Hi,
The background: we are using the differential rotation correction for SUVI, but since the off-disk parts do not have a HeliographicStonyhurst coordinate, they get set to NaN in the output image. We do need the off-disk parts for context though, so right now we are clumsily puzzling the on-disk and off-disk parts back together. From what I understand, the "assume_spherical_screen" method could mitigate this problem, but I don't understand how to combine it with the reproject example above. When I just try a simple
with Helioprojective.assume_spherical_screen(suvimap.observer_coordinate):
with transform_with_sun_center():
arr, _ = reproject_interp(suvimap, out_wcs, out_shape)
I only get an odd hourglass shape of the data, with the rest set to NaN.
Any help greatly appreciated!
Cheers,
Chris