Code covered by the BSD License
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CalcEA(M,ecc,tol)
Orbit eccentric anomaly, Kepler's equation keplers equation
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Groundtrack(Kepler,GMSTo,Tf,f...
Orbit groundtrack plot Latitude longitude lat long
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Hohmann(R_init,R_fin,U)
Orbit Hohmann transfer
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JD(yr,day)
Julian Date
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KeplerCOE(Ro,Vo,dT,U,tol)
Orbit Kepler position velocity
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NodeChange(dO,inc,Vinit)
Node change right ascension of the ascending node RAAN raan orbit
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R1(x)
Rotation matrix direction cosine matrix
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R2(x)
Rotation matrix direction cosine matrix
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R3(x)
Rotation matrix direction cosine matrix
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RVtoLatLong(ECEF)
orbit radius velocity latitude longitude ECEF
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TwoBody(t,X,U)
Two body Orbit gravity
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dInc(V,dI,fpa)
Inclination change orbit gravity
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dVdI(R_init,R_fin,Inc,U,Tol)
Inclination change velocity change orbit hohmann transfer
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ecef2eci(ECEF, GST, V_ECEF)
Orbit ECEF ECI Coordinate conversion
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eci2ecef(ECI, GST, V_ECI)
Orbit ECEF ECI Coordinate conversion
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elorb(R,V,U,tol)
Kepler orbital elements ECI Position orbit conversion
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nuFromM(M,ecc,tol)
Kepler Orbit Anomaly true mean
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nuFromTp(Tp,ecc,n,tol)
Kepler Orbit Anomaly true time periapse perigee
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plotorb(ECEF, V_ECEF, mu, Rbo...
Orbit gravity plot orbit spherical
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randv(a,ecc,inc,Omega,w,nu,U)
Kepler orbital elements ECI Position orbit conversion
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topo(ECEF, lat, long, h, Rp)
Orbit range elevation azimuth position ground station site latitude longitude
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zeroTo360(x,unit)
Angle reduce reduction degrees radians
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Constants.m
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View all files
from
Orbital Mechanics Library
by Richard Rieber
A compilation of all of the functions I wrote for my orbital mechanics class
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| RVtoLatLong(ECEF)
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%orbit radius velocity latitude longitude ECEF
% Richard Rieber
% October 17, 2006
% rrieber@gmail.com
%
% [Lat, Long] = RVtoLatLong(ECEF)
%
% Revision 8/21/07: Added H1 line for lookfor functionality.
%
% Revision 9/25/07 - Fixed typo referring to velocity in comments.
% Velocity not needed in this function.
%
% Revision 9/20/09: Removed GMST since it isn't used
%
% Purpose: This fuction convertes ECEF coordinates to Geocentric latitude
% and longitude given ECEF radius in km. Valid for any planetary
% body.
%
% Inputs: o ECI - A 3x1 vector of Earth-Centered Inertial (IJK)
% coordinates in km.
%
% Outputs: o Lat - Geocentic latitude of spacecraft in radians
% o Long - Longitude of spacecraft in radians
%
function [Lat, Long] = RVtoLatLong(ECEF)
if nargin < 1
error('Too few inputs. See help RVtoLatLong')
elseif nargin > 1
error('Too many inputs. See help RVtoLatLong')
end
if length(ECEF) ~= 3
error('ECI length incorrect. See help RVtoLatLong')
end
if nargout ~= 2
error('Incorrect number of outputs. See help RVtoLatLong')
end
r_delta = norm(ECEF(1:2));
sinA = ECEF(2)/r_delta;
cosA = ECEF(1)/r_delta;
Long = atan2(sinA,cosA);
if Long < -pi
Long = Long + 2*pi;
end
Lat = asin(ECEF(3)/norm(ECEF));
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