Propagation on higher frequencies. K0FF
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Geo>K0FF
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June 15, 2000
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Everyone seems puzzeled as to why conditions are not so hot on the upper frequencies during this "peak" of the sunspot cycle.
First of all, on the upper frequencies, DX occurs via F2 between the months of Sept thru April, for the Nothern Hemisphere. We here in the midwest experienced our first F2 opening of this cycle on 6M on Nov 8th 1999. We were working 9J2BO with low power for 3 days in a row. Using a combination of Es-link-to-TEP, multihop Es and a little F2, I worked 34 DXCC countries on 6 in 1999, and was heard in several more.Europe, Africa, Central America, South America, Alaska, Hawaii, South Pacific..all this from Missouri, where we are farther from the DX by one hop than the coastal stations. What more can you expect from 6M?
This band was specifically chosen over a proposed 42 Mc allotment, after WW2, by the ARRL, to supply us with a "challenge". That was their philosophy, and it worked. 42 Mc would have been "just another low band", per an article in QST, 1946.
In the summertime we see Es openings on 6 and 10, and these are not as intense during the peaks as they are during the nulls. In 95-96, we were tearing up 6M with European openings in June and July (4 hops for me).
Even during the peak months, there will be waxing and waning days. These occur on a 5 day and 27 day sub-cycle. this effectris more noticed on 6 than 10, as the MUF generaly still goes above 30 Mc but not as high as 50.On 6 especially there are aslo specific times of the day that are better for specific paths, depending on you location, and has to do with the angle of the sun between you and the target DX. Also different types of propagation will arrive at different angles from the horizon, making the performance of the antenna a big factor. Most successfull 6M ops have at least 2 antenna systems, on for Es (high angle) and one for F2(low angle). I have 3 systems, and one is elevatable in its orientation to the horizon, and it and one other are changeble in height from as low as 12 feet to as high as 85 feet. I use a single 11 el at 105 feet as a reference. A good compromise 6M antenna is 5 to 9 elements at 55 feet. An ideal antenna would be two 5 to 9 element beams stacked at 48 and 60 feet, and have variable phasing. This would catch either Es or F2.
Aslo 6M prop is better on the downward side of the peak than it is on the upward side, so watch out for the next few years, for reports of spectacular DX being worked with low power on 6M.
I have followed these patterns for over 35 years and have come up with a "Magic Calendar" for 6M, that shows the most likly days that DX may occur from my area, and use this to plan vacations, trips etc, with pretty good results... There is a lot more order to the supposed randomness of VHF DXing than generally recognized. ( I include 10M in the term VHF as it has many of the same characterisstics as 6, and indeed before the definitions were changed after WW@, anything above 30 Mc was considered UHF, so I gess 10M was truley VHF then..)
Remember 50.100 to 50.125 for INTERCONTENENTAL DX QSOs only.
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Don't count your chickens before they hatch
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by WA4RX on June 18, 2000
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Alas, all hope is not lost! Yesterday, 6.17.00, and today, 6.18.00, HF activity was picking up considerably. Consider checking some of the less common bands like 17m and 12m.
There was plenty of DX coming through today on 17meters. This is a great band-fast becoming my favorite. Plus, it's much more casual than the competitive 20 meter band.
Last night, 15 meters was wide open until midnight EST--very strange!
That is the thrill of ham radio--it follows the GUMP philosophy-"it's like a box of chocolates..you never know what you're gonna yet.."
Good DX!
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RE: Magic Calendar for 6
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by N4XX on September 28, 2000
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Plot the solar flux and A or k indices on a daily basis. More and more, as this cycle matures, you will see that they rise and fall with a 27-day periodicity (the time it takes the Sun to revolve once on its axis (approximately)). This will help you decide when it's best to be on the air. Specifically, if the condx are good today, chances are they will be good 27 days from now. Solar flare activity, and hence, geomagnetic activity on Earth, peaks two years after the sunspot cycle peak, so the next two years will have in increasing number of geomagnetic storms that will catch you by surprise. But if you play the 27-day game for the next six years, you should be able to time your operations to catch the best conditions about 80% of the time. The technique does not work well in the early years of a sunspot cycle because the early spots rarely stick around for more than one revolution of the Sun.
By the way, the VHFer's feast often is the HFer's famine. If the geomagnetic activity is high, there's a good chance that HF conditions will be poor while auroral propagation on the VHF bands will be fantastic.
If you want to learn more, George Jacobs, Bob Rose, and I wrote a book called The Shortwave Propagation Handbook that is available from CQ.
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