KuangshiAi commited on
Commit
dc736c1
·
1 Parent(s): b7f8c04

update with camera info

Browse files
eval_cases/paraview/paraview_cases.yaml CHANGED
@@ -23,6 +23,8 @@
23
 
24
  Use a white background. Render at 1024x1024.
25
 
 
 
26
  Save the visualization image as "ABC/results/{agent_mode}/ABC.png".
27
  (Optional, but must save if use paraview) Save the paraview state as "ABC/results/{agent_mode}/ABC.pvsm".
28
  (Optional, but must save if use python script) Save the python script as "ABC/results/{agent_mode}/ABC.py".
@@ -84,6 +86,8 @@
84
 
85
  Use a gray-blue background (RGB: 0.329, 0.349, 0.427). Render at 1280x1280. Do not show a color bar.
86
 
 
 
87
  Save the visualization image as "Bernard/results/{agent_mode}/Bernard.png".
88
  (Optional, but must save if use paraview) Save the paraview state as "Bernard/results/{agent_mode}/Bernard.pvsm".
89
  (Optional, but must save if use pvpython script) Save the python script as "Bernard/results/{agent_mode}/Bernard.py".
@@ -114,6 +118,8 @@
114
 
115
  Use a white background. Render at 1280x1280. Do not show a color bar or coordinate axes.
116
 
 
 
117
  Save the visualization image as "bonsai/results/{agent_mode}/bonsai.png".
118
  (Optional, but must save if use paraview) Save the paraview state as "bonsai/results/{agent_mode}/bonsai.pvsm".
119
  (Optional, but must save if use pvpython script) Save the python script as "bonsai/results/{agent_mode}/bonsai.py".
@@ -168,7 +174,9 @@
168
 
169
  6. Use a white background. Find an optimal view. Render at 1280x1280. Do not show a color bar or coordinate axes.
170
 
171
- 7. Save your work:
 
 
172
  Save the visualization image as "carp/results/{agent_mode}/carp.png".
173
  Save the answers to the analysis questions in plain text as "carp/results/{agent_mode}/answers.txt".
174
  (Optional, but must save if use paraview) Save the paraview state as "carp/results/{agent_mode}/carp.pvsm".
@@ -245,6 +253,8 @@
245
 
246
  Use a white background. Render at 1280x1280.
247
 
 
 
248
  Save the paraview state as "crayfish_streamline/results/{agent_mode}/crayfish_streamline.pvsm".
249
  Save the visualization image as "crayfish_streamline/results/{agent_mode}/crayfish_streamline.png".
250
  (Optional, if use python script) Save the python script as "crayfish_streamline/results/{agent_mode}/crayfish_streamline.py".
@@ -279,7 +289,9 @@
279
 
280
  4. Use a white background. Find an optimal view. Render at 1280x1280. Do not show a color bar or coordinate axes.
281
 
282
- 5. Save your work:
 
 
283
  Save the visualization image as "engine/results/{agent_mode}/engine.png".
284
  (Optional, but must save if use paraview) Save the paraview state as "engine/results/{agent_mode}/engine.pvsm".
285
  (Optional, but must save if use pvpython script) Save the python script as "engine/results/{agent_mode}/engine.py".
@@ -324,7 +336,9 @@
324
 
325
  3. Use a white background. Find an optimal view. Render at 1280x1280. Do not show a color bar or coordinate axes.
326
 
327
- 4. Save your work:
 
 
328
  Save the visualization image as "foot/results/{agent_mode}/foot.png".
329
  Save the answers to the analysis questions in plain text as "foot/results/{agent_mode}/answers.txt".
330
  (Optional, but must save if use paraview) Save the paraview state as "foot/results/{agent_mode}/foot.pvsm".
@@ -372,7 +386,9 @@
372
 
373
  4. Use a white background. Find an optimal view. Render at 1280x1280. Do not show a color bar or coordinate axes.
374
 
375
- 5. Save your work:
 
 
376
  Save the visualization image as "lobster/results/{agent_mode}/lobster.png".
377
  Save the answers to the analysis questions in plain text as "lobster/results/{agent_mode}/answers.txt".
378
  (Optional, but must save if use paraview) Save the paraview state as "lobster/results/{agent_mode}/lobster.pvsm".
@@ -402,6 +418,7 @@
402
  Color the stream ribbon by magnetic field magnitude using the 'Cool to Warm' colormap. Enable surface lighting with specular reflection for better 3D perception.
403
  Add a color bar labeled 'Magnetic Field Magnitude'.
404
  Use a white background. Set an isometric camera view. Render at 1024x1024 resolution.
 
405
  Save the visualization image as "mhd-magfield_streamribbon/results/{agent_mode}/mhd-magfield_streamribbon.png".
406
  (Optional, but must save if use paraview) Save the paraview state as "mhd-magfield_streamribbon/results/{agent_mode}/mhd-magfield_streamribbon.pvsm".
407
  (Optional, but must save if use pvpython script) Save the python script as "mhd-magfield_streamribbon/results/{agent_mode}/mhd-magfield_streamribbon.py".
@@ -426,7 +443,8 @@
426
  Compute true pathlines by tracking particles through the time-varying velocity field using the ParticlePath filter. Apply TemporalShiftScale (scale=20) and TemporalInterpolator (interval=0.5) to extend particle travel and smooth trajectories.
427
  Seed 26 points along a line on the z-axis at x=64, y=64 (from z=20 to z=108). Use static seeds with termination time 80.
428
  Render pathlines as tubes with radius 0.3. Color by velocity magnitude using the 'Viridis (matplotlib)' colormap.
429
- Add a color bar for velocity magnitude. Use a white background. Set an isometric camera view. Render at 1024x1024.
 
430
  Save the visualization image as "mhd-turbulence_pathline/results/{agent_mode}/mhd-turbulence_pathline.png".
431
  (Optional, but must save if use paraview) Save the paraview state as "mhd-turbulence_pathline/results/{agent_mode}/mhd-turbulence_pathline.pvsm".
432
  (Optional, but must save if use pvpython script) Save the python script as "mhd-turbulence_pathline/results/{agent_mode}/mhd-turbulence_pathline.py".
@@ -453,6 +471,7 @@
453
  Create ribbon surfaces from the pathlines using the Ribbon filter with width 1.5 and a fixed default normal to prevent twisting. Apply Smooth filter (500 iterations) and generate surface normals for smooth shading.
454
  Set surface opacity to 0.85. Color by velocity magnitude using the 'Cool to Warm' colormap (range 0.1-0.8). Add specular highlights (0.5).
455
  Add a color bar for velocity magnitude. Use a white background. Set an isometric camera view. Render at 1024x1024.
 
456
  Save the visualization image as "mhd-turbulence_pathribbon/results/{agent_mode}/mhd-turbulence_pathribbon.png".
457
  (Optional, but must save if use paraview) Save the paraview state as "mhd-turbulence_pathribbon/results/{agent_mode}/mhd-turbulence_pathribbon.pvsm".
458
  (Optional, but must save if use pvpython script) Save the python script as "mhd-turbulence_pathribbon/results/{agent_mode}/mhd-turbulence_pathribbon.py".
@@ -475,6 +494,7 @@
475
  Generate 3D streamlines seeded from a line source along the z-axis at x=64, y=64 (from z=0 to z=127), with 50 seed points.
476
  Color the streamlines by velocity magnitude using the 'Turbo' colormap. Set streamline tube radius to 0.3 using the Tube filter.
477
  Add a color bar labeled 'Velocity Magnitude'. Use a white background. Set an isometric camera view. Render at 1024x1024.
 
478
  Save the visualization image as "mhd-turbulence_streamline/results/{agent_mode}/mhd-turbulence_streamline.png".
479
  (Optional, but must save if use paraview) Save the paraview state as "mhd-turbulence_streamline/results/{agent_mode}/mhd-turbulence_streamline.pvsm".
480
  (Optional, but must save if use pvpython script) Save the python script as "mhd-turbulence_streamline/results/{agent_mode}/mhd-turbulence_streamline.py".
@@ -588,6 +608,7 @@
588
  Color the arrows by velocity magnitude using the 'Viridis (matplotlib)' colormap. Use a sampling stride of 3.
589
  Add a color bar labeled 'Velocity Magnitude'.
590
  Use a white background. Set the camera to view along the negative y-axis. Render at 1024x1024.
 
591
  Save the visualization image as "rti-velocity_glyph/results/{agent_mode}/rti-velocity_glyph.png".
592
  (Optional, but must save if use paraview) Save the paraview state as "rti-velocity_glyph/results/{agent_mode}/rti-velocity_glyph.pvsm".
593
  (Optional, but must save if use pvpython script) Save the python script as "rti-velocity_glyph/results/{agent_mode}/rti-velocity_glyph.py".
@@ -613,6 +634,7 @@
613
  Color all three slices by velocity magnitude using the 'Turbo' colormap.
614
  Add a color bar labeled 'Velocity Magnitude'.
615
  Use a white background. Set an isometric camera view that shows all three slices. Render at 1024x1024.
 
