Propagation 

Part 2

 
During each solar cycle, there is plenty of time to work DX with a little RF radiating from a wet noodle ; )  With a highly refractive ionosphere and little path absorption, it doesn't take much antenna to work the world.

Some may say - what's difference between an S9 signal with a low-dipole or an S-9 +20db signal with a tall tower and directional antenna? The main thing is that you can hear and work the DX! For the most part, when conditions are good, that's absolutely correct.

It explains why there are many hams all over the world, who have received their WAC QRP awards ( that's Worked all Continents with less than 1 watt! ). These fellows are a rare breed that understand propagation and know how to use it to their advantage. Another advantage they have is that 99% of them work CW : )

For the better part of most solar cycles, a low dipole will get you DXCC and beyond in a hurry so please don't sweat your antenna. I'm sure your log reflects what I'm saying.

On the opposite side of the coin, things do change for the worst with any solar cycle. When we only have a couple of years before the bottom of the cycle, where the upper HF bands that gave us an intrinsic DX advantage aren't opening much at all, and 14Mhz acts much like 28Mhz, closing shortly after sundown, every decibel you can muster can mean the difference between making the contact or not.

It doesn't have to be the bottom of the cycle either - solar flares, coronal mass ejections and other detrimental solar activity that can diminish the ionospheres ability to refract HF signals can put a big frown on any Dx'ers face! A lot of this kind of activity actually happens at the height of most solar cycles.

As for antennas and height, imagine that for every 3db advantage in antenna
performance, the power requirements at each end of a Dx circuit are cut by one half. So, yes, there isn't much difference between hearing signals at S9 and 20db over, but that same 20db advantage makes a big difference when it's needed - when signals are marginal at best.

The bottom line is that it's all relative - just about any RF radiator will work with Dx, but with varying degrees of success. It's true that higher and higher antenna heights with directional antennas, increase ones ability to copy long-haul Dx with greater signal strength, which is especially dramatic when conditions are marginal. Those that run the bigger arrays will allow those with minimal antennas, like mobiles and portables to work the world! I know, I've worked 50 countries CW mobile, but none of it was mobile-to-mobile.  : )

In contrast, low antennas do work well enough to work mucho Dx. So, even though the main-lobe of a low antenna is radiating at high angles, there is still enough low angle radiation to capture enough signal arriving at those low angles to work more than your fair share of DX. Signals may not be great all the time, as with a more elaborate antenna system, but if the Dx is above the noise, and he hears you, you have at it! Breaking Dx pile-ups may take a few more calls, but that's relative too. As long as the contact gets in the log, run what you hung and enjoy.

Here's an assignment for you OM - when was the last time you worked S.Korea or Japan? This weekend, run "W6EL Propagation Prediction Software" for openings to Japan and tune the band when the signals are supposed to peek. Remember, the software predicts openings and signal strengths based on ionospheric model statistics. If it says Japan will open on 15 meters 25 percent of the time in the month of December with a SF of 150 at 23:00Z, then chances are, the band will open 7 days out of the month. If it opens more often due to a burst of solar energy, so be it!

One more thing - how about running the NCDXF Software and listen for the beacon network. You don't have to know CW at 22wpm with the software. When you think the band is dead due to the lack of signals, use the network and assess conditions for yourself.

 

    Are you still glad you asked me that question?

--AA2AE

This has been another Marconi Moment.

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Last revised: March 21, 2003 13:13.