Topband: Correlation
Bill Tippett
btippett at alum.mit.edu
Mon Mar 8 09:46:22 EST 2004
Not to beat a dead horse on this but there is VERY
strong correlation with the low flux and stable geomagnetic
conditions which exist at solar cycle lows. The following
data was gathered for the RM-10352 petition by K1ZM and
myself. Granted, it is virtually impossible to predict 160
conditions from one day to the next, but there is very strong
long-term correlation to the stage of the solar cycle. This
can also be observed by looking at the year all-time
DX contest records were set on 160. Current records for
both modes of the CQ WW Contests were set in 1996.
73, Bill W4ZV
http://users.vnet.net/btippett/rm_petition.htm
Comparison of 160 m Contact Levels by US Multi-Multi Contest Entrants Over Time
The matrix appearing below represents the aggregation of 160 m contact
totals of the 5 top-scoring USA multi-multi entrants during 48 hours in the
CQWW CW DX Contests from 1975 - 2000. A definite trendline of increasing
contact totals can be seen as well as variations caused by solar cycle
maxima and minima. Solar maxima present somewhat unfavorable conditions on
1.8 MHz due to increased levels of signal absorption. Solar minima offer
favorable conditions for 160 m enthusiasts due to decreased absorption. The
matrix indicates increasing activity levels on 160 m throughout the period
with short periods of reduced activity around solar maxima.
Year Contacts (Sum of Top 5 USA Multi-Multi QSO's on 160 m in CQ CW DX Tests)
1975 214
1976 300 Cycle Minimum June 1976
1977 295
1978 229
1979 235 Cycle 21 Maximum December 1979
1980 215
1981 298
1982 230
1983 407
1984 502
1985 647
1986 546 Cycle Minimum September 1986
1987 495
1988 391
1989 392 Cycle 22 Maximum June 1989
1990 523
1991 381
1992 433
1993 890
1994 781
1995 1299
1996 1474 Cycle Minimum May 1996
1997 704
1998 898
1999 996
2000 1092 Cycle 23 Maximum April 2000
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