[Bf-extensions-cvs] [1df44726] master: Added Lamp , Radiosity, and World presets

Sun Jan 28 13:47:24 CET 2018

Commit: 1df44726b049543330d033fd7685771007eae06d
Author: Maurice Raybaud
Date:   Sun Jan 28 13:47:02 2018 +0100
Branches: master
https://developer.blender.org/rBA1df44726b049543330d033fd7685771007eae06d

Added Lamp , Radiosity, and World presets

===================================================================

A	presets/pov/lamp/01_(5400K)_Direct_Sun.py
A	presets/pov/lamp/02_(5400K)_High_Noon_Sun.py
A	presets/pov/lamp/03_(6000K)_Daylight_Window.py
A	presets/pov/lamp/04_(6000K)_2500W_HMI_(Halogen_Metal_Iodide).py
A	presets/pov/lamp/05_(4000K)_100W_Metal_Halide.py
A	presets/pov/lamp/06_(3200K)_100W_Quartz_Halogen.py
A	presets/pov/lamp/07_(2850K)_100w_Tungsten.py
A	presets/pov/lamp/08_(2600K)_40w_Tungsten.py
A	presets/pov/lamp/09_(5000K)_75W_Full_Spectrum_Fluorescent_T12.py
A	presets/pov/lamp/10_(4300K)_40W_Vintage_Fluorescent_T12.py
A	presets/pov/lamp/11_(5000K)_18W_Standard_Fluorescent_T8.py
A	presets/pov/lamp/12_(4200K)_18W_Cool_White_Fluorescent_T8.py
A	presets/pov/lamp/13_(3000K)_18W_Warm_Fluorescent_T8.py
A	presets/pov/lamp/14_(6500K)_54W_Grow_Light_Fluorescent_T5-HO.py
A	presets/pov/lamp/15_(3200K)_40W_Induction_ Fluorescent.py
A	presets/pov/lamp/16_(2100K)_150W_High_Pressure_Sodium.py
A	presets/pov/lamp/17_(1700K)_135W_Low_Pressure_Sodium.py
A	presets/pov/lamp/18_(6800K)_175W_Mercury_Vapor.py
A	presets/pov/lamp/19_(5200K)_700W_Carbon_Arc.py
A	presets/pov/lamp/20_(6500K)_15W_LED_Spot.py
A	presets/pov/lamp/21_(2700K)_7W_OLED_Panel.py
A	presets/pov/lamp/22_(30000K)_40W_Black_Light_Fluorescent.py
A	presets/pov/lamp/23_(30000K)_40W_Black_Light_Bulb.py
A	presets/pov/lamp/24_(1850K)_Candle.py
A	presets/pov/radiosity/01_Debug.py
A	presets/pov/radiosity/02_Fast.py
A	presets/pov/radiosity/03_Normal.py
A	presets/pov/radiosity/04_Two_Bounces.py
A	presets/pov/radiosity/05_Final.py
A	presets/pov/radiosity/06_Outdoor_Low_Quality.py
A	presets/pov/radiosity/07_Outdoor_High_Quality.py
A	presets/pov/radiosity/08_Outdoor_(Sun)Light.py
A	presets/pov/radiosity/09_Indoor_Low_Quality.py
A	presets/pov/radiosity/10_Indoor_High_Quality.py
A	presets/pov/world/1_Clear_Blue_Sky.py
A	presets/pov/world/2_Partly_Hazy_Sky.py
A	presets/pov/world/3_Overcast_Sky.py
A	presets/pov/world/4_Cartoony_Sky.py
A	presets/pov/world/5_Under_Water.py
M	render_povray/__init__.py
M	render_povray/render.py
M	render_povray/shading.py
M	render_povray/ui.py

