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author | Mattias Andrée <maandree@kth.se> | 2021-02-19 22:10:26 +0100 |
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committer | Mattias Andrée <maandree@kth.se> | 2021-02-19 22:10:26 +0100 |
commit | ec7baa81e8fd4bec924d6adf3ee880af621a10ba (patch) | |
tree | 700434a1a65c55584dff270ed45e4bdfd46f6ab3 /src | |
parent | Add blue hour (diff) | |
download | solar-python-ec7baa81e8fd4bec924d6adf3ee880af621a10ba.tar.gz solar-python-ec7baa81e8fd4bec924d6adf3ee880af621a10ba.tar.bz2 solar-python-ec7baa81e8fd4bec924d6adf3ee880af621a10ba.tar.xz |
Imrpove makefile and flatten the hier a bit
Signed-off-by: Mattias Andrée <maandree@kth.se>
Diffstat (limited to 'src')
-rw-r--r-- | src/solar_python.py | 846 |
1 files changed, 0 insertions, 846 deletions
diff --git a/src/solar_python.py b/src/solar_python.py deleted file mode 100644 index e336ab4..0000000 --- a/src/solar_python.py +++ /dev/null @@ -1,846 +0,0 @@ -# solar-python — Solar data calculation and prediction library for Python -# Copyright © 2014, 2015 Mattias Andrée (maandree@member.fsf.org) -# -# This program is free software: you can redistribute it and/or modify -# it under the terms of the GNU Affero General Public License as published by -# the Free Software Foundation, either version 3 of the License, or -# (at your option) any later version. -# -# This program is distributed in the hope that it will be useful, -# but WITHOUT ANY WARRANTY; without even the implied warranty of -# MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the -# GNU Affero General Public License for more details. -# -# You should have received a copy of the GNU Affero General Public License -# along with this program. If not, see <http://www.gnu.org/licenses/>. - - - -SOLAR_APPARENT_RADIUS = 32.0 / 60.0 -''' -:float Approximate apparent size of the Sun in degrees -''' - - -SOLAR_ELEVATION_PRESUNSET_POSTSUNRISE = 32.0 / 60.0 -''' -:float The Sun's elevation the beginning of sunset and - end of sunrise, measured in degrees -''' - -SOLAR_ELEVATION_SUNSET_SUNRISE = -32.0 / 60.0 -''' -:float The Sun's elevation the (end of) at sunset and - (beginning of) sunrise, measured in degrees -''' - -SOLAR_ELEVATION_CIVIL_DUSK_DAWN = -6.0 -''' -:float The Sun's elevation at civil dusk and civil - dawn, measured in degrees -''' - -SOLAR_ELEVATION_NAUTICAL_DUSK_DAWN = -12.0 -''' -:float The Sun's elevation at nautical dusk and - nautical dawn, measured in degrees -''' - -SOLAR_ELEVATION_AMATEUR_ASTRONOMICAL_DUSK_DAWN = -15.0 -''' -:float The Sun's elevation at amateur astronomical dusk - and amateur astronomical dawn, measured in degrees -''' - -SOLAR_ELEVATION_ASTRONOMICAL_DUSK_DAWN = -18.0 -''' -:float The Sun's elevation at astronomical dusk - and astronomical dawn, measured in degrees -''' - -SOLAR_ELEVATION_RANGE_TWILIGHT = (-18.0, 0.0) -''' -:(float, float) The Sun's lowest and highest elevation during - all periods of twilight, measured in degrees -''' - -SOLAR_ELEVATION_RANGE_CIVIL_TWILIGHT = (-6.0, SOLAR_ELEVATION_SUNSET_SUNRISE) -''' -:(float, float) The Sun's lowest and highest elevation - during civil twilight, measured in degrees -''' - -SOLAR_ELEVATION_RANGE_NAUTICAL_TWILIGHT = (-12.0, SOLAR_ELEVATION_SUNSET_SUNRISE) -''' -:(float, float) The Sun's lowest and highest elevation - during nautical twilight, measured in degrees -''' - -SOLAR_ELEVATION_RANGE_ASTRONOMICAL_TWILIGHT = (-18.0, SOLAR_ELEVATION_SUNSET_SUNRISE) -''' -:(float, float) The Sun's lowest and highest elevation during - astronomical twilight, measured in degrees -''' - -SOLAR_ELEVATION_RANGE_AMATEUR_ASTRONOMICAL_TWILIGHT = (-18.0, -15.0) -''' -:(float, float) The Sun's lowest and highest elevation during - amateur astronomical twilight, measured in degrees -''' - -SOLAR_ELEVATION_RANGE_GOLDEN_HOUR = (-4.0, 6.0) -''' -:(float, float) The Sun's lowest and highest elevation during - the golden "hour" (also known as magic hour), - measured in degrees. These elevations are - approximate. -''' - -SOLAR_ELEVATION_RANGE_BLUE_HOUR = (-6.0, -4.0) -''' -:(float, float) The Sun's lowest and highest elevation during - the blue "hour", measured in degrees. These - elevations are approximate. -''' - - - -# The following functions are used to calculate the result for `sun` -# (most of them) but could be used for anything else. There name is -# should tell you enough, `t` (and `noon`) is in Julian Centuries -# except for in the convertion methods. - - -def julian_day_to_epoch(t): - ''' - Converts a Julian Day timestamp to a POSIX time timestamp - - @param t:float The time in Julian Days - @return :float The time in POSIX time - ''' - return (t - 2440587.5) * 86400.0 - - -def epoch_to_julian_day(t): - ''' - Converts a POSIX time timestamp to a Julian Day timestamp - - @param t:float The time in POSIX time - @return :float The time in Julian Days - ''' - return t / 86400.0 + 2440587.5 - - -def julian_day_to_julian_centuries(t): - ''' - Converts a Julian Day timestamp to a Julian Centuries timestamp - - @param t:float The time in Julian Days - @return :float The time in Julian Centuries - ''' - return (t - 2451545.0) / 36525.0 - - -def julian_centuries_to_julian_day(t): - ''' - Converts a Julian Centuries timestamp to a Julian Day timestamp - - @param t:float The time in Julian Centuries - @return :float The time in Julian Days - ''' - return t * 36525.0 + 2451545.0 - - -def epoch_to_julian_centuries(t): - ''' - Converts a POSIX time timestamp to a Julian Centuries timestamp - - @param t:float The time in POSIX time - @return :float The time in Julian Centuries - ''' - 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 - - @param t:float The time in Julian Centuries - @return :float The time in POSIX time - ''' - return julian_day_to_epoch(julian_centuries_to_julian_day(t)) - - -def epoch(): - ''' - Get current POSIX time - - @return :float The current POSIX time - ''' - import time - return time.time() - - -def julian_day(): - ''' - Get current Julian Day time - - @return :float The current Julian Day time - ''' - return epoch_to_julian_day(epoch()) - - -def julian_centuries(): - ''' - Get current Julian Centuries time (100 Julian days since J2000) - - @return :float The current Julian Centuries time - ''' - return epoch_to_julian_centuries(epoch()) - - -def radians(deg): - ''' - Convert an angle from degrees to radians - - @param deg:float The angle in degrees - @return :float The angle in radians - ''' - import math - return deg * math.pi / 180 - - -def degrees(rad): - ''' - Convert an angle from radians to degrees - - @param rad:float The angle in radians - @return :float The angle in degrees - ''' - import math - return rad * 180 / math.pi - - -def sun_geometric_mean_longitude(t): - ''' - Calculates the Sun's geometric mean longitude - - @param t:float The time in Julian Centuries - @return :float The Sun's geometric mean longitude in radians - ''' - return radians((0.0003032 * t ** 2 + 36000.76983 * t + 280.46646) % 360) - # CANNIBALISERS: - # The result of this function should always be positive, this - # means that after division modulo 360 but before `radians`, - # you will need to add 360 if the value is negative. This can - # only happen if `t` is negative, which can only happen for date - # times before 2000-(01)Jan-01 12:00:00 UTC par division modulo - # implementations with the signess of at least the left operand. - # More precively, it happens between circa 1970-(01)Jan-11 - # 16:09:02 UTC and circa 374702470660351740 seconds before - # January 1, 1970 00:00 UTC, which is so far back in time - # it cannot be reliable pinned down to the right year, but it - # is without a shadow of a doubt looooong before the Earth - # was formed, is right up there with the age of the Milky Way - # and the universe itself. - - -def sun_geometric_mean_anomaly(t): - ''' - Calculates the Sun's geometric mean anomaly - - @param t:float The time in Julian Centuries - @return :float The Sun's geometric mean anomaly in radians - ''' - return radians(-0.0001537 * t ** 2 + 35999.05029 * t + 357.52911) - - -def earth_orbit_eccentricity(t): - ''' - Calculates the Earth's orbit eccentricity - - @param t:float The time in Julian Centuries - @return :float The Earth's orbit eccentricity - ''' - 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 - the true anomaly and the mean anomaly - - @param t:float The time in Julian Centuries - @return :float The Sun's equation of the centre, in radians - ''' - import math - a = sun_geometric_mean_anomaly(t) - rc = math.sin(1 * a) * (-0.000014 * t ** 2 - 0.004817 * t + 1.914602) - rc += math.sin(2 * a) * (-0.000101 * t + 0.019993) - rc += math.sin(3 * a) * 0.000289 - return radians(rc) - - -def sun_real_longitude(t): - ''' - Calculates the Sun's real longitudinal position - - @param t:float The time in Julian Centuries - @return :float The longitude, in radians - ''' - 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 - - @param t:float The time in Julian Centuries - @return :float The longitude, in radians - ''' - import math - rc = degrees(sun_real_longitude(t)) - 0.00569 - 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 - - @param t:float The time in Julian Centuries - @return :float The uncorrected mean obliquity, in radians - ''' - rc = 0.001813 * t ** 3 - 0.00059 * t ** 2 - 46.815 * t + 21.448 - rc = 26 + rc / 60 - 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 - - @param t:float The time in Julian Centuries - @return :float The mean obliquity, in radians - ''' - import math - rc = -1934.136 * t + 125.04 - rc = 0.00256 * math.cos(radians(rc)) - rc += degrees(mean_ecliptic_obliquity(t)) - return radians(rc) - - -def solar_declination(t): - ''' - Calculates the Sun's declination - - @param t:float The time in Julian Centuries - @return :float The Sun's declination, in radians - ''' - import math - rc = math.sin(corrected_mean_ecliptic_obliquity(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 - - @param t:float The time in Julian Centuries - @return :float The equation of time, in degrees - ''' - import math - l = sun_geometric_mean_longitude(t) - e = earth_orbit_eccentricity(t) - m = sun_geometric_mean_anomaly(t) - y = corrected_mean_ecliptic_obliquity(t) - y = math.tan(y / 2) ** 2 - rc = y * math.sin(2 * l) - rc += (4 * y * math.cos(2 * l) - 2) * e * math.sin(m) - rc -= 0.5 * y ** 2 * math.sin(4 * l) - 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 - - @param longitude:float The longitude in degrees eastwards - from Greenwich, negative for westwards - @param declination:float The declination, in radians - @param elevation:float The Sun's elevation, in radians - @return :float The solar hour angle, in radians - ''' - import math - if elevation == 0: - return 0 - rc = math.cos(abs(elevation)) - rc -= math.sin(radians(latitude)) * math.sin(declination) - rc /= math.cos(radians(latitude)) * math.cos(declination) - 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 - - @param longitude:float The longitude in degrees eastwards - from Greenwich, negative for westwards - @param declination:float The declination, in radians - @param hour_angle:float The solar hour angle, in radians - @return :float The Sun's elevation, in radians - ''' - import math - rc = math.cos(radians(latitude)) - rc *= math.cos(hour_angle) * math.cos(declination) - 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 - - @param t:float A time close to the sought time, - in Julian Centuries - @param longitude:float The longitude in degrees eastwards from - Greenwich, negative for westwards - @return :float The time, in Julian Centuries, - of the closest solar noon - ''' - t, rc = julian_centuries_to_julian_day(t), longitude - for (k, m) in ((-360, 0), (1440, -0.5)): - rc = julian_day_to_julian_centuries(t + m + rc / k) - 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 - - @param t:float A time close to the sought time, - in Julian Centuries - @param noon:float The time of the closest solar noon - @param latitude:float The latitude in degrees northwards from - the equator, negative for southwards - @param longitude:float The longitude in degrees eastwards from - Greenwich, negative for westwards - @param elevation:float The solar elevation, in radians - @return :float The time, in Julian Centuries, - of the specified elevation - ''' - rc = noon - rc, et = solar_declination(rc), equation_of_time(rc) - rc = hour_angle_from_elevation(latitude, rc, elevation) - rc = 720 - 4 * (longitude + degrees(rc)) - et - - rc = julian_day_to_julian_centuries(julian_centuries_to_julian_day(t) + rc / 1440) - rc, et = solar_declination(rc), equation_of_time(rc) - rc = hour_angle_from_elevation(latitude, rc, elevation) - rc = 720 - 4 * (longitude + degrees(rc)) - et - return rc - - -def solar_elevation_from_time(t, latitude, longitude): - ''' - Calculates