Last major update issued on April 6, 2015 at 05:30 UT
[Solar and geomagnetic
data - last month (updated daily)]
[Solar wind and electron fluence charts (updated daily)]
[Solar cycles 23-24 (last update April 1, 2015)] [Cycle 24 progress (last update April 1, 2015) ]
[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 to unsettled on April 5. Solar wind speed at SOHO ranged between 462 and 569 km/s under the influence of a high speed stream from CH661.
Solar flux at 20h UTC on 2.8 GHz was 122.2 (decreasing 0.7 over the last solar rotation). The 90 day 10.7 flux at 1 AU was 128.4. The Potsdam WDC planetary A index was 6 (STAR Ap - based on the mean of three hour interval ap indices: 5.9). Three hour interval K indices: 22111113 (planetary), 22112223 (Boulder).
The background x-ray flux is at the class B4 level.
At the time of counting spots (see image time), spots were observed in 13 active regions using 2K resolution (SN: 200) and 10 active regions using 1K resolution (SN: 135) SDO images on the visible solar disk.
Region 12317 [N12W83] developed significantly and
was mostly quiet.
Region 12318 [N08E43] was quiet and stable.
Region 12319 [S09W09] decayed slowly and quietly.
Region 12320 [S12E29] developed further becoming a compact region. Magnetically the region currently has a fairly simple layout.
Spotted regions not numbered (or interpreted
differently) by SWPC:
S4339 [N08W72] developed slowly and quietly.
S4342 [S26E04] was quiet and stable.
S4345 [N10E48] was quiet and stable.
S4346 [N10W00] developed slowly and quietly.
S4347 [N27W15] was quiet and stable.
New region S4348 [S16E38] was observed with penumbra spots.
New region S4349 [S15E12] emerged with a penumbra spot.
New region S4350 [N21W67] emerged with a penumbra spot.
New region S4351 [N31E36] emerged with a penumbra spot.
|Magnitude||Peak time (UTC)||Location||AR||Recorded by||Comment|
|C3.1||03:42||NW limb||SDO/EVE||C1.9 @ GOES15 - peak 03:36 UT|
|C3.8 (LDE)||21:06||S12E30||12320||SDO/EVE||C3.0 @ GOES15 - peak 21:03 UT|
Flare activity according to SDO/EVE/ESP XRS-B proxy
April 3-5: No obviously Earth directed CMEs were observed.
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 to fair.
The geomagnetic field is expected to be mostly quiet on April 6-8.
|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
|Total spot count:||26||70||37|
|Sunspot number:||66||200||137||(total spot count + 10 * number of spotted regions)|
|Weighted SN:||41||92||59||(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):||40||70||75||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||(122.0)||8.8 (2A) / 52.6 (2B) / 62.6 (2C)||(53.4 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). 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.