|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 12. Solar wind speed at SOHO ranged between 301 and 382 km/s. The total field of the IMF was at a high level, however, Bz was predominantly northwards resulting in only a mildly disturbed geomagnetic field. Bz at ACE swung moderately southwards after 04:30 UT on February 13, this could cause active and minor storm intervals.
Solar flux at 20h UTC on 2.8 GHz was 112.2 (increasing 12.3 over the last solar rotation). The 90 day 10.7 flux at 1 AU was 105.4. The Potsdam WDC planetary A index was 11 (STAR Ap - based on the mean of three hour interval ap indices: 10.8). Three hour interval K indices: 32233222 (planetary), 33233322 (Boulder).
The background x-ray flux is at the class B3 level.
At the time of counting spots (see image time), spots were observed in 9 active regions using 2K resolution (SN: 184) and 6 active regions using 1K resolution (SN: 102) SDO images on the visible solar disk.
Region 12496 [N08W36] was quiet and stable.
Region 12497 [N13W21] has multiple magnetic deltas in the largest penumbra. Further M class flares are possible.
Region 12498 [N18E17] was quiet and stable.
New region 12499 [N11E41] rotated into view on February 10 and was numbered by SWPC 2 days later as the region began to decay.
Spotted regions not numbered (or interpreted differently) by SWPC:
S5086 [S19W20] was quiet and stable.
S5091 [N14W80] decayed slowly and quietly.
S5100 [N05E65] was quiet and stable.
New region S5102 [N25E37] emerged with a tiny spot.
New region S5103 [S34W13] emerged with a tiny spot.
|Magnitude||Peak time (UT)||Location||AR||Recorded by||Comment|
February 10, 12: No obviously Earth directed CMEs were observed in
available LASCO imagery.
February 11: A halo CME was observed after the C8 LDE in AR 12497. The CME could reach Earth on February 14.
history (since October 2002)]
[Compare today's report to the situation one solar rotation ago: 28 days ago 27 days ago 26 days ago]
An extension (CH715) of the southern polar coronal hole will rotate across the central meridian on February 13-14.
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 quiet to active on February 13 with a chance of minor storm intervals. Quiet to major storm conditions are possible on February 14-15 due to effects from the February 11 CME. A high speed stream associated with CH715 could cause unsettled to minor storm conditions on February 16-17.
|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
SWPC has moved AR 12492 to the location of AR S5091
rotated out of view
|Total spot count:||24||94||42|
|Sunspot number:||74||184||102||(total spot count + 10 * number of spotted regions)|
|Relative sunspot number (Wolf number):||81||101||87||k * (sunspot number)
As of July 1, 2015: k = 1.1 for SWPC, k = 0.55 for MSN 2K, k = 0.85 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||100.2||56.6||(60.2 projected, -1.7)||10.0|
|2016.02||113.4||31.8 (2A) / 76.8 (2B) / 89.6 (2C)||(57.8 projected, -2.4)||(7.9)|
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.