the Sun's elevation as apparent - from a geographical position - - @param t:float The time in Julian Centuries - @param latitude:float The latitude in degrees northwards from - the equator, negative for southwards - @param longitude:float The longitude in degrees eastwards from - Greenwich, negative for westwards - @return :float The Sun's apparent elevation at the specified - time as seen from the specified position, - measured in radians - ''' - rc = julian_centuries_to_julian_day(t) - rc = (rc - float(int(rc + 0.5)) - 0.5) * 1440 - rc = 720 - rc - equation_of_time(t) - rc = radians(rc / 4 - longitude) - return elevation_from_hour_angle(latitude, solar_declination(t), rc) - - -def solar_elevation(latitude, longitude, t = None): - ''' - Calculates the Sun's elevation as apparent - from a geographical position - - @param latitude:float The latitude in degrees northwards from - the equator, negative for southwards - @param longitude:float The longitude in degrees eastwards from - Greenwich, negative for westwards - @param t:float? The time in Julian Centuries, `None` - for the current time - @return :float The Sun's apparent elevation at the specified - time as seen from the specified position, - measured in degrees - ''' - rc = julian_centuries() if t is None else t - rc = solar_elevation_from_time(rc, latitude, longitude) - return degrees(rc) - - - -def have_sunrise_and_sunset(latitude, t = None): - ''' - Determine whether solar declination currently is - so that there can be sunrises and sunsets. If not, - you either have 24-hour daytime or 24-hour nighttime. - - @param latitude:float The latitude in degrees northwards from - the equator, negative for southwards - @param t:float? The time in Julian Centuries, `None` - for the current time - @return Whether there can be sunrises and - sunsets where you are located - ''' - t = julian_centuries() if t is None else t - d = degrees(solar_declination(t)) - ## Convert everything to the Northern hemisphere - latitude = abs(latitude) - if d >= 0: - ## Northern summer - return -90 + d < latitude < 90 - d - else: - ## Northern winter - return -90 - d < latitude < 90 + d - - -def is_summer(latitude, t = None): - ''' - Determine whether it is summer - - @param latitude:float The latitude in degrees northwards from - the equator, negative for southwards - @param t:float? The time in Julian Centuries, `None` - for the current time - @return Whether it is summer on the hemisphere - you are located on - ''' - t = julian_centuries() if t is None else t - d = solar_declination(t) - return (d > 0) == (latitude > 0) - - -def is_winter(latitude, t = None): - ''' - Determine whether it is winter - - @param latitude:float The latitude in degrees northwards from - the equator, negative for southwards - @param t:float? The time in Julian Centuries, `None` - for the current time - @return Whether it is winter on the hemisphere - you are located on - ''' - t = julian_centuries() if t is None else t - d = solar_declination(t) - return not ((d > 0) == (latitude > 0)) - - - -def solar_prediction(delta, requested, fun, epsilon = 0.000001, span = 0.01, t = None): - ''' - Predict the time point of the next or previous - time an arbitrary condition is meet - - @param delta:float Iteration step size, negative for past - event, positive for future event - @param requested:float The value returned by `fun` for which to - calculate the time point of occurrence - @param fun:(t:float)→float Function that calculate the data of interest - @param epsilon:float The tolerance for the result - @param span:float The number of Julian Centuries (0,01 for - one year) to restrict the search to - @param t:float? The time in Julian Centuries, `None` for - the current time - @return :float? The calculated time point, `None` if none - were found within the specified time span - ''' - fun_ = lambda t : fun(t) - requested - t = julian_centuries() if t is None else t - t1 = t2 = t - v1 = v0 = fun_(t) - - # Predicate time point to within a small time span - while True: - if abs(t2 - t) > span: - return None - t2 += delta - v2 = fun_(t2) - if (v1 <= 0 <= v2) or ((0 >= v1 >= v2) and (0 <= v0)): - break - if (v1 >= 0 >= v2) or ((0 <= v1 <= v2) and (0 >= v0)): - break - t1 = t2 - v2 = v1 - - # Binary search