def __init__(self, fMoonMeanElongation, fSunMeanAnomaly, fMoonMeanAnomaly, fMoonArgumentOfLatitude, fEccentricity):
toolObjectSerializable.__init__(self)
self._fMoonMeanElongation = fMoonMeanElongation
self._fSunMeanAnomaly = fSunMeanAnomaly
self._fMoonMeanAnomaly = fMoonMeanAnomaly
self._fMoonArgumentOfLatitude = fMoonArgumentOfLatitude
self._fEccentricity = fEccentricity
def __init__(self, sPlanetName):
toolObjectSerializable.__init__(self)
self._sName = sPlanetName
self._sType = "planet"
self._fLongPerihelion = 0.0 # w1 = longitude of perihelion
self._fLongAscNodeInDeg = 0.0 # N = longitude of the ascending node
self._fArgPerihelInDeg = 0.0 # w = argument of perihelion
self._fMeanLongInDeg = 0.0 # L = mean longitude
self._fInclEclipInDeg = 0.0
# i = inclination to the ecliptic (plane of the Earth's orbit)
self._fMeanAnoInDeg = 0.0 # M = mean anomaly (0 at perihelion; increases uniformly with time)
self._fPerihelionDistInUA = 0.0 # q = perihelion distance
self._fMeanDistSunInAU = 0.0 # a = semi-major axis, or mean distance from Sun
self._fEccentricInDeg = 0.0 # e = eccentricity (0=circle, 0-1=ellipse, 1=parabola)
self._fAphelionDistInUA = 0.0 # Q = aphelion distance
self._fOrbPeriodInYears = 0.0 # P = orbital period (years if a is in AU, astronomical units)
self._fEccentricAnoInDeg = 0.0 # E = Eccentric Anomaly
self._fTrueAnoInDeg = 0.0 # v = True Anomaly
self._fSunDistInUA = 0.0 # r = Sun's distance
self._fLongitudeEcliptic = 0.0 # LonEcl = Longitude Ecliptic
self._fLatitudeEcliptic = 0.0 # LatEcl = Longitude Ecliptic
self._fGeocentricCoordX = 0.0 # xg = Geocentric Coordinate X
self._fGeocentricCoordY = 0.0 # yg = Geocentric Coordinate Y
self._fGeocentricCoordZ = 0.0 # zg = Geocentric Coordinate Z
self._fRAInDeg = 0.0
# RA = Right Ascension
self._fDecInDeg = 0.0
# Dec = Declination
self._fTopoRAInDeg = 0.0
# TopoRA = Right Ascension
self._fTopoDecInDeg = 0.0
def __init__(self, sDate, sTime):
toolObjectSerializable.__init__(self)
self._date = sDate # date as YYYYMMDD
self._time = sTime # Time as HHMMSS (GMT)
self._iYear = int(sDate[0:4])
self._iMonth = int(sDate[4:6])
self._iDay = int(sDate[6:8])
self._iHour = int(sTime[0:2])
self._iMinute = int(sTime[2:4])
self._iSecond = int(sTime[4:6])
self._fJuliandDay = 0.0
self._fJuliandEphemerisDay = 0.0
self._fJulianCenturies = 0.0
self._fJulianEphemerisCenturies = 0
self._fDeltaT = 0.0
self._fMeanSideralTimeGreenwich = 0.0
self._fApparentSideralTimeGreenwich = 0.0
self._fApparentGeometricLongitude = {}
self._fApparentGeocentricLongitude = {}
self._fApparentGeocentricLatitude = {}
self._fApparentRightAscension = {}
self._fArgumentOfLatitude = {}
self._fAscendNodeLongitude = {}
self._fDeclination = {}
self._fDistanceInKm = {}
self._fDistanceInUA = {}
self._fEquationCenter = {}
self._fEccentricity = {}
self._fGeocentricLatitude = {}
self._fGeocentricLongitude = {}
self._fGeometricMeanLongitude = {}
self._fIllumination = {}
self._fMeanAscendingNodeLongitude = {}
self._fMeanAnomaly = {}
self._fMeanElongation = {}
self._fMeanLongitude = {}
self._fMeanObliquityEcliptic = {}
self._fNutationInLongitude = {}
self._fOpticalLibrationInLongitude = {}
self._fOpticalLibrationInLatitude = {}
self._fPhaseAngle = {}
self._fPositionAngle = {}
self._fRightAscension = {}
self._fSelenographicColongitude = {}
self._fSubSolarSelenographicLongitude = {}
self._fSubSolarSelenographicLatitude = {}
self._fTrueAnomaly = {}
self._fTrueGeometricLongitude = {}
self._fTrueObliquityEcliptic = {}
self._compute()
def __init__(self):
