Closed KelSolaar closed 10 years ago
Here is the current relevant list of mappings and a proposal for some aliases: https://docs.google.com/spreadsheets/d/1Xfto7D6VAmEnT9EaZsjO5l_dnziRhd0AEVsBWZnp5_w/edit?usp=sharing
I'm not sure I am a fan of the numeric aliases. While they are nice and short to write, they are impossible to interpret while reading the code that is using them.
I'd propose to use terse, but meaningful strings that contain enough information to at least give the reader an idea what he is seeing.
A few example (just of the top of my head, not supposed to be definitive)
Verbose name | alias |
---|---|
Small Areas, Uniform Background & Surrounds | small_uniform |
Normal Scenes | normal |
Television & CRT, Dim Surrounds | crt_dim |
CIE 1931 2 Degree Standard Observer | cie_2_1931 |
CIE 2012 2 Degree Standard Observer | cie_2_2012 |
Yeah that's the exact feeling I got when feeding the spreadsheet, I'll work toward a better proposal following your model.
Here is a proposal Michael, if it looks good, I'll roll it:
Mapping | Alias |
---|---|
CHROMATIC_ADAPTATION_METHODS | |
XYZ Scaling | |
Bradford | |
Von Kries | |
Fairchild | |
CAT02 | |
CIECAM02_VIEWING_CONDITIONS | |
Average | |
Dim | |
Dark | |
HUNT_VIEWING_CONDITIONS | |
Small Areas, Uniform Background & Surrounds | small_uniform |
Normal Scenes | normal |
Television & CRT, Dim Surrounds | tv_dim |
Large Transparencies On Light Boxes | light_boxes |
Projected Transparencies, Dark Surrounds | dark |
LLAB_VIEWING_CONDITIONS | |
Reference Samples & Images, Average Surround, Subtending > 4 | ref_average_4_plus |
Reference Samples & Images, Average Surround, Subtending < 4 | ref_average_4_minus |
Television & VDU Displays, Dim Surround | tv_dim |
Cut Sheet Transparency, Dim Surround | sheet_dim |
35mm Projection Transparency, Dark Surround | dark |
RLAB_VIEWING_CONDITIONS | |
Average | |
Dim | |
Dark | |
COLOURCHECKERS | |
BabelColor Average | average |
ColorChecker 2005 | crc_2005 |
ColorChecker 1976 | |
COLOURCHECKERS_SPDS | |
BabelColor Average | |
ColorChecker N Ohta | |
BANDPASS_CORRECTION_METHODS | |
Stearns 1988 | |
LIGHTNESS_FUNCTIONS | |
Lightness Glasser 1958 | |
Lightness Wyszecki 1964 | |
Lightness 1976 | l_star |
LUMINANCE_FUNCTIONS | |
Luminance Newhall 1943 | |
Luminance 1976 | l_star |
Luminance ASTM D1535-08 | astm |
LMS_CMFS | |
Stockman & Sharpe 2 Degree Cone Fundamentals | |
RGB_CMFS | |
Wright & Guild 1931 2 Degree RGB CMFs | |
Stiles & Burch 1955 2 Degree RGB CMFs | |
Stiles & Burch 1959 10 Degree RGB CMFs | |
STANDARD_OBSERVERS_CMFS | |
CIE 1931 2 Degree Standard Observer | cie_2_1931 |
CIE 1964 10 Degree Standard Observer | cie_10_1964 |
CIE 2012 2 Degree Standard Observer | |
CIE 2012 10 Degree Standard Observer | |
CMFS | |
PHOTOPIC_LEFS | |
CIE 1924 Photopic Standard Observer | cie_2_1924 |
Judd Modified CIE 1951 Photopic Standard Observer | |
Judd-Vos Modified CIE 1978 Photopic Standard Observer | |
CIE 1964 Photopic 10 Degree Standard Observer | cie_10_1964 |