616
  Save the visualization image as "rti-velocity_slices/results/{agent_mode}/rti-velocity_slices.png".
617
  (Optional, but must save if use paraview) Save the paraview state as "rti-velocity_slices/results/{agent_mode}/rti-velocity_slices.pvsm".
618
  (Optional, but must save if use pvpython script) Save the python script as "rti-velocity_slices/results/{agent_mode}/rti-velocity_slices.py".
@@ -635,6 +657,7 @@
635
  Seed 26 static points along a line on the z-axis at x=64, y=64 (from z=20 to z=108). Use StaticSeeds=True, ForceReinjectionEveryNSteps=1 (reinjection at every sub-timestep), and set TerminationTime=200.
636
  Render the resulting streaklines as tubes with radius 0.3. Color the tubes by velocity magnitude ("magnitude") using the 'Cool to Warm (Extended)' colormap. Add a color bar for velocity magnitude.
637
  Use a white background. Set an isometric camera view and render at 1024×1024.
 
638
  Save the visualization image as "rti-velocity_streakline/results/{agent_mode}/rti-velocity_streakline.png".
639
  (Optional, but must save if use paraview) Save the paraview state as "rti-velocity_streakline/results/{agent_mode}/rti-velocity_streakline.pvsm".
640
  (Optional, but must save if use pvpython script) Save the python script as "rti-velocity_streakline/results/{agent_mode}/rti-velocity_streakline.py".
@@ -655,7 +678,7 @@
655
  question: |
656
  Task:
657
 
658
- Load the tornado dataset from "solar-plume/data/solar-plume_126x126x512_float32_scalar3.raw", the information about this dataset:
659
  solar-plume (Vector)
660
  Data Scalar Type: float
661
  Data Byte Order: little Endian
@@ -663,13 +686,15 @@
663
  Number of Scalar Components: 3
664
  Data loading is very important, make sure you correctly load the dataset according to their features.
665
 
666
- Add a "stream tracer" filter under the tornado data to display streamline, set the "Seed type" to "Point Cloud" and set the center of point cloud to 3D position [50, 50, 320] with a radius 30, then hide the point cloud sphere.
667
 
668
  Add a "tube" filter under the "stream tracer" filter to enhance the streamline visualization. Set the radius to 0.5. In the pipeline browser panel, hide everything except the "tube" filter.
669
 
670
 
671
  Please think step by step and make sure to fulfill all the visualization goals mentioned above.
672
 
 
 
673
  Use a white background. Find an optimal view. Render at 1280x1280. Do not show a color bar or coordinate axes.
674
 
675
  Save the visualization image as "solar-plume/results/{agent_mode}/solar-plume.png".
@@ -708,6 +733,8 @@
708
 
709
  Use a white background. Find an optimal view. Render at 1280x1280. Do not show a color bar or coordinate axes.
710
 
 
 
711
  Save the visualization image as "supernova_isosurface/results/{agent_mode}/supernova_isosurface.png".
712
  (Optional, but must save if use paraview) Save the paraview state as "supernova_isosurface/results/{agent_mode}/supernova_isosurface.pvsm".
713
  (Optional, but must save if use pvpython script) Save the python script as "supernova_isosurface/results/{agent_mode}/supernova_isosurface.py".
@@ -749,6 +776,8 @@
749
 
750
  Use a white background. Render at 1280x1280.
751
 
 
 
752
  Save the visualization image as "supernova_streamline/results/{agent_mode}/supernova_streamline.png".
753
  (Optional, but must save if use paraview) Save the paraview state as "supernova_streamline/results/{agent_mode}/supernova_streamline.pvsm".
754
  (Optional, but must save if use pvpython script) Save the python script as "supernova_streamline/results/{agent_mode}/supernova_streamline.py".
@@ -785,6 +814,8 @@
785
 
786
  Use a white background. Find an optimal view. Render at 1280x1280. Do not show a color bar or coordinate axes.
787
 
 
 
788
  Save the visualization image as "tangaroa_streamribbon/results/{agent_mode}/tangaroa_streamribbon.png".
789
  (Optional, but must save if use paraview) Save the paraview state as "tangaroa_streamribbon/results/{agent_mode}/tangaroa_streamribbon.pvsm".
790
  (Optional, but must save if use pvpython script) Save the python script as "tangaroa_streamribbon/results/{agent_mode}/tangaroa_streamribbon.py".
@@ -810,6 +841,7 @@
810
  Also add contour lines of velocity magnitude on the same slice at values [0.3, 0.6, 0.9, 1.2] using the Contour filter on the slice output.
811
  Display contour lines in white. Add a color bar labeled 'Velocity Magnitude'.
812
  Light gray background (RGB: 0.9, 0.9, 0.9). Top-down camera. Render at 1024x1024.
 
813
  Save the visualization image as "tgc-velocity_contour/results/{agent_mode}/tgc-velocity_contour.png".
814
  (Optional, but must save if use paraview) Save the paraview state as "tgc-velocity_contour/results/{agent_mode}/tgc-velocity_contour.pvsm".
815
  (Optional, but must save if use pvpython script) Save the python script as "tgc-velocity_contour/results/{agent_mode}/tgc-velocity_contour.py".
@@ -845,6 +877,7 @@
845
  Add an "Outline" filter to display the dataset bounding box (black).
846
 
847
  Use a white background (RGB: 1.0, 1.0, 1.0). Find an optimal view. Render at 1280x1280. Show both color bar and coordinate axes.
 
848
  Save the visualization image as "tornado/results/{agent_mode}/tornado.png".
849
  (Optional, but must save if use paraview) Save the paraview state as "tornado/results/{agent_mode}/tornado.pvsm".
850
  (Optional, but must save if use pvpython script) Save the python script as "tornado/results/{agent_mode}/tornado.py".
@@ -879,6 +912,7 @@
879
  In the pipeline browser panel, hide all stream tracers and only show the ribbon filters and the outline.
880
 
881
  Use a white background (RGB: 1.0, 1.0, 1.0). Find an optimal view. Render at 1280x1280. Do not show a color bar or coordinate axes.
 
882
  Save the visualization image as "twoswirls_streamribbon/results/{agent_mode}/twoswirls_streamribbon.png".
883
  (Optional, but must save if use paraview) Save the paraview state as "twoswirls_streamribbon/results/{agent_mode}/twoswirls_streamribbon.pvsm".
884
  (Optional, but must save if use pvpython script) Save the python script as "twoswirls_streamribbon/results/{agent_mode}/twoswirls_streamribbon.py".
@@ -918,7 +952,9 @@
918
 
919
  6. Use a white background. Find an optimal view. Render at 1280x1280. Do not show a color bar or coordinate axes.
920
 
921
- 7. Save your work:
 
 
922
  Save the visualization image as "vortex/results/{agent_mode}/vortex.png".
923
  (Optional, but must save if use paraview) Save the paraview state as "vortex/results/{agent_mode}/vortex.pvsm".
924
  (Optional, but must save if use pvpython script) Save the python script as "vortex/results/{agent_mode}/vortex.py".
 
23
 
24
  Use a white background. Render at 1024x1024.
25
 
26
+ Set the viewpoint parameters as: [-150.99, 391.75, 219.64] to position; [32.38, 120.41, 81.63] to focal point; [0.23, -0.31, 0.92] to camera up direction.
27
+
28
  Save the visualization image as "ABC/results/{agent_mode}/ABC.png".
29
  (Optional, but must save if use paraview) Save the paraview state as "ABC/results/{agent_mode}/ABC.pvsm".
30
  (Optional, but must save if use python script) Save the python script as "ABC/results/{agent_mode}/ABC.py".
 
86
 
87
  Use a gray-blue background (RGB: 0.329, 0.349, 0.427). Render at 1280x1280. Do not show a color bar.
88
 
89
+ Set the viewpoint parameters as: [-81.99, -141.45, 89.86] to position; [65.58, 26.29, 28.48] to focal point; [0.18, 0.20, 0.96] to camera up direction.
90
+
91
  Save the visualization image as "Bernard/results/{agent_mode}/Bernard.png".
92
  (Optional, but must save if use paraview) Save the paraview state as "Bernard/results/{agent_mode}/Bernard.pvsm".
93
  (Optional, but must save if use pvpython script) Save the python script as "Bernard/results/{agent_mode}/Bernard.py".
 
118
 
119
  Use a white background. Render at 1280x1280. Do not show a color bar or coordinate axes.
120
 
121
+ Set the viewpoint parameters as: [-765.09, 413.55, 487.84] to position; [-22.76, 153.30, 157.32] to focal point; [0.30, 0.95, -0.07] to camera up direction.
122
+
123
  Save the visualization image as "bonsai/results/{agent_mode}/bonsai.png".
124
  (Optional, but must save if use paraview) Save the paraview state as "bonsai/results/{agent_mode}/bonsai.pvsm".
125
  (Optional, but must save if use pvpython script) Save the python script as "bonsai/results/{agent_mode}/bonsai.py".
 
174
 
175
  6. Use a white background. Find an optimal view. Render at 1280x1280. Do not show a color bar or coordinate axes.
176
 
177
+ 7. Set the viewpoint parameters as: [265.81, 1024.69, 131.23] to position; [141.24, 216.61, 243.16] to focal point; [0.99, -0.14, 0.07] to camera up direction.
178
+
179
+ 8. Save your work:
180
  Save the visualization image as "carp/results/{agent_mode}/carp.png".
181
  Save the answers to the analysis questions in plain text as "carp/results/{agent_mode}/answers.txt".
182
  (Optional, but must save if use paraview) Save the paraview state as "carp/results/{agent_mode}/carp.pvsm".
 