toolObjectSerializable.__init__(self)
self._sStartDate = "" # YYYYMMDD
self._sStartTime = "" # HHMMSS
self._iNbSlots = 0 #
self._observerLongitude = 0.0 #
self._observerLatitude = 0.0 #
self._date = {} # date for each slot (YYYYMMDD) (key=slotID)
self._time = {
} # time for the beginning of the slot (HHMMSS) (key=slotID)
self._sunAltitude = {} # sun's altitude for each slot (key=slotID)
self._sunMeanLongInDeg = {
} # sun's mean longitude for each slot (key=slotID)
self._objects = {
} # ephemerides for each objects (dictionary of EphemeridesDataObject, with key = ObjectID)
self._dicMemBuffer = {}
self._bBufferInitialized = False
def __init__(self, sID, sType, sCategory, sName, sPictureName):
toolObjectSerializable.__init__(self)
self._sID = sID
self._sType = sType
self._sCategory = sCategory
self._sName = sName
self._sPictureName = sPictureName
self._Azimut = {} #
self._Altitude = {} #
self._RightAscension = {} #
self._Declination = {} #
self._Distance = {} #
self._MeanLong = {} #
self._Colongitude = {} #
self._SelenographicLongitude = {} #
self._SelenographicLatitude = {} #
self._Phase = {}
self._Illumination = {}
self._PositionAngle = {}
self._VisibilityStatus = {}
def __init__(self, sLocalStartDate, sLocalStartTime,
fLocalTimeDifferenceWithGMT):
toolObjectSerializable.__init__(self)
self._LocalStartdate = sLocalStartDate # date as YYYYMMDD (Local Time)
self._LocalStartTime = sLocalStartTime # Time as HHMMSS (Local Time)
self._fLocalTimeDifferenceWithGMT = fLocalTimeDifferenceWithGMT
self._iYear = int(self._LocalStartdate[0:4])
self._iMonth = int(self._LocalStartdate[4:6])
self._iDay = int(self._LocalStartdate[6:8])
self._iHours = int(self._LocalStartTime[0:2])
self._iMinutes = int(self._LocalStartTime[2:4])
self._iSeconds = int(self._LocalStartTime[4:8])
self._dtLocalDateTime = datetime.datetime(self._iYear, self._iMonth,
self._iDay, self._iHours,
self._iMinutes,
self._iSeconds)
self._dtGMTLocalDateTime = self._dtLocalDateTime - datetime.timedelta(
hours=self._fLocalTimeDifferenceWithGMT)
self._fLocalDateValue = self.__computeDateValueFromDateAndTime(
self._LocalStartdate, self._LocalStartTime)
self._LocalStartTimeSlotBasedHour0 = None
def __init__(self):
toolObjectSerializable.__init__(self)
self._sName = "Sun"
self._sType = "Star"
self._oMeeusAlgorithm = None
self._fObliqEclipInDeg = 0.0
# ecl = obliquity of the ecliptic
self._fLongAscNodeInDeg = 0.0
# N = longitude of the ascending node
self._fInclEclipInDeg = 0.0
# i = inclination to the ecliptic (plane of the Earth's orbit)
self._fArgPerihelInDeg = 0.0
# w = argument of perihelion
self._fMeanDistSunInAU = 0.0
# a = semi-major axis, or mean distance from Sun
self._fEccentricInDeg = 0.0
# e = eccentricity (0=circle, 0-1=ellipse, 1=parabola)
self._fMeanAnoInDeg = 0.0
# M = mean anomaly (0 at perihelion; increases uniformly with time)
self._fLongPerihelion = 0.0
# w1 = longitude of perihelion
self._fMeanLongInDeg = 0.0
# L = mean longitude
self._fPerihelionDistInUA = 0.0
# q = perihelion distance
self._fAphelionDistInUA = 0.0
# Q = aphelion distance
self._fOrbPeriodInYears = 0.0
# P = orbital period (years if a is in AU, astronomical units)
self._fEccentricAnoInDeg = 0.0
# E = Eccentric Anomaly
self._fSunDistInUA = 0.0
# r = Sun's distance
self._fTrueAnoInDeg = 0.0
# v = True Anomaly
self._fRAInDeg = 0.0
# RA = Right Ascension
self._fDecInDeg = 0.0
def __init__(self):
toolObjectSerializable.__init__(self)
self._sName = "Moon"
self._sType = "Moon"
self._oMeeusAlgorithm = None
