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Акс:Sirius type double star animation 1.gif

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Мавод аз Википедиа — донишномаи озод

Sirius_type_double_star_animation_1.gif ((800 × 600 пиксел, ҳаҷми парванда: 5,06 Мбайт, навъи MIME: image/gif), looped, 100 frames, 5,0 s)

Ин файл аз Викианбор ва дар дигар лоиҳаҳо метавонад истифода шавад. Тафсилоти ин файл саҳифаи тафсилоти файл дар зер нишон дода шудааст.

Хулоса

Тавсифот
English: Star pair like Sirius. Artist rendering.
Сана
Манбаъ Кори худ
Муаллиф Merikanto

POV-Ray and ImageMagick source code

ImageMagick script

magick convert -delay 5 -loop 0 *.png sirius_type_double_star_animation_1.gif

POV-Ray 3.8 .ini file

POV-Ray animation ini file

Antialias=Off Antialias_Threshold=0.1

Antialias_Depth=2 Quality=11

Input_File_Name="sirisu3.pov"

Initial_Frame=1 Final_Frame=100 Initial_Clock=0 Final_Clock=360

Cyclic_Animation=on Pause_when_Done=off

POV-Ray 3.8 source code

///////////////////////////// // // Sirius-type double star // // POV-Ray 3.8 source code // // 30.9.2023 v 0000.0001 // /////////////////////////////

  1. include "functions.inc"
  2. include "rand.inc"
  3. include "shapes3.inc"


  1. declare tau_ofset=90;
  1. declare taunolla=clock+tau_ofset;
  1. declare randi1=rand(1);
  2. declare randi2=rand(2);
  3. declare randi3=rand(3);
  1. declare tau1=radians(taunolla);
  2. declare tau2=radians(taunolla+180.0);
  1. declare ra=3;
  2. declare rb=3;
  3. declare ax = sin(tau1)*ra+0.5;
  4. declare ay = cos(tau1)*ra;
  1. declare bx = sin(tau2)*rb-0.5;
  2. declare by = cos(tau2)*rb;

//## stella atmosphere

  1. declare atm_thickness1=1.5 ;


  1. declare samples1=30; // media samples, greater value slower to render


camera { location <0,25,-150>*1 look_at 0 angle 5 }

  1. macro convection_pigment(c)

crackle pigment_map{ [0.0 rgb c*0.2] [0.2 rgb c] [0.9 rgb c] [1.0 rgb 1.0]

} warp{turbulence 1}

  1. end


  1. declare stella_object_type_1= object {
        sphere {0,1 } 
   // ovus {1,0.7 rotate x*90 rotate y*-90}
   //object { Egg_Shape (1.15,1.55)  rotate x*90 rotate y*-90}
   

// texture { pigment {color rgb <1,1/2,0>} finish {ambient 0 }} }

  1. declare stella_object_type_2= object {
        difference 
       {
        sphere {0,1+atm_thickness1 } 
        sphere {0,1.001 } 
       }

}

//#declare star_pigment_1= pigment { wrinkles turbulence 0.4 scale 0.005 translate taunolla/360 color_map { [0 color rgb starcolor1a] [1 color rgb starcolor1c] } }


  1. macro makestar1(color1, color2, color3, color4)

object { union {


  // main sequence stella

object {

 object { stella_object_type_1  }   
 // texture {pigment {color rgb  color1} finish {ambient 1} }

// texture { pigment { convection_pigment(color1) scale 0.05} finish {ambient 1} }

   texture { 
     wrinkles scale 0.02
 //   granite  scale 0.1
         translate x*tau1*0.2
   warp { turbulence 0.5 }
   texture_map {

     [0 pigment { wrinkles turbulence 0.4 scale 0.005  translate taunolla/360   color_map {   [0 color rgb color1] [1 color rgb color3] }} finish {ambient 1}]    
     [0.85 pigment { wrinkles turbulence 0.4 scale 0.005  translate taunolla/360   color_map {   [0 color rgb color1] [1 color rgb color3] }} finish {ambient 1/2}]  
     [0.9 pigment { wrinkles turbulence 0.4 scale 0.005  translate taunolla/360   color_map {   [0 color rgb color1] [1 color rgb color3] }} finish {ambient 2/5}]   
     [1 pigment { wrinkles turbulence 0.4 scale 0.005  translate taunolla/360   color_map {   [0 color rgb color1] [1 color rgb color3] }} finish {ambient 0.2}]    
 } 
          
 
} // ...tex
        
   scale 1
} // stella object
 


// stella korona try 1

object {
 object {stella_object_type_2}
   pigment{rgbt 1}
       hollow

      interior{ 
   media{ method 3      
        //   absorption (1-color1)*1 // darkening
          emission color3*3/10
       //  scattering{ 4,(1-color1)// Type
         
        //   } // end scattering
          density{ 
          // #declare qq=tau1/(pi*2);
          
 function {   
       pow( 1*sqrt(1*(x*x+y*y+z*z)),-6 )  
//   * pow( f_granite(  atan2(x,y), atan2(x,z),atan2(y,z)),1/1)
//   * pow( f_granite( atan2(x+f_wrinkles(x,y,z),y+f_granite(x,y,z)*0.2), 1,1),z)  
   * pow( f_granite( atan2(x+f_wrinkles(x,y,z),y+f_granite(x,y,z)*0.2), 1,1),2)  
  • 0.5

