📄 rayfan.m
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function [x,t,phi]=rayfan(v,z,z1,z2,p)
% RAYFAN: shoots a fan of rays given their ray parameters for v(z)
%
% [x,t,phi]=rayfan(v,z,z1,z2,p)
%
% rayfan shots a fan of rays through the stratified earth. It is
% identical to rayfan_a except that the fan is described by a p vector
% rather than an angle vector.
% v = vector of layer velocities
% z = vector of depths to the tops of each layer. Thus V(k) is
% the velocity between z(k) and z(k+1). Z should be sorted into
% ascending order.
% z1 = depth the ray starts at
% z2 = depth the ray ends at
% p = vector of ray parameters defining the fan
% x = horizontal distance the ray travels (one for each p)
% t = traveltime along the ray ( in seconds ) (one for each p)
% NOTE: Critically refracted rays will return inf for both x an t
% phi = angle (from the vertical) of the ray at z2 (degrees) (one for each p)
%
% G.F. Margrave, CREWES Project, July 1995
%
% NOTE: It is illegal for you to use this software for a purpose other
% than non-profit education or research UNLESS you are employed by a CREWES
% Project sponsor. By using this software, you are agreeing to the terms
% detailed in this software's Matlab source file.
% BEGIN TERMS OF USE LICENSE
%
% This SOFTWARE is maintained by the CREWES Project at the Department
% of Geology and Geophysics of the University of Calgary, Calgary,
% Alberta, Canada. The copyright and ownership is jointly held by
% its author (identified above) and the CREWES Project. The CREWES
% project may be contacted via email at: crewesinfo@crewes.org
%
% The term 'SOFTWARE' refers to the Matlab source code, translations to
% any other computer language, or object code
%
% Terms of use of this SOFTWARE
%
% 1) Use of this SOFTWARE by any for-profit commercial organization is
% expressly forbidden unless said organization is a CREWES Project
% Sponsor.
%
% 2) A CREWES Project sponsor may use this SOFTWARE under the terms of the
% CREWES Project Sponsorship agreement.
%
% 3) A student or employee of a non-profit educational institution may
% use this SOFTWARE subject to the following terms and conditions:
% - this SOFTWARE is for teaching or research purposes only.
% - this SOFTWARE may be distributed to other students or researchers
% provided that these license terms are included.
% - reselling the SOFTWARE, or including it or any portion of it, in any
% software that will be resold is expressly forbidden.
% - transfering the SOFTWARE in any form to a commercial firm or any
% other for-profit organization is expressly forbidden.
%
% END TERMS OF USE LICENSE
%preliminaries
z=z(:);
v=v(:);
p=p(:)'; %make p a row vector
nz=length(z);
%adjust z1 and z2 so that they won't be exactly on layer boundaries
zt=min([z1 z2]);
if(zt==z1)
z1=z1+100000*eps;
z2=z2-100000*eps;
else
z1=z1-100000*eps;
z2=z2+100000*eps;
end
if( z1< z(1) | z2< z(1) )
error(' start or end depth outside model range');
end
%determine layers propagated through
ind=find(z>=z1);
if(isempty(ind))
ibeg=nz;
else
ibeg=ind(1)-1;
end
%compute sin and check for critical angle
ind=find(z>=z2);
if(isempty(ind))
iend=nz;
else
iend=ind(1)-1;
end
if(ibeg~=iend)
% these are the layers propagated thru
iprop=ibeg:sign(iend-ibeg):iend;
else
iprop=ibeg;
end
sn = v(iprop)*p;
%
% sn is an n by m matrix where n is the length of iprop (the number of
% layers propagated through) and m is the length of p (the number of
% unique ray parameters to use). Each column of sn corresponds to a
% single ray parameter and contains the sin of the vertical angle;
%
[ichk,pchk]=find(sn>1);
% if(~isempty(ichk))
% %assign zeros for critical refractions
% sn(ichk,pchk)=zeros(size(sn(ichk,pchk)));
% end
%compute x and t
np=length(iprop);
cs=sqrt(1-sn.*sn);
zprop=[z1;z(iprop(2:np));z2];
vprop=v(iprop)*ones(1,length(p));
thk=abs(diff(zprop))*ones(1,length(p));
if(size(sn,1)>1)
x=sum( (thk.*sn)./cs);
t=sum(thk./(vprop.*cs));
else %single layer case
x=(thk.*sn)./cs;
t=thk./(vprop.*cs);
end
if(~isempty(ichk))
x(pchk)=inf*ones(size(pchk));
t(pchk)=inf*ones(size(pchk));
end
% final angle
if(nargout>2)
phi=180*asin(sn(np,:))/pi;
end
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