Last major update issued on October 27, 2013 at 06:15 UTC.
[Solar and geomagnetic data - last month (updated
[Solar wind and electron fluence charts (updated daily)]
[Solar cycles 23-24 (last update October 1, 2013)] [Cycle 24 progress (last update October 1, 2013) ]
[Solar cycles 1-20]
[Graphical comparison of cycles 21, 22, 23 and 24 (last update October 1, 2013)]
[Graphical comparison of cycles 10, 12, 13, 14, 16 and 24 (last update October 1, 2013)]
[Historical solar and geomagnetic data charts 1954-2006 (last update April 5, 2007)]
[Archived reports since January 2003 (last update October 9, 2013)]
[POES auroral activity level since October
2009 - updated January 26, 2013]
[Solar polar fields vs solar cycles - updated October 10, 2013]
[Presentation 3rd SSN Workshop, Tucson, 2013 (pdf)]
The geomagnetic field was very quiet on October 26. Solar wind speed at SOHO ranged between 270 and 358 km/s. ACE data indicates the arrival of a weak CME near 22h UT, however, the interplanetary magnetic field has been predominantly northwards since then.
Solar flux measured at 17h UTC on 2.8 GHz was 160.2 (the measurement at 20h was flare enhanced, increasing 57.1 over the last solar rotation). The 90 day 10.7 flux at 1 AU was 116.0. 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: 00000001 (planetary), 10001211 (Boulder).
The background x-ray flux was at the class C1 level.
At the time of counting spots (see image time) spots were observed in 11 active regions in 2K resolution (SN: 228) and 10 active regions in 1K resolution (SN: 169) SDO images on the visible solar disk.
Region 11872 [S18W78] was quiet and stable.
Region 11873 [N12W80] developed slowly and was quiet.
Region 11875 [N06W52] decayed slowly and has a magnetic delta structure in the trailing spot section. M class flares are possible. C5+ flares: M1.2 at 09:23 (not reported by SWPC) UTC.
Region 11877 [S12W29] lost negative polarity umbrae but still has polarity intermixing. C5+ flares: C5.2 at 08:46, C8.8 at 17:15, C7.7 at 19:20 UTC.
Region 11879 [S12W14] decayed in the trailing spot section.
Region 11881 [S22E08] was quiet and stable.
Region 11882 [S09E49] produced several M class flares and has at least two magnetic delta structures. Major flaring is possible. C5+ flares: M2.3/1B at 06:06, M1.5 at 09:37, M1.8/1N long duration event peaking at 11:08 (associated with a partial halo CME), C6.5 at 17:32, M1.0 at 19:53 UTC.
New region 11883 [N02E75] rotated into view.
New region 11884 [S12E80] rotated into view. It is not yet clear whether this and AR 11885 are tow independent groups or one group. M flares are possible. C5+ flares: M3.1 at 19:27 UTC.
New region 11885 [S18E77] rotated into view.
Spotted regions not numbered by SWPC:
S2776 [N08W18] lost the trailing spots.
October 24: A faint halo CME was observed after the M9 event in AR 11877
early in the day.
October 25: A faint asymmetric halo CME was observed after the X1.7 event at 08h while a significantly larger full halo asymmetric CME was observed after the X2.1 flare near 15h. The latter CME will likely reach Earth on October 27.
October 26: An asymmetric halo CME was observed after the M1.8 LDE near 11h. Due to many other CMEs it is difficult to determine if this one was full or partial halo. The CME could reach Earth on October 29.
Coronal hole history (since October
Compare today's report to the situation one solar rotation ago: 28 days ago 27 days ago 26 days ago
No obvious coronal holes are currently in or near Earth facing positions.
Long distance low and medium frequency (below 2 MHz) propagation along paths north of due west over high and upper middle latitudes is good. Propagation on long distance northeast-southwest paths is poor.
The geomagnetic field is expected to be quiet to minor storm on October 27-29 due to CME effects, occasional major storm intervals are possible when the CME observed after the X2 event on Oct.25 arrives.
|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: 0-20% probability, Yellow: 20-60% probability, Red: 60-100% 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:||81||118||69|
|Sunspot number:||171||228||169||(total spot count + 10 * number of spotted regions)|
|Weighted SN:||131||176||127||(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):||103||80||93||k * (sunspot number). k = 0.6 for SWPC, k = 0.35 for STAR SDO 2K, k = 0.55 for STAR SDO 1K|
|Month||Average measured solar flux||International sunspot number (SIDC)||Smoothed sunspot number||Average ap
|2011.11||153.5 (cycle peak)||96.7 (cycle peak)||61.1 (+1.2)||5.55|
likely cycle 24 max
|2013.04||124.8||72.4||(56.2 projected, -1.3)||5.40|
|2013.05||131.4||78.7||(55.8 projected, -0.4)||9.73|
|2013.06||110.1||52.5||(56.0 projected, +0.2)||12.60|
|2013.07||115.5||57.0||(56.1 projected, +0.1)||9.47|
|2013.08||114.6||66.0||(55.9 projected, -0.2)||8.27|
|2013.09||102.6||36.9||(55.4 projected, -0.5)||5.23|
|2013.10||128.1 (1)||101.6 (2A) / 121.2 (2B) / 70.6 (2C)||(53.9 projected, -1.5)||(8.13)|
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 SIDC 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 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.