Table 6.234 — DRM_SEC_3D_Location

Property

Description

Class

  • <DRM SEC 3D Location>

Superclass

Subclass

  • None.

Definition

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

See 8.5.12 Solar ecliptic SRFT of ISO/IEC 18026 for a complete definition.

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

Class diagram

Figure 6.290 — DRM_SEC_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_SEC_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)

  • SRFs derived from the Solar Ecliptic SRFT are convenient for representing such data as:

    1. interplanetary magnetic field observations;
    2. solar wind velocity data; and
    3. satellite trajectories.