To: | [email protected] |
---|---|
Subject: | Re: LF: Strong signal 29501 tonight |
From: | Paul Nicholson <[email protected]> |
Date: | Fri, 14 Mar 2014 11:51:50 +0000 |
Authentication-results: | mx.google.com; spf=neutral (google.com: 195.171.43.25 is neither permitted nor denied by best guess record for domain of [email protected]) smtp.mail=[email protected] |
Delivered-to: | [email protected] |
In-reply-to: | <3293FF91BB5841DB9C5C1F480B6A4943@White> |
References: | <[email protected]> <3293FF91BB5841DB9C5C1F480B6A4943@White> |
Reply-to: | [email protected] |
Sender: | [email protected] |
User-agent: | Mozilla/5.0 (X11; Linux i686; rv:17.0) Gecko/20130106 Thunderbird/17.0.2 |
Signal reports: WH2XBA/1 on 29499 http://abelian.org/vlf/tmp/29499_140314a.gif http://abelian.org/vlf/tmp/29499_140314b.gif Average S/N in 278 uHz: 14.4dB; Significance after 6 hours: 17.5 sigma; WHX2XBA/4 on 29501 http://abelian.org/vlf/tmp/29501_140314a.gif http://abelian.org/vlf/tmp/29501_140314b.gif Average S/N in 278 uHz: 13.8dB; Significance after 6 hours: 17.1 sigma; Comparison of phase change: http://abelian.org/vlf/tmp/140314a.gif These signals have a message carrying capability of around 180 bits in 6 hours at one code symbol per minute. Unfortunately, none of the data modes used by radio amateurs could come anywhere close to that theoretical limit at VLF. -- Paul Nicholson -- |
<Prev in Thread] | Current Thread | [Next in Thread> |
---|---|---|
|
Previous by Date: | LF: Re: Plasma TV and CPL QRM, André Guyé |
---|---|
Next by Date: | Re: LF: Strong signal 29501 tonight, Dexter McIntyre W4DEX |
Previous by Thread: | Re: LF: Strong signal 29501 tonight, Markus Vester |
Next by Thread: | Re: LF: Strong signal 29501 tonight, Dexter McIntyre W4DEX |
Indexes: | [Date] [Thread] [Top] [All Lists] |