Last major update issued on April 7, 2015 at 05:20 UT
[Solar and geomagnetic
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[Solar wind and electron fluence charts (updated daily)]
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[Solar cycles 1-20]
[Graphical comparison of cycles 21, 22, 23 and 24 (last update April 1, 2015)]
[Graphical comparison of cycles 10, 12, 13, 14, 16 and 24 (last update April 1, 2015)]
[Historical solar and geomagnetic data charts 1954-2006 (last update April 5, 2007)]
[Archived reports since January 2003 (last update April 1, 2015)]
[Noon SDO sunspot count 1K Reference: 4K (large file) (updated daily)]
[POES auroral activity
level October 2009 - December 2012]
[Solar polar fields vs solar cycles - updated March 15, 2015]
[Presentations: 3rd SSN Workshop, Tucson, 2013 (pdf) / 4th SSN Workshop, Locarno, 2014]
The geomagnetic field was quiet on April 6. Solar wind speed at SOHO ranged between 445 and 551 km/s.
Solar flux at 17h UTC on 2.8 GHz was 117.2 (decreasing 3.7 over the last solar rotation, the measurement at 20h UT was flare enhanced). The 90 day 10.7 flux at 1 AU was 128.2. The Potsdam WDC planetary A index was 4 (STAR Ap - based on the mean of three hour interval ap indices: 4.4). Three hour interval K indices: 22101011 (planetary), 23113221 (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 10 active regions using 2K resolution (SN: 178) and 8 active regions using 1K resolution (SN: 120) SDO images on the visible solar disk.
Region 12318 [N08E31] was quiet and stable.
Region 12319 [S10W19] was quiet and stable.
Region 12320 [S12E16] developed polarity intermixing. Further C flares are possible.
Spotted regions not numbered (or interpreted
differently) by SWPC:
S4345 [N10E35] was quiet and stable.
S4346 [N16W10] decayed slowly and quietly.
S4348 [S15E27] was quiet and stable.
S4350 [N21W82] developed slowly and quietly.
New region S4352 [S19E33] was observed with penumbra spots.
New region S4353 [S37W33] emerged with a penumbra spot at a high latitude.
New region S4354 [S05W22] emerged with penumbra spots.
|Magnitude||Peak time (UTC)||Location||AR||Recorded by||Comment|
|C3.6 (LDE)||18:57||SDO/EVE||filament eruption to the west of AR 12320
faint CME @ SOHO/LASCO C2
|C4.5||19:06||S14E14||12320||SDO/EVE||C3.0 @ GOES15 - peak 19:06 UT
impulsive flare superimposed on LDE
Flare activity according to SDO/EVE/ESP XRS-B proxy
April 4-5: No obviously
Earth directed CMEs were observed.
April 6: A faint CME was observed after a C3 LDE near AR 12320. The CME could reach Earth on April 9.
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 trans equatorial coronal hole (CH662) was in an Earth facing position on April 5. No geomagnetic disturbances have been associated with CH662 during previous rotations.
Long distance low and medium frequency (below 2 MHz) propagation along paths north of due west over upper middle latitudes is poor to fair. Propagation on long distance northeast-southwest paths is poor.
The geomagnetic field is expected to be quiet on April 7-9. There is a slim possibility that a weak CME could arrive late on April 9 and cause a few unsettled intervals that day and on April 10.
|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) 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 overlay
rotated out of view
actual location: N11W98
SWPC probably observed AR S4339!!
|Total spot count:||38||78||40|
|Sunspot number:||78||178||120||(total spot count + 10 * number of spotted regions)|
|Weighted SN:||53||89||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):||47||62||66||k * (sunspot number). k = 0.6 for SWPC, k = 0.35 for MSN 2K, k = 0.55 for MSN 1K (MSN=Magnetic Sunspot Number)|
|Month||Average solar flux||International sunspot number
|Smoothed sunspot number||Average
|166.3||102.3 (cycle peak)||78.4 (+1.1)||10.70|
(likely solar max)
|2014.10||153.4||152.9||60.6||(67.3 projected, -3.6)||8.96|
|2014.11||154.8||151.4||70.1||(64.7 projected, -2.6)||9.33|
|2014.12||158.7||153.8||78.0||(62.4 projected, -2.3)||11.24|
|2015.01||141.9||137.3||67.0||(60.2 projected, -2.2)||9.46|
|2015.02||129.1||126.0||44.8||(58.4 projected, -1.8)||9.92|
|2015.03||126.0||124.6||38.4||(56.1 projected, -2.3)||15.5|
|2015.04||(121.2)||11.4 (2A) / 56.3 (2B) / 63.5 (2C)||(53.4 projected, -2.7)||(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). The official WDC-SILSO international sunspot number is typically 30-50% lower. 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.
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 the UTC day. Comments and suggestions are always welcome.
SDO images are courtesy of NASA/SDO and the AIA, EVE, and HMI science teams.