the small time span for the exact time point - for _itr in range(1000): - tm = (t1 + t2) / 2 - v1 = fun_(t1) - v2 = fun_(t2) - vm = fun_(tm) - if abs(v1 - v2) < epsilon: - return tm - if v1 < v2: - if 0 < vm: - t2 = tm - else: - t1 = tm - elif v1 > v2: - if 0 > vm: - t2 = tm - else: - t1 = tm - return tm - - - -def future_past_equinox(delta, t = None): - ''' - Predict the time point of the next or previous equinox - - @param delta:float Iteration step size, negative for - past event, positive for future event - @param t:float? The time in Julian Centuries, `None` - for the current time - @return :float The calculated time point - ''' - return solar_prediction(delta, 0, solar_declination, t = t) - - -def future_equinox(t = None): - ''' - Predict the time point of the next equinox - - @param t:float? The time in Julian Centuries, `None` - for the current time - @return :float The calculated time point - ''' - return future_past_equinox(0.01 / 2000, t) - - -def past_equinox(t = None): - ''' - Predict the time point of the previous equinox - - @param t:float? The time in Julian Centuries, `None` - for the current time - @return :float The calculated time point - ''' - return future_past_equinox(0.01 / -2000, t) - - - -def future_past_solstice(delta, t = None): - ''' - Predict the time point of the next or previous solstice - - @param delta:float Iteration step size, negative for - past event, positive for future event - @param t:float? The time in Julian Centuries, `None` - for the current time - @return :float The calculated time point - ''' - e = 0.00001 - fun = solar_declination - dfun = lambda t : (fun(t + e) - fun(t - e)) / (2 * e) - return solar_prediction(delta, 0, dfun, t = t) - - -def future_solstice(t = None): - ''' - Predict the time point of the next solstice - - @param t:float? The time in Julian Centuries, - `None` for the current time - @return :float The calculated time point - ''' - return future_past_solstice(0.01 / 2000, t) - - -def past_solstice(t = None): - ''' - Predict the time point of the previous solstice - - @param t:float? The time in Julian Centuries, - `None` for the current time - @return :float The calculated time point - ''' - return future_past_solstice(0.01 / -2000, t) - - - -def future_past_elevation(delta, latitude, longitude, elevation, t = None): - ''' - Predict the time point of the next or previous time - the Sun reaches or reached a specific elevation - - @param delta:float Iteration step size, negative for past - event, positive for future event - @param latitude:float The latitude in degrees northwards from - the equator, negative for southwards - @param longitude:float The longitude in degrees eastwards from - Greenwich, negative for westwards - @param elevation:float The elevation of interest - @param t:float? The time in Julian Centuries, `None` - for the current time - @return :float? The calculated time point, `None` if - none were found within a year - ''' - fun = lambda t : solar_elevation(latitude, longitude, t) - return solar_prediction(delta, elevation, fun, t = t) - - -def future_elevation(latitude, longitude, elevation, t = None): - ''' - Predict the time point of the next time the Sun - reaches a specific elevation - - @param latitude:float The latitude in degrees northwards from - the equator, negative for southwards - @param longitude:float The longitude in degrees eastwards from - Greenwich, negative for westwards - @param elevation:float The elevation of interest - @param t:float? The time in Julian Centuries, `None` - for the current time - @return :float? The calculated time point, `None` if - none were found within a year - ''' - return future_past_elevation(0.01 / 2000, latitude, longitude, elevation, t) - - -def past_elevation(latitude, longitude, elevation, t = None): - ''' - Predict the time point of the previous time the Sun - reached a specific elevation - - @param latitude:float The latitude in degrees northwards from - the equator, negative for southwards - @param longitude:float The longitude in degrees eastwards from - Greenwich, negative for westwards - @param elevation:float The elevation of interest - @param t:float? The time in Julian Centuries, `None` - for the current time - @return :float? The calculated time point, `None` if - none were found within a year - ''' - return future_past_elevation(0.01 / -2000, latitude, longitude, elevation, t) - - - -def future_past_elevation_derivative(delta, latitude, longitude, derivative, t = None): - ''' - Predict the time point of the next or previous time the - Sun reaches or reached a specific elevation derivative - - @param delta:float Iteration step size, negative for past - event, positive for future event - @param latitude:float The latitude in degrees northwards from - the equator, negative for southwards - @param longitude:float The longitude in degrees eastwards from - Greenwich, negative for westwards - @param derivative:float The elevation derivative value of interest - @param t:float? The time in Julian Centuries, `None` - for the current time - @return :float? The calculated time point, `None` if - none were found within a year - ''' - e = 0.00001 - fun = lambda t : solar_elevation(latitude, longitude, t) - dfun = lambda t : (fun(t + e) - fun(t - e)) / (2 * e) - return solar_prediction(delta, derivative, dfun, t = t) - - -def future_elevation_derivative(latitude, longitude, derivative, t = None): - ''' - Predict the time point of the next time the - Sun reaches a specific elevation derivative - - @param latitude:float The latitude in degrees northwards from - the equator, negative for southwards - @param longitude:float The longitude in degrees eastwards from - Greenwich, negative for westwards - @param derivative:float The elevation derivative value of interest - @param t:float? The time in Julian Centuries, `None` - for the current time - @return :float? The calculated time point, `None` if - none were found within a year - ''' - return future_past_elevation_derivative(0.01 / 2000, latitude, longitude, derivative, t) - - -def past_elevation_derivative(latitude, longitude, derivative, t = None): - ''' - Predict the time point of the previous time - the Sun reached a specific elevation derivative - - @param latitude:float The latitude in degrees northwards from - the equator, negative for southwards - @param longitude:float The longitude in degrees eastwards from - Greenwich, negative for westwards - @param derivative:float The elevation derivative value of interest - @param t:float? The time in Julian Centuries, `None` - for the current time - @return :float? The calculated time point, `None` - if none were found within a year - ''' - return future_past_elevation_derivative(0.01 / -2000, latitude, longitude, derivative, t) - - - -# TODO: This algorithm is imprecise, gives an incorrent sunrise and I do not fully know its behaviour -def sunrise_equation(latitude, longitude, t = None): - import math - # Calculate Julian Cycle - j_cent = julian_centuries() if t is None else t - j_date = julian_centuries_to_julian_day(j_cent) - j_cycle = int(j_date - 2451545.0009 - longitude / 360 + 0.5) - - # Calculate approximate solar noon and solar man anomaly - approx_solar_noon = 451545.0009 + longitude / 360 + j_cycle - solar_mean_anomaly = int(357.5291 + 0.98560028 * (j_cycle - 2451545)) % 360 - - # Calculate solar equation of centre - equation_of_centre = 1.9148 * math.sin(1 * solar_mean_anomaly) - equation_of_centre += 0.0200 * math.sin(2 * solar_mean_anomaly) - equation_of_centre += 0.0003 * math.sin(3 * solar_mean_anomaly) - - # Calculate solar ecliptic longitude - ecliptic_longitude = (solar_mean_anomaly + 102.9372 + equation_of_centre + 180) % 360 - - # Calculate solar transit - solar_transit = approx_solar_noon + 0.0053 * math.sin(solar_mean_anomaly) - solar_transit -= 0.0069 * math.sin(2 * ecliptic_longitude) - - # Calculate solar declination - declination = math.asin(math.sin(ecliptic_longitude) * math.sin(radians(23.45))) - - # Calculate solar hour angle - hour_angle = math.sin(radians(-0.83)) - hour_angle -= math.sin(latitude) * math.sin(declination) - hour_angle /= math.cos(latitude) * math.cos(declination) - hour_angle = degrees(math.acos(hour_angle)) - - # Calculate time of sunset and sunrise - sunset = 2451545.0009 + (hour_angle + longitude) / 360 - sunset += j_cycle + solar_transit - approx_solar_noon - sunrise = 2 * solar_transit - sunset - - # Convert to Julian Centuries - return (julian_day_to_julian_centuries(sunset), - julian_day_to_julian_centuries(sunrise)) - |