suncalculator.java

world wind java sdk 源码

package gov.nasa.worldwind.examples.sunlight;

import gov.nasa.worldwind.geom.LatLon;

import java.util.Calendar;

/**
 * @author Michael de Hoog - from http://www.psa.es/sdg/sunpos.htm
 * @version $Id: SunCalculator.java 10406 2009-04-22 18:28:45Z patrickmurris $
 */
public class SunCalculator
{
	public static LatLon subsolarPoint(Calendar time)
	{
		// Main variables
		double elapsedJulianDays;
		double decimalHours;
		double eclipticLongitude;
		double eclipticObliquity;
		double rightAscension, declination;

		// Calculate difference in days between the current Julian Day 
		// and JD 2451545.0, which is noon 1 January 2000 Universal Time
		{
			// Calculate time of the day in UT decimal hours
			decimalHours = time.get(Calendar.HOUR_OF_DAY)
					+ (time.get(Calendar.MINUTE) + time.get(Calendar.SECOND) / 60.0)
					/ 60.0;
			// Calculate current Julian Day
			long aux1 = (time.get(Calendar.MONTH) - 14) / 12;
			long aux2 = (1461 * (time.get(Calendar.YEAR) + 4800 + aux1)) / 4
					+ (367 * (time.get(Calendar.MONTH) - 2 - 12 * aux1)) / 12
					- (3 * ((time.get(Calendar.YEAR) + 4900 + aux1) / 100)) / 4
					+ time.get(Calendar.DAY_OF_MONTH) - 32075;
			double julianDate = (double) (aux2) - 0.5 + decimalHours / 24.0;
			// Calculate difference between current Julian Day and JD 2451545.0 
			elapsedJulianDays = julianDate - 2451545.0;
		}

		// Calculate ecliptic coordinates (ecliptic longitude and obliquity of the 
		// ecliptic in radians but without limiting the angle to be less than 2*Pi 
		// (i.e., the result may be greater than 2*Pi)
		{
			double omega = 2.1429 - 0.0010394594 * elapsedJulianDays;
			double meanLongitude = 4.8950630 + 0.017202791698 * elapsedJulianDays; // Radians
			double meanAnomaly = 6.2400600 + 0.0172019699 * elapsedJulianDays;
			eclipticLongitude = meanLongitude + 0.03341607
					* Math.sin(meanAnomaly) + 0.00034894
					* Math.sin(2 * meanAnomaly) - 0.0001134 - 0.0000203
					* Math.sin(omega);
			eclipticObliquity = 0.4090928 - 6.2140e-9 * elapsedJulianDays
					+ 0.0000396 * Math.cos(omega);
		}

		// Calculate celestial coordinates ( right ascension and declination ) in radians 
		// but without limiting the angle to be less than 2*Pi (i.e., the result may be 
		// greater than 2*Pi)
		{
			double sin_EclipticLongitude = Math.sin(eclipticLongitude);
			double dY = Math.cos(eclipticObliquity) * sin_EclipticLongitude;
			double dX = Math.cos(eclipticLongitude);
			rightAscension = Math.atan2(dY, dX);
			if (rightAscension < 0.0)
				rightAscension = rightAscension + Math.PI * 2.0;
			declination = Math.asin(Math.sin(eclipticObliquity)
					* sin_EclipticLongitude);
		}

		double greenwichMeanSiderealTime = 6.6974243242 + 0.0657098283
				* elapsedJulianDays + decimalHours;
		double longitude = rightAscension
				- Math.toRadians(greenwichMeanSiderealTime * 15.0);
		
		longitude += Math.PI;

		while (declination > Math.PI / 2.0)
			declination -= Math.PI;
		while (declination <= -Math.PI / 2.0)
			declination += Math.PI;
		while (longitude > Math.PI)
			longitude -= Math.PI * 2.0;
		while (longitude <= -Math.PI)
			longitude += Math.PI * 2.0;

		return LatLon.fromRadians(declination, longitude);
	}
}