253
 
254
  Use a white background. Render at 1280x1280.
255
 
256
+ Set the viewpoint parameters as: [435.04, -325.38, 567.82] to position; [111.64, 202.81, -21.96] to focal point; [-0.099, 0.714, 0.693] to camera up direction.
257
+
258
  Save the paraview state as "crayfish_streamline/results/{agent_mode}/crayfish_streamline.pvsm".
259
  Save the visualization image as "crayfish_streamline/results/{agent_mode}/crayfish_streamline.png".
260
  (Optional, if use python script) Save the python script as "crayfish_streamline/results/{agent_mode}/crayfish_streamline.py".
 
289
 
290
  4. Use a white background. Find an optimal view. Render at 1280x1280. Do not show a color bar or coordinate axes.
291
 
292
+ 5. Set the viewpoint parameters as: [-184.58, 109.48, -431.72] to position; [134.05, 105.62, 88.92] to focal point; [0.01, 1.0, -0.001] to camera up direction.
293
+
294
+ 6. Save your work:
295
  Save the visualization image as "engine/results/{agent_mode}/engine.png".
296
  (Optional, but must save if use paraview) Save the paraview state as "engine/results/{agent_mode}/engine.pvsm".
297
  (Optional, but must save if use pvpython script) Save the python script as "engine/results/{agent_mode}/engine.py".
 
336
 
337
  3. Use a white background. Find an optimal view. Render at 1280x1280. Do not show a color bar or coordinate axes.
338
 
339
+ 4. Set the viewpoint parameters as: [-576.41, -264.41, -153.48] to position; [127.5, 127.5, 127.5] to focal point; [-0.52, 0.38, 0.76] to camera up direction.
340
+
341
+ 5. Save your work:
342
  Save the visualization image as "foot/results/{agent_mode}/foot.png".
343
  Save the answers to the analysis questions in plain text as "foot/results/{agent_mode}/answers.txt".
344
  (Optional, but must save if use paraview) Save the paraview state as "foot/results/{agent_mode}/foot.pvsm".
 
386
 
387
  4. Use a white background. Find an optimal view. Render at 1280x1280. Do not show a color bar or coordinate axes.
388
 
389
+ 5. Set the viewpoint parameters as: [543.52, -957.0, 1007.87] to position; [150.0, 161.5, 38.5] to focal point; [-0.15, 0.62, 0.77] to camera up direction.
390
+
391
+ 6. Save your work:
392
  Save the visualization image as "lobster/results/{agent_mode}/lobster.png".
393
  Save the answers to the analysis questions in plain text as "lobster/results/{agent_mode}/answers.txt".
394
  (Optional, but must save if use paraview) Save the paraview state as "lobster/results/{agent_mode}/lobster.pvsm".
 
418
  Color the stream ribbon by magnetic field magnitude using the 'Cool to Warm' colormap. Enable surface lighting with specular reflection for better 3D perception.
419
  Add a color bar labeled 'Magnetic Field Magnitude'.
420
  Use a white background. Set an isometric camera view. Render at 1024x1024 resolution.
421
+ Set the viewpoint parameters as: [200.0, 200.0, 200.0] to position; [63.5, 63.5, 63.5] to focal point; [0.0, 0.0, 1.0] to camera up direction.
422
  Save the visualization image as "mhd-magfield_streamribbon/results/{agent_mode}/mhd-magfield_streamribbon.png".
423
  (Optional, but must save if use paraview) Save the paraview state as "mhd-magfield_streamribbon/results/{agent_mode}/mhd-magfield_streamribbon.pvsm".
424
  (Optional, but must save if use pvpython script) Save the python script as "mhd-magfield_streamribbon/results/{agent_mode}/mhd-magfield_streamribbon.py".
 
443
  Compute true pathlines by tracking particles through the time-varying velocity field using the ParticlePath filter. Apply TemporalShiftScale (scale=20) and TemporalInterpolator (interval=0.5) to extend particle travel and smooth trajectories.
444
  Seed 26 points along a line on the z-axis at x=64, y=64 (from z=20 to z=108). Use static seeds with termination time 80.
445
  Render pathlines as tubes with radius 0.3. Color by velocity magnitude using the 'Viridis (matplotlib)' colormap.
446
+ Add a color bar for velocity magnitude. Set the viewpoint parameters as: [200.0, 200.0, 200.0] to position; [63.5, 63.5, 63.5] to focal point; [0.0, 0.0, 1.0] to camera up direction.
447
+ Use a white background. Set an isometric camera view. Render at 1024x1024.
448
  Save the visualization image as "mhd-turbulence_pathline/results/{agent_mode}/mhd-turbulence_pathline.png".
449
  (Optional, but must save if use paraview) Save the paraview state as "mhd-turbulence_pathline/results/{agent_mode}/mhd-turbulence_pathline.pvsm".
450
  (Optional, but must save if use pvpython script) Save the python script as "mhd-turbulence_pathline/results/{agent_mode}/mhd-turbulence_pathline.py".
 
471
  Create ribbon surfaces from the pathlines using the Ribbon filter with width 1.5 and a fixed default normal to prevent twisting. Apply Smooth filter (500 iterations) and generate surface normals for smooth shading.
472
  Set surface opacity to 0.85. Color by velocity magnitude using the 'Cool to Warm' colormap (range 0.1-0.8). Add specular highlights (0.5).
473
  Add a color bar for velocity magnitude. Use a white background. Set an isometric camera view. Render at 1024x1024.
474
+ Set the viewpoint parameters as: [200.0, 200.0, 200.0] to position; [63.5, 63.5, 63.5] to focal point; [0.0, 0.0, 1.0] to camera up direction.
475
  Save the visualization image as "mhd-turbulence_pathribbon/results/{agent_mode}/mhd-turbulence_pathribbon.png".
476
  (Optional, but must save if use paraview) Save the paraview state as "mhd-turbulence_pathribbon/results/{agent_mode}/mhd-turbulence_pathribbon.pvsm".
477
  (Optional, but must save if use pvpython script) Save the python script as "mhd-turbulence_pathribbon/results/{agent_mode}/mhd-turbulence_pathribbon.py".
 
494
  Generate 3D streamlines seeded from a line source along the z-axis at x=64, y=64 (from z=0 to z=127), with 50 seed points.
495
  Color the streamlines by velocity magnitude using the 'Turbo' colormap. Set streamline tube radius to 0.3 using the Tube filter.
496
  Add a color bar labeled 'Velocity Magnitude'. Use a white background. Set an isometric camera view. Render at 1024x1024.
497
+ Set the viewpoint parameters as: [200.0, 200.0, 200.0] to position; [63.5, 63.5, 63.5] to focal point; [0.0, 0.0, 1.0] to camera up direction.
498
  Save the visualization image as "mhd-turbulence_streamline/results/{agent_mode}/mhd-turbulence_streamline.png".
499
  (Optional, but must save if use paraview) Save the paraview state as "mhd-turbulence_streamline/results/{agent_mode}/mhd-turbulence_streamline.pvsm".
500
  (Optional, but must save if use pvpython script) Save the python script as "mhd-turbulence_streamline/results/{agent_mode}/mhd-turbulence_streamline.py".
 
608
  Color the arrows by velocity magnitude using the 'Viridis (matplotlib)' colormap. Use a sampling stride of 3.
609
  Add a color bar labeled 'Velocity Magnitude'.
610
  Use a white background. Set the camera to view along the negative y-axis. Render at 1024x1024.
611
+ Set the viewpoint parameters as: [63.5, 250.0, 63.5] to position; [63.5, 64.0, 63.5] to focal point; [0.0, 0.0, 1.0] to camera up direction.
612
  Save the visualization image as "rti-velocity_glyph/results/{agent_mode}/rti-velocity_glyph.png".
613
  (Optional, but must save if use paraview) Save the paraview state as "rti-velocity_glyph/results/{agent_mode}/rti-velocity_glyph.pvsm".
614
  (Optional, but must save if use pvpython script) Save the python script as "rti-velocity_glyph/results/{agent_mode}/rti-velocity_glyph.py".
 
634
  Color all three slices by velocity magnitude using the 'Turbo' colormap.
635
  Add a color bar labeled 'Velocity Magnitude'.
636
  Use a white background. Set an isometric camera view that shows all three slices. Render at 1024x1024.
637
+ Set the viewpoint parameters as: [200.0, 200.0, 200.0] to position; [63.5, 63.5, 63.5] to focal point; [0.0, 0.0, 1.0] to camera up direction.
638
  Save the visualization image as "rti-velocity_slices/results/{agent_mode}/rti-velocity_slices.png".
639
  (Optional, but must save if use paraview) Save the paraview state as "rti-velocity_slices/results/{agent_mode}/rti-velocity_slices.pvsm".
640
  (Optional, but must save if use pvpython script) Save the python script as "rti-velocity_slices/results/{agent_mode}/rti-velocity_slices.py".
 
