The current solar terminator (the non-sunlit part of the Earth) is shown in blue. (Origin: Ben Elsen’s fix of Mike Bostock’s original)
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Earth, night and day sides.
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<!DOCTYPE html> | |
<meta charset="utf-8"> | |
<style> | |
.night { | |
stroke: steelblue; | |
fill: steelblue; | |
fill-opacity: .3; | |
} | |
</style> | |
<body> | |
<script src="http://d3js.org/d3.v3.min.js"></script> | |
<script src="http://d3js.org/d3.geo.projection.v0.min.js"></script> | |
<script src="http://d3js.org/topojson.v0.min.js"></script> | |
<script> | |
var width = 960, | |
height = 500; | |
var projection = d3.geo.cylindricalEqualArea() | |
.parallel(38.5) | |
.scale(196) | |
.precision(.1); | |
var circle = d3.geo.circle() | |
.angle(89.9975572); | |
var path = d3.geo.path() | |
.projection(projection); | |
var svg = d3.select("body").append("svg") | |
.attr("width", width) | |
.attr("height", height); | |
d3.json("/d/4090846/world-50m.json", function(error, world) { | |
svg.append("path") | |
.datum(topojson.object(world, world.objects.land)) | |
.attr("class", "land") | |
.attr("d", path); | |
var night = svg.append("path") | |
.attr("class", "night") | |
.attr("d", path); | |
redraw(); | |
setInterval(redraw, 250); | |
function redraw() { | |
var sunPos = getSolarWGSPosition( Date.now() ); | |
var darknessAngle = 90 - Math.asin( (constants.meanRsun - constants.meanRearth) / sunPos.range ) * constants.rad2deg; | |
night.datum(circle.origin([ -180+sunPos.lon, -sunPos.lat ]).angle(darknessAngle)).attr("d", path); | |
} | |
}); | |
var getSolarWGSPosition = function getSolarWGSPosition(time) { | |
var eci_pos = getSolarECI(time); | |
var wgs_pos = ECItoWGS84(eci_pos, time); | |
return {lat: wgs_pos.latitude, lon: wgs_pos.longitude, range: eci_pos.w}; | |
}; | |
var getSolarECI = function getSolarECI(time) { | |
var mjd, year, T, M, L, e, C, O, Lsa, nu, R, eps; | |
var jd_utc = unix2jd( time / 1000 ); | |
mjd = jd_utc - 2415020.0; | |
year = 1900 + mjd / 365.25; | |
T = (mjd + constants.deltaUTCTT / 86400) / 36525.0; | |
M = (( 358.47583 + ((35999.04975 * T) % 360) - (0.000150 + 0.0000033 * T) * (T*T) ) % 360) * constants.deg2rad; | |
L = ((279.69668 + ((36000.76892 * T) % 360.0) + 0.0003025 * (T*T) ) % 360) * constants.deg2rad; | |
e = 0.01675104 - (0.0000418 + 0.000000126 * T) * T; | |
C = ((1.919460 - (0.004789 + 0.000014 * T) * T) * Math.sin(M) + (0.020094 - 0.000100 * T) * Math.sin(2 * M) + 0.000293 * Math.sin(3 * M)) * constants.deg2rad; | |
O = ((259.18 - 1934.142 * T) % 360) * constants.deg2rad; | |
Lsa = (L + C -((0.00569 - 0.00479 * Math.sin(O)) * constants.deg2rad)) % (2*Math.PI); | |
nu = (M + C) % (2*Math.PI); | |
R = 1.0000002 * (1.0 - (e*e)) / (1.0 + e * Math.cos(nu)); | |
eps = ((23.452294 - (0.0130125 + (0.00000164 - 0.000000503 * T) * T) * T + 0.00256 * Math.cos(O)) * constants.deg2rad); | |
R = constants.au * R; | |
var x = R * Math.cos (Lsa); | |
var y = R * Math.sin (Lsa) * Math.cos (eps); | |
var z = R * Math.sin (Lsa) * Math.sin (eps); | |
var w = R; | |
return { x : x, y : y, z : z, w : w } | |
}; | |
var ECItoWGS84 = function ECItoWGS84(eci, time) { | |
var jd_utc = unix2jd( time / 1000 ); | |
var theta = Math.atan2(eci.y, eci.x); // radians | |
var lon = (theta - thetaG_JD(jd_utc)) % (2*Math.PI); // radians | |
var r = Math.sqrt( (eci.x*eci.x) + (eci.y*eci.y) ); | |
var e2 = constants.f * (2 - constants.f); | |
var lat = Math.atan2(eci.z, r); // radians | |
var sin_phi, phi, c; | |
do { | |
phi = lat; | |
sin_phi = Math.sin(phi); | |
c = 1 / Math.sqrt(1 - e2 * (sin_phi*sin_phi)); | |
lat = Math.atan2(eci.z + constants.eqRearth * c * e2 * sin_phi, r); | |
} while (Math.abs(lat - phi) > 1e-10); | |
var alt = r / Math.cos(lat) - constants.eqRearth * c; // kilometers | |
if (lat > (Math.PI / 2)) { | |
lat -= (2 * Math.PI); | |
} | |
if (lon < -Math.PI) { | |
lon += 2*Math.PI; | |
} | |
return { | |
latitude: lat * constants.rad2deg, | |
longitude: lon * constants.rad2deg, | |
altitude: alt, | |
theta: theta * constants.rad2deg | |
}; | |
}; | |
// ** Astronomical, Geodetic & Mathematical Constants ** // | |
var constants = { | |
au: 149597870700, // [m] Astronomical unit | |
deltaUTCTT: 67.184, | |
deg2rad: 0.017453292519943295, | |
rad2deg: 57.29577951308232, | |
omega_E: 1.00273790934, | |
f: 1/298.257222101, // Earth, reciprocal of flattening IERS 2010 | |
eqRearth: 6378.1366, // Equatorial radius | |
meanRearth: 6371.0, // Mean radius | |
meanRsun: 1.392684e8, // Mean radius sun | |
omega: 7.292115e-5, // Nominal mean angular vel. of Earth rotation | |
}; | |
// Converts a UNIX timestamp to JD (Julian Date) | |
var unix2jd = function unix2jd(timestamp) { | |
return (timestamp / 86400.0) + 2440587.5; | |
}; | |
var thetaG_JD = function thetaG_JD(jd) { | |
// Reference: The 1992 Astronomical Almanac, page B6. | |
var UT, TU, GMST; | |
UT = (jd + 0.5) % 1; | |
jd = jd - UT; | |
TU = (jd - 2451545.0) / 36525; | |
GMST = 24110.54841 + TU * (8640184.812866 + TU * (0.093104 - TU * 6.2e-6)); | |
GMST = (GMST + 86400 * constants.omega_E * UT) % 86400; | |
return (2*Math.PI) * GMST / 86400; | |
}; | |
</script> |
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