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Tips for Processing LRGB and HaRGB Images: Getting the C o l o r Right!. By Chris Schur. Introduction. With Digital Imaging as the mainstay for astrophotograpy today, color balance remains an elusive target. - PowerPoint PPT Presentation
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Tips for Processing LRGB and HaRGBTips for Processing LRGB and HaRGB Images: Getting the Images: Getting the CCoolloorr Right!Right!
By Chris SchurBy Chris Schur
IntroductionIntroduction
With Digital Imaging as the mainstay for astrophotograpy today, With Digital Imaging as the mainstay for astrophotograpy today, color balance remains an elusive target.color balance remains an elusive target.
Here we will discuss key points on locking in accurate color Here we will discuss key points on locking in accurate color balance for Deep Sky Images that use LRGB methodology.balance for Deep Sky Images that use LRGB methodology.
Our topics will include:Our topics will include: Setting a reference for our gray scaleSetting a reference for our gray scale Understanding the LRGB hue and saturation shiftUnderstanding the LRGB hue and saturation shift Correcting the shift in LRGB imagesCorrecting the shift in LRGB images Understanding the Hydrogen Alpha contribution to an imageUnderstanding the Hydrogen Alpha contribution to an image The role of Hydrogen Beta in the final color of nebulaThe role of Hydrogen Beta in the final color of nebula Tactfully combining Hydrogen and RGB data for balanced imagesTactfully combining Hydrogen and RGB data for balanced images
How the Eye Perceives ColorHow the Eye Perceives Color
Setting the Reference: The Setting the Reference: The SunSun
Kitt Peak Solar Observatory
An actual G2V CalibrationAn actual G2V Calibration
Sample G2V Calibrated Image: M3Sample G2V Calibrated Image: M3
Sample G2V Calibrated Image: M81 Sample G2V Calibrated Image: M81
Ha/L RGB Hue ShiftsHa/L RGB Hue Shifts
LRGB Images: The Color Shift LRGB Images: The Color Shift Problem: Salmon PinksProblem: Salmon Pinks
Lab image detailsLab image details Some math details – Why the shift?Some math details – Why the shift?
Conversion to Lab starts with RGB -> CIE XYZ Conversion to Lab starts with RGB -> CIE XYZ space then to Lab.space then to Lab.
Conversion math reveals a coupling of G and LConversion math reveals a coupling of G and L ““Salmon Pink” is light red + a bit of green addedSalmon Pink” is light red + a bit of green added Increasing L in value in conversion elevates GIncreasing L in value in conversion elevates G So by adding additional L, we shift reds to salmonSo by adding additional L, we shift reds to salmon
Correcting the Hue ShiftCorrecting the Hue Shift
Next, Correct the SaturationNext, Correct the Saturation
The Final ComparisonThe Final Comparison
The Final Result:The Final Result:
Adding H-Alpha Data to the Image:Adding H-Alpha Data to the Image:-Why?-Why?
For Emission Nebula can be 85% of photonsFor Emission Nebula can be 85% of photons But - But - H-alphaH-alpha is is veryvery close to the near IR band = 70% total close to the near IR band = 70% total AND AND H-BetaH-Beta is very close to the center of the Blue band = 15% is very close to the center of the Blue band = 15%
Hydrogen Hydrogen enhanced images are enhanced images are Simply StunningSimply Stunning, ,
and provide additional and provide additional Significant StructureSignificant Structure..
-How?-How? We then add it to the closest wavelengths: We then add it to the closest wavelengths: RED, RED, BLUE.BLUE.
Emission Nebula:Emission Nebula:The Process of adding The Process of adding HydroHydrogengen Data – Data – How NOT to do it…How NOT to do it…
Star Color distortionStar Color distortion
By adding By adding H-alphaH-alpha data we change the data we change the G2V balance of the star imagesG2V balance of the star images
We can We can maintainmaintain the balance by the balance by combining combining HydroHydrogengen data frame with data frame with the original the original R R && BB frame using frame using LightenLighten..
Restoring G2V balance with LightenRestoring G2V balance with Lighten
Second Example: M16 in SerpensSecond Example: M16 in Serpens
Final DiscussionFinal Discussion Understanding how adding additional Luminance Understanding how adding additional Luminance
data will affect the entire Lab Color Schemedata will affect the entire Lab Color Scheme Tastefully adding Hydrogen data into RGB images Tastefully adding Hydrogen data into RGB images
while retaining G2V balance is possiblewhile retaining G2V balance is possible