Пример #1
0
def calc_time(lower_bound, upper_bound, location, attribute, value,
              pressure=101325, temperature=12, xtol=1.0e-12):
    """
    Calculate the time between lower_bound and upper_bound
    where the attribute is equal to value. Uses PyEphem for
    solar position calculations.

    Parameters
    ----------
    lower_bound : datetime.datetime
    upper_bound : datetime.datetime
    location : pvlib.Location object
    attribute : str
        The attribute of a pyephem.Sun object that
        you want to solve for. Likely options are 'alt'
        and 'az' (which must be given in radians).
    value : int or float
        The value of the attribute to solve for
    pressure : int or float, optional
        Air pressure in Pascals. Set to 0 for no
        atmospheric correction.
    temperature : int or float, optional
        Air temperature in degrees C.
    xtol : float, optional
        The allowed error in the result from value

    Returns
    -------
    datetime.datetime

    Raises
    ------
    ValueError
        If the value is not contained between the bounds.
    AttributeError
        If the given attribute is not an attribute of a
        PyEphem.Sun object.
    """

    try:
        import scipy.optimize as so
    except ImportError:
        raise ImportError('The calc_time function requires scipy')

    obs, sun = _ephem_setup(location, pressure, temperature)

    def compute_attr(thetime, target, attr):
        obs.date = thetime
        sun.compute(obs)
        return getattr(sun, attr) - target

    lb = datetime_to_djd(lower_bound)
    ub = datetime_to_djd(upper_bound)

    djd_root = so.brentq(compute_attr, lb, ub,
                         (value, attribute), xtol=xtol)

    return djd_to_datetime(djd_root, location.tz)
Пример #2
0
def calc_time(lower_bound,
              upper_bound,
              latitude,
              longitude,
              attribute,
              value,
              altitude=0,
              pressure=101325,
              temperature=12,
              horizon='+0:00',
              xtol=1.0e-12):
    """
    Calculate the time between lower_bound and upper_bound
    where the attribute is equal to value. Uses PyEphem for
    solar position calculations.

    Parameters
    ----------
    lower_bound : datetime.datetime
    upper_bound : datetime.datetime
    latitude : float
    longitude : float
    attribute : str
        The attribute of a pyephem.Sun object that
        you want to solve for. Likely options are 'alt'
        and 'az' (which must be given in radians).
    value : int or float
        The value of the attribute to solve for
    altitude : float, default 0
        Distance above sea level.
    pressure : int or float, optional, default 101325
        Air pressure in Pascals. Set to 0 for no
        atmospheric correction.
    temperature : int or float, optional, default 12
        Air temperature in degrees C.
    horizon : string, optional, default '+0:00'
        arc degrees:arc minutes from geometrical horizon for sunrise and
        sunset, e.g., horizon='+0:00' to use sun center crossing the
        geometrical horizon to define sunrise and sunset,
        horizon='-0:34' for when the sun's upper edge crosses the
        geometrical horizon
    xtol : float, optional, default 1.0e-12
        The allowed error in the result from value

    Returns
    -------
    datetime.datetime

    Raises
    ------
    ValueError
        If the value is not contained between the bounds.
    AttributeError
        If the given attribute is not an attribute of a
        PyEphem.Sun object.
    """

    try:
        import scipy.optimize as so
    except ImportError:
        raise ImportError('The calc_time function requires scipy')

    obs, sun = _ephem_setup(latitude, longitude, altitude, pressure,
                            temperature, horizon)

    def compute_attr(thetime, target, attr):
        obs.date = thetime
        sun.compute(obs)
        return getattr(sun, attr) - target

    lb = datetime_to_djd(lower_bound)
    ub = datetime_to_djd(upper_bound)

    djd_root = so.brentq(compute_attr, lb, ub, (value, attribute), xtol=xtol)

    return djd_to_datetime(djd_root)
Пример #3
0
def calc_time(lower_bound,
              upper_bound,
              location,
              attribute,
              value,
              pressure=101325,
              temperature=12,
              xtol=1.0e-12):
    """
    Calculate the time between lower_bound and upper_bound
    where the attribute is equal to value. Uses PyEphem for
    solar position calculations.

    Parameters
    ----------
    lower_bound : datetime.datetime
    upper_bound : datetime.datetime
    location : pvlib.Location object
    attribute : str
        The attribute of a pyephem.Sun object that
        you want to solve for. Likely options are 'alt'
        and 'az' (which must be given in radians).
    value : int or float
        The value of the attribute to solve for
    pressure : int or float, optional
        Air pressure in Pascals. Set to 0 for no
        atmospheric correction.
    temperature : int or float, optional
        Air temperature in degrees C.
    xtol : float, optional
        The allowed error in the result from value

    Returns
    -------
    datetime.datetime

    Raises
    ------
    ValueError
        If the value is not contained between the bounds.
    AttributeError
        If the given attribute is not an attribute of a
        PyEphem.Sun object.
    """

    try:
        import scipy.optimize as so
    except ImportError:
        raise ImportError('The calc_time function requires scipy')

    obs, sun = _ephem_setup(location, pressure, temperature)

    def compute_attr(thetime, target, attr):
        obs.date = thetime
        sun.compute(obs)
        return getattr(sun, attr) - target

    lb = datetime_to_djd(lower_bound)
    ub = datetime_to_djd(upper_bound)

    djd_root = so.brentq(compute_attr, lb, ub, (value, attribute), xtol=xtol)

    return djd_to_datetime(djd_root, location.tz)
Пример #4
0
def calc_time(lower_bound, upper_bound, latitude, longitude, attribute, value,
              altitude=0, pressure=101325, temperature=12, horizon='+0:00',
              xtol=1.0e-12):
    """
    Calculate the time between lower_bound and upper_bound
    where the attribute is equal to value. Uses PyEphem for
    solar position calculations.

    Parameters
    ----------
    lower_bound : datetime.datetime
    upper_bound : datetime.datetime
    latitude : float
    longitude : float
    attribute : str
        The attribute of a pyephem.Sun object that
        you want to solve for. Likely options are 'alt'
        and 'az' (which must be given in radians).
    value : int or float
        The value of the attribute to solve for
    altitude : float, default 0
        Distance above sea level.
    pressure : int or float, optional, default 101325
        Air pressure in Pascals. Set to 0 for no
        atmospheric correction.
    temperature : int or float, optional, default 12
        Air temperature in degrees C.
    horizon : string, optional, default '+0:00'
        arc degrees:arc minutes from geometrical horizon for sunrise and
        sunset, e.g., horizon='+0:00' to use sun center crossing the
        geometrical horizon to define sunrise and sunset,
        horizon='-0:34' for when the sun's upper edge crosses the
        geometrical horizon
    xtol : float, optional, default 1.0e-12
        The allowed error in the result from value

    Returns
    -------
    datetime.datetime

    Raises
    ------
    ValueError
        If the value is not contained between the bounds.
    AttributeError
        If the given attribute is not an attribute of a
        PyEphem.Sun object.
    """

    try:
        import scipy.optimize as so
    except ImportError:
        raise ImportError('The calc_time function requires scipy')

    obs, sun = _ephem_setup(latitude, longitude, altitude,
                            pressure, temperature, horizon)

    def compute_attr(thetime, target, attr):
        obs.date = thetime
        sun.compute(obs)
        return getattr(sun, attr) - target

    lb = datetime_to_djd(lower_bound)
    ub = datetime_to_djd(upper_bound)

    djd_root = so.brentq(compute_attr, lb, ub,
                         (value, attribute), xtol=xtol)

    return djd_to_datetime(djd_root)