Last major update issued on May 28, 2005 at 04:15 UTC.
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The geomagnetic field was very quiet to quiet on May 27. Solar wind speed ranged between 275 and 313 km/sec. A weak solar wind shock was observed at ACE near 03:25 UTC on May 28.
Solar flux measured at 20h UTC on 2.8 GHz was 95.5. The planetary
A
index was 4 (STAR Ap - based on the mean of three hour interval ap
indices: 4.3).
Three hour interval K indices: 11111211 (planetary), 11111000 (Boulder).
The background x-ray flux is at the class B2 level.
At midnight there were 3 spotted regions on the visible solar disk. The solar flare activity level was moderate. A total of 3 C and 1 M class events was recorded during the day.
Region 10766 had small spots emerging and disappearing all day. The region was quiet.
Region 10767 developed further in both the leading and intermediate spot section. A magnetic delta has formed inside
the large, irregularly shaped intermediate penumbra. Further M class flares are possible. Flare:
C2.5 at 05:07, C6.9 at 06:35, M1.1/2F at 12:30 and C1.1 at 19:40 UTC.
Region 10768 decayed and had only tiny spots left at the end of the day.
May 25 and 27: No obviously fully or partly potentially geoeffective CMEs were observed.
May 26: A full halo CME was observed after a filament eruption in region 10767 during the early afternoon. This CME will
likely reach Earth on May 29. Further material was added later in the day after the C8 long duration event in region 10767.
Coronal hole
history (since late October 2002)
Compare today's report with the situation one solar rotation ago: 28
days ago 27 days ago 26
days ago
A recurrent coronal hole (CH167) in the northern hemisphere was in an Earth facing position on May 24-26. CH167 has lost most of its area over the last rotation. A coronal hole in the southern hemisphere could rotate into an Earth facing position on May 29.
Processed SOHO/EIT 284 image at 01:06 UTC on May 28. The darkest areas on the solar disk are likely coronal holes.
The geomagnetic field is expected to be quiet to active on May 28 and unsettled to major storm on May 29-30 as a CME is likely to reach Earth near noon on May 29.
Coronal holes (1) | Coronal mass ejections (2) | M and X class flares (3) |
1) Effects from a coronal hole could reach Earth
within the next 5 days. When the high speed stream has arrived
the color changes to green.
2) Material from a CME is likely to impact 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.
Long distance low and medium frequency (below 2 MHz) propagation along east-west paths over high and upper middle latitudes is very poor. Propagation along long distance north-south paths is fair. Trans Atlantic propagation conditions are normally monitored every night on 1470 kHz. Dominant station tonight: Radio Cristal del Uruguay and Radio Rafaela (Argentina). 1510 kHz was again a lively frequency with Radio Rincón (Uruguay) delivering an amazing signal for such a low powered transmitter.
Compare to the previous day's image.
Data for all numbered solar regions according to the Solar Region Summary provided by NOAA/SEC. Comments are my own, as is the STAR spot count (spots observed at or inside a few hours before midnight) and data for regions not numbered by SEC or where SEC has observed no spots. SEC active region numbers in the table below and in the active region map above are the historic SEC/USAF numbers.
Active region | Date numbered | SEC spot count |
STAR spot count |
Location at midnight | Area | Classification | Comment |
---|---|---|---|---|---|---|---|
10765 | 2005.05.19 | N08W42 | plage | ||||
10766 | 2005.05.21 | 1 | 4 | N13W06 | 0010 | HRX | classification was BXO at midnight |
10767 | 2005.05.21 | 17 | 40 | S08W02 | 0240 | EKI |
beta-gamma-delta
area was 0420 at midnight |
10768 | 2005.05.26 | 3 | 3 | S08W63 | 0020 | DRO | classification was BXO at midnight, area 0000 |
Total spot count: | 21 | 47 | |||||
SSN: | 51 | 77 |
Month | Average solar flux at Earth |
International sunspot number | Smoothed sunspot number |
---|---|---|---|
2000.04 | 184.2 | 125.5 | 120.8 cycle 23 sunspot max. |
2000.07 | 202.3 | 170.1 | 119.8 |
2001.12 | 235.1 | 132.2 | 114.6 (-0.9) |
2004.03 | 112.0 | 49.1 | 47.1 (-2.2) |
2004.04 | 101.2 | 39.3 | 45.5 (-1.6) |
2004.05 | 99.8 | 41.5 | 43.8 (-1.7) |
2004.06 | 97.4 | 43.2 | 41.6 (-2.2) |
2004.07 | 119.1 | 51.1 | 40.2 (-1.4) |
2004.08 | 109.6 | 40.9 | 39.2 (-1.0) |
2004.09 | 103.1 | 27.7 | 37.5 (-1.7) |
2004.10 | 105.9 | 48.0 | 35.9 (-1.6) |
2004.11 | 113.2 | 43.5 | (34.8 predicted, -1.1) |
2004.12 | 94.5 | 17.9 | (33.4 predicted, -1.4) |
2005.01 | 102.2 | 31.3 | (30.9 predicted, -2.5) |
2005.02 | 97.2 | 29.1 | (28.3 predicted, -2.6) |
2005.03 | 89.9 | 24.8 | (26.5 predicted, -1.8) |
2005.04 | 86.0 | 24.4 | (24.6 predicted, -1.9) |
2005.05 | 100.1 (1) | 56.3 (2) | (22.0 predicted, -2.6) |
1) Running average based on the daily 20:00 UTC observed solar flux
value at 2800 MHz.
2) Unofficial, accumulated value based on the Boulder (NOAA/SEC)
sunspot number. The official international sunspot number is typically
30-50% less.
This report has been prepared by Jan Alvestad. It is based partly on my own observations and analysis, and partly on data from some of these solar data sources. All time references are to the UTC day. Comments and suggestions are always welcome.
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