CIE 2008 2 Degree Physiologically Relevant LEF | |
CIE 2008 10 Degree Physiologically Relevant LEF | |
SCOTOPIC_LEFS | |
CIE 1951 Scotopic Standard Observer | cie_1951 |
LEFS | |
ILLUMINANTS | |
CIE 1931 2 Degree Standard Observer | cie_2_1931 |
CIE 1964 10 Degree Standard Observer | cie_10_1964 |
RGB_COLOURSPACES | |
ACES_RGB_COLOURSPACE | aces |
ACES_RGB_LOG_COLOURSPACE | |
ACES_RGB_PROXY_10_COLOURSPACE | |
ACES_RGB_PROXY_12_COLOURSPACE | |
ADOBE_RGB_1998_COLOURSPACE | adobe_1998 |
ADOBE_WIDE_GAMUT_RGB_COLOURSPACE | |
ALEXA_WIDE_GAMUT_RGB_COLOURSPACE | |
APPLE_RGB_COLOURSPACE | |
BEST_RGB_COLOURSPACE | |
BETA_RGB_COLOURSPACE | |
CIE_RGB_COLOURSPACE | |
C_LOG_COLOURSPACE | |
COLOR_MATCH_RGB_COLOURSPACE | |
DCI_P3_COLOURSPACE | |
DON_RGB_4_COLOURSPACE | |
ECI_RGB_V2_COLOURSPACE | |
EKTA_SPACE_PS_5_COLOURSPACE | |
MAX_RGB_COLOURSPACE | |
NTSC_RGB_COLOURSPACE | |
PAL_SECAM_RGB_COLOURSPACE | |
PROPHOTO_RGB_COLOURSPACE | prophoto |
REC_709_COLOURSPACE | |
REC_2020_COLOURSPACE | |
RUSSELL_RGB_COLOURSPACE | |
S_LOG_COLOURSPACE | |
SMPTE_C_RGB_COLOURSPACE | |
sRGB_COLOURSPACE | |
XTREME_RGB_COLOURSPACE | |
MUNSELL_VALUE_FUNCTIONS | |
Munsell Value Priest 1920 | |
Munsell Value Munsell 1933 | |
Munsell Value Moon 1943 | |
Munsell Value Saunderson 1944 | |
Munsell Value Ladd 1955 | |
Munsell Value McCamy 1987 | |
Munsell Value ASTM D1535-08 | astm |
UV_TO_CCT_METHODS | |
Ohno 2013 | ohno |
Robertson 1968 | robertson |
CCT_TO_UV_METHODS | |
Ohno 2013 | ohno |
Robertson 1968 | robertson |
XY_TO_CCT_METHODS | |
McCamy 1992 | mcamy |
Hernandez 1999 | hernandez |
CCT_TO_XY_METHODS | |
Kang 2002 | kang |
CIE Illuminant D Series | d |
Looks great!
What do you think of extending the two dark
s to projected_dark
?
Just dark
might be too general and give the impression of a default value.
Yeah agreed, here we go:
Mapping | Alias |
---|---|
CHROMATIC_ADAPTATION_METHODS | |
XYZ Scaling | |
Bradford | |
Von Kries | |
Fairchild | |
CAT02 | |
CIECAM02_VIEWING_CONDITIONS | |
Average | |
Dim | |
Dark | |
HUNT_VIEWING_CONDITIONS | |
Small Areas, Uniform Background & Surrounds | small_uniform |
Normal Scenes | normal |
Television & CRT, Dim Surrounds | tv_dim |
Large Transparencies On Light Boxes | light_boxes |
Projected Transparencies, Dark Surrounds | projected_dark |
LLAB_VIEWING_CONDITIONS | |
Reference Samples & Images, Average Surround, Subtending > 4 | ref_average_4_plus |
Reference Samples & Images, Average Surround, Subtending < 4 | ref_average_4_minus |
Television & VDU Displays, Dim Surround | tv_dim |
Cut Sheet Transparency, Dim Surround | sheet_dim |
35mm Projection Transparency, Dark Surround | projected_dark |
RLAB_VIEWING_CONDITIONS | |
Average | |
Dim | |
Dark | |
COLOURCHECKERS | |
BabelColor Average | average |
ColorChecker 2005 | crc_2005 |
ColorChecker 1976 | |
COLOURCHECKERS_SPDS | |
BabelColor Average | |
ColorChecker N Ohta | |
BANDPASS_CORRECTION_METHODS | |
Stearns 1988 | |
LIGHTNESS_FUNCTIONS | |
