HeliocentricEarthEcliptic#
- class sunpy.coordinates.HeliocentricEarthEcliptic(*args, **kwargs)[source]#
Bases:
SunPyBaseCoordinateFrame
A coordinate or frame in the Heliocentric Earth Ecliptic (HEE) system.
The origin is the center of the Sun.
The X-axis (0 degrees longitude and 0 degrees latitude) is aligned with the Sun-Earth line.
The Z-axis (+90 degrees latitude) is aligned with the component perpendicular to the X-axis of the mean ecliptic pole at the observation time.
- Parameters:
data (
BaseRepresentation
orNone
) – A representation object orNone
to have no data (or use the coordinate component arguments, see below).lon (
Angle
orQuantity
, optional) – The longitude coordinate for this object (lat
must also be given anddata
must beNone
). Not needed ifdata
is given.lat (
Angle
orQuantity
, optional) – The latitude coordinate for this object (lon
must also be given anddata
must beNone
). Not needed ifdata
is given.distance (
Quantity
, optional) – The distance coordinate from Sun center for this object. Not needed ifdata
is given.obstime (
tuple
,list
,str
,pandas.Timestamp
,pandas.Series
,pandas.DatetimeIndex
,datetime.datetime
,datetime.date
,numpy.datetime64
,numpy.ndarray
,astropy.time.Time
) – The time of the observation. This is used to determine the position of solar-system bodies (e.g., the Sun and the Earth) as needed to define the origin and orientation of the frame.representation_type (
BaseRepresentation
, str, optional) – A representation class or string name of a representation class. This may change the valid coordinate component arguments from the defaults (see above). For example, passingrepresentation_type='cartesian'
will make the frame expect Cartesian coordinate component arguments (typically,x
,y
, andz
).copy (bool, optional) – If
True
(default), make copies of the input coordinate arrays.
Attributes Summary
Default representation for differential data (e.g., velocity)
Default representation for position data
Mapping for frame-specific component names
Attributes Documentation
- default_differential#
Default representation for differential data (e.g., velocity)
- default_representation#
Default representation for position data
- frame_attributes = {'obstime': <sunpy.coordinates.frameattributes.TimeFrameAttributeSunPy object>}#
- frame_specific_representation_info#
Mapping for frame-specific component names
- name = 'heliocentricearthecliptic'#