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The definitions of two spacecraft coordinates, SGA and SSI, are indicated.
The original and averaged vectors are despun into non-rotating spacecraft coordinates and geophysical coordinates.
Magnetic field and ion velocity components are plotted in GSM coordinates together with electric field variations in spacecraft coordinates.
Red, green, and blue curves are for B x−sat, B y−sat, and B z−sat components in spacecraft coordinates, respectively.
In local spacecraft coordinates, the Hp component points toward the north pole, the He component Earthward, and the Hn component eastward.
Data are converted into the physical magnetic field vectors in the rotating spacecraft coordinates by calibration parameters, namely sensitivity, offset, and alignment.
Similar(54)
The spacecraft coordinate system ((X_text {sc}), (Y_text {sc}), (Z_text {sc})) is also given in the figure.
Here the suffix 'sc' stands for the spacecraft coordinate system, and 'cmp' stands for the component (instrument) coordinate system.
Spin averages are generated from the vectors in the non-rotating spacecraft coordinate and converted to vectors in the geophysical coordinates.
We have identified a 4.31 ± 0.14 cm error in the Z (cross-track) direction that defines the center-of-mass of the SARAL satellite in the spacecraft coordinate system, and we have tuned the SLR and DORIS tracking point offsets.
The intrinsic field-of-view of IMA is 4.5° × 360° in the spacecraft X–Z plane, divided into 16 azimuthal sectors of 22.5° (see Barabash and the ASPERA-3 team, 2006) their figure 37 or Nilsson et al. (2006a) their figure 1 for a schematic description of the IMA field-of-view as well as a definition of the spacecraft coordinate system).
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