)|
|Cycle 24 progress (February 1, 2016)||Noon SDO sunspot count 1K Reference: 4K (large file) (*)|
|Solar cycles 1-24 (July 17, 2015)||POES auroral activity level October 2009 - December 2012|
|Comparison of cycles 21, 22, 23 and 24 (February 1, 2016)||3rd SSN Workshop, Tucson, 2013|
|Comparison of cycles 12, 13, 14, 16 and 24 (February 1, 2016)||4th SSN Workshop, Locarno, 2014|
|Solar polar fields vs. solar cycles (January 29, 2016)|
The geomagnetic field was quiet to unsettled on February 19 under the decreasig influence of a high speed stream from CH715. Solar wind speed at SOHO ranged between 436 and 559 km/s.
Solar flux at 20h UTC on 2.8 GHz was 94.0 (decreasing 4.9 over the last solar rotation). The 90 day 10.7 flux at 1 AU was 104.9. The Potsdam WDC planetary A index was 14 (STAR Ap - based on the mean of three hour interval ap indices: 14.0). Three hour interval K indices: 33233332 (planetary), 24333322 (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 11 active regions using 2K resolution (SN: 178) and 7 active regions using 1K resolution (SN: 98) SDO images on the visible solar disk.
Region 12501 [N04E10] was quiet and stable.
Region 12502 [N08W42] decayed slowly and quietly.
Region 12503 [N05W30] decayed and lost the trailing spots. Unfortunately SWPC lost track of this region and appears to be counting the spots belonging to another region further northeast.
New region 12504 [N13W02] emerged on February 18 and was numbered by SWPC the next day.
Spotted regions not numbered (or interpreted differently) by SWPC:
S5109 [S02W10] decayed slowly and quietly.
S5111 [S20E05] was quiet and stable.
S5113 [N08W18] developed further and was mostly quiet. C flares are likely.
S5116 [N08W11] decayed slowly and quietly.
New region S5121 [N10E77] rotated into view with a tiny spot.
New region S5122 [S08W36] emerged with a tiny spot.
New region S5123 [S18W50] emerged with tiny spots.
|Magnitude||Peak time (UT)||Location||AR||Recorded by||Comment|
February 17-19: No obviously Earth directed CMEs were observed in available LASCO imagery.
history (since October 2002)]
[Compare today's report to the situation one solar rotation ago: 28 days ago 27 days ago 26 days ago]
The southern parts of a large, recurrent northern hemisphere coronal hole (CH716) could rotate into an Earth facing position on February 20-22. CH716 was too far to the north to cause a disturbance during the previous rotation.
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 on February 20 and quiet on February 21-22. A high speed stream from CH716 could cause unsettled to active conditions on February 23-25.
|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). 4K 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 overlays
difficult to make sense of SWPC data, there is no CRO region at N05W27,
they are probably counting the spots of AR S5113
|Total spot count:||12||68||28|
|Sunspot number:||42||178||98||(total spot count + 10 * number of spotted regions)|
|Weighted SN:||20||81||41||(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):||46||89||78||k * (sunspot number)
As of February 19, 2015: k = 1.1 for SWPC, k = 0.45 for MSN 2K, k = 0.80 for MSN 1K (MSN=Magnetic Sunspot Number)
|Month||Average solar flux||International sunspot number
|Smoothed sunspot number (4)||Average
|166.3||146.1 (cycle peak)||110.5 (+1.2)||10.70|
|2014.04||143.9||144.8||112.5||116.4 (+2.1) (solar max)||7.88|
|2015.08||105.4||108.0||64.6||(66.1 projected, -2.1)||14.58|
|2015.09||101.7||102.7||78.1||(66.1 projected, +0.0)||15.78|
|2015.10||104.1||103.3||61.7||(65.7 projected, -0.4)||14.02|
|2015.11||109.3||106.9||63.2||(63.6 projected, -2.1)||12.09|
|2015.12||113.1||109.5||57.7||(61.9 projected, -1.7)||14.29|
|2016.01||103.4||100.1||56.6||(60.2 projected, -1.7)||9.4|
|2016.02||(109.5)||43.2 (2A) / 66.0 (2B) / 89.0 (2C)||(57.8 projected, -2.4)||(12.0)|
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).
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.
4) Updated to new data set from WDC-SILSO on July 1, 2015
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 Universal Time. Comments and suggestions are always welcome.
SDO images are courtesy of NASA/SDO and the AIA, EVE, and HMI science teams.