Table 6.243 — DRM_SME_3D_Location

Property

Description

Class

  • <DRM SME 3D Location>

Superclass

Subclass

  • None.

Definition

An instance of this DRM class specifies a coordinate for an SRF based on the Solar Magnetic Ecliptic SRFT.

See 8.5.14 Solar magnetic ecliptic SRFT of ISO/IEC 18026 for a complete definition.

The coordinate field specifies the set of coordinate-component values.

Class diagram

Figure 6.300 — DRM_SME_3D_Location

Inherited field elements

Field name

Range

Field data type

None

   

Field elements

Field name

Range

Field data type

coordinate

 

SRM_Spherical_3D_Coordinate

Default field values

Default field values for DRM_SME_3D_Location

Associated to (one-way) (inherited)

  • None.

Associated to (one-way)

  • None.

Associated by (one-way) (inherited)

  • None.

Associated by (one-way)

  • None.

Associated with (two-way) (inherited)

  • None.

Associated with (two-way)

  • None.

Composed of (two-way) (inherited)

  • None.

Composed of (two-way)

  • None.

Composed of (two-way metadata) (inherited)

  • None.

Composed of (two-way metadata)

  • None.

Component of (two-way) (inherited)

Component of (two-way)

  • None.

Constraints

Clarifications

None.

Example(s)

  • An SRF derived from the Solar Magnetic Ecliptic SRFT is convenient for representing such data as:
    1. magnetopause and shock boundary positions,
    2. magnetosheath and magnetotail fields, and
    3. magnetosheath solar wind velocities (since the orientation of the magnetic dipole axis alters the otherwise cylindrical symmetry of the solar wind flow).