+ pow( 1*sqrt(1*(x*x+y*y+z*z)),-6 )*0.2 }

  //    translate x*tau1*0.2
   density_map
          { 
           [0 rgb color1*0.000000000] 
       //   [0.1 rgb color3*1]
          //   [0+atm_thickness1 rgb color3*1]
         
           [1 rgb color1*3] 
            }
          } // 
          samples samples1 
    }  // ... density
 } // ... interior
//  scale 1.0+atm_thickness1

// scale 0.9

} // ... obj stella atm


} // union } // object

  1. end // end makestar1 macro


  1. macro makestar2(color1, color2, color3, color4)

object { union {

  // main sequence stella

object {

 object { stella_object_type_1  }   
  texture {pigment {color rgb  color1} finish {ambient 1} }

// texture { pigment { convection_pigment(color1) scale 0.05} finish {ambient 1} }

// texture {

//     wrinkles scale 0.02
 //   granite  scale 0.1
//         translate x*tau1*0.2
//   warp { turbulence 0.5 }
//   texture_map {

//     [0 pigment { wrinkles turbulence 0.4 scale 0.005  translate taunolla/360   color_map {   [0 color rgb color1] [1 color rgb color3] }} finish {ambient 1}]    
//     [0.85 pigment { wrinkles turbulence 0.4 scale 0.005  translate taunolla/360   color_map {   [0 color rgb color1] [1 color rgb color3] }} finish {ambient 0.6}]  
//     [0.9 pigment { wrinkles turbulence 0.4 scale 0.005  translate taunolla/360   color_map {   [0 color rgb color1] [1 color rgb color3] }} finish {ambient 0.4}]   
//     [1 pigment { wrinkles turbulence 0.4 scale 0.005  translate taunolla/360   color_map {   [0 color rgb color1] [1 color rgb color3] }} finish {ambient 0.0}]    

// }

          // } // ...tex
        
   scale 1
} // stella object
 


// stella korona2 try 1

object {
 object {stella_object_type_1}
   pigment{rgbt 1}
       hollow

      interior{ 
   media{ method 3      
        //   absorption (1-color1)*1 // darkening
          emission color3*1/10
       //  scattering{ 4,(1-color1)// Type
         
        //   } // end scattering
          density{ 
      //    #declare qq=tau1/(pi*2);
 function {   

// pow( 1*sqrt(1*(x*x+y*y+z*z)),-6 )


//   * pow( f_granite(  atan2(x,y), atan2(x,z),atan2(y,z)),1/1)

// * pow( f_granite( atan2(x+f_wrinkles(x,y,z),y+f_granite(x,y,z)*0.1), 1,1),1/1) //*0.5 //+ pow( 1*sqrt(1*(x*x+y*y+z*z)),-6 )*0.2 // pow( 1/3*sqrt(4*(x*x+y*y+z*z)),-5 )*1

pow(f_spherical(x,y,z),2)*2
*f_wrinkles(x,y,z) *2
  • pow( f_granite( atan2(x,y)/2, atan2(x,z)/2,atan2(y,z)/2),1/1)

}

  //    translate x*tau1*0.2
   density_map
          { 
           [0 rgb color1*0.000000000] 
       //   [0.1 rgb color3*1]
          //   [0+atm_thickness1 rgb color3*1]
         
           [1 rgb color1*20] 
            }
          } // 
          samples samples1 
    }  // ... density
 } // ... interior
  scale 3

// scale 0.9

} // ... obj stella atm


} // union } // object

  1. end // end makestar1 macro


// star 1

  #declare color1=<1,1,1>*1.2;
#declare color2=<1,1,1,0>*1.2;   
  1. declare color3=<1,1,1.4>*1;
#declare color4=<1,1,1.4,0>*1;  


union {

makestar1(color1, color2, color3, color4 )    
  scale 1.68*1   
   rotate taunolla
// scale 1
    translate <ax,0,ay>*1 
  }

// star 2

  #declare color1=<1,1,2>*2;
#declare color2=<1,1,3,0>;   
  1. declare color3=<1,1,1.5>*2;
#declare color4=<1,1,1.5,0>;  

union {

makestar2(color1, color2, color3, color4 )   
   rotate taunolla 
   scale 1/5
    translate <bx,0,by>*1 
  }

Иҷозатнома

I, the copyright holder of this work, hereby publish it under the following license:
w:en:Creative Commons
тахсис саҳми яксон
This file is licensed under the Creative Commons Attribution-Share Alike 4.0 International license.
Шумо озодед:
  • мубодилот намудан – копӣ, паҳн ва фиристадани асар
  • ремикс кардан – татбиқи кор
Under the following conditions:
  • тахсис – You must give appropriate credit, provide a link to the license, and indicate if changes were made. You may do so in any reasonable manner, but not in any way that suggests the licensor endorses you or your use.
  • саҳми яксон – If you remix, transform, or build upon the material, you must distribute your contributions under the same or compatible license as the original.

Captions

Add a one-line explanation of what this file represents
Double star that has A-spectral class star and white dwaf

Items portrayed in this file

тавсифҳо

source of file Англисӣ

30 сентябри 2023

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нусхаи феълӣ17:36, 30 сентябри 2023Акси бандангуштӣ аз нусхаи то 17:36, 30 сентябри 2023800 × 600 (5,06 Мбайт)MerikantoUploaded own work with UploadWizard

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