Solar Terrestrial Activity Report

Last major update issued on December 1, 2003 at 04:45 UTC.

[Solar and geomagnetic data - last month (updated daily)]
[Solar wind and electron fluence charts (updated daily)]
[Solar cycles 21-23 (last update November 4, 2003)]
[Solar cycles 1-20]
[Graphical comparison of cycles 21, 22 and 23 (last update November 4, 2003)]
[Graphical comparison of cycles 2, 10, 13, 17, 20 and 23 (last update November 4, 2003)]
[Historical solar and geomagnetic data charts 1954-2003 (last update October 15, 2003)]
[Archived reports (last update November 22, 2003)]

Recent activity

The geomagnetic field was quiet to unsettled on November 30. Solar wind speed ranged between 365 and 544 km/sec. A very weak moderately high speed coronal stream was observed early in the day. After 09h UTC ACE data did not any longer indicate the presence of that stream and a weak disturbance (unidentified source) dominated the solar wind for the remainder of the day.

Solar flux measured at 20h UTC on 2.8 GHz was 152.8. The planetary A index was 10 (STAR Ap - based on the mean of three hour interval ap indices: 11.3).
Three hour interval K indices: 22223332 (planetary), 22213332 (Boulder).

The background x-ray flux is at the class B6 level.

At midnight there were 10 spotted regions on the visible disk. Solar flare activity was low. A total of 4 C class events were recorded during the day.

Region 10507 decayed slowly and is rotating over the northwest limb.
Region 10508 decayed very quickly and lost about three quarters of the penumbral area. The region will rotate over the southwest limb tomorrow. Flares: C1.1 at 03:00, C1.2 at 10:11 and C2.1 at 15:31 UTC.
Region 10509 decayed slowly and quietly.
Region 10510 decayed quietly and lost penumbra on all spots. Rudimentary penumbra is still visible on quite a few of the many small spots.
Region 10511 decayed slowly and quietly.
Region 10513 was quiet and stable.
Region 10515 decayed and could become spotless today.
Region 10516 developed slowly and quietly.
New region 10517 rotated into view at the southeast limb. This is currently the most interesting region on the visible disk. Further C class flaring is likely, a minor M class flare is possible. Flares: C4.6 at 000:11 UTC.

Spotted regions not numbered by NOAA/SEC:
[S318] A new region emerged just southeast of region 10516 on November 30. Location at midnight: S22E47.

Coronal mass ejections (CMEs)

November 28-30: No partly or fully earth directed CMEs observed.

Coronal holes

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 trans equatorial coronal hole (CH70) was in a geoeffective position on November 30 and December 1.

Processed SOHO/EIT 284 image at 19:05 UTC on November 30. The darkest areas on the solar disk are likely coronal holes.

Forecast

The geomagnetic field is expected to be quiet to unsettled on December 1-2. On December 3-4 unsettled to major storm conditions are likely due to a high speed stream from coronal hole CH70.

Long distance low 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 poor. [Trans Atlantic propagation conditions are currently monitored every night on 1470 kHz. Dominant station tonight: Radio Cristal del Uruguay with CPN Radio (Peru) noted at times].

Coronal holes (1) Coronal mass ejections (2) M and X class flares (3)
Coronal hole indicator CME indicator M and X class flare indicator

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.

Active solar regions (Recent map)

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
10507 2003.11.18 8 10 N07W82 0320 DAO beta-gamma-delta
10508 2003.11.19 15 16 S19W71 0230 DAI classification was DSO
at midnight, area 0090
10509 2003.11.24 2 6 S11W24 0040 HAX classification was CAO
at midnight
10510 2003.11.24 27 25 S23W16 0090 DAI classification was DRI
at midnight, area 0040
10511 2003.11.25 6 7 S15W44 0030 BXO classification was CSO
at midnight
10512 2003.11.25 1   N06W36 0010 HSX spotless
10513 2003.11.26 2 1 N13E18 0070 HSX  
10514 2003.11.27     S15W85     spotless
10515 2003.11.28 8 6 S02E42 0030 BXO area was 0010
at midnight
10516 2003.11.28 7 14 S17E44 0090 DAO  
10517 2003.11.30 2 6 S07E67 0160 CAO formerly region S317
classification was DAO
at midnight, area 0260
S314 emerged on
2003.11.27
    S15W17     plage
S318 emerged on
2003.11.30
  5 S22E47 0020 BXO  
Total spot count: 78 96
SSN: 178 196

Monthly solar cycle data

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)
2002.10 167.0 97.5 90.5 (-4.1)
2002.11 168.7 95.5 85.2 (-5.3)
2002.12 157.2 80.8 82.0 (-3.2)
2003.01 144.0 79.7 80.9 (-1.1)
2003.02 124.5 46.0 78.5 (-2.4)
2003.03 131.4 61.1 74.1 (-4.4)
2003.04 126.4 60.0 70.3 (-3.8)
2003.05 115.7 55.2 (66.8 predicted, -3.5)
2003.06 129.3 77.4 (63.0 predicted, -3.8)
2003.07 127.7 85.0 (59.3 predicted, -3.7)
2003.08 122.1 72.7 (56.3 predicted, -3.0)
2003.09 112.2 48.8 (54.3 predicted, -2.0)
2003.10 151.7 65.6 (51.6 predicted, -2.7)
2003.11 140.8 (1) 103.0 (2) (48.9 predicted, -2.7)

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 sources noted in solar links. All time references are to the UTC day. Comments and suggestions are always welcome.


[DX-Listeners' Club]