657
  Seed 26 static points along a line on the z-axis at x=64, y=64 (from z=20 to z=108). Use StaticSeeds=True, ForceReinjectionEveryNSteps=1 (reinjection at every sub-timestep), and set TerminationTime=200.
658
  Render the resulting streaklines as tubes with radius 0.3. Color the tubes by velocity magnitude ("magnitude") using the 'Cool to Warm (Extended)' colormap. Add a color bar for velocity magnitude.
659
  Use a white background. Set an isometric camera view and render at 1024×1024.
660
+ Set the viewpoint parameters as: [200.0, 200.0, 200.0] to position; [63.5, 63.5, 63.5] to focal point; [0.0, 0.0, 1.0] to camera up direction.
661
  Save the visualization image as "rti-velocity_streakline/results/{agent_mode}/rti-velocity_streakline.png".
662
  (Optional, but must save if use paraview) Save the paraview state as "rti-velocity_streakline/results/{agent_mode}/rti-velocity_streakline.pvsm".
663
  (Optional, but must save if use pvpython script) Save the python script as "rti-velocity_streakline/results/{agent_mode}/rti-velocity_streakline.py".
 
678
  question: |
679
  Task:
680
 
681
+ Load the solar plume dataset from "solar-plume/data/solar-plume_126x126x512_float32_scalar3.raw", the information about this dataset:
682
  solar-plume (Vector)
683
  Data Scalar Type: float
684
  Data Byte Order: little Endian
 
686
  Number of Scalar Components: 3
687
  Data loading is very important, make sure you correctly load the dataset according to their features.
688
 
689
+ Add a "stream tracer" filter under the solar plume data to display streamline, set the "Seed type" to "Point Cloud" and set the center of point cloud to 3D position [50, 50, 320] with a radius 30, then hide the point cloud sphere.
690
 
691
  Add a "tube" filter under the "stream tracer" filter to enhance the streamline visualization. Set the radius to 0.5. In the pipeline browser panel, hide everything except the "tube" filter.
692
 
693
 
694
  Please think step by step and make sure to fulfill all the visualization goals mentioned above.
695
 
696
+ Set the viewpoint parameters as: [62.51, -984.78, 255.45] to position; [62.51, 62.46, 255.45] to focal point; [0, 0, 1] to camera up direction.
697
+
698
  Use a white background. Find an optimal view. Render at 1280x1280. Do not show a color bar or coordinate axes.
699
 
700
  Save the visualization image as "solar-plume/results/{agent_mode}/solar-plume.png".
 
733
 
734
  Use a white background. Find an optimal view. Render at 1280x1280. Do not show a color bar or coordinate axes.
735
 
736
+ Set the viewpoint parameters as: [567.97, 80.17, 167.28] to position; [125.09, 108.83, 121.01] to focal point; [-0.11, -0.86, 0.50] to camera up direction.
737
+
738
  Save the visualization image as "supernova_isosurface/results/{agent_mode}/supernova_isosurface.png".
739
  (Optional, but must save if use paraview) Save the paraview state as "supernova_isosurface/results/{agent_mode}/supernova_isosurface.pvsm".
740
  (Optional, but must save if use pvpython script) Save the python script as "supernova_isosurface/results/{agent_mode}/supernova_isosurface.py".
 
776
 
777
  Use a white background. Render at 1280x1280.
778
 
779
+ Set the viewpoint parameters as: [41.38, 73.91, -282.0] to position; [49.45, 49.50, 49.49] to focal point; [0.01, 1.0, 0.07] to camera up direction.
780
+
781
  Save the visualization image as "supernova_streamline/results/{agent_mode}/supernova_streamline.png".
782
  (Optional, but must save if use paraview) Save the paraview state as "supernova_streamline/results/{agent_mode}/supernova_streamline.pvsm".
783
  (Optional, but must save if use pvpython script) Save the python script as "supernova_streamline/results/{agent_mode}/supernova_streamline.py".
 
814
 
815
  Use a white background. Find an optimal view. Render at 1280x1280. Do not show a color bar or coordinate axes.
816
 
817
+ Set the viewpoint parameters as: [372.27, 278.87, 214.44] to position; [169.85, 76.46, 12.02] to focal point; [-0.41, 0.82, -0.41] to camera up direction.
818
+
819
  Save the visualization image as "tangaroa_streamribbon/results/{agent_mode}/tangaroa_streamribbon.png".
820
  (Optional, but must save if use paraview) Save the paraview state as "tangaroa_streamribbon/results/{agent_mode}/tangaroa_streamribbon.pvsm".
821
  (Optional, but must save if use pvpython script) Save the python script as "tangaroa_streamribbon/results/{agent_mode}/tangaroa_streamribbon.py".
 
841
  Also add contour lines of velocity magnitude on the same slice at values [0.3, 0.6, 0.9, 1.2] using the Contour filter on the slice output.
842
  Display contour lines in white. Add a color bar labeled 'Velocity Magnitude'.
843
  Light gray background (RGB: 0.9, 0.9, 0.9). Top-down camera. Render at 1024x1024.
844
+ Set the viewpoint parameters as: [31.5, 31.5, 100.0] to position; [31.5, 31.5, 32.0] to focal point; [0.0, 1.0, 0.0] to camera up direction.
845
  Save the visualization image as "tgc-velocity_contour/results/{agent_mode}/tgc-velocity_contour.png".
846
  (Optional, but must save if use paraview) Save the paraview state as "tgc-velocity_contour/results/{agent_mode}/tgc-velocity_contour.pvsm".
847
  (Optional, but must save if use pvpython script) Save the python script as "tgc-velocity_contour/results/{agent_mode}/tgc-velocity_contour.py".
 
877
  Add an "Outline" filter to display the dataset bounding box (black).
878
 
879
  Use a white background (RGB: 1.0, 1.0, 1.0). Find an optimal view. Render at 1280x1280. Show both color bar and coordinate axes.
880
+ Set the viewpoint parameters as: [142.01, -36.46, 93.96] to position; [31.5, 31.5, 31.5] to focal point; [-0.35, 0.25, 0.90] to camera up direction.
881
  Save the visualization image as "tornado/results/{agent_mode}/tornado.png".
882
  (Optional, but must save if use paraview) Save the paraview state as "tornado/results/{agent_mode}/tornado.pvsm".
883
  (Optional, but must save if use pvpython script) Save the python script as "tornado/results/{agent_mode}/tornado.py".
 
912
  In the pipeline browser panel, hide all stream tracers and only show the ribbon filters and the outline.
913
 
914
  Use a white background (RGB: 1.0, 1.0, 1.0). Find an optimal view. Render at 1280x1280. Do not show a color bar or coordinate axes.
915
+ Set the viewpoint parameters as: [30.51, -154.18, 144.99] to position; [30.51, 31.5, 30.91] to focal point; [0.0, 0.53, 0.85] to camera up direction.
916
  Save the visualization image as "twoswirls_streamribbon/results/{agent_mode}/twoswirls_streamribbon.png".
917
  (Optional, but must save if use paraview) Save the paraview state as "twoswirls_streamribbon/results/{agent_mode}/twoswirls_streamribbon.pvsm".
918
  (Optional, but must save if use pvpython script) Save the python script as "twoswirls_streamribbon/results/{agent_mode}/twoswirls_streamribbon.py".
 
952
 
953
  6. Use a white background. Find an optimal view. Render at 1280x1280. Do not show a color bar or coordinate axes.
954
 
955
+ 7. Set the viewpoint parameters as: [308.85, 308.85, 308.85] to position; [63.5, 63.5, 63.5] to focal point; [-0.41, 0.82, -0.41] to camera up direction.
956
+
957
+ 8. Save your work:
958
  Save the visualization image as "vortex/results/{agent_mode}/vortex.png".
959
  (Optional, but must save if use paraview) Save the paraview state as "vortex/results/{agent_mode}/vortex.pvsm".
960
  (Optional, but must save if use pvpython script) Save the python script as "vortex/results/{agent_mode}/vortex.py".
paraview/ABC/task_description.txt CHANGED
@@ -16,6 +16,8 @@ Show the dataset bounding box as an outline.
16
 
17
  Use a white background. Render at 1024x1024.
18
 
 
 
19
  Save the visualization image as "ABC/results/{agent_mode}/ABC.png".
20
  (Optional, but must save if use paraview) Save the paraview state as "ABC/results/{agent_mode}/ABC.pvsm".
21
  (Optional, but must save if use python script) Save the python script as "ABC/results/{agent_mode}/ABC.py".
 
16
 
17
  Use a white background. Render at 1024x1024.
18
 
19
+ Set the viewpoint parameters as: [-150.99, 391.75, 219.64] to position; [32.38, 120.41, 81.63] to focal point; [0.23, -0.31, 0.92] to camera up direction.
20
+
21
  Save the visualization image as "ABC/results/{agent_mode}/ABC.png".
22
  (Optional, but must save if use paraview) Save the paraview state as "ABC/results/{agent_mode}/ABC.pvsm".
23
  (Optional, but must save if use python script) Save the python script as "ABC/results/{agent_mode}/ABC.py".
paraview/Bernard/task_description.txt CHANGED
@@ -16,6 +16,8 @@ In the pipeline browser panel, hide all stream tracers and only show the tube fi
16
 
17
  Use a gray-blue background (RGB: 0.329, 0.349, 0.427). Render at 1280x1280. Do not show a color bar.
18
 
 
 
19
  Save the visualization image as "Bernard/results/{agent_mode}/Bernard.png".
20
  (Optional, but must save if use paraview) Save the paraview state as "Bernard/results/{agent_mode}/Bernard.pvsm".
21
  (Optional, but must save if use pvpython script) Save the python script as "Bernard/results/{agent_mode}/Bernard.py".
 
