|Charts (* = updated daily)||Data and archive|
|Solar wind (*)||Solar and geomagnetic data - last month (*)|
|Electron fluence (*)||Archived daily reports and monthly data since 2003.01 (December 4, 2016)|
|Solar cycle||Solar cycles 23-24 (December 1, 2016)||Historical solar and geomagnetic data charts 1954-2006 (April 5, 2007)|
|Cycle 24 progress (December 1, 2016)||Noon SDO sunspot count 1K / 4K (*)|
|Solar cycles 1-24 (July 17, 2015)||POES auroral activity level October 2009 - December 2012|
|Comparison of cycles 21, 22, 23 and 24 (December 1, 2016)||3rd SSN Workshop, Tucson, 2013|
|Comparison of cycles 12, 13, 14, 16 and 24 (December 1, 2016)||4th SSN Workshop, Locarno, 2014|
|Solar polar fields vs. solar cycles (December 4, 2016)|
The geomagnetic field was very quiet on December 3. Solar wind speed at SOHO ranged between 282 and 312 km/s.
Solar flux at 20h UTC on 2.8 GHz was 84.7 (increasing 8.5 over the last solar rotation). The average 90 day 10.7 flux at 1 AU was 83.0. The Potsdam WDC planetary A index was 2 (STAR Ap - based on the mean of three hour interval ap indices: 1.5). Three hour interval K indices: 00000010 (planetary), 01100110 (Boulder).
The background x-ray flux is at the class B1 level.
At the time of counting spots (see image time), spots were observed in 5 active regions using 2K resolution (SN: 76) and 4 active regions using 1K resolution (SN: 60) SDO images on the visible solar disk.
Region 12612 [N09W61] decayed slowly and quietly.
Region 12614 [N06W34] decayed and could soon become spotless.
Region 12615 [S06W06] developed slowly with a magnetic delta forming on the northern side of the main trailing penumbra. C and minor M class flares are possible.
Region 12616 [N17W27] decayed and could soon become spotless.
Spotted regions not numbered (or interpreted differently)
New region S5526 [S08W30] emerged with tiny spots.
|Magnitude||Peak time (UT)||Location||AR||Recorded by||Comment|
December 1-3: 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]
A recurrent small southern hemisphere coronal hole (CH776) was in an Earth facing position on December 1. CH776 didn't cause a geomagnetic disturbance during the previous solar rotation. A recurrent trans equatorial coronal hole (CH777) will likely rotate across the central meridian on December 5-8.
Long distance low and medium frequency (below 2 MHz) propagation along paths north of due west over upper middle latitudes is fair to good. Propagation on long distance northeast-southwest paths is poor.
The geomagnetic field is expected to be quiet on December 4-6. On December 4-5 there is a chance of unsettled intervals due to effects from CH776.
|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
area : 0003
|Total spot count:||22||26||20|
|Sunspot number:||62||76||60||(total spot count + 10 * number of spotted regions)|
|Weighted SN:||32||36||30||(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):||68||42||48||k * (sunspot number)
As of May 7, 2016: k = 1.1 for SWPC, k = 0.55 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|
|2016.06||81.9||84.5||20.9||(42.0 projected, -2.9)||8.44|
|2016.07||86.0||88.9||32.5||(39.1 projected, -2.9)||9.43|
|2016.08||85.0||87.1||50.7||(36.3 projected, -2.8)||9.61|
|2016.09||87.7||88.7||44.7||(33.6 projected, -2.7)||14.54|
|2016.10||86.1||85.6||33.6||(31.6 projected, -2.0)||15.33|
|2016.11||78.6||76.9||21.4||(29.8 projected, -1.8)||8.6|
|2016.12||(84.5)||5.5 (2A) / 56.7 (2B) / 30.8 (2C)||(28.3 projected, -1.5)||(2.2)|
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).
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.