===================================================================

diff --git a/presets/pov/lamp/01_(5400K)_Direct_Sun.py b/presets/pov/lamp/01_(5400K)_Direct_Sun.py
new file mode 100644
index 00000000..7f53ce06
--- /dev/null
+++ b/presets/pov/lamp/01_(5400K)_Direct_Sun.py
@@ -0,0 +1,10 @@
+#Since the dawn of time
+
+import bpy
+bpy.context.object.data.type = 'SUN'
+lampdata = bpy.context.object.data
+
+lampdata.color = (1.0, 1.0, 0.9843137264251709)
+lampdata.energy = 1.2 #100 000lux
+#lampdata.distance = 0.001
+#lampdata.falloff_type = 'INVERSE_SQUARE'
\ No newline at end of file
diff --git a/presets/pov/lamp/02_(5400K)_High_Noon_Sun.py b/presets/pov/lamp/02_(5400K)_High_Noon_Sun.py
new file mode 100644
index 00000000..6d3083a6
--- /dev/null
+++ b/presets/pov/lamp/02_(5400K)_High_Noon_Sun.py
@@ -0,0 +1,17 @@
+#Since the dawn of time
+
+import bpy
+bpy.context.object.rotation_euler = (0,0,0)#And loc HIGH
+bpy.context.object.location = (0,0,700000000)
+bpy.context.object.data.type = 'AREA'
+lampdata = bpy.context.object.data
+
+lampdata.shape = 'SQUARE'
+lampdata.size = 30000000#0.02
+#lampdata.size_y = 0.02
+lampdata.shadow_ray_samples_x = 2
+#lampdata.shadow_ray_samples_y = 3
+lampdata.color = (1.0, 1.0, 1.0)
+lampdata.energy = 1.094316#91193 #lux
+lampdata.distance =695699968
+
diff --git a/presets/pov/lamp/03_(6000K)_Daylight_Window.py b/presets/pov/lamp/03_(6000K)_Daylight_Window.py
new file mode 100644
index 00000000..a9781f57
--- /dev/null
+++ b/presets/pov/lamp/03_(6000K)_Daylight_Window.py
@@ -0,0 +1,13 @@
+#Since the dawn of time
+
+import bpy
+bpy.context.object.data.type = 'AREA'
+lampdata = bpy.context.object.data
+
+lampdata.size = 1.2
+lampdata.size_y = 2.10
+lampdata.shadow_ray_samples_x = 2
+lampdata.shadow_ray_samples_y = 3
+lampdata.color = (1.0, 1.0, 1.0)
+lampdata.energy = 1.094316#91193 #lux
+lampdata.distance = 1.0
diff --git a/presets/pov/lamp/04_(6000K)_2500W_HMI_(Halogen_Metal_Iodide).py b/presets/pov/lamp/04_(6000K)_2500W_HMI_(Halogen_Metal_Iodide).py
new file mode 100644
index 00000000..0bfa95d8
--- /dev/null
+++ b/presets/pov/lamp/04_(6000K)_2500W_HMI_(Halogen_Metal_Iodide).py
@@ -0,0 +1,14 @@
+#After 1969
+#made specifically for film and entertainment applications
+
+import bpy
+bpy.context.object.data.type = 'SPOT'
+lampdata = bpy.context.object.data
+
+lampdata.show_cone = True
+lampdata.spot_size = 0.872665
+lampdata.spot_blend = 0.9
+lampdata.color = (0.99, 0.9882352948188782, 0.998)
+lampdata.energy = 223.81796 #240000lm/21.446(=lux)*0.004*2.5(distance) *2 for distance is the point of half strength
+lampdata.distance = 0.001
+lampdata.falloff_type = 'INVERSE_SQUARE'
\ No newline at end of file
diff --git a/presets/pov/lamp/05_(4000K)_100W_Metal_Halide.py b/presets/pov/lamp/05_(4000K)_100W_Metal_Halide.py
new file mode 100644
index 00000000..e91d3f9a
--- /dev/null
+++ b/presets/pov/lamp/05_(4000K)_100W_Metal_Halide.py
@@ -0,0 +1,14 @@
+#After 1962
+#Common uses: outdoor lighting where good color rendering is needed, television/film lighting, sports fields, car headlights, flood lights, heavy flashlights, green house applications
+
+import bpy
+bpy.context.object.data.type = 'SPOT'
+lampdata = bpy.context.object.data
+
+lampdata.show_cone = True
+lampdata.spot_size = 0.6
+lampdata.spot_blend = 0.9
+lampdata.color = (0.9490196108818054, 0.9882352948188782, 1.0)
+lampdata.energy = 20.98293#9000lm/21.446(=lux)*0.004*6.25(distance) *2 for distance is the point of half strength
