Hi all, 

thanks @erget for trying to clarify this issue! It's causing some confusion in 
the community, as it's a tricky thing to understand. I'm fully in line with 
your last recap. 

As it's already been mentioned here, imho one thing that each description 
should really clarify (including the one from PROJ), is that this gimbal 
scanning geometry we are describing for the geostationary projection is 
independent of the actual scanning geometry of the actual instrument in orbit. 
It rather describes how the image is aquired by a fictitious, simplified, 
two-axis gimbal imaging instrument in an idealized geostationary position.

Elaborating on this, for future newbies like me delving into this issue: 
Higher-lever geostationary imagery (e.g. SEVIRI L1.5, FCI L1c, and GOES-R L1b) 
is rectified to a specified regular azimuth/elevation grid. With this, each 
image pixel has a pair of azimuth and elevation angles, that define how this 
idealized gimbal needs to be rotated to reach that specific pointing towards 
Earth. The sweep-angle axis describes which convention is used to define these 
azimuth/elevation rotations (either the "standing" gimbal as in the image 
above, or a turned-over version). The origin of the reference frame used to 
define these angles (i.e. the center of the gimbal and the intersection of the 
two rotation axes), is fixed and placed on an ideal satellite position. With 
this, each pixel of the rectified image is always at the same location on 
Earth, independently of the instrument scanning pattern, and the wobbling and 
drifting of the satellite in the non-perfect and perturbed geostationary orbit. 
This ideal satellite position is specified by the other variables of the 
geostationary projection. 

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