From ab7edbdecb82a654c300d88d75227e3a5c211a1f Mon Sep 17 00:00:00 2001 From: Mattias Andrée Date: Sat, 29 Mar 2014 14:30:29 +0100 Subject: whitespace MIME-Version: 1.0 Content-Type: text/plain; charset=UTF-8 Content-Transfer-Encoding: 8bit Signed-off-by: Mattias Andrée --- src/solar.py | 26 ++++++++++++++++++++++++++ 1 file changed, 26 insertions(+) (limited to 'src') diff --git a/src/solar.py b/src/solar.py index 041d427..24370c1 100644 --- a/src/solar.py +++ b/src/solar.py @@ -98,6 +98,7 @@ def julian_day_to_epoch(t): ''' return (t - 2440587.5) * 86400.0 + def epoch_to_julian_day(t): ''' Converts a POSIX time timestamp to a Julian Day timestamp @@ -107,6 +108,7 @@ def epoch_to_julian_day(t): ''' return t / 86400.0 + 2440587.5 + def julian_day_to_julian_centuries(t): ''' Converts a Julian Day timestamp to a Julian Centuries timestamp @@ -116,6 +118,7 @@ def julian_day_to_julian_centuries(t): ''' return (t - 2451545.0) / 36525.0 + def julian_centuries_to_julian_day(t): ''' Converts a Julian Centuries timestamp to a Julian Day timestamp @@ -125,6 +128,7 @@ def julian_centuries_to_julian_day(t): ''' return t * 36525.0 + 2451545.0 + def epoch_to_julian_centuries(t): ''' Converts a POSIX time timestamp to a Julian Centuries timestamp @@ -134,6 +138,7 @@ def epoch_to_julian_centuries(t): ''' return julian_day_to_julian_centuries(epoch_to_julian_day(t)) + def julian_centuries_to_epoch(t): ''' Converts a Julian Centuries timestamp to a POSIX time timestamp @@ -143,6 +148,7 @@ def julian_centuries_to_epoch(t): ''' return julian_day_to_epoch(julian_centuries_to_julian_day(t)) + def epoch(): ''' Get current POSIX time @@ -151,6 +157,7 @@ def epoch(): ''' return time.time() + def julian_day(): ''' Get current Julian Day time @@ -159,6 +166,7 @@ def julian_day(): ''' return epoch_to_julian_day(epoch()) + def julian_centuries(): ''' Get current Julian Centuries time (100 Julian days since J2000) @@ -167,6 +175,7 @@ def julian_centuries(): ''' return epoch_to_julian_centuries(epoch()) + def radians(deg): ''' Convert an angle from degrees to radians @@ -176,6 +185,7 @@ def radians(deg): ''' return deg * math.pi / 180 + def degrees(rad): ''' Convert an angle from radians to degrees @@ -185,6 +195,7 @@ def degrees(rad): ''' return rad * 180 / math.pi + def sun_geometric_mean_longitude(t): ''' Calculates the Sun's geometric mean longitude @@ -194,6 +205,7 @@ def sun_geometric_mean_longitude(t): ''' return radians((0.0003032 * t ** 2 + 36000.76983 * t + 280.46646) % 360) + def sun_geometric_mean_anomaly(t): ''' Calculates the Sun's geometric mean anomaly @@ -203,6 +215,7 @@ def sun_geometric_mean_anomaly(t): ''' return radians(-0.0001537 * t ** 2 + 35999.05029 * t + 357.52911) + def earth_orbit_eccentricity(t): ''' Calculates the Earth's orbit eccentricity @@ -212,6 +225,7 @@ def earth_orbit_eccentricity(t): ''' return -0.0000001267 * t ** 2 - 0.000042037 * t + 0.016708634 + def sun_equation_of_centre(t): ''' Calculates the Sun's equation of the centre, the difference between @@ -226,6 +240,7 @@ def sun_equation_of_centre(t): rc += math.sin(3 * a) * 0.000289 return radians(rc) + def sun_real_longitude(t): ''' Calculates the Sun's real longitudinal position @@ -236,6 +251,7 @@ def sun_real_longitude(t): rc = sun_geometric_mean_longitude(t) return rc + sun_equation_of_centre(t) + def sun_apparent_longitude(t): ''' Calculates the Sun's apparent longitudinal position @@ -247,6 +263,7 @@ def sun_apparent_longitude(t): rc -= 0.00478 * math.sin(radians(-1934.136 * t + 125.04)) return radians(rc) + def mean_ecliptic_obliquity(t): ''' Calculates the mean ecliptic obliquity of the Sun's apparent motion without variation correction @@ -259,6 +276,7 @@ def mean_ecliptic_obliquity(t): rc = 23 + rc / 60 return radians(rc) + def corrected_mean_ecliptic_obliquity(t): ''' Calculates the mean ecliptic obliquity of the Sun's apparent motion with variation correction @@ -271,6 +289,7 @@ def corrected_mean_ecliptic_obliquity(t): rc += degrees(mean_ecliptic_obliquity(t)) return radians(rc) + def solar_declination(t): ''' Calculates the Sun's declination @@ -282,6 +301,7 @@ def solar_declination(t): rc *= math.sin(sun_apparent_longitude(t)) return math.asin(rc) + def equation_of_time(t): ''' Calculates the equation of time, the discrepancy between apparent and mean solar time @@ -300,6 +320,7 @@ def equation_of_time(t): rc -= 1.25 * e ** 2 * math.sin(2 * m) return 4 * degrees(rc) + def hour_angle_from_elevation(latitude, declination, elevation): ''' Calculates the solar hour angle from the Sun's elevation @@ -317,6 +338,7 @@ def hour_angle_from_elevation(latitude, declination, elevation): rc = math.acos(rc) return -rc if (rc < 0) == (elevation < 0) else rc; + def elevation_from_hour_angle(latitude, declination, hour_angle): ''' Calculates the Sun's elevation from the solar hour angle @@ -331,6 +353,7 @@ def elevation_from_hour_angle(latitude, declination, hour_angle): rc += math.sin(radians(latitude)) * math.sin(declination) return math.asin(rc) + def time_of_solar_noon(t, longitude): ''' Calculates the time of the closest solar noon @@ -345,6 +368,7 @@ def time_of_solar_noon(t, longitude): rc = 720 - 4 * longitude - equation_of_time(rc) return rc + def time_of_solar_elevation(t, noon, latitude, longitude, elevation): ''' Calculates the time the Sun has a specified apparent elevation at a geographical position @@ -367,6 +391,7 @@ def time_of_solar_elevation(t, noon, latitude, longitude, elevation): rc = 720 - 4 * (longitude + degrees(rc)) - et return rc + def solar_elevation_from_time(t, latitude, longitude): ''' Calculates the Suns elevation as apparent from a geographical position @@ -383,6 +408,7 @@ def solar_elevation_from_time(t, latitude, longitude): rc = radians(rc / 4 - longitude) return elevation_from_hour_angle(latitude, solar_declination(t), rc) + def solar_elevation(latitude, longitude, t = None): ''' Calculates the Suns elevation as apparent from a geographical position -- cgit v1.2.3-70-g09d2