+lampdata.distance = 0.025
+lampdata.falloff_type = 'INVERSE_SQUARE'
\ No newline at end of file
diff --git a/presets/pov/lamp/06_(3200K)_100W_Quartz_Halogen.py b/presets/pov/lamp/06_(3200K)_100W_Quartz_Halogen.py
new file mode 100644
index 00000000..b58edf17
--- /dev/null
+++ b/presets/pov/lamp/06_(3200K)_100W_Quartz_Halogen.py
@@ -0,0 +1,16 @@
+#since 1960, no longer manufactured since 2016
+#8mm projectors
+#used in many automobiles headlamps ; outdoor lighting systems ; watercraft ; desktop lamps (smaller power).
+#theatrical and studio (film and television) fixtures, including Ellipsoidal reflector spotlights, Source Four, and Fresnels; PAR Cans 
+
+import bpy
+bpy.context.object.data.type = 'SPOT'
+lampdata = bpy.context.object.data
+
+lampdata.show_cone = True
+lampdata.spot_size = 1.9
+lampdata.spot_blend = 0.9
+lampdata.color = (1.0, 0.9450980424880981, 0.8784313797950745)
+lampdata.energy = 12.43433#5000/21.446 #lumen values/20 or lux when available used as a basis
+lampdata.distance = 0.015#energy calculated for length 0.075 but width gives better result
+lampdata.falloff_type = 'INVERSE_SQUARE'
diff --git a/presets/pov/lamp/07_(2850K)_100w_Tungsten.py b/presets/pov/lamp/07_(2850K)_100w_Tungsten.py
new file mode 100644
index 00000000..72675de3
--- /dev/null
+++ b/presets/pov/lamp/07_(2850K)_100w_Tungsten.py
@@ -0,0 +1,10 @@
+#1908 - today
+
+import bpy
+bpy.context.object.data.type = 'POINT'
+lampdata = bpy.context.object.data
+
+lampdata.color = (1.0, 0.8392156958580017, 0.6666666865348816)
+lampdata.energy = 7.46060#3.7303#1000/21.446/(lampdistance/candledistance)  #lumen values/21.446 or lux when available used as a basis
+lampdata.distance = 0.05
+lampdata.falloff_type = 'INVERSE_SQUARE'
\ No newline at end of file
diff --git a/presets/pov/lamp/08_(2600K)_40w_Tungsten.py b/presets/pov/lamp/08_(2600K)_40w_Tungsten.py
new file mode 100644
index 00000000..88ef46a0
--- /dev/null
+++ b/presets/pov/lamp/08_(2600K)_40w_Tungsten.py
@@ -0,0 +1,10 @@
+#since 1908
+
+import bpy
+bpy.context.object.data.type = 'POINT'
+lampdata = bpy.context.object.data
+
+lampdata.color = (1.0, 0.8196078431372549, 0.6980392156862745)
+lampdata.energy = 2.98424#400/21.446 #lumen values/21.446 or lux when available used as a basis
+lampdata.distance = 0.05
+lampdata.falloff_type = 'INVERSE_SQUARE'
\ No newline at end of file
diff --git a/presets/pov/lamp/09_(5000K)_75W_Full_Spectrum_Fluorescent_T12.py b/presets/pov/lamp/09_(5000K)_75W_Full_Spectrum_Fluorescent_T12.py
new file mode 100644
index 00000000..b0a23eda
--- /dev/null
+++ b/presets/pov/lamp/09_(5000K)_75W_Full_Spectrum_Fluorescent_T12.py
@@ -0,0 +1,14 @@
+#Available since 1979 (Triphosphor lamps)
+
+import bpy
+bpy.context.object.data.type = 'AREA'
+lampdata = bpy.context.object.data
+
+lampdata.size = 0.038
+lampdata.size_y = 2.40284
+lampdata.shadow_ray_samples_x = 1
+lampdata.shadow_ray_samples_y = 2
+lampdata.color = (1.0, 0.95686274766922, 0.9490200281143188)
+lampdata.energy = 4.45304#4775lm/21.446(=lux)*0.004(distance) *2 for distance is the point of half strength 6200lm?
+lampdata.distance = 1.0 #dist values multiplied by 10 for area lights for same power as bulb/spot/...
+#lampdata.falloff_type = 'INVERSE_SQUARE'
\ No newline at end of file
diff --git a/presets/pov/lamp/10_(4300K)_40W_Vintage_Fluorescent_T12.py b/presets/pov/lamp/10_(4300K)_40W_Vintage_Fluorescent_T12.py
new file mode 100644
index 00000000..d03ce6fd
