Solar Terrestrial Activity Report

Last major update issued on April 2, 2007 at 03:25 UTC.

[Solar and geomagnetic data - last month (updated daily)]
[Solar wind and electron fluence charts (updated daily)
[Solar cycles 21-23 (last update March 10, 2007)]
[Solar cycles 1-20]
[Graphical comparison of cycles 21, 22 and 23 (last update March 10, 2007)]
[Graphical comparison of cycles 2, 10, 13, 17, 20 and 23 (last update March 10, 2007)]
[Historical solar and geomagnetic data charts 1954-2005 (last update March 3, 2006)]
[Archived reports (last update February 6, 2007)]

Recent activity

The geomagnetic field was unsettled to minor storm on April 1. Solar wind speed ranged between 379 and 573 km/s (average speed was 505 km/s, increasing 172 km/s over the previous day) under the influence of a high speed stream from CH263.

Solar flux measured at 20h UTC on 2.8 GHz was 71.7. The planetary A index was 30 (STAR Ap - based on the mean of three hour interval ap indices: 30.0). Three hour interval K indices: 54544334 (planetary), 54544333 (Boulder).

The background x-ray flux is below the class A1 level.

At midnight there was 1 spotted region on the visible solar disk. The solar flare activity level was very low. No C class events were recorded during the day.

Region 10949 reemerged with a few small spots in the leading positive polarity area.

Coronal mass ejections (CMEs)

March 30 - April 1: No obvious fully or partially Earth directed CMEs were observed in LASCO imagery.

Coronal holes

Coronal hole history (since late October 2002)
Compare today's report to the situation one solar rotation ago: 28 days ago 27 days ago 26 days ago

A recurrent coronal hole (CH263) in the southern hemisphere was in an Earth facing position on March 28-30.

Processed SOHO/EIT 195 image at 17:00 UTC on April 1. The darkest areas on the solar disk are likely coronal holes.

Forecast

The geomagnetic field is expected to be unsettled to be quiet to active on April 2-3 due to a high speed stream from CH263. Mostly quiet conditions are likely on April 4-6.

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.

Propagation

Daily monitoring will not resume until a local noise problem (related to construction work on a neighboring property) has been fixed. Occasional monitoring reports will be submitted when propagation is good.

March 23, 2007: Strong signals were noted from a number of USA east coast stations. Some stations from the Canadian Atlantic provinces had signals exceeding S9 (on a Drake R8A).

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
10949 2007.03.28 3 4 N08E08 0050 CRO classification was AXX at midnight, area 0010
Total spot count: 3 4  
SSN: 13 14  

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)
2006.01 83.4 15.3 20.8 (-2.2)
2006.02 76.5 4.9 18.6 (-2.2)
2006.03 75.4 10.6 17.4 (-1.2)
2006.04 89.0 30.2 17.1 (-0.3)
2006.05 80.9 22.3 17.3 (+0.2)
2006.06 76.5 13.9 16.3 (-1.0)
2006.07 75.7 12.2 15.3 (-1.0)
2006.08 79.0 12.9 15.6 (+0.3)
2006.09 77.8 14.4 15.6 (+0.0)
2006.10 74.3 10.4 (14.3 predicted, -1.3)
2006.11 86.3 21.5 (12.6 predicted, -1.7)
2006.12 84.5 13.6 (11.6 predicted, -1.0)
2007.01 83.3 16.9 (11.2 predicted, -0.4)
2007.02 77.7 10.6 (11.1 predicted, -0.1)
2007.03 72.2 4.8 (11.3 predicted, +0.2)
2007.03 71.7 (1) 0.4 (2) (11.9 predicted, +0.6)

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% 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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