adhan-extended
Version:
High precision Islamic prayer time library (extended)
62 lines (40 loc) • 3.11 kB
JavaScript
;
Object.defineProperty(exports, "__esModule", {
value: true
});
exports["default"] = void 0;
var _Astronomical = _interopRequireDefault(require("./Astronomical"));
var _MathUtils = require("./MathUtils");
function _interopRequireDefault(obj) { return obj && obj.__esModule ? obj : { "default": obj }; }
function _defineProperties(target, props) { for (var i = 0; i < props.length; i++) { var descriptor = props[i]; descriptor.enumerable = descriptor.enumerable || false; descriptor.configurable = true; if ("value" in descriptor) descriptor.writable = true; Object.defineProperty(target, descriptor.key, descriptor); } }
function _createClass(Constructor, protoProps, staticProps) { if (protoProps) _defineProperties(Constructor.prototype, protoProps); if (staticProps) _defineProperties(Constructor, staticProps); Object.defineProperty(Constructor, "prototype", { writable: false }); return Constructor; }
function _classCallCheck(instance, Constructor) { if (!(instance instanceof Constructor)) { throw new TypeError("Cannot call a class as a function"); } }
var SolarCoordinates = /*#__PURE__*/_createClass(function SolarCoordinates(julianDay) {
_classCallCheck(this, SolarCoordinates);
var T = _Astronomical["default"].julianCentury(julianDay);
var L0 = _Astronomical["default"].meanSolarLongitude(T);
var Lp = _Astronomical["default"].meanLunarLongitude(T);
var Omega = _Astronomical["default"].ascendingLunarNodeLongitude(T);
var Lambda = (0, _MathUtils.degreesToRadians)(_Astronomical["default"].apparentSolarLongitude(T, L0));
var Theta0 = _Astronomical["default"].meanSiderealTime(T);
var dPsi = _Astronomical["default"].nutationInLongitude(T, L0, Lp, Omega);
var dEpsilon = _Astronomical["default"].nutationInObliquity(T, L0, Lp, Omega);
var Epsilon0 = _Astronomical["default"].meanObliquityOfTheEcliptic(T);
var EpsilonApparent = (0, _MathUtils.degreesToRadians)(_Astronomical["default"].apparentObliquityOfTheEcliptic(T, Epsilon0));
/* declination: The declination of the sun, the angle between
the rays of the Sun and the plane of the Earth's
equator, in degrees.
Equation from Astronomical Algorithms page 165 */
this.declination = (0, _MathUtils.radiansToDegrees)(Math.asin(Math.sin(EpsilonApparent) * Math.sin(Lambda)));
/* rightAscension: Right ascension of the Sun, the angular distance on the
celestial equator from the vernal equinox to the hour circle,
in degrees.
Equation from Astronomical Algorithms page 165 */
this.rightAscension = (0, _MathUtils.unwindAngle)((0, _MathUtils.radiansToDegrees)(Math.atan2(Math.cos(EpsilonApparent) * Math.sin(Lambda), Math.cos(Lambda))));
/* apparentSiderealTime: Apparent sidereal time, the hour angle of the vernal
equinox, in degrees.
Equation from Astronomical Algorithms page 88 */
this.apparentSiderealTime = Theta0 + dPsi * 3600 * Math.cos((0, _MathUtils.degreesToRadians)(Epsilon0 + dEpsilon)) / 3600;
});
exports["default"] = SolarCoordinates;
//# sourceMappingURL=SolarCoordinates.js.map