--- /dev/null
+++ b/presets/pov/lamp/10_(4300K)_40W_Vintage_Fluorescent_T12.py
@@ -0,0 +1,14 @@
+#since 1939 , T12 no longer manufactured since T8 propagated
+
+import bpy
+bpy.context.object.data.type = 'AREA'
+lampdata = bpy.context.object.data
+
+lampdata.size = 0.038
+lampdata.size_y = 1.2192
+lampdata.shadow_ray_samples_x = 1
+lampdata.shadow_ray_samples_y = 2
+lampdata.color = (0.901, 1.0, 0.979)
+lampdata.energy = 2.14492#2300lm/21.446(=lux)*0.004*2.5(distance) *2 for distance is the point of half strength
+lampdata.distance = 1.0 #dist values multiplied by 10 for area lights for same power as bulb/spot/...
+#lampdata.falloff_type = 'INVERSE_SQUARE'
\ No newline at end of file
diff --git a/presets/pov/lamp/11_(5000K)_18W_Standard_Fluorescent_T8.py b/presets/pov/lamp/11_(5000K)_18W_Standard_Fluorescent_T8.py
new file mode 100644
index 00000000..6fef1763
--- /dev/null
+++ b/presets/pov/lamp/11_(5000K)_18W_Standard_Fluorescent_T8.py
@@ -0,0 +1,13 @@
+#since 1973 
+
+import bpy
+bpy.context.object.data.type = 'AREA'
+lampdata = bpy.context.object.data
+
+lampdata.size = 0.026
+lampdata.size_y = 0.59
+lampdata.shadow_ray_samples_x = 1
+lampdata.shadow_ray_samples_y = 2
+lampdata.color = (0.95686274766922, 1.0, 0.9803921580314636)
+lampdata.energy = 1.25898#1350lm/21.446(=lux)*0.004*2.5(distance) *2 for distance is the point of half strength
+lampdata.distance = 1.0 #dist values multiplied by 10 for area lights for same power as bulb/spot/...
diff --git a/presets/pov/lamp/12_(4200K)_18W_Cool_White_Fluorescent_T8.py b/presets/pov/lamp/12_(4200K)_18W_Cool_White_Fluorescent_T8.py
new file mode 100644
index 00000000..83f8dd4e
--- /dev/null
+++ b/presets/pov/lamp/12_(4200K)_18W_Cool_White_Fluorescent_T8.py
@@ -0,0 +1,15 @@
+#Available since 1979
+#more common than the warm white
+
+import bpy
+bpy.context.object.data.type = 'AREA'
+lampdata = bpy.context.object.data
+
+lampdata.size = 0.026
+lampdata.size_y = 0.59
+lampdata.shadow_ray_samples_x = 1
+lampdata.shadow_ray_samples_y = 2
+lampdata.color = (0.8313725590705872, 0.9215686321258545, 1.0)
+lampdata.energy = 1.25898#1350lm/21.446(=lux)*0.004*2.5(distance) *2 for distance is the point of half strength
+lampdata.distance = 1.0 #dist values multiplied by 10 for area lights for same power as bulb/spot/...
+#lampdata.falloff_type = 'INVERSE_SQUARE'
\ No newline at end of file
diff --git a/presets/pov/lamp/13_(3000K)_18W_Warm_Fluorescent_T8.py b/presets/pov/lamp/13_(3000K)_18W_Warm_Fluorescent_T8.py
new file mode 100644
index 00000000..e1cee557
--- /dev/null
+++ b/presets/pov/lamp/13_(3000K)_18W_Warm_Fluorescent_T8.py
@@ -0,0 +1,14 @@
+#Available since 1979
+#developed to get closer to tungsten atmospher in interiors
+
+import bpy
+bpy.context.object.data.type = 'AREA'
+lampdata = bpy.context.object.data
+
+lampdata.size = 0.026
+lampdata.size_y = 0.59
+lampdata.shadow_ray_samples_x = 1
+lampdata.shadow_ray_samples_y = 2
+lampdata.color = (1.0, 0.95686274766922, 0.8980392217636108)
+lampdata.energy = 1.25898#1350lm/21.446(=lux)*0.004*2.5(distance) *2 for distance is the point of half strength
+lampdata.distance = 1.0 #dist values multiplied by 10 for area lights for same power as bulb/spot/...
diff --git a/presets/pov/lamp/14_(6500K)_54W_Grow_Light_Fluorescent_T5-HO.py b/presets/pov/lamp/14_(6500K)_54W_Grow_Light_Fluorescent_T5-HO.py
new file mode 100644
index 00000000..55f84ab8
--- /dev/null
+++ b/

@@ Diff output truncated at 10240 characters. @@