Lightness Glasser 1958 | |
Lightness Wyszecki 1964 | |
Lightness 1976 | l_star |
LUMINANCE_FUNCTIONS | |
Luminance Newhall 1943 | |
Luminance 1976 | l_star |
Luminance ASTM D1535-08 | astm |
LMS_CMFS | |
Stockman & Sharpe 2 Degree Cone Fundamentals | |
RGB_CMFS | |
Wright & Guild 1931 2 Degree RGB CMFs | |
Stiles & Burch 1955 2 Degree RGB CMFs | |
Stiles & Burch 1959 10 Degree RGB CMFs | |
STANDARD_OBSERVERS_CMFS | |
CIE 1931 2 Degree Standard Observer | cie_2_1931 |
CIE 1964 10 Degree Standard Observer | cie_10_1964 |
CIE 2012 2 Degree Standard Observer | |
CIE 2012 10 Degree Standard Observer | |
CMFS | |
PHOTOPIC_LEFS | |
CIE 1924 Photopic Standard Observer | cie_2_1924 |
Judd Modified CIE 1951 Photopic Standard Observer | |
Judd-Vos Modified CIE 1978 Photopic Standard Observer | |
CIE 1964 Photopic 10 Degree Standard Observer | cie_10_1964 |
CIE 2008 2 Degree Physiologically Relevant LEF | |
CIE 2008 10 Degree Physiologically Relevant LEF | |
SCOTOPIC_LEFS | |
CIE 1951 Scotopic Standard Observer | cie_1951 |
LEFS | |
ILLUMINANTS | |
CIE 1931 2 Degree Standard Observer | cie_2_1931 |
CIE 1964 10 Degree Standard Observer | cie_10_1964 |
RGB_COLOURSPACES | |
ACES_RGB_COLOURSPACE | aces |
ACES_RGB_LOG_COLOURSPACE | |
ACES_RGB_PROXY_10_COLOURSPACE | |
ACES_RGB_PROXY_12_COLOURSPACE | |
ADOBE_RGB_1998_COLOURSPACE | adobe_1998 |
ADOBE_WIDE_GAMUT_RGB_COLOURSPACE | |
ALEXA_WIDE_GAMUT_RGB_COLOURSPACE | |
APPLE_RGB_COLOURSPACE | |
BEST_RGB_COLOURSPACE | |
BETA_RGB_COLOURSPACE | |
CIE_RGB_COLOURSPACE | |
C_LOG_COLOURSPACE | |
COLOR_MATCH_RGB_COLOURSPACE | |
DCI_P3_COLOURSPACE | |
DON_RGB_4_COLOURSPACE | |
ECI_RGB_V2_COLOURSPACE | |
EKTA_SPACE_PS_5_COLOURSPACE | |
MAX_RGB_COLOURSPACE | |
NTSC_RGB_COLOURSPACE | |
PAL_SECAM_RGB_COLOURSPACE | |
PROPHOTO_RGB_COLOURSPACE | prophoto |
REC_709_COLOURSPACE | |
REC_2020_COLOURSPACE | |
RUSSELL_RGB_COLOURSPACE | |
S_LOG_COLOURSPACE | |
SMPTE_C_RGB_COLOURSPACE | |
sRGB_COLOURSPACE | |
XTREME_RGB_COLOURSPACE | |
MUNSELL_VALUE_FUNCTIONS | |
Munsell Value Priest 1920 | |
Munsell Value Munsell 1933 | |
Munsell Value Moon 1943 | |
Munsell Value Saunderson 1944 | |
Munsell Value Ladd 1955 | |
Munsell Value McCamy 1987 | |
Munsell Value ASTM D1535-08 | astm |
UV_TO_CCT_METHODS | |
Ohno 2013 | ohno |
Robertson 1968 | robertson |
CCT_TO_UV_METHODS | |
Ohno 2013 | ohno |
Robertson 1968 | robertson |
XY_TO_CCT_METHODS | |
McCamy 1992 | mcamy |
Hernandez 1999 | hernandez |
CCT_TO_XY_METHODS | |
Kang 2002 | kang |
CIE Illuminant D Series | d |
Sorry for the nitpicking:
babel_average
d
could be cie_d
It's not nitpicking, we have to get those right! :)
McCamy 1992, mccamy 1992, MCCAMY 1992
babel_average
, speaks more than average
cie_d
.Which leads me to the CAMs and others for more consistency: the CIE is trimming the first two numbers in the years: CIECAM97, CIECAM02 and you did the same for the others which is fine and consistent. I'm wondering if we shouldn't do the same for all the objects in the API?
