The Flowing Clue: La Source Unveiled – page 2, panels 2 – 4

“The Flowing Clue: La Source Unveiled” page 2, panels 2-4

These are the rest of the supporting characters in my short fluids-related crime story. I enjoyed developing them and making concept drawings early on.  However, simplifying those for this inking stage, so that the characters would hopefully be recognizable and easy enough to draw multiple times from various angles was not trivial. In fact, I had to come back to these panels and tweak them quite a bit as I progressed further into the book.

The Flowing Clue: La Source Unveiled – page 2, panel 1

“The Flowing Clue: La Source Unveiled” page 2, panel 1

Here is the ink of the first panel on the second page of my fluids comic book. The second page was easier to conceptualize than the first one, since it was a straightforward introduction of the supporting characters. Among them, I had a clearest vision of this one, Trevis, and as a consequence, he changed the least from the initial character design stage.

Nebula processing workflow: a Foraxx palette from a one-shot colour image

IC 1848 – The Soul Nebula

My current workflow for processing one-shot colour images of deep-space objects, particularly nebulae, heavily relies on the process of reconstruction a foraxx palette outlined in this video by Paulyman Astro (https://youtu.be/Gy42AeZ_XB4?si=lNb4B7a0jVKWi4I1).

The video is very detailed, and it has been exceptionally useful for me, but I found myself scrolling through it and pausing so much that I wanted to have a written summary of the steps that I could quickly refer to. Apologies in advance, if the following steps appear out-of-context – they are really short notes that would make sense to those who have used the Pixinsight software and worked with the foraxx palette.

Before this image processing is even started, I generate an integrated image using the following pre-processing sequence (see this guide by Adam Block for details: https://youtu.be/VKOTCuqD2Qs?si=EdbONwT8GO_DUAkR) :

First of all, all the individual exposures (light frames), which are typically 5-min long each, are calibrated with “flats”, “dark flats” and “darks” using the WeightedBatchPreprocessing script. 

Then, the resulted de-bayered images are aligned using the StarAlignment process.

Finally, the aligned images are integrated using the ImageIntergation process with Winthorised Sigma Clipping background rejection method. This produces the “integration.xisf” image, which is the basis for the nebula processing workflow itself:

  1. Right-click on the identifier tab at the top-left of the image frame and set the new identifier to ‘osc’ (for ‘One-Shot Colour’).
  2. Use Process>All processes>ScreenTransferFunction to preview a stretched image. I unlock the RGB channels before pressing the “nuke” button to avoid a high colour cast. This is not important though, because nothing is actually being done to the image – this is just a preview.
  3. Use Process>All processes>DynamicCrop to crop the image.
  4. Use AutomaticBackgroundExrtactor with Function degree (under Interpolation and Output) set to 1 and Target Image Correction to ‘Subtraction’. This works if there is simply some light pollution gradient in the image and little to no vignetting. Otherwise, use the DynamicBackgroundExtraction process.
  5. Split the RGB channels using an icon in the toolbar.
  6. Set the identifier of the Red channel to ‘ha’ for “Hydrogen alpha”.
  7. Combine the Green and the Blue channel using the following Pixelmath expression: 0.5*B+0.5*G. Give the resulting image an identifier ‘oiii’. 
  8. Use StarExterminator process to extract the stars. Check “Generate Star Image” and “Unscreen Stars” boxes. Drag the triangle from the process window onto the ha window and then onto the oiii window.
  9. Use Generalized Hyperbolic Stretch (GHS) script or process to stretch the ‘ha’ and the ‘oiii’ (starless) images.
    • First stretch: Just right of the peak. Local stretch intensity ~10. Stretch factor ~3.
    • Second stretch: Secondary drop-off (log view). Local stretch intensity ~5.
  10. Foraxx process: Create the false Green channel (‘ho’) using the Pixelmath expression: (ha*oiii)^~(ha*oiii). Press the square button.
  11. Boost the brightness of the ‘ho’ image by doing the first-level stretch in GHS.
  12. Create the colour image by using the Pixelmath expression (uncheck ‘Use a single RGB/K expression’, set Color space to ‘RGB color’):
    • R: ha
    • G: ho*ha+~ho*oiii
    • B: oiii
  13. Apply CurvesTransformation. Start with saturation, proceed to individual channels.
  14. Apply NoiseExterminator with default values or Denoise ~0.9, Detail ~0.55.
  15. Stretch ‘ha_stars’ and ‘oiii_stars’ using HistogramTransformation. Use checkmark to track the histogram and use live preview to monitor the stretch amount. Drag middle slider to the left.
  16. Apply the Foraxx process (step 10) to ‘ha_stars’ and ‘oiii_stars’.
  17. Use CurvesTransformation to boost saturation of ‘foraxx_stars’.
  18. Put the stars back using the Pixelmath expression: ~(~foraxx*~foraxx_stars).

And this is it! Here are some examples of my application of this process applied to various emission nebulae.

Sharpless 157 – The Lobster Claw Nebula
NGC 7000 – Cygnus Wall
NGC 7822 – The Cosmic Question Mark Nebula

NGC 7822 – The Cosmic Question Mark

This emission nebula is one of the youngest star-forming regions in our galaxy. Some components of it are only few million years old. In the cosmic time scale, this is basically star birth happening in front of our eyes. This nebula also contains the hottest star found within 1 kpc of our Sun, the BD+66 1673, which has the surface temperature of 45,000 K and the luminosity 100,000 times that of the Sun. It is primarily responsible for ionizing the gas of the nebula and for compressing it by the strong stellar wind, leading to creation of new stars. 

This light travelled for 3,000 years before reaching my yard in Victoria, BC in June 2024.

NGC 7822 is a large target, filling the full-frame sensor of my camera attached to a 478 mm-long telescope. This is a 3.5 hr-long RGB exposure at f/5.9, processed using a Foraxx palette.

The Flowing Clue: La Source Unveiled – panels 4,5

“The Flowing Clue: La Source Unveiled” page 1, panels 4, 5

This is the ink of the last two panels on the first page of my fluids comic book. The first closeup of one of the main characters required quite a bit of thinking through in order to simplify the original character design. Professionals like Victoria Ying say that by the end of the inking process one becomes very good at drawing the main characters, because they appear so often. I am certainly looking forward to that, but in the meantime, I was quite glad to simply finish the first page.

The Flowing Clue: La Source Unveiled – panel 3

“The Flowing Clue: La Source Unveiled” page 1, panel 3

Here is the ink of the third panel of my fluids comic book. When I was laying out this panel, I made a decision to use a 3D model for the backgrounds, and now that I am several pages into inking, I am certainly glad that I did so. Considering that the story takes place in the same room full of small details, maintaining consistency of the set without the ability to simply re-position the camera would have been impossible.

My fluids comic book

“The Flowing Clue: La Source Unveiled” page 1, panels 1-2

I’ve been working on a fictional short story, hopefully the first in a series, on the subject of my academic research and teaching – fluid mechanics. As a colleague of mine said about teaching fluids at the university level, “fluids is a dry subject”. In the hope of making it a bit more entertaining, I’decided to try a manga format. It’s a crime story set in the not-very-distant future with the working title “The Flowing Clue: La Source Unveiled”

Here are the inks of the first two panels. Stay tuned for the updates on this work in progress.

M94 – The Croc’s Eye Galaxy

I captured this image of the Croc’s Eye Galaxy (M94, also called the Cat’s Eye Galaxy) yesterday in my yard in Victoria, BC, using a total of 3 hours of exposure. It’s an unusual galaxy – it has a an inner ring with a diameter of 5,400 light-years and an outer one with a diameter of 45,000 light-years. Pressure from the galactic core compresses the gas and dust clouds in the outer ring, where gravity pulls them together to form new stars. These stars pull in more gas and dust, resulting in a relatively empty region separating them from yet another layer of gas at the periphery of the galaxy.

M94 has a remarkably low amount of dark matter for a galaxy – the stars comprise almost all of its mass. Their light travelled for 16 million years before reaching my telescope.