16
 
17
  Use a gray-blue background (RGB: 0.329, 0.349, 0.427). Render at 1280x1280. Do not show a color bar.
18
 
19
+ Set the viewpoint parameters as: [-81.99, -141.45, 89.86] to position; [65.58, 26.29, 28.48] to focal point; [0.18, 0.20, 0.96] to camera up direction.
20
+
21
  Save the visualization image as "Bernard/results/{agent_mode}/Bernard.png".
22
  (Optional, but must save if use paraview) Save the paraview state as "Bernard/results/{agent_mode}/Bernard.pvsm".
23
  (Optional, but must save if use pvpython script) Save the python script as "Bernard/results/{agent_mode}/Bernard.py".
paraview/bonsai/task_description.txt CHANGED
@@ -13,6 +13,8 @@ Please think step by step and make sure to fulfill all the visualization goals m
13
 
14
  Use a white background. Render at 1280x1280. Do not show a color bar or coordinate axes.
15
 
 
 
16
  Save the visualization image as "bonsai/results/{agent_mode}/bonsai.png".
17
  (Optional, but must save if use paraview) Save the paraview state as "bonsai/results/{agent_mode}/bonsai.pvsm".
18
  (Optional, but must save if use pvpython script) Save the python script as "bonsai/results/{agent_mode}/bonsai.py".
 
13
 
14
  Use a white background. Render at 1280x1280. Do not show a color bar or coordinate axes.
15
 
16
+ Set the viewpoint parameters as: [-765.09, 413.55, 487.84] to position; [-22.76, 153.30, 157.32] to focal point; [0.30, 0.95, -0.07] to camera up direction.
17
+
18
  Save the visualization image as "bonsai/results/{agent_mode}/bonsai.png".
19
  (Optional, but must save if use paraview) Save the paraview state as "bonsai/results/{agent_mode}/bonsai.pvsm".
20
  (Optional, but must save if use pvpython script) Save the python script as "bonsai/results/{agent_mode}/bonsai.py".
paraview/carp/task_description.txt CHANGED
@@ -33,7 +33,9 @@ D. ~40%
33
 
34
  6. Use a white background. Find an optimal view. Render at 1280x1280. Do not show a color bar or coordinate axes.
35
 
36
- 7. Save your work:
 
 
37
  Save the visualization image as "carp/results/{agent_mode}/carp.png".
38
  Save the answers to the analysis questions in plain text as "carp/results/{agent_mode}/answers.txt".
39
  (Optional, but must save if use paraview) Save the paraview state as "carp/results/{agent_mode}/carp.pvsm".
 
33
 
34
  6. Use a white background. Find an optimal view. Render at 1280x1280. Do not show a color bar or coordinate axes.
35
 
36
+ 7. Set the viewpoint parameters as: [265.81, 1024.69, 131.23] to position; [141.24, 216.61, 243.16] to focal point; [0.99, -0.14, 0.07] to camera up direction.
37
+
38
+ 8. Save your work:
39
  Save the visualization image as "carp/results/{agent_mode}/carp.png".
40
  Save the answers to the analysis questions in plain text as "carp/results/{agent_mode}/answers.txt".
41
  (Optional, but must save if use paraview) Save the paraview state as "carp/results/{agent_mode}/carp.pvsm".
paraview/crayfish_streamline/task_description.txt CHANGED
@@ -19,6 +19,8 @@ In the pipeline browser panel, hide all stream tracers and only show the tube fi
19
 
20
  Use a white background. Render at 1280x1280.
21
 
 
 
22
  Save the paraview state as "crayfish_streamline/results/{agent_mode}/crayfish_streamline.pvsm".
23
  Save the visualization image as "crayfish_streamline/results/{agent_mode}/crayfish_streamline.png".
24
  (Optional, if use python script) Save the python script as "crayfish_streamline/results/{agent_mode}/crayfish_streamline.py".
 
19
 
20
  Use a white background. Render at 1280x1280.
21
 
22
+ Set the viewpoint parameters as: [435.04, -325.38, 567.82] to position; [111.64, 202.81, -21.96] to focal point; [-0.099, 0.714, 0.693] to camera up direction.
23
+
24
  Save the paraview state as "crayfish_streamline/results/{agent_mode}/crayfish_streamline.pvsm".
25
  Save the visualization image as "crayfish_streamline/results/{agent_mode}/crayfish_streamline.png".
26
  (Optional, if use python script) Save the python script as "crayfish_streamline/results/{agent_mode}/crayfish_streamline.py".
paraview/engine/task_description.txt CHANGED
@@ -17,7 +17,9 @@ Instructions:
17
 
18
  4. Use a white background. Find an optimal view. Render at 1280x1280. Do not show a color bar or coordinate axes.
19
 
20
- 5. Save your work:
 
 
21
  Save the visualization image as "engine/results/{agent_mode}/engine.png".
22
  (Optional, but must save if use paraview) Save the paraview state as "engine/results/{agent_mode}/engine.pvsm".
23
  (Optional, but must save if use pvpython script) Save the python script as "engine/results/{agent_mode}/engine.py".
 
17
 
18
  4. Use a white background. Find an optimal view. Render at 1280x1280. Do not show a color bar or coordinate axes.
19
 
20
+ 5. Set the viewpoint parameters as: [-184.58, 109.48, -431.72] to position; [134.05, 105.62, 88.92] to focal point; [0.01, 1.0, -0.001] to camera up direction.
21
+
22
+ 6. Save your work:
23
  Save the visualization image as "engine/results/{agent_mode}/engine.png".
24
  (Optional, but must save if use paraview) Save the paraview state as "engine/results/{agent_mode}/engine.pvsm".
25
  (Optional, but must save if use pvpython script) Save the python script as "engine/results/{agent_mode}/engine.py".
paraview/foot/task_description.txt CHANGED
@@ -22,7 +22,9 @@ D. Neither the phalanges nor the metatarsals are clearly visible
22
 
23
  3. Use a white background. Find an optimal view. Render at 1280x1280. Do not show a color bar or coordinate axes.
24
 
25
- 4. Save your work:
 
 
26
  Save the visualization image as "foot/results/{agent_mode}/foot.png".
27
  Save the answers to the analysis questions in plain text as "foot/results/{agent_mode}/answers.txt".
28
  (Optional, but must save if use paraview) Save the paraview state as "foot/results/{agent_mode}/foot.pvsm".
 
22
 
23
  3. Use a white background. Find an optimal view. Render at 1280x1280. Do not show a color bar or coordinate axes.
24
 
25
+ 4. Set the viewpoint parameters as: [-576.41, -264.41, -153.48] to position; [127.5, 127.5, 127.5] to focal point; [-0.52, 0.38, 0.76] to camera up direction.
26
+
27
+ 5. Save your work:
28
  Save the visualization image as "foot/results/{agent_mode}/foot.png".
29
  Save the answers to the analysis questions in plain text as "foot/results/{agent_mode}/answers.txt".
30
  (Optional, but must save if use paraview) Save the paraview state as "foot/results/{agent_mode}/foot.pvsm".
paraview/lobster/task_description.txt CHANGED
@@ -24,7 +24,9 @@ D. 10 walking legs
24
 
25
  4. Use a white background. Find an optimal view. Render at 1280x1280. Do not show a color bar or coordinate axes.
26
 
27
- 5. Save your work:
 
 
28
  Save the visualization image as "lobster/results/{agent_mode}/lobster.png".
29
  Save the answers to the analysis questions in plain text as "lobster/results/{agent_mode}/answers.txt".
30
  (Optional, but must save if use paraview) Save the paraview state as "lobster/results/{agent_mode}/lobster.pvsm".
 
24
 
25
  4. Use a white background. Find an optimal view. Render at 1280x1280. Do not show a color bar or coordinate axes.
26
 
27
+ 5. Set the viewpoint parameters as: [543.52, -957.0, 1007.87] to position; [150.0, 161.5, 38.5] to focal point; [-0.15, 0.62, 0.77] to camera up direction.
28
+
29
+ 6. Save your work:
30
  Save the visualization image as "lobster/results/{agent_mode}/lobster.png".
31
  Save the answers to the analysis questions in plain text as "lobster/results/{agent_mode}/answers.txt".
32
  (Optional, but must save if use paraview) Save the paraview state as "lobster/results/{agent_mode}/lobster.pvsm".
paraview/mhd-magfield_streamribbon/task_description.txt CHANGED
@@ -4,6 +4,7 @@ The stream ribbon should be traced along the magnetic field lines.
4
  Color the stream ribbon by magnetic field magnitude using the 'Cool to Warm' colormap. Enable surface lighting with specular reflection for better 3D perception.
5
  Add a color bar labeled 'Magnetic Field Magnitude'.
6
  Use a white background. Set an isometric camera view. Render at 1024x1024 resolution.
 
7
  Save the visualization image as "mhd-magfield_streamribbon/results/{agent_mode}/mhd-magfield_streamribbon.png".
8
  (Optional, but must save if use paraview) Save the paraview state as "mhd-magfield_streamribbon/results/{agent_mode}/mhd-magfield_streamribbon.pvsm".
9
  (Optional, but must save if use pvpython script) Save the python script as "mhd-magfield_streamribbon/results/{agent_mode}/mhd-magfield_streamribbon.py".
 
4
  Color the stream ribbon by magnetic field magnitude using the 'Cool to Warm' colormap. Enable surface lighting with specular reflection for better 3D perception.
5
  Add a color bar labeled 'Magnetic Field Magnitude'.
6
  Use a white background. Set an isometric camera view. Render at 1024x1024 resolution.
7
+ Set the viewpoint parameters as: [200.0, 200.0, 200.0] to position; [63.5, 63.5, 63.5] to focal point; [0.0, 0.0, 1.0] to camera up direction.
8
  Save the visualization image as "mhd-magfield_streamribbon/results/{agent_mode}/mhd-magfield_streamribbon.png".
9
  (Optional, but must save if use paraview) Save the paraview state as "mhd-magfield_streamribbon/results/{agent_mode}/mhd-magfield_streamribbon.pvsm".
10
  (Optional, but must save if use pvpython script) Save the python script as "mhd-magfield_streamribbon/results/{agent_mode}/mhd-magfield_streamribbon.py".
paraview/mhd-turbulence_pathline/task_description.txt CHANGED
@@ -3,6 +3,7 @@ Compute true pathlines by tracking particles through the time-varying velocity f
3
  Seed 26 points along a line on the z-axis at x=64, y=64 (from z=20 to z=108). Use static seeds with termination time 80.
4
  Render pathlines as tubes with radius 0.3. Color by velocity magnitude using the 'Viridis (matplotlib)' colormap.
5
  Add a color bar for velocity magnitude. Use a white background. Set an isometric camera view. Render at 1024x1024.
 
6
  Save the visualization image as "mhd-turbulence_pathline/results/{agent_mode}/mhd-turbulence_pathline.png".
7
  (Optional, but must save if use paraview) Save the paraview state as "mhd-turbulence_pathline/results/{agent_mode}/mhd-turbulence_pathline.pvsm".
8
  (Optional, but must save if use pvpython script) Save the python script as "mhd-turbulence_pathline/results/{agent_mode}/mhd-turbulence_pathline.py".
 
3
  Seed 26 points along a line on the z-axis at x=64, y=64 (from z=20 to z=108). Use static seeds with termination time 80.
4
  Render pathlines as tubes with radius 0.3. Color by velocity magnitude using the 'Viridis (matplotlib)' colormap.
5
  Add a color bar for velocity magnitude. Use a white background. Set an isometric camera view. Render at 1024x1024.
6
+ Add a color bar for velocity magnitude. Set the viewpoint parameters as: [200.0, 200.0, 200.0] to position; [63.5, 63.5, 63.5] to focal point; [0.0, 0.0, 1.0] to camera up direction.
7
  Save the visualization image as "mhd-turbulence_pathline/results/{agent_mode}/mhd-turbulence_pathline.png".
8
  (Optional, but must save if use paraview) Save the paraview state as "mhd-turbulence_pathline/results/{agent_mode}/mhd-turbulence_pathline.pvsm".
9
  (Optional, but must save if use pvpython script) Save the python script as "mhd-turbulence_pathline/results/{agent_mode}/mhd-turbulence_pathline.py".
paraview/mhd-turbulence_pathribbon/task_description.txt CHANGED
@@ -4,6 +4,7 @@ Seed 26 points along a line on the z-axis at x=64, y=64 (from z=20 to z=108). Us
4
  Create ribbon surfaces from the pathlines using the Ribbon filter with width 1.5 and a fixed default normal to prevent twisting. Apply Smooth filter (500 iterations) and generate surface normals for smooth shading.
5
  Set surface opacity to 0.85. Color by velocity magnitude using the 'Cool to Warm' colormap (range 0.1-0.8). Add specular highlights (0.5).
6
  Add a color bar for velocity magnitude. Use a white background. Set an isometric camera view. Render at 1024x1024.
 
7
  Save the visualization image as "mhd-turbulence_pathribbon/results/{agent_mode}/mhd-turbulence_pathribbon.png".
8
  (Optional, but must save if use paraview) Save the paraview state as "mhd-turbulence_pathribbon/results/{agent_mode}/mhd-turbulence_pathribbon.pvsm".
9
  (Optional, but must save if use pvpython script) Save the python script as "mhd-turbulence_pathribbon/results/{agent_mode}/mhd-turbulence_pathribbon.py".
 
4
  Create ribbon surfaces from the pathlines using the Ribbon filter with width 1.5 and a fixed default normal to prevent twisting. Apply Smooth filter (500 iterations) and generate surface normals for smooth shading.
5
  Set surface opacity to 0.85. Color by velocity magnitude using the 'Cool to Warm' colormap (range 0.1-0.8). Add specular highlights (0.5).
6
  Add a color bar for velocity magnitude. Use a white background. Set an isometric camera view. Render at 1024x1024.
7
+ Set the viewpoint parameters as: [200.0, 200.0, 200.0] to position; [63.5, 63.5, 63.5] to focal point; [0.0, 0.0, 1.0] to camera up direction.
8
  Save the visualization image as "mhd-turbulence_pathribbon/results/{agent_mode}/mhd-turbulence_pathribbon.png".
9
  (Optional, but must save if use paraview) Save the paraview state as "mhd-turbulence_pathribbon/results/{agent_mode}/mhd-turbulence_pathribbon.pvsm".
10
  (Optional, but must save if use pvpython script) Save the python script as "mhd-turbulence_pathribbon/results/{agent_mode}/mhd-turbulence_pathribbon.py".
paraview/mhd-turbulence_streamline/task_description.txt CHANGED
@@ -2,6 +2,7 @@ Load the MHD turbulence velocity field dataset "mhd-turbulence_streamline/data/m
2
  Generate 3D streamlines seeded from a line source along the z-axis at x=64, y=64 (from z=0 to z=127), with 50 seed points.
3
  Color the streamlines by velocity magnitude using the 'Turbo' colormap. Set streamline tube radius to 0.3 using the Tube filter.
4
  Add a color bar labeled 'Velocity Magnitude'. Use a white background. Set an isometric camera view. Render at 1024x1024.
 
5
  Save the visualization image as "mhd-turbulence_streamline/results/{agent_mode}/mhd-turbulence_streamline.png".
6
  (Optional, but must save if use paraview) Save the paraview state as "mhd-turbulence_streamline/results/{agent_mode}/mhd-turbulence_streamline.pvsm".
7
  (Optional, but must save if use pvpython script) Save the python script as "mhd-turbulence_streamline/results/{agent_mode}/mhd-turbulence_streamline.py".
 
2
  Generate 3D streamlines seeded from a line source along the z-axis at x=64, y=64 (from z=0 to z=127), with 50 seed points.
3
  Color the streamlines by velocity magnitude using the 'Turbo' colormap. Set streamline tube radius to 0.3 using the Tube filter.
4
  Add a color bar labeled 'Velocity Magnitude'. Use a white background. Set an isometric camera view. Render at 1024x1024.
5
+ Set the viewpoint parameters as: [200.0, 200.0, 200.0] to position; [63.5, 63.5, 63.5] to focal point; [0.0, 0.0, 1.0] to camera up direction.
6
  Save the visualization image as "mhd-turbulence_streamline/results/{agent_mode}/mhd-turbulence_streamline.png".
7
  (Optional, but must save if use paraview) Save the paraview state as "mhd-turbulence_streamline/results/{agent_mode}/mhd-turbulence_streamline.pvsm".
8
  (Optional, but must save if use pvpython script) Save the python script as "mhd-turbulence_streamline/results/{agent_mode}/mhd-turbulence_streamline.py".
paraview/rti-velocity_glyph/task_description.txt CHANGED
@@ -4,6 +4,7 @@ Place arrow glyphs on the slice, oriented by the velocity vector. Use uniform ar
4
  Color the arrows by velocity magnitude using the 'Viridis (matplotlib)' colormap. Use a sampling stride of 3.
5
  Add a color bar labeled 'Velocity Magnitude'.
6
  Use a white background. Set the camera to view along the negative y-axis. Render at 1024x1024.
 
7
  Save the visualization image as "rti-velocity_glyph/results/{agent_mode}/rti-velocity_glyph.png".
8
  (Optional, but must save if use paraview) Save the paraview state as "rti-velocity_glyph/results/{agent_mode}/rti-velocity_glyph.pvsm".
9
  (Optional, but must save if use pvpython script) Save the python script as "rti-velocity_glyph/results/{agent_mode}/rti-velocity_glyph.py".
 
4
  Color the arrows by velocity magnitude using the 'Viridis (matplotlib)' colormap. Use a sampling stride of 3.
5
  Add a color bar labeled 'Velocity Magnitude'.
6
  Use a white background. Set the camera to view along the negative y-axis. Render at 1024x1024.
7
+ Set the viewpoint parameters as: [63.5, 250.0, 63.5] to position; [63.5, 64.0, 63.5] to focal point; [0.0, 0.0, 1.0] to camera up direction.
8
  Save the visualization image as "rti-velocity_glyph/results/{agent_mode}/rti-velocity_glyph.png".
9
  (Optional, but must save if use paraview) Save the paraview state as "rti-velocity_glyph/results/{agent_mode}/rti-velocity_glyph.pvsm".
10
  (Optional, but must save if use pvpython script) Save the python script as "rti-velocity_glyph/results/{agent_mode}/rti-velocity_glyph.py".
paraview/rti-velocity_slices/task_description.txt CHANGED
@@ -3,6 +3,7 @@ Create three orthogonal slices: at x=64 (YZ-plane), y=64 (XZ-plane), and z=64 (X
3
  Color all three slices by velocity magnitude using the 'Turbo' colormap.
4
  Add a color bar labeled 'Velocity Magnitude'.
5
  Use a white background. Set an isometric camera view that shows all three slices. Render at 1024x1024.
 
6
  Save the visualization image as "rti-velocity_slices/results/{agent_mode}/rti-velocity_slices.png".
7
  (Optional, but must save if use paraview) Save the paraview state as "rti-velocity_slices/results/{agent_mode}/rti-velocity_slices.pvsm".
8
  (Optional, but must save if use pvpython script) Save the python script as "rti-velocity_slices/results/{agent_mode}/rti-velocity_slices.py".
 
3
  Color all three slices by velocity magnitude using the 'Turbo' colormap.
4
  Add a color bar labeled 'Velocity Magnitude'.
5
  Use a white background. Set an isometric camera view that shows all three slices. Render at 1024x1024.
6
+ Set the viewpoint parameters as: [200.0, 200.0, 200.0] to position; [63.5, 63.5, 63.5] to focal point; [0.0, 0.0, 1.0] to camera up direction.
7
  Save the visualization image as "rti-velocity_slices/results/{agent_mode}/rti-velocity_slices.png".
8
  (Optional, but must save if use paraview) Save the paraview state as "rti-velocity_slices/results/{agent_mode}/rti-velocity_slices.pvsm".
9
  (Optional, but must save if use pvpython script) Save the python script as "rti-velocity_slices/results/{agent_mode}/rti-velocity_slices.py".
paraview/rti-velocity_streakline/task_description.txt CHANGED
@@ -4,6 +4,7 @@ Compute streaklines as a discrete approximation of continuous particle injection
4
  Seed 26 static points along a line on the z-axis at x=64, y=64 (from z=20 to z=108). Use StaticSeeds=True, ForceReinjectionEveryNSteps=1 (reinjection at every sub-timestep), and set TerminationTime=200.
5
  Render the resulting streaklines as tubes with radius 0.3. Color the tubes by velocity magnitude ("magnitude") using the 'Cool to Warm (Extended)' colormap. Add a color bar for velocity magnitude.
6
  Use a white background. Set an isometric camera view and render at 1024×1024.
 
7
  Save the visualization image as "rti-velocity_streakline/results/{agent_mode}/rti-velocity_streakline.png".
8
  (Optional, but must save if use paraview) Save the paraview state as "rti-velocity_streakline/results/{agent_mode}/rti-velocity_streakline.pvsm".
9
  (Optional, but must save if use pvpython script) Save the python script as "rti-velocity_streakline/results/{agent_mode}/rti-velocity_streakline.py".
 
4
  Seed 26 static points along a line on the z-axis at x=64, y=64 (from z=20 to z=108). Use StaticSeeds=True, ForceReinjectionEveryNSteps=1 (reinjection at every sub-timestep), and set TerminationTime=200.
5
  Render the resulting streaklines as tubes with radius 0.3. Color the tubes by velocity magnitude ("magnitude") using the 'Cool to Warm (Extended)' colormap. Add a color bar for velocity magnitude.
6
  Use a white background. Set an isometric camera view and render at 1024×1024.
7
+ Set the viewpoint parameters as: [200.0, 200.0, 200.0] to position; [63.5, 63.5, 63.5] to focal point; [0.0, 0.0, 1.0] to camera up direction.
8
  Save the visualization image as "rti-velocity_streakline/results/{agent_mode}/rti-velocity_streakline.png".
9
  (Optional, but must save if use paraview) Save the paraview state as "rti-velocity_streakline/results/{agent_mode}/rti-velocity_streakline.pvsm".
10
  (Optional, but must save if use pvpython script) Save the python script as "rti-velocity_streakline/results/{agent_mode}/rti-velocity_streakline.py".
paraview/solar-plume/task_description.txt CHANGED
@@ -1,6 +1,6 @@
1
  Task:
2
 
3
- Load the tornado dataset from "solar-plume/data/solar-plume_126x126x512_float32_scalar3.raw", the information about this dataset:
4
  solar-plume (Vector)
5
  Data Scalar Type: float
6
  Data Byte Order: little Endian
@@ -8,13 +8,15 @@ Data Extent: 126x126x512
8
  Number of Scalar Components: 3
9
  Data loading is very important, make sure you correctly load the dataset according to their features.
10
 
11
- Add a “stream tracer” filter under the tornado data to display streamline, set the "Seed type" to "Point Cloud" and set the center of point cloud to 3D position [50, 50, 320] with a radius 30, then hide the point cloud sphere.
12
 
13
  Add a "tube" filter under the "stream tracer" filter to enhance the streamline visualization. Set the radius to 0.5. In the pipeline browser panel, hide everything except the "tube" filter.
14
 
15
 
16
  Please think step by step and make sure to fulfill all the visualization goals mentioned above.
17
 
 
 
18
  Use a white background. Find an optimal view. Render at 1280x1280. Do not show a color bar or coordinate axes.
19
 
20
  Save the visualization image as "solar-plume/results/{agent_mode}/solar-plume.png".
 
1
  Task:
2
 
3
+ Load the solar plume dataset from "solar-plume/data/solar-plume_126x126x512_float32_scalar3.raw", the information about this dataset:
4
  solar-plume (Vector)
5
  Data Scalar Type: float
6
  Data Byte Order: little Endian
 
8
  Number of Scalar Components: 3
9
  Data loading is very important, make sure you correctly load the dataset according to their features.
10
 
11
+ Add a “stream tracer” filter under the solar plume data to display streamline, set the "Seed type" to "Point Cloud" and set the center of point cloud to 3D position [50, 50, 320] with a radius 30, then hide the point cloud sphere.
12
 
13
  Add a "tube" filter under the "stream tracer" filter to enhance the streamline visualization. Set the radius to 0.5. In the pipeline browser panel, hide everything except the "tube" filter.
14
 
15
 
16
  Please think step by step and make sure to fulfill all the visualization goals mentioned above.
17
 
18
+ Set the viewpoint parameters as: [62.51, -984.78, 255.45] to position; [62.51, 62.46, 255.45] to focal point; [0, 0, 1] to camera up direction.
19
+
20
  Use a white background. Find an optimal view. Render at 1280x1280. Do not show a color bar or coordinate axes.
21
 
22
  Save the visualization image as "solar-plume/results/{agent_mode}/solar-plume.png".
paraview/supernova_isosurface/GS/supernova_isosurface_gs.pvsm CHANGED
@@ -1,3 +1,3 @@
1
  version https://git-lfs.github.com/spec/v1
2
- oid sha256:c7a2fe0fd0e2d02159312061cf47f767327cac69b07cdc58790f0a17109a7af3
3
- size 516350
 
1
  version https://git-lfs.github.com/spec/v1
2
+ oid sha256:354b5a3e81aa3c8ee0c794faf3b03e80ad8878d1761f4a45ab80a66a3151334b
3
+ size 516122
paraview/supernova_isosurface/task_description.txt CHANGED
@@ -14,6 +14,8 @@ Please think step by step and make sure to fulfill all the visualization goals m
14
 
15
  Use a white background. Find an optimal view. Render at 1280x1280. Do not show a color bar or coordinate axes.
16
 
 
 
17
  Save the visualization image as "supernova_isosurface/results/{agent_mode}/supernova_isosurface.png".
18
  (Optional, but must save if use paraview) Save the paraview state as "supernova_isosurface/results/{agent_mode}/supernova_isosurface.pvsm".
19
  (Optional, but must save if use pvpython script) Save the python script as "supernova_isosurface/results/{agent_mode}/supernova_isosurface.py".
 
14
 
15
  Use a white background. Find an optimal view. Render at 1280x1280. Do not show a color bar or coordinate axes.
16
 
17
+ Set the viewpoint parameters as: [567.97, 80.17, 167.28] to position; [125.09, 108.83, 121.01] to focal point; [-0.11, -0.86, 0.50] to camera up direction.
18
+
19
  Save the visualization image as "supernova_isosurface/results/{agent_mode}/supernova_isosurface.png".
20
  (Optional, but must save if use paraview) Save the paraview state as "supernova_isosurface/results/{agent_mode}/supernova_isosurface.pvsm".
21
  (Optional, but must save if use pvpython script) Save the python script as "supernova_isosurface/results/{agent_mode}/supernova_isosurface.py".
paraview/supernova_streamline/task_description.txt CHANGED
@@ -21,6 +21,8 @@ In the pipeline browser panel, hide the stream tracer and only show the tube fil
21
 
22
  Use a white background. Render at 1280x1280.
23
 
 
 
24
  Save the visualization image as "supernova_streamline/results/{agent_mode}/supernova_streamline.png".
25
  (Optional, but must save if use paraview) Save the paraview state as "supernova_streamline/results/{agent_mode}/supernova_streamline.pvsm".
26
  (Optional, but must save if use pvpython script) Save the python script as "supernova_streamline/results/{agent_mode}/supernova_streamline.py".
 
