Tips for Processing LRGB and HaRGB Images: Getting the Color Right! - PowerPoint PPT Presentation

About This Presentation
Title:

Tips for Processing LRGB and HaRGB Images: Getting the Color Right!

Description:

How the Eye Perceives Color. Setting the Reference: The ... 'Salmon Pink' is light red a bit of green added. Increasing L in value in conversion elevates G ... – PowerPoint PPT presentation

Number of Views:95
Avg rating:3.0/5.0
Slides: 21
Provided by: chr1318
Category:

less

Transcript and Presenter's Notes

Title: Tips for Processing LRGB and HaRGB Images: Getting the Color Right!


1
Tips for Processing LRGB and HaRGB Images
Getting the Color Right!
  • By Chris Schur

2
Introduction
  • With Digital Imaging as the mainstay for
    astrophotograpy today, color balance remains an
    elusive target.
  • Here we will discuss key points on locking in
    accurate color balance for Deep Sky Images that
    use LRGB methodology.
  • Our topics will include
  • Setting a reference for our gray scale
  • Understanding the LRGB hue and saturation shift
  • Correcting the shift in LRGB images
  • Understanding the Hydrogen Alpha contribution to
    an image
  • The role of Hydrogen Beta in the final color of
    nebula
  • Tactfully combining Hydrogen and RGB data for
    balanced images

3
How the Eye Perceives Color
4
Setting the Reference The Sun
Kitt Peak Solar Observatory
5
An actual G2V Calibration
6
Sample G2V Calibrated Image M3
7
Sample G2V Calibrated Image M81
8
Ha/L RGB Hue Shifts
9
LRGB Images The Color Shift Problem Salmon
Pinks
10
Lab image details
  • Some math details Why the shift?
  • Conversion to Lab starts with RGB -gt CIE XYZ
    space then to Lab.
  • Conversion math reveals a coupling of G and L
  • Salmon Pink is light red a bit of green added
  • Increasing L in value in conversion elevates G
  • So by adding additional L, we shift reds to salmon

11
Correcting the Hue Shift
12
Next, Correct the Saturation
13
The Final Comparison
14
The Final Result
15
Adding H-Alpha Data to the Image-Why?
  • For Emission Nebula can be 85 of photons
  • But - H-alpha is very close to the near IR band
    70 total
  • AND H-Beta is very close to the center of the
    Blue band 15
  • Hydrogen enhanced images are Simply Stunning,
  • and provide additional Significant Structure.
  • -How?
  • We then add it to the closest wavelengths RED,
    BLUE.

16
Emission NebulaThe Process of adding Hydrogen
Data How NOT to do it
17
Star Color distortion
  • By adding H-alpha data we change the G2V balance
    of the star images
  • We can maintain the balance by combining Hydrogen
    data frame with the original R B frame using
    Lighten.

18
Restoring G2V balance with Lighten
19
Second Example M16 in Serpens
20
Final Discussion
  • Understanding how adding additional Luminance
    data will affect the entire Lab Color Scheme
  • Tastefully adding Hydrogen data into RGB images
    while retaining G2V balance is possible
Write a Comment
User Comments (0)
About PowerShow.com