|[AMRadio] Microphone recomendation|
bbruhns at erols.com
bbruhns at erols.com
Tue Sep 22 11:16:23 EDT 2009
I used about 15 megs of grid-leak with a D-104 in the early 70s, and I was picking up a strong 9 Hz rumble that was probably from a nearby main road. The D-104 is a good choice for super-high Z inputs because it has a strong response peak around 3 KHz. This makes brighter, clearer audio, which improves things - especially with people listening on selective receivers.
Bacon (the old Bacon), WA3WDR
Sent from my Verizon Wireless BlackBerry
From: "Jim Tonne" <tonne at comcast.net>
Date: Tue, 22 Sep 2009 11:07:19
To: Discussion of AM Radio in the Amateur Service<amradio at mailman.qth.net>
Subject: Re: [AMRadio] Microphone recomendation
I have been lurking here and reading the discussion
which seems to me to have reduced itself down to a
kind of "my daddy is better than your daddy" kind of
The person who said the D104 microphone could be
thought of as a voltage generator in series with a
500 pF capacitor hit the nail on the head! Exactly
correct (although I thought it might be a *slightly*
higher capacitance value).
I have spent a few minutes with LTspice and made
a plot which clearly shows what happens when you
change the value of the load on the D104 microphone.
With a 10 megohm load the -3 dB point will be right
at 30 Hz.
Please, fellows, take a quick peek at this plot:
The bottom line of this note is that going higher than
10 megohms for a load is nonsense. Pure nonsense.
- Jim W4ENE
Our Main Website: http://www.amfone.net
AMRadio mailing list
Searchable Archives: http://email@example.com/
List Rules (must read!): http://w5ami.net/amradiofaq.html
List Home: http://mailman.qth.net/mailman/listinfo/amradio
Post: AMRadio at mailman.qth.net
To unsubscribe, send an email to amradio-request at mailman.qth.net with
the word unsubscribe in the message body.
This list hosted by: http://www.qsl.net
Please help support this email list: http://www.qsl.net/donate.html
More information about the AMRadio mailing list
This page last updated 17 Oct 2017.