Hi

> On Aug 7, 2020, at 10:48 PM, Bill Byrom <[email protected]> wrote:
> 
> Whit Griffith N5SU was the Chief Radio Scientist (or some similar title) for 
> Continental Electronics in the 1980's in Dallas. In around 1990 Whit gave a 
> slide show presentation to a Dallas Amateur Radio Club meeting at the 
> National Communications Museum, a project at the Dallas Communication Complex 
> in Irving started by Bill Bragg KA5PIP (SK) who became the voice of BIG TEX. 
> Whit showed amazing photos of the VLF transmitter and antenna they had 
> installed in Germany - I believe it was DHO38 at 23.4 kHz. The 
> helix/variometer room was huge, and the antenna used large cables strung 
> between tall towers as a capacitive top hat, and included an impressive 
> ground system.
> 
> The radiation resistance of a VLF vertical antenna is very low. At 100 kHz 
> one wavelength is 3 km (9,843 feet). So if an antenna was 412 m tall (1,352 
> feet), it would only be 0.137 wavelength long. The low radiation resistance 
> of such a short antenna requires a high antenna current. At high power levels 
> (1 MW or even more), the antenna current can be several hundreds of amps, and 
> this can produce very high voltages across reactive components of the antenna 
> system and matching network.
> 
> The result is that high power VLF transmitting stations require a lot of 
> land, a very expensive and large antenna and matching system which retunes 
> itself as the weather changes the antenna impedance, expensive provisions for 
> lightning and high wind protection, an expensive transmitter, and a very high 
> cost for the utility power and maintenance. 
> --
> Bill Byrom N5BB
> 
> 

One of the WWVB transmitters *might* fit in a large garage. The antenna 
matching gear at the base
of one of the antennas …. no way. It’s closer to the size of a small house. Of 
course as VLF stations 
go, WWVB is “low power”. 

Same basic issue, lots of weird interactions and a need to keep the signal very 
precise. Not as easy
as it might seem.

Bob


> 
> On Fri, Aug 7, 2020, at 7:16 PM, Bob kb8tq wrote:
>> Hi
>> 
>> Back in the day, if you hung out for a while in the lobby at Continental 
>> Electronics, you would notice a
>> model of an old style transmitter over by one wall. Go over and look a it 
>> for a a while and all the usual
>> parts were there. Couple of big tubes, big matching coil insulators here and 
>> there. Eventually you would 
>> notice this tiny spec down by the bottom of the model … hmmm … wonder what 
>> that is? 
>> 
>> Eventually one might figure out that the tiny spec was a person. The model 
>> was of an Omega transmitter ….
>> 
>> Bob
>> 
>>> On Aug 7, 2020, at 7:33 PM, jimlux <[email protected]> wrote:
>>> 
>>> On 8/7/20 4:13 PM, Bill Byrom wrote:
>>>> See this 1961 IRE paper at the NIST website:
>>>> https://tf.nist.gov/general/pdf/2303.pdf
>>>> IRE merged with AIEE in 1963 to form IEEE.
>>>> Figure 7 shows the calculated amplitude transfer of the ground wave signal 
>>>> vs frequency and distance. Note that for 100 kHz signals, the ground wave 
>>>> signal is reasonably strong at 2,000 miles but lousy at 5,000 miles.
>>>> As this paper notes, the sky wave reflections are delayed, and this delay 
>>>> depends on the ionization state of the ionosphere along the propagation 
>>>> path. This delay is shown in figure 2.
>>>> Figure 6 shows differences between daytime and nighttime propagation of 
>>>> pulsed signals. The received signal is a combination of the ground wave 
>>>> signal and one or more skywave signals (which are delayed with respect to 
>>>> the ground wave signal).
>>>> --
>>>> Bill Byrom N5BB
>>> 
>>> and such stuff is why Omega worked at VLF frequencies - none of that pesky 
>>> skywave - lambda=30km and you're ALWAYS below ionospheric cutoff. Alas, 
>>> they made some boneheaded mistakes like making one of the frequencies an 
>>> exact multiple of 60Hz.
>>> 
>>> There is something positively Tesla-ian about Omega with high power low 
>>> frequency transmitters into physically enormous antennas - like the one 
>>> with the top hat across the fjord.  None of this tiny L-band patch antenna 
>>> stuff inside a wristwatch.
>>> 
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