Managed to get some HA data of the Vela SNR. The system is now totally free of noticeable flexure.
So this is what we have in raw NB data.
HA 8x32 minutes, NII 10x32 minutes and OIII 9x32 minutes.
This is just HA and NII with HA to red channel and NII to green. 8MB
http://d1355990.i49.quadrahosting.co...SNR_HA_NII.jpg
This is HA to red, NII to green and OIII to blue. 8MB
http://d1355990.i49.quadrahosting.co...A_NII_OIII.jpg
I have tried to process all NB wavelengths the same and have not adjusted levels so what you see is close to the relative intensities of each emission line.
The much larger older Gum nebula behind the Vela SNR emit more HA than NII. You can see this as red background at the bottom and top left in the HA NII image. See the diagram from APOD below which shows our Sun's neighbourhood.
The gas cloud structure of the Vela SNR is quite fractal in nature and looks a bit like a what a much older version of the Crab Nebula M1 would look like.
Bert