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Right now the only supported option in PySPEDAS is 'xgse'. We should implement the others:
; 'Xgse', (DEFAULT) translates from gse or gsm into FAC
; Definition(works on GSE, or GSM):
; X Axis = on plane defined by Xgse - Z
; Second coordinate definition: Y = Z x X_gse
; Third coordinate, X completes orthogonal RHS
; (right hand system) triad: XYZ
; Note: X_gse is a unit vector pointing in direction from
; earth to the sun
; 'Rgeo',translate from geo into FAC using radial position vector
; Rgeo is radial position vector, positive radialy outwards.
; Second coordinate definition: Y = Z x Rgeo (eastward)
; Third coordinate, X completes orthogonal RHS XYZ.
; 'mRgeo',translate into FAC using radial position vector
; mRgeo is radial position vector, positive radially inwards.
; Second coordinate definition: Y = Z x mRgeo (westward)
; Third coordinate, X completes orthogonal RHS XYZ.
; 'Phigeo', translate into FAC using azimuthal position vector
; Phigeo is the azimuthal geo position vector, positive Eastward
; First coordinate definition: X = Phigeo x Z (positive outwards)
; Second coordinate, Y ~ Phigeo (eastward) completes orthogonal RHS XYZ
; 'mPhigeo', translate into FAC using azimuthal position vector
; mPhigeo is minus the azimuthal geo position vector; positive Westward
; First coordinate definition: X = mPhigeo x Z (positive inwards)
; Second coordinate, Y ~ mPhigeo (Westward) completes orthogonal RHS XYZ
; 'Phism', translate into FAC using azimuthal Solar Magnetospheric vector.
; Phism is "phi" vector of satellite position in SM coordinates.
; Y Axis = on plane defined by Phism-Z, normal to Z
; Second coordinate definition: X = Phism x Z
; Third completes orthogonal RHS XYZ
; 'mPhism', translate into FAC using azimuthal Solar Magnetospheric vector.
; mPhism is minus "phi" vector of satellite position in SM coordinates.
; Y Axis = on plane defined by Phism-Z, normal to Z
; Second coordinate definition: X = mPhism x Z
; Third completes orthogonal RHS XYZ
; 'Ygsm', translate into FAC using cartesian Ygsm position as other dimension.
; Y Axis on plane defined by Ygsm and Z
; First coordinate definition: X = Ygsm x Z
; Third completes orthogonal RHS XYZ
There are several places where individual missions implement their own method of computing basis vectors for the transforms listed above, for example, see erg_pgs_make_fac.py.
The text was updated successfully, but these errors were encountered:
Right now the only supported option in PySPEDAS is 'xgse'. We should implement the others:
There are several places where individual missions implement their own method of computing basis vectors for the transforms listed above, for example, see erg_pgs_make_fac.py.
The text was updated successfully, but these errors were encountered: