COMPOSITION
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StudioBinder – Roger Deakins on How to Choose a Camera Lens — Cinematography Composition TechniquesRead more: StudioBinder – Roger Deakins on How to Choose a Camera Lens — Cinematography Composition Techniqueshttps://www.studiobinder.com/blog/camera-lens-buying-guide/ https://www.studiobinder.com/blog/e-books/camera-lenses-explained-volume-1-ebook 
DESIGN
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Realistic Avengers action figuresRead more: Realistic Avengers action figureshttp://kotaku.com/5911846/these-avengers-action-figures-look-so-real-youll-think-theyre-tiny-actors http://www.sideshowtoy.com/?page_id=37555&ref=Avengers2012 http://www.sideshowtoy.com/?page_id=4489&sku=9017301&ref=ref=avengersLP_9017301#!prettyPhoto/0/ http://animagetoyznews.blogspot.co.nz/ 
COLOR
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Space bodies’ components and light spectroscopyRead more: Space bodies’ components and light spectroscopywww.plutorules.com/page-111-space-rocks.html This help’s us understand the composition of components in/on solar system bodies. Dips in the observed light spectrum, also known as, lines of absorption occur as gasses absorb energy from light at specific points along the light spectrum. These dips or darkened zones (lines of absorption) leave a finger print which identify elements and compounds. In this image the dark absorption bands appear as lines of emission which occur as the result of emitted not reflected (absorbed) light. Lines of absorption  Lines of emission Lines of emission    
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Björn Ottosson – OKlch color spaceRead more: Björn Ottosson – OKlch color spaceBjörn Ottosson proposed OKlch in 2020 to create a color space that can closely mimic how color is perceived by the human eye, predicting perceived lightness, chroma, and hue. The OK in OKLCH stands for Optimal Color. - L: Lightness (the perceived brightness of the color)
- C: Chroma (the intensity or saturation of the color)
- H: Hue (the actual color, such as red, blue, green, etc.)
  Also read: 
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Thomas Mansencal – Colour Science for PythonRead more: Thomas Mansencal – Colour Science for Pythonhttps://thomasmansencal.substack.com/p/colour-science-for-python https://www.colour-science.org/ Colour is an open-source Python package providing a comprehensive number of algorithms and datasets for colour science. It is freely available under the BSD-3-Clause terms. 
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Colour – MacBeth Chart Checker DetectionRead more: Colour – MacBeth Chart Checker Detectiongithub.com/colour-science/colour-checker-detection A Python package implementing various colour checker detection algorithms and related utilities.  
LIGHTING
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NVidia DiffusionRenderer – Neural Inverse and Forward Rendering with Video Diffusion Models. How NVIDIA reimagined relightingRead more: NVidia DiffusionRenderer – Neural Inverse and Forward Rendering with Video Diffusion Models. How NVIDIA reimagined relightinghttps://www.fxguide.com/quicktakes/diffusing-reality-how-nvidia-reimagined-relighting/ https://research.nvidia.com/labs/toronto-ai/DiffusionRenderer/ 
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Tracing Spherical harmonics and how Weta used them in productionRead more: Tracing Spherical harmonics and how Weta used them in productionA way to approximate complex lighting in ultra realistic renders. All SH lighting techniques involve replacing parts of standard lighting equations with spherical functions that have been projected into frequency space using the spherical harmonics as a basis. http://www.cs.columbia.edu/~cs4162/slides/spherical-harmonic-lighting.pdf Spherical harmonics as used at Weta Digital 
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Vahan Sosoyan MakeHDR – an OpenFX open source plug-in for merging multiple LDR images into a single HDRIRead more: Vahan Sosoyan MakeHDR – an OpenFX open source plug-in for merging multiple LDR images into a single HDRIhttps://github.com/Sosoyan/make-hdr Feature notes- Merge up to 16 inputs with 8, 10 or 12 bit depth processing
- User friendly logarithmic Tone Mapping controls within the tool
- Advanced controls such as Sampling rate and Smoothness
 Available at cross platform on Linux, MacOS and Windows Works consistent in compositing applications like Nuke, Fusion, Natron. NOTE: The goal is to clean the initial individual brackets before or at merging time as much as possible. 
 This means:- keeping original shooting metadata
- de-fringing
- removing aberration (through camera lens data or automatically)
- at 32 bit
- in ACEScg (or ACES) wherever possible
  
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What light is best to illuminate gems for resaleRead more: What light is best to illuminate gems for resalewww.palagems.com/gem-lighting2 Artificial light sources, not unlike the diverse phases of natural light, vary considerably in their properties. As a result, some lamps render an object’s color better than others do. The most important criterion for assessing the color-rendering ability of any lamp is its spectral power distribution curve. Natural daylight varies too much in strength and spectral composition to be taken seriously as a lighting standard for grading and dealing colored stones. For anything to be a standard, it must be constant in its properties, which natural light is not. For dealers in particular to make the transition from natural light to an artificial light source, that source must offer: 
 1- A degree of illuminance at least as strong as the common phases of natural daylight.
 2- Spectral properties identical or comparable to a phase of natural daylight.A source combining these two things makes gems appear much the same as when viewed under a given phase of natural light. From the viewpoint of many dealers, this corresponds to a naturalappearance. The 6000° Kelvin xenon short-arc lamp appears closest to meeting the criteria for a standard light source. Besides the strong illuminance this lamp affords, its spectrum is very similar to CIE standard illuminants of similar color temperature.   
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Photography basics: Why Use a (MacBeth) Color Chart?Read more: Photography basics: Why Use a (MacBeth) Color Chart?Start here: https://www.pixelsham.com/2013/05/09/gretagmacbeth-color-checker-numeric-values/ https://www.studiobinder.com/blog/what-is-a-color-checker-tool/ In LightRoom in Final Cut in Nuke Note: In Foundry’s Nuke, the software will map 18% gray to whatever your center f/stop is set to in the viewer settings (f/8 by default… change that to EV by following the instructions below). 
 You can experiment with this by attaching an Exposure node to a Constant set to 0.18, setting your viewer read-out to Spotmeter, and adjusting the stops in the node up and down. You will see that a full stop up or down will give you the respective next value on the aperture scale (f8, f11, f16 etc.).One stop doubles or halves the amount or light that hits the filmback/ccd, so everything works in powers of 2. 
 So starting with 0.18 in your constant, you will see that raising it by a stop will give you .36 as a floating point number (in linear space), while your f/stop will be f/11 and so on.If you set your center stop to 0 (see below) you will get a relative readout in EVs, where EV 0 again equals 18% constant gray. In other words. Setting the center f-stop to 0 means that in a neutral plate, the middle gray in the macbeth chart will equal to exposure value 0. EV 0 corresponds to an exposure time of 1 sec and an aperture of f/1.0. This will set the sun usually around EV12-17 and the sky EV1-4 , depending on cloud coverage. To switch Foundry’s Nuke’s SpotMeter to return the EV of an image, click on the main viewport, and then press s, this opens the viewer’s properties. Now set the center f-stop to 0 in there. And the SpotMeter in the viewport will change from aperture and fstops to EV. 
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What is the Light Field?Read more: What is the Light Field?http://lightfield-forum.com/what-is-the-lightfield/ The light field consists of the total of all light rays in 3D space, flowing through every point and in every direction. How to Record a Light Field- a single, robotically controlled camera
- a rotating arc of cameras
- an array of cameras or camera modules
- a single camera or camera lens fitted with a microlens array
 
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