SB PROP @ ARRL $ARLP052 ARLP052 Propagation DE KT7H QST DE W1AW Propagation Forecast Bulletin 52 ARLP052 From Tad Cook, KT7H Seattle, WA December 31, 1993 To All Radio Amateurs Solar activity took a large unexpected jump last week, averaging more than 34 points better than the week prior. The greatest solar flux was on December 27, reaching 140.4, the highest since May 30, 1993 when it was 140. Prior to that, the last time the flux was higher was on April 8, 1993 when it was 143.1 The best part of this event for radio amateurs was that there was no increase in geomagnetic disturbances. In fact, the A and K indices were very quiet. There has been a forecast for a recurring coronal hole to wreak havoc around the last day of the year, but as of this writing, it has not appeared. Perhaps the big rise in activity is part of the moderate increase in flux that was forecast for this Fall and Winter season, before the solar cycle continues it's retreat toward a probable minimum in about 3 years. 1993 has been a year of declining solar activity, and this should continue through 1994, 1995, and the following year. The latest long term forecast shows average monthly flux values rising about five to fifteen points until April 1994, and then dropping to about ten points lower than the current level by the end of 1994. As we begin the new year, look for typical winter conditions with 80 and 160 meters benefitting from low noise levels and long nights. 40 meters should be a good DX band starting around sundown, and the higher bands during the daytime. In January the flux should reach a minimum around the 17th or 18th, dipping below 100, and then rise back to the current higher levels around the end of the month. Sunspot Numbers from December 23 through 29 were 70, 117, 120, 92, 107, 108 and 112, with a mean of 103.7. 10.7 cm flux was 105, 111.2, 119.1, 125, 140.4, 133.6 and 128.7, with a mean of 123.3 Beginning this week the sample path projections will take a slightly more cautious approach to when band openings begin. It is difficult to make these forecasts for all levels of amateur radio stations, given the wide range of antennas and station environments. There will now also be weightings used to make the forecast, particularly on the lower frequencies to account for average low band antennas at most stations. The projection this week is from West Suffield, Connecticut to Germany. Look for 80 and 75 meters to open after 2030z, peak from 2330z to 0630z, and end after 0900z. 40 meters looks good from 1900z to 0800z or 1000z, peaking around 2130z to 0730z, which is the period that darkness prevails over both ends of the path. Check 30 meters from 1230z until 1900z, and again around 0330z to 0500z. 20 meters also looks good from 1230z to 1900z, with the peak periods at the beginning and the end of the opening. 17 meters should be usable from 1330z to 1730z, and 15 meters from 1430z to 1700z. 12 meters has some possibility of openings on some days from 1500z to 1630z. 10 meters does not look promising, but on some days there may be openings around 1600z. /EX