UV_TO_CCT_METHODS = CaseInsensitiveMapping(
{'Ohno 2013': uv_to_CCT_ohno2013,
'Robertson 1968': uv_to_CCT_robertson1968})
Would become:
UV_TO_CCT_METHODS = CaseInsensitiveMapping(
{'Ohno 2013': uv_to_CCT_ohno13,
'Robertson 1968': uv_to_CCT_robertson68})
And now we could add the ohno13
and robertson68
aliases.
I'm somewhat torn.
The names of the CIE models are just the official names, I would not change anything there, and while ohno13
and robertson68
look perfectly fine to me, there might be cases where the meaning of the number as a year might get lost and things start to look very confusing to the casual observer (e.g., cie_2_31
versus cie_10_64
). Also we are in a place (well time actually...) where a lower number can denote a newer date (e.g., for the CIE 2012 Observers), which might also lead to confusion.
Overall I'd say using the whole year might be safer. Or we might compromise the name+YY for the name based aliases and the full year everywhere else.
Yeah, it's not very easy to come up with something nice here (It's the main reason I have chosen the very big long descriptive names so there are no ambiguities). What about this:
Mapping | Alias |
---|---|
CHROMATIC_ADAPTATION_METHODS | |
XYZ Scaling | |
Bradford | |
Von Kries | |
Fairchild | |
CAT02 | |
CIECAM02_VIEWING_CONDITIONS | |
Average | |
Dim | |
Dark | |
HUNT_VIEWING_CONDITIONS | |
Small Areas, Uniform Background & Surrounds | small_uniform |
Normal Scenes | normal |
Television & CRT, Dim Surrounds | tv_dim |
Large Transparencies On Light Boxes | light_boxes |
Projected Transparencies, Dark Surrounds | projected_dark |
LLAB_VIEWING_CONDITIONS | |
Reference Samples & Images, Average Surround, Subtending > 4 | ref_average_4_plus |
Reference Samples & Images, Average Surround, Subtending < 4 | ref_average_4_minus |
Television & VDU Displays, Dim Surround | tv_dim |
Cut Sheet Transparency, Dim Surround | sheet_dim |
35mm Projection Transparency, Dark Surround | projected_dark |
RLAB_VIEWING_CONDITIONS | |
Average | |
Dim | |
Dark | |
COLOURCHECKERS | |
BabelColor Average | babel_average |
ColorChecker 2005 | crc2005 |
ColorChecker 1976 | |
COLOURCHECKERS_SPDS | |
BabelColor Average | |
ColorChecker N Ohta | |
BANDPASS_CORRECTION_METHODS | |
Stearns 1988 | |
LIGHTNESS_FUNCTIONS | |
Lightness Glasser 1958 | |
Lightness Wyszecki 1964 | |
Lightness 1976 | l_star1976 |
LUMINANCE_FUNCTIONS | |
Luminance Newhall 1943 | |
Luminance 1976 | l_star1976 |
Luminance ASTM D1535-08 | astm2008 |
LMS_CMFS | |
Stockman & Sharpe 2 Degree Cone Fundamentals | |
RGB_CMFS | |
Wright & Guild 1931 2 Degree RGB CMFs | |
Stiles & Burch 1955 2 Degree RGB CMFs | |
Stiles & Burch 1959 10 Degree RGB CMFs | |
STANDARD_OBSERVERS_CMFS | |
CIE 1931 2 Degree Standard Observer | cie_2_1931 |
CIE 1964 10 Degree Standard Observer | cie_10_1964 |
CIE 2012 2 Degree Standard Observer | |
CIE 2012 10 Degree Standard Observer | |
