Files
OpenSpace/shaders/grid_vs.glsl
michal 700f590a2a SPICE-time dependency, retrieval of spice ephemerides and rotational matrix + coordinate references.
Added functionality:
- New class renderablesphericalgrid is repurposed code from powerscaledsphere class.
  Due to z-buffer issues used as reference grid to confirm planetary orbits are correct.
  This has been a major problem as prior we had no visual reference.
  Now we have a Galactic-, Celestial- and Ecliptic-coordinate grid.
  To this also added separate shader: grid_vs.glsl / grid_fs.glsl
  These grids have a static-rotational matrix derived from partiview (thanks to Brian)
  since spice req. to-from frame to compute rotational matrix.

Time dependency:
- Added struct RuntimeData - which for now only contains openspace time and is passed to all renderables
- All renderables accept runtimeData, keep private reference and use for computation of rotational matrix
- This obviously carries corresponding changes to Scenegraph and ScenegraphNode.

Spicemanager:
- Added function that more easily provides access to rotational matrix used in spice
 (used in renderableplanet for computing planetary objects spin around axis)

Ephemeris-classes:
- Now compute ephemeris from spice based on timeepoch in runtimedata
  TODO: once z-buffer fixed - set ephemeris correctly as meters (not kilometers)

Renderengine:
- Advances time with the advanceTime method in RuntimeData struct

ISSUES:
- Our Y axis NOT same as SPICE or star-catalogue, all renderables rotated now 90deg, needs redefinition,
  lots of debugging and major headaches before this conclusion.
- Depth buffer needs to be fixed in order to properly place planets.
- Spice kernels have finite time-range, when time stops - simulation ends - ugly fix: reset time to zero.
  Possible fix: kernels de431 (part 1-2) cover huge timespan and most likely have functions to extrapolate time,
  drawback is that they are 1,7 gb each.

TODO:
- Compute and draw dynamic ephemeries for each renderable. Either do full year sweep then update for each point or
  create a tail of linesegments for each planet. Dont know yet how to do this, would like spicephemeris to be
  sub-class of Renderable (have own render() method) - good/bad?
2014-09-19 20:32:33 -04:00

108 lines
3.4 KiB
GLSL

/**
Copyright (C) 2012-2014 Jonas Strandstedt
Permission is hereby granted, free of charge, to any person obtaining
a copy of this software and associated documentation files (the "Software"),
to deal in the Software without restriction, including without limitation
the rights to use, copy, modify, merge, publish, distribute, sublicense,
and/or sell copies of the Software, and to permit persons to whom the
Software is furnished to do so, subject to the following conditions:
The above copyright notice and this permission notice shall be included in
all copies or substantial portions of the Software.
THE SOFTWARE IS PROVIDED "AS IS", WITHOUT WARRANTY OF ANY KIND, EXPRESS OR
IMPLIED, INCLUDING BUT NOT LIMITED TO THE WARRANTIES OF MERCHANTABILITY,
FITNESS FOR A PARTICULAR PURPOSE AND NONINFRINGEMENT. IN NO EVENT SHALL THE
AUTHORS OR COPYRIGHT HOLDERS BE LIABLE FOR ANY CLAIM, DAMAGES OR OTHER
LIABILITY, WHETHER IN AN ACTION OF CONTRACT, TORT OR OTHERWISE, ARISING FROM,
OUT OF OR IN CONNECTION WITH THE SOFTWARE OR THE USE OR OTHER DEALINGS IN
THE SOFTWARE.
*/
#version 400 core
uniform mat4 ViewProjection;
uniform mat4 ModelTransform;
uniform vec4 campos;
uniform mat4 camrot;
uniform vec2 scaling;
uniform vec4 objpos;
uniform vec4 gridColor;
layout(location = 0) in vec4 in_position;
//in vec3 in_position;
layout(location = 1) in vec2 in_st;
layout(location = 2) in vec3 in_normal;
out vec2 vs_st;
out vec3 vs_stp;
out vec4 vs_normal;
out vec4 vs_position;
const float k = 10.0;
const float dgr_to_rad = 0.0174532925;
vec4 psc_addition(vec4 v1, vec4 v2) {
float ds = v2.w - v1.w;
if(ds >= 0) {
float p = pow(k,-ds);
return vec4(v1.x*p + v2.x, v1.y*p + v2.y, v1.z*p + v2.z, v2.w);
} else {
float p = pow(k,ds);
return vec4(v1.x + v2.x*p, v1.y + v2.y*p, v1.z + v2.z*p, v1.w);
}
}
vec4 psc_to_meter(vec4 v1, vec2 v2) {
float factor = v2.x * pow(k,v2.y + v1.w);
return vec4(v1.xyz * factor, 1.0);
}
vec4 psc_scaling(vec4 v1, vec2 v2) {
float ds = v2.y - v1.w;
if(ds >= 0) {
return vec4(v1.xyz * v2.x * pow(k,v1.w), v2.y);
} else {
return vec4(v1.xyz * v2.x * pow(k,v2.y), v1.w);
}
}
void main()
{
// set variables
vs_st = in_st;
//vs_stp = in_position.xyz;
vs_normal = normalize(ModelTransform * vec4(in_normal,0));
// fetch model and view translation
//vec4 vertex_translate = ModelTransform[3];
// rotate and scale vertex with model transform and add the translation
vec3 local_vertex_pos = mat3(ModelTransform) * in_position.xyz;
//vec4 lvp = ModelTransform * in_position;
// PSC addition; local vertex position and the object power scaled world position
vs_position = psc_addition(vec4(local_vertex_pos,in_position.w),objpos);
//vs_position = psc_addition(lvp,objpos);
// PSC addition; rotated and viewscaled vertex and the cmaeras negative position
vs_position = psc_addition(vs_position,vec4(-campos.xyz,campos.w));
// rotate the camera
local_vertex_pos = mat3(camrot) * vs_position.xyz;
vs_position = vec4(local_vertex_pos, vs_position.w);
//vs_position = camrot* vs_position;
// rescales the scene to fit inside the view frustum
// is set from the main program, but these are decent values
// scaling = vec2(1.0, -8.0);
// project using the rescaled coordinates,
//vec4 vs_position_rescaled = psc_scaling(vs_position, scaling);
vec4 vs_position_rescaled = psc_to_meter(vs_position, scaling);
//vs_position = vs_position_rescaled;
// project the position to view space
gl_Position = ViewProjection * vs_position_rescaled;
}