|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 (July 2, 2016)|
|Solar cycle||Solar cycles 23-24 (July 1, 2016)||Historical solar and geomagnetic data charts 1954-2006 (April 5, 2007)|
|Cycle 24 progress (July 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 (July 1, 2016)||3rd SSN Workshop, Tucson, 2013|
|Comparison of cycles 12, 13, 14, 16 and 24 (July 1, 2016)||4th SSN Workshop, Locarno, 2014|
|Solar polar fields vs. solar cycles (July 9, 2016)|
The geomagnetic field was quiet to minor storm on July 19. Solar wind speed at SOHO ranged between 289 and 451 km/s. A fairly strong solar wind shock was observed at 23:09 UT at SOHO with a sudden jump in solar wind speed from 300 to 450 km/s. This was likely the earlier than expected arrival of the July 17 CME. The total field of the interplanetary magnetic field peaked near 35 nT, an unusually high value. Minor geomagnetic storming was recorded after the shock arrival.
Solar flux at 17h UTC on 2.8 GHz was 106.1 (increasing 27.8 over the last solar rotation. The value recorded at 20h UT was 5-6% lower than those at 17 and 23h and has therefore been marked as a possible bad measurement). The 90 day 10.7 flux at 1 AU was 90.0. The Potsdam WDC planetary A index was 8 (STAR Ap - based on the mean of three hour interval ap indices: 8.4). Three hour interval K indices: 10001115 (planetary), 11112315 (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 4 active regions using 2K resolution (SN: 85) and 4 active regions using 1K resolution (SN: 58) SDO images on the visible solar disk.
Region 12565 [N04W33] gained small spots and
produced low level C flares.
Region 12567 [N05W23] developed with the main penumbra increasing in area and positive polarity spots emerging at the northern edge of that penumbra. M class flaring is possible.
Region 12569 [N15E13] decayed slowly and quietly.
Spotted regions not numbered (or interpreted differently) by SWPC:
S5372 [S15W01] was quiet and stable.
|Magnitude||Peak time (UT)||Location||AR||Recorded by||Comment|
July 18-19: No obviously Earth directed CMEs were observed in available
July 17: A faint CME was likely associated with a long duration C1 event in ARs 12565/12567. The CME reached Earth late on July 19.
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 northern hemisphere coronal hole (CH750) was in an Earth facing position on July 18-19.
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 unsettled to major storm on July 20 due to CME effects. July 21-22 could see quiet to unsettled conditions due to effects from CH750.
|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
|Total spot count:||28||45||28|
|Sunspot number:||58||85||58||(total spot count + 10 * number of spotted regions)|
|Weighted SN:||53||68||51||(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):||64||47||46||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|
|2016.01||103.4||100.1||56.6||(54.5 projected, -3.4)||9.4|
|2016.02||103.6||101.0||57.2||(51.5 projected, -3.0)||9.9|
|2016.03||91.5||90.6||54.9||(47.9 projected, -3.4)||10.58|
|2016.04||93.3||94.0||38.0||(44.5 projected, -3.4)||9.03|
|2016.05||93.0||95.3||52.1||(41.8 projected, -2.7)||11.65|
|2016.06||81.9||84.5||20.9||(39.3 projected, -2.5)||8.44|
|2016.07||(89.4)||24.2 (2A) / 39.6 (2B) / 34.3 (2C)||(36.6 projected, -2.7)||(8.6)|
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.