Sg-ifying names.
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@@ -59,12 +59,12 @@ void CelestialBody::updatePosition(double mjd, Star *ourSun)
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xv, yv, xh, yh, zh, xg, yg, zg, xe, ye, ze;
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updateOrbElements(mjd);
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actTime = fgCalcActTime(mjd);
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actTime = sgCalcActTime(mjd);
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// calcualate the angle bewteen ecliptic and equatorial coordinate system
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ecl = DEG_TO_RAD * (23.4393 - 3.563E-7 *actTime);
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eccAnom = fgCalcEccAnom(M, e); //calculate the eccentric anomaly
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eccAnom = sgCalcEccAnom(M, e); //calculate the eccentric anomaly
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xv = a * (cos(eccAnom) - e);
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yv = a * (sqrt (1.0 - e*e) * sin(eccAnom));
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v = atan2(yv, xv); // the planet's true anomaly
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@@ -111,7 +111,7 @@ void CelestialBody::updatePosition(double mjd, Star *ourSun)
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};
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/****************************************************************************
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* double CelestialBody::fgCalcEccAnom(double M, double e)
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* double CelestialBody::sgCalcEccAnom(double M, double e)
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* this private member calculates the eccentric anomaly of a celestial body,
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* given its mean anomaly and eccentricity.
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*
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@@ -136,7 +136,7 @@ void CelestialBody::updatePosition(double mjd, Star *ourSun)
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* the eccentric anomaly
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*
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****************************************************************************/
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double CelestialBody::fgCalcEccAnom(double M, double e)
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double CelestialBody::sgCalcEccAnom(double M, double e)
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{
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double
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eccAnom, E0, E1, diff;
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@@ -60,8 +60,8 @@ protected: // make the data protected, in order to give the
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double magnitude;
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double lonEcl, latEcl;
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double fgCalcEccAnom(double M, double e);
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double fgCalcActTime(double mjd);
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double sgCalcEccAnom(double M, double e);
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double sgCalcActTime(double mjd);
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void updateOrbElements(double mjd);
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public:
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@@ -149,7 +149,7 @@ inline CelestialBody::CelestialBody(double Nf, double Ns,
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***************************************************************************/
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inline void CelestialBody::updateOrbElements(double mjd)
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{
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double actTime = fgCalcActTime(mjd);
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double actTime = sgCalcActTime(mjd);
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M = DEG_TO_RAD * (MFirst + (MSec * actTime));
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w = DEG_TO_RAD * (wFirst + (wSec * actTime));
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N = DEG_TO_RAD * (NFirst + (NSec * actTime));
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@@ -158,7 +158,7 @@ inline void CelestialBody::updateOrbElements(double mjd)
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a = aFirst + (aSec * actTime);
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}
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/*****************************************************************************
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* inline double CelestialBody::fgCalcActTime(double mjd)
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* inline double CelestialBody::sgCalcActTime(double mjd)
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* this private member function returns the offset in days from the epoch for
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* wich the orbital elements are calculated (Jan, 1st, 2000).
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*
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@@ -166,7 +166,7 @@ inline void CelestialBody::updateOrbElements(double mjd)
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*
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* return value: the (fractional) number of days until Jan 1, 2000.
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****************************************************************************/
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inline double CelestialBody::fgCalcActTime(double mjd)
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inline double CelestialBody::sgCalcActTime(double mjd)
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{
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return (mjd - 36523.5);
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}
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@@ -88,12 +88,12 @@ void Moon::updatePosition(double mjd, double lst, double lat, Star *ourSun)
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geoRa, geoDec;
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updateOrbElements(mjd);
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actTime = fgCalcActTime(mjd);
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actTime = sgCalcActTime(mjd);
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// calculate the angle between ecliptic and equatorial coordinate system
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// in Radians
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ecl = ((DEG_TO_RAD * 23.4393) - (DEG_TO_RAD * 3.563E-7) * actTime);
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eccAnom = fgCalcEccAnom(M, e); // Calculate the eccentric anomaly
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eccAnom = sgCalcEccAnom(M, e); // Calculate the eccentric anomaly
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xv = a * (cos(eccAnom) - e);
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yv = a * (sqrt(1.0 - e*e) * sin(eccAnom));
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v = atan2(yv, xv); // the moon's true anomaly
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@@ -67,7 +67,7 @@ void Saturn::updatePosition(double mjd, Star *ourSun)
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{
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CelestialBody::updatePosition(mjd, ourSun);
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double actTime = fgCalcActTime(mjd);
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double actTime = sgCalcActTime(mjd);
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double ir = 0.4897394;
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double Nr = 2.9585076 + 6.6672E-7*actTime;
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double B = asin (sin(declination) * cos(ir) -
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@@ -84,9 +84,9 @@ void Star::updatePosition(double mjd)
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updateOrbElements(mjd);
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actTime = fgCalcActTime(mjd);
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actTime = sgCalcActTime(mjd);
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ecl = DEG_TO_RAD * (23.4393 - 3.563E-7 * actTime); // Angle in Radians
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eccAnom = fgCalcEccAnom(M, e); // Calculate the eccentric Anomaly (also known as solving Kepler's equation)
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eccAnom = sgCalcEccAnom(M, e); // Calculate the eccentric Anomaly (also known as solving Kepler's equation)
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xv = cos(eccAnom) - e;
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yv = sqrt (1.0 - e*e) * sin(eccAnom);
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