Example #1
0
        public static AASPhysicalSunDetails Calculate(double JD)
        {
            double theta = AASCoordinateTransformation.MapTo0To360Range((JD - 2398220) * 360 / 25.38);
            double I     = 7.25;
            double K     = 73.6667 + 1.3958333 * (JD - 2396758) / 36525;

            //Calculate the apparent longitude of the sun (excluding the effect of nutation)
            double L       = AASEarth.EclipticLongitude(JD);
            double R       = AASEarth.RadiusVector(JD);
            double SunLong = L + 180 - AASCoordinateTransformation.DMSToDegrees(0, 0, 20.4898 / R);

            double epsilon = AASNutation.TrueObliquityOfEcliptic(JD);

            //Convert to radians
            epsilon = AASCoordinateTransformation.DegreesToRadians(epsilon);
            SunLong = AASCoordinateTransformation.DegreesToRadians(SunLong);
            K       = AASCoordinateTransformation.DegreesToRadians(K);
            I       = AASCoordinateTransformation.DegreesToRadians(I);
            theta   = AASCoordinateTransformation.DegreesToRadians(theta);

            double x = Math.Atan(-Math.Cos(SunLong) * Math.Tan(epsilon));
            double y = Math.Atan(-Math.Cos(SunLong - K) * Math.Tan(I));

            AASPhysicalSunDetails details = new AASPhysicalSunDetails();

            details.P  = AASCoordinateTransformation.RadiansToDegrees(x + y);
            details.B0 = AASCoordinateTransformation.RadiansToDegrees(Math.Asin(Math.Sin(SunLong - K) * Math.Sin(I)));

            double eta = Math.Atan(Math.Tan(SunLong - K) * Math.Cos(I));

            details.L0 = AASCoordinateTransformation.MapTo0To360Range(AASCoordinateTransformation.RadiansToDegrees(eta - theta));

            return(details);
        }
Example #2
0
        public static AASPhysicalSunDetails Calculate(double JD)
        {
            double theta = AASCoordinateTransformation.MapTo0To360Range((JD - 2398220) * 360 / 25.38);
            double I = 7.25;
            double K = 73.6667 + 1.3958333 * (JD - 2396758) / 36525;

            //Calculate the apparent longitude of the sun (excluding the effect of nutation)
            double L = AASEarth.EclipticLongitude(JD);
            double R = AASEarth.RadiusVector(JD);
            double SunLong = L + 180 - AASCoordinateTransformation.DMSToDegrees(0, 0, 20.4898 / R);

            double epsilon = AASNutation.TrueObliquityOfEcliptic(JD);

            //Convert to radians
            epsilon = AASCoordinateTransformation.DegreesToRadians(epsilon);
            SunLong = AASCoordinateTransformation.DegreesToRadians(SunLong);
            K = AASCoordinateTransformation.DegreesToRadians(K);
            I = AASCoordinateTransformation.DegreesToRadians(I);
            theta = AASCoordinateTransformation.DegreesToRadians(theta);

            double x = Math.Atan(-Math.Cos(SunLong) * Math.Tan(epsilon));
            double y = Math.Atan(-Math.Cos(SunLong - K) * Math.Tan(I));

            AASPhysicalSunDetails details = new AASPhysicalSunDetails();

            details.P = AASCoordinateTransformation.RadiansToDegrees(x + y);
            details.B0 = AASCoordinateTransformation.RadiansToDegrees(Math.Asin(Math.Sin(SunLong - K) * Math.Sin(I)));

            double eta = Math.Atan(Math.Tan(SunLong - K) * Math.Cos(I));
            details.L0 = AASCoordinateTransformation.MapTo0To360Range(AASCoordinateTransformation.RadiansToDegrees(eta - theta));

            return details;
        }