Last major update issued on March 30, 2006 at 04:15 UTC.
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The geomagnetic field was quiet to unsettled on March 28. Solar wind speed ranged between 318 and 363 (all day average 338) km/sec.
Solar flux measured at 20h UTC on 2.8 GHz was 81.7. The planetary A index
was 6 (STAR Ap - based on the mean of three hour interval ap
indices: 6.0).
Three hour interval K indices: 12012322 (planetary), 12113202 (Boulder).
The background x-ray flux is at the class A8 level.
At midnight there were 2 spotted regions on the visible solar disk. The solar flare activity level was very low. No C class events were recorded during the day.
Region 10865 developed slowly and remains capable of producing
occasional C flares.
New region 10866 rotated into view at the southeast limb on March 28 and
was numbered the next day by SEC.
March 27-29: No partly or fully Earth directed CMEs were observed in LASCO imagery.
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 coronal hole (CH218) in the northern hemisphere will likely rotate to an Earth facing position on April 2. A coronal hole in the southern hemisphere is probably too far to the south to be geoeffective.
Processed SOHO/EIT 284 image at 01:06 UTC on March 30. The darkest areas on the solar disk are likely coronal holes.
The geomagnetic field is expected to be quiet to unsettled on March 30 - April 1.
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) 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.
Long distance low and medium frequency (below 2 MHz) propagation along east-west paths over high and upper middle latitudes is poor. Propagation on long distance northeast-southwest paths is poor. Trans Atlantic propagation conditions are normally monitored every night on 1470 kHz. Dominant station tonight: Radio Vibración (Venezuela). On 610 kHz several stations were noted with either WIOD Miami or Radio Rebelde (Cuba) usually on top.
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 |
---|---|---|---|---|---|---|---|
10865 | 2006.03.28 | 10 | 15 | S12E48 | 0130 | DSO | classification was DSI at midnight |
10866 | 2006.03.29 | 1 | 1 | S06E69 | 0070 | HSX | formerly region S637 |
Total spot count: | 11 | 16 | |||||
SSN: | 31 | 36 |
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) |
2005.01 | 102.2 | 31.3 | 34.6 (-0.6) |
2005.02 | 97.2 | 29.2 | 33.9 (-0.7) |
2005.03 | 89.9 | 24.5 | 33.5 (-0.4) |
2005.04 | 86.0 | 24.2 | 31.6 (-1.9) |
2005.05 | 99.3 | 42.7 | 28.9 (-2.7) |
2005.06 | 93.7 | 39.3 | 28.8 (-0.1) |
2005.07 | 96.4 | 40.1 | 29.1 (+0.3) |
2005.08 | 90.5 | 36.4 | 27.4 (-1.7) |
2005.09 | 91.1 | 21.9 | (25.6 predicted, -1.8) |
2005.10 | 77.0 | 8.5 | (23.8 predicted, -1.8) |
2005.11 | 86.3 | 18.0 | (21.4 predicted, -2.4) |
2005.12 | 90.7 | 41.2 | (18.5 predicted, -2.9) |
2006.01 | 83.4 | 15.4 | (15.4 predicted, -3.1) |
2006.02 | 76.5 | 4.7 | (12.3 predicted, -3.1) |
2006.03 | 74.8 (1) | 18.8 (2) | (10.1 predicted, -2.2) |
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% lower.
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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