21
 
22
  Use a white background. Render at 1280x1280.
23
 
24
+ Set the viewpoint parameters as: [41.38, 73.91, -282.0] to position; [49.45, 49.50, 49.49] to focal point; [0.01, 1.0, 0.07] to camera up direction.
25
+
26
  Save the visualization image as "supernova_streamline/results/{agent_mode}/supernova_streamline.png".
27
  (Optional, but must save if use paraview) Save the paraview state as "supernova_streamline/results/{agent_mode}/supernova_streamline.pvsm".
28
  (Optional, but must save if use pvpython script) Save the python script as "supernova_streamline/results/{agent_mode}/supernova_streamline.py".
paraview/tangaroa_streamribbon/task_description.txt CHANGED
@@ -18,6 +18,8 @@ Please think step by step and make sure to fulfill all the visualization goals m
18
 
19
  Use a white background. Find an optimal view. Render at 1280x1280. Do not show a color bar or coordinate axes.
20
 
 
 
21
  Save the visualization image as "tangaroa_streamribbon/results/{agent_mode}/tangaroa_streamribbon.png".
22
  (Optional, but must save if use paraview) Save the paraview state as "tangaroa_streamribbon/results/{agent_mode}/tangaroa_streamribbon.pvsm".
23
  (Optional, but must save if use pvpython script) Save the python script as "tangaroa_streamribbon/results/{agent_mode}/tangaroa_streamribbon.py".
 
18
 
19
  Use a white background. Find an optimal view. Render at 1280x1280. Do not show a color bar or coordinate axes.
20
 
21
+ Set the viewpoint parameters as: [372.27, 278.87, 214.44] to position; [169.85, 76.46, 12.02] to focal point; [-0.41, 0.82, -0.41] to camera up direction.
22
+
23
  Save the visualization image as "tangaroa_streamribbon/results/{agent_mode}/tangaroa_streamribbon.png".
24
  (Optional, but must save if use paraview) Save the paraview state as "tangaroa_streamribbon/results/{agent_mode}/tangaroa_streamribbon.pvsm".
25
  (Optional, but must save if use pvpython script) Save the python script as "tangaroa_streamribbon/results/{agent_mode}/tangaroa_streamribbon.py".
paraview/tgc-velocity_contour/task_description.txt CHANGED
@@ -3,6 +3,7 @@ Extract a slice at z=32 and color it by velocity magnitude using 'Viridis (matpl
3
  Also add contour lines of velocity magnitude on the same slice at values [0.3, 0.6, 0.9, 1.2] using the Contour filter on the slice output.
4
  Display contour lines in white. Add a color bar labeled 'Velocity Magnitude'.
5
  Light gray background (RGB: 0.9, 0.9, 0.9). Top-down camera. Render at 1024x1024.
 
6
  Save the visualization image as "tgc-velocity_contour/results/{agent_mode}/tgc-velocity_contour.png".
7
  (Optional, but must save if use paraview) Save the paraview state as "tgc-velocity_contour/results/{agent_mode}/tgc-velocity_contour.pvsm".
8
  (Optional, but must save if use pvpython script) Save the python script as "tgc-velocity_contour/results/{agent_mode}/tgc-velocity_contour.py".
 
3
  Also add contour lines of velocity magnitude on the same slice at values [0.3, 0.6, 0.9, 1.2] using the Contour filter on the slice output.
4
  Display contour lines in white. Add a color bar labeled 'Velocity Magnitude'.
5
  Light gray background (RGB: 0.9, 0.9, 0.9). Top-down camera. Render at 1024x1024.
6
+ Set the viewpoint parameters as: [31.5, 31.5, 100.0] to position; [31.5, 31.5, 32.0] to focal point; [0.0, 1.0, 0.0] to camera up direction.
7
  Save the visualization image as "tgc-velocity_contour/results/{agent_mode}/tgc-velocity_contour.png".
8
  (Optional, but must save if use paraview) Save the paraview state as "tgc-velocity_contour/results/{agent_mode}/tgc-velocity_contour.pvsm".
9
  (Optional, but must save if use pvpython script) Save the python script as "tgc-velocity_contour/results/{agent_mode}/tgc-velocity_contour.py".
paraview/tornado/task_description.txt CHANGED
@@ -13,6 +13,7 @@ Add a "Glyph" filter on the original data using Arrow glyph type. Orient arrows
13
  Add an "Outline" filter to display the dataset bounding box (black).
14
 
15
  Use a white background (RGB: 1.0, 1.0, 1.0). Find an optimal view. Render at 1280x1280. Show both color bar and coordinate axes.
 
16
  Save the visualization image as "tornado/results/{agent_mode}/tornado.png".
17
  (Optional, but must save if use paraview) Save the paraview state as "tornado/results/{agent_mode}/tornado.pvsm".
18
  (Optional, but must save if use pvpython script) Save the python script as "tornado/results/{agent_mode}/tornado.py".
 
13
  Add an "Outline" filter to display the dataset bounding box (black).
14
 
15
  Use a white background (RGB: 1.0, 1.0, 1.0). Find an optimal view. Render at 1280x1280. Show both color bar and coordinate axes.
16
+ Set the viewpoint parameters as: [142.01, -36.46, 93.96] to position; [31.5, 31.5, 31.5] to focal point; [-0.35, 0.25, 0.90] to camera up direction.
17
  Save the visualization image as "tornado/results/{agent_mode}/tornado.png".
18
  (Optional, but must save if use paraview) Save the paraview state as "tornado/results/{agent_mode}/tornado.pvsm".
19
  (Optional, but must save if use pvpython script) Save the python script as "tornado/results/{agent_mode}/tornado.py".
paraview/twoswirls_streamribbon/task_description.txt CHANGED
@@ -16,6 +16,7 @@ Show the dataset bounding box as an outline (black, opacity 0.3).
16
  In the pipeline browser panel, hide all stream tracers and only show the ribbon filters and the outline.
17
 
18
  Use a white background (RGB: 1.0, 1.0, 1.0). Find an optimal view. Render at 1280x1280. Do not show a color bar or coordinate axes.
 
19
  Save the visualization image as "twoswirls_streamribbon/results/{agent_mode}/twoswirls_streamribbon.png".
20
  (Optional, but must save if use paraview) Save the paraview state as "twoswirls_streamribbon/results/{agent_mode}/twoswirls_streamribbon.pvsm".
21
  (Optional, but must save if use pvpython script) Save the python script as "twoswirls_streamribbon/results/{agent_mode}/twoswirls_streamribbon.py".
 
16
  In the pipeline browser panel, hide all stream tracers and only show the ribbon filters and the outline.
17
 
18
  Use a white background (RGB: 1.0, 1.0, 1.0). Find an optimal view. Render at 1280x1280. Do not show a color bar or coordinate axes.
19
+ Set the viewpoint parameters as: [30.51, -154.18, 144.99] to position; [30.51, 31.5, 30.91] to focal point; [0.0, 0.53, 0.85] to camera up direction.
20
  Save the visualization image as "twoswirls_streamribbon/results/{agent_mode}/twoswirls_streamribbon.png".
21
  (Optional, but must save if use paraview) Save the paraview state as "twoswirls_streamribbon/results/{agent_mode}/twoswirls_streamribbon.pvsm".
22
  (Optional, but must save if use pvpython script) Save the python script as "twoswirls_streamribbon/results/{agent_mode}/twoswirls_streamribbon.py".
paraview/vortex/task_description.txt CHANGED
@@ -21,7 +21,9 @@ Instructions:
21
 
22
  6. Use a white background. Find an optimal view. Render at 1280x1280. Do not show a color bar or coordinate axes.
23
 
24
- 7. Save your work:
 
 
25
  Save the visualization image as "vortex/results/{agent_mode}/vortex.png".
26
  (Optional, but must save if use paraview) Save the paraview state as "vortex/results/{agent_mode}/vortex.pvsm".
27
  (Optional, but must save if use pvpython script) Save the python script as "vortex/results/{agent_mode}/vortex.py".
 
21
 
22
  6. Use a white background. Find an optimal view. Render at 1280x1280. Do not show a color bar or coordinate axes.
23
 
24
+ 7. Set the viewpoint parameters as: [308.85, 308.85, 308.85] to position; [63.5, 63.5, 63.5] to focal point; [-0.41, 0.82, -0.41] to camera up direction.
25
+
26
+ 8. Save your work:
27
  Save the visualization image as "vortex/results/{agent_mode}/vortex.png".
28
  (Optional, but must save if use paraview) Save the paraview state as "vortex/results/{agent_mode}/vortex.pvsm".
29
  (Optional, but must save if use pvpython script) Save the python script as "vortex/results/{agent_mode}/vortex.py".