New Process: NarrowbandNormalization

Love this one! I just tried it out on my data from last night. Orion Xt10g with a ZWO 294 MC and L-enhance filter. 800x5 subs.
Here's the original image and then the Narrowband Normalized one:
 

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  • NGC7380_2023_09_26_APP_St_1_DBE-PI-Blur-Noise-CROP-Curve-PS-SM.jpg
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  • 01-NGC7380_2023_09_26_APP_St_1_DBE-PI-Blur-Noise-CROP-Curve-PS2-NarrowBand-2-SM.jpg
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Fabulous process. For me it's finally taken the heartache out of NB colour balancing and made it so much easier. I knew that I had good data, but spent far too long trying to get the colour balance right.

Thank you both. Much appreciated.

Soul Nebula starless SHO stretched and post-NB normalisation with RGB stars.

Soul_NBnormalisation.jpg
 
Bill Blanshan and I have been working on a new process designed to help balance the channels within a narrowband image. The process links in to the PixInsight real-time preview functionality so you can see the effect of the various parameters on your image before applying them. Bill has made a video explaining its use which you can find here. There is also full documentation available, linked from with the process. The process is designed to run on the new 1.8.9-2 version of PixInsight. You can obtain it from the following repository: https://www.cosmicphotons.com/pi-modules/narrowbandnormalization/

Clear Skies, Mike
(Visit my website for more PixInsight scripts)
Although I do understand why this balancing of channels is done: but is it not just physics within the target which "tells me" in the data that the, say, H-alpha emission is "much " stronger, than, say, S[II] emission.?
So, if I want to produce a physically correct representation of that target in my exposure, why should I change the "color" distribution (or, the physic) unless for esthetic reasons ?
 
Although I do understand why this balancing of channels is done: but is it not just physics within the target which "tells me" in the data that the, say, H-alpha emission is "much " stronger, than, say, S[II] emission.?
So, if I want to produce a physically correct representation of that target in my exposure, why should I change the "color" distribution (or, the physic) unless for esthetic reasons ?
Well, a SHO image is, fundamentally, about aesthetics. The intensity differences between the channels can be huge, and if you treat them with the same scaling you won't see much. The processing is largely about seeing what elements are where, not how much of them there is. From a science standpoint, SHO images help us get an initial sense of structure, but any actual science is conducted on the individual channels, not on the SHO composite. (Likewise for any narrowband data composited into some kind of RGB image.)
 
Although I do understand why this balancing of channels is done: but is it not just physics within the target which "tells me" in the data that the, say, H-alpha emission is "much " stronger, than, say, S[II] emission.?
So, if I want to produce a physically correct representation of that target in my exposure, why should I change the "color" distribution (or, the physic) unless for esthetic reasons ?
Isn't all narrowband processing for aesthetic reasons? Unless you are working on scientific research, all AP is for aesthetic reasons any way.
 
Although I do understand why this balancing of channels is done: but is it not just physics within the target which "tells me" in the data that the, say, H-alpha emission is "much " stronger, than, say, S[II] emission.?
So, if I want to produce a physically correct representation of that target in my exposure, why should I change the "color" distribution (or, the physic) unless for esthetic reasons ?
My image processing is largely about aesthetics, although curiosity naturally leads me to understanding what the data actually represents. But I'd never interest other people in deep space if I only presented scientifically-accurate images that are overwhelmingly green in the SHO palette. A palette to me is what it is to other artists; a set of colours to describe an object. I'm quite happy to use artistic licence to show where the different emissions are coming from. It's an extension of stretching an image luminance to reveal hidden detail within the shadows. This NB normalisation process is in effect just a form of colour stretching.
 
My image processing is largely about aesthetics, although curiosity naturally leads me to understanding what the data actually represents. But I'd never interest other people in deep space if I only presented scientifically-accurate images that are overwhelmingly green in the SHO palette. A palette to me is what it is to other artists; a set of colours to describe an object. I'm quite happy to use artistic licence to show where the different emissions are coming from. It's an extension of stretching an image luminance to reveal hidden detail within the shadows. This NB normalisation process is in effect just a form of colour stretching.
Not to mention that the physics behind analyzing narrowband data is non-trivial. For instance, equal intensities of H-alpha and [O III] do not mean you have equal amounts or densities of H and O. The intensity is determined by other factors, such as the nature and sources of the ionizing radiation, the quantum details of the specific transitions, and other factors, as well. So the same thing that results in a good aesthetic result actually makes the final image more scientifically useful, as well, by letting us see the distributions of the different elements.
 
This script- or it's download location no longer works. I installed it, the script window doesn't show up in Pixinsight. It's either not compatible with the latest PI or the depository no longer valid.
 
Hmm... I get a 404 no server access error. However, I might try what you recommended.
That normally happens when you try to access the link directly via your web browser. You need to copy the link to your repository list and then check for updates. Did you do this?
 
Yes, I did this but it did not help. I had to reset all updates, delete the link to the narrowbandnormalization from the repository and add it again. Finally everything works as it should.
Thank you both, unimatrix and Mike1485.
 
Yes, I did this but it did not help. I had to reset all updates, delete the link to the narrowbandnormalization from the repository and add it again. Finally everything works as it should.
Thank you both, unimatrix and Mike1485.
Glad you got it working!
CS, Mike
 
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