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Python Dataset.attrs['lat']方法代码示例

本文整理汇总了Python中xarray.Dataset.attrs['lat']方法的典型用法代码示例。如果您正苦于以下问题:Python Dataset.attrs['lat']方法的具体用法?Python Dataset.attrs['lat']怎么用?Python Dataset.attrs['lat']使用的例子?那么恭喜您, 这里精选的方法代码示例或许可以为您提供帮助。您也可以进一步了解该方法所在xarray.Dataset的用法示例。


在下文中一共展示了Dataset.attrs['lat']方法的1个代码示例,这些例子默认根据受欢迎程度排序。您可以为喜欢或者感觉有用的代码点赞,您的评价将有助于系统推荐出更棒的Python代码示例。

示例1: radec2azel

# 需要导入模块: from xarray import Dataset [as 别名]
# 或者: from xarray.Dataset import attrs['lat'] [as 别名]
def radec2azel(scale: xarray.Dataset,
               latlon: Tuple[float, float], time: datetime=None) -> xarray.Dataset:

    if latlon is None or not isinstance(scale, xarray.Dataset):
        return None

    if time is None:
        with fits.open(scale.filename, mode='readonly') as f:
            try:
                t = f[0].header['FRAME']  # TODO this only works from Solis?
            except KeyError:
                logging.error('no time given in file or manually, cannot compute az/el')
                return None
        time = parse(t)
        logging.info('using FITS header for time')
    elif isinstance(time, datetime):
        pass
    elif isinstance(time, (float, int)):  # assume UT1_Unix
        time = datetime.utcfromtimestamp(time)
    else:  # user override of frame time
        time = parse(time)

    print('image time:', time)
# %% knowing camera location, time, and sky coordinates observed, convert to az/el for each pixel
    az, el = pymap3d.radec2azel(scale['ra'], scale['dec'], latlon[0], latlon[1], time)
# %% collect output
    scale['az'] = (('y', 'x'), az)
    scale['el'] = (('y', 'x'), el)
    scale.attrs['lat'] = latlon[0]
    scale.attrs['lon'] = latlon[1]
    scale.attrs['time'] = time

    return scale
开发者ID:scienceopen,项目名称:astrometry_azel,代码行数:35,代码来源:base.py


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