CMFS | |
PHOTOPIC_LEFS | |
CIE 1924 Photopic Standard Observer | cie_2_1924 |
Judd Modified CIE 1951 Photopic Standard Observer | |
Judd-Vos Modified CIE 1978 Photopic Standard Observer | |
CIE 1964 Photopic 10 Degree Standard Observer | cie_10_1964 |
CIE 2008 2 Degree Physiologically Relevant LEF | |
CIE 2008 10 Degree Physiologically Relevant LEF | |
SCOTOPIC_LEFS | |
CIE 1951 Scotopic Standard Observer | cie_1951 |
LEFS | |
ILLUMINANTS | |
CIE 1931 2 Degree Standard Observer | cie_2_1931 |
CIE 1964 10 Degree Standard Observer | cie_10_1964 |
RGB_COLOURSPACES | |
ACES_RGB_COLOURSPACE | aces |
ACES_RGB_LOG_COLOURSPACE | |
ACES_RGB_PROXY_10_COLOURSPACE | |
ACES_RGB_PROXY_12_COLOURSPACE | |
ADOBE_RGB_1998_COLOURSPACE | adobe1998 |
ADOBE_WIDE_GAMUT_RGB_COLOURSPACE | |
ALEXA_WIDE_GAMUT_RGB_COLOURSPACE | |
APPLE_RGB_COLOURSPACE | |
BEST_RGB_COLOURSPACE | |
BETA_RGB_COLOURSPACE | |
CIE_RGB_COLOURSPACE | |
C_LOG_COLOURSPACE | |
COLOR_MATCH_RGB_COLOURSPACE | |
DCI_P3_COLOURSPACE | |
DON_RGB_4_COLOURSPACE | |
ECI_RGB_V2_COLOURSPACE | |
EKTA_SPACE_PS_5_COLOURSPACE | |
MAX_RGB_COLOURSPACE | |
NTSC_RGB_COLOURSPACE | |
PAL_SECAM_RGB_COLOURSPACE | |
PROPHOTO_RGB_COLOURSPACE | prophoto |
REC_709_COLOURSPACE | |
REC_2020_COLOURSPACE | |
RUSSELL_RGB_COLOURSPACE | |
S_LOG_COLOURSPACE | |
SMPTE_C_RGB_COLOURSPACE | |
sRGB_COLOURSPACE | |
XTREME_RGB_COLOURSPACE | |
MUNSELL_VALUE_FUNCTIONS | |
Munsell Value Priest 1920 | |
Munsell Value Munsell 1933 | |
Munsell Value Moon 1943 | |
Munsell Value Saunderson 1944 | |
Munsell Value Ladd 1955 | |
Munsell Value McCamy 1987 | |
Munsell Value ASTM D1535-08 | astm2008 |
UV_TO_CCT_METHODS | |
Ohno 2013 | ohno2013 |
Robertson 1968 | robertson1968 |
CCT_TO_UV_METHODS | |
Ohno 2013 | ohno2013 |
Robertson 1968 | robertson1968 |
XY_TO_CCT_METHODS | |
McCamy 1992 | mcamy1992 |
Hernandez 1999 | hernandez1999 |
CCT_TO_XY_METHODS | |
Kang 2002 | kang2002 |
CIE Illuminant D Series | cie_d |
The l_starYYYY
look slightly weird to me because they have an underscore in the name but none before the year. But that's consistent with the nameYYYY scheme so I can live with that.
Everything else looks fine to me.
Lstar1976
so that we remove the underscore and there is no confusion between L and i?
Sounds good. On 17 Aug 2014 23:58, "Thomas Mansencal" notifications@github.com wrote:
Lstar1976 so that we remove the underscore and there is no confusion between L and i?
— Reply to this email directly or view it on GitHub https://github.com/colour-science/colour/issues/97#issuecomment-52438375 .
As devil is in details we have now un uppercase letter in the alias (Which shouldn't be an issue because of case insensitivity), oh well... Let's go for that!
For instance when accessing the CIE 1931 2° Standard Observer illuminants we have right now to use the following form:
we can for instance have a shortcut like this: