Return-Path: Received: from mtain-mj08.r1000.mx.aol.com (mtain-mj08.r1000.mail.aol.com [172.21.164.92]) by air-md05.mail.aol.com (v129.4) with ESMTP id MAILINMD052-8b854cca5feb33b; Fri, 29 Oct 2010 01:47:23 -0400 Received: from post.thorcom.com (post.thorcom.com [195.171.43.25]) by mtain-mj08.r1000.mx.aol.com (Internet Inbound) with ESMTP id 0A6D9380000A7; Fri, 29 Oct 2010 01:47:20 -0400 (EDT) Received: from majordom by post.thorcom.com with local (Exim 4.14) id 1PBhm7-0004Ay-3c for rs_out_1@blacksheep.org; Fri, 29 Oct 2010 06:45:15 +0100 Received: from [195.171.43.32] (helo=relay1.thorcom.net) by post.thorcom.com with esmtp (Exim 4.14) id 1PBhm6-0004Ap-Fl for rsgb_lf_group@blacksheep.org; Fri, 29 Oct 2010 06:45:14 +0100 Received: from mailt.toya.net.pl ([217.113.224.9] ident=postfix) by relay1.thorcom.net with esmtp (Exim 4.63) (envelope-from ) id 1PBhm4-0000aL-2z for rsgb_lf_group@blacksheep.org; Fri, 29 Oct 2010 06:45:14 +0100 Received: from mail.toya.net.pl (localhost.localdomain [127.0.0.1]) by mail.toya.net.pl (Postfix) with ESMTP id F13BB20000613 for ; Fri, 29 Oct 2010 07:45:10 +0200 (CEST) Received: by mail.toya.net.pl (Postfix, from userid 5001) id E67032000060F; Fri, 29 Oct 2010 07:45:10 +0200 (CEST) Received: from [192.168.1.100] (unknown [10.3.153.39]) (Authenticated sender: unimlyn) by mail.toya.net.pl (Postfix) with ESMTPA id 59EC420000613 for ; Fri, 29 Oct 2010 07:45:08 +0200 (CEST) Message-ID: <4CCA5F64.60606@toya.net.pl> Date: Fri, 29 Oct 2010 07:45:08 +0200 From: Piotr Mlynarski User-Agent: Thunderbird 2.0.0.24 (Windows/20100228) MIME-Version: 1.0 To: rsgb_lf_group@blacksheep.org X-AV-Checked: ClamAV using ClamSMTP X-Spam-Score: 0.0 (/) X-Spam-Report: autolearn=disabled,none Subject: LF: vlf experiments-numerical considerations Content-Type: text/plain; charset=ISO-8859-2; format=flowed Content-Transfer-Encoding: 7bit X-Spam-Checker-Version: SpamAssassin 2.63 (2004-01-11) on post.thorcom.com X-Spam-Level: X-Spam-Status: No, hits=0.0 required=5.0 tests=none autolearn=no version=2.63 X-SA-Exim-Scanned: Yes Sender: owner-rsgb_lf_group@blacksheep.org Precedence: bulk Reply-To: rsgb_lf_group@blacksheep.org X-Listname: rsgb_lf_group X-SA-Exim-Rcpt-To: rs_out_1@blacksheep.org X-SA-Exim-Scanned: No; SAEximRunCond expanded to false x-aol-global-disposition: S X-AOL-REROUTE: YES x-aol-sid: 3039400c89b04cca5fe86439 X-AOL-IP: 195.171.43.25 X-AOL-SPF: domain : blacksheep.org SPF : none X-Mailer: Unknown (No Version) Dear LF Group, Dreamers Recently, after 7th Stefan experiment on VLF band i came back to the numerical programme i have written few months ago which gives us some insight about the e-field strength produced by Stefan TX setup along with its kite antenna. Following Alan Melia suggestions concerning the ways of displaying results i have sent here few graphs illustrating the e-field strength vs distance for a given frequency. The programme has been written basing upon earth-ionosphere waveguide model proposed by David F. Lowenfels: http://dspace.mit.edu/bitstream/handle/1721.1/16973/53712465.pdf?sequence=1 (again, i am grateful to Paul Nicholson for this link) The numerical simulation covers wide range of frequencies starting from several Hertz up to 24 Khz with an assumption that EM energy is transmitted from vertical electric field antennae ( so it does apply to Stefan kite antenna ) By the time the code was almost completed i've promised to put here, on the reflector, the source code so everybody could play her/himself with it for specific purposes. It is written in Fortran and can be downloaded from: http://www.toya.net.pl/~mlynarski/mpj.zip ( i am sorry that instead of two weeks it took me few months to complete something which was almost completed - well, please, do not ask why ... :) ) Basically, the programme solves normal mode equations for the TEM mode propagation in a spherical waveguide ( eqns: 5.2 - 5.11 of Lowenfels paper). The numerical essence of the present source code is connected with the calculation of the Legendre Function of a complex degree "nu" where the complex "nu" accounts for the dispersive and dissipative properties of the earth-ionosphere waveguide. For that purpose I have used an algorithm described in Jones and Burke paper published in J.Phys.A: Math.Gen, Vol.23, 3159(1990) I did partial optimization of the fortran code , however, the used algorithm of zonal harmonic series expansion is very efficient itself so the program should work on modest PC machines and yet producing the final result in a reasonable time ( seconds of CPU time for , say, 1000 steps of frequency etc...) After download and decompression the user will get 4 files: propvlf.f head.f dane.dat out.dat The main fortran subroutine which calculates the propagation model is in propvlf.f file. The C(omment) lines at the begining of this subroutine describe its input/output formal parameters. The second fortran file head.f is a simple example of so-called main program showing how the subroutine is called with user defined numerical inputs ( dane.dat file) the out.dat file contains one line of numerical result which along with dane.dat file can be used as a reference when adopting/testing the program. Of course, the user can easily modify the header program by defining loops over frequency, distance with incremental steps allowing for different graphical displays, presentations etc... The code is rather portable (generic names were used for intrinsic functions) so basically any fortran compiler on most platforms should do its work without problems - if otherwise, please contact me either on or off the reflector. Finally, please, feel absolutely free to change, adopt, modify, add , delete etc.. any part of this code. I did it for our/dreamers/ purposes inspired by the wonderful (TX) work done by Stefan and others who do also a smart work of RX'ing. Unfortunately, i could not take part in 8th Stefan experiment, though i am preparing my RX stuff for the 9th one :) 73, Piotr, sq7mpj qth: Lodz /jo91rs/