Changes between Version 8 and Version 9 of u/lchamandy


Ignore:
Timestamp:
08/08/19 13:01:48 (6 years ago)
Author:
Luke
Comment:

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  • u/lchamandy

    v8 v9  
    4949[http://www.pas.rochester.edu/~lchamandy/Graphics/RGB/Post-sink_particle/Post-modified_Lane_Emden/Run151/Paper1/Figure8_velocity_151/v_phi_over_v_Kepler_corot_rel_2_vVec_corot_rel_2_v_phi_over_v_Kepler_corot_rel_2_sliceP2_faceon_lview_30.0Rsun_P1dir_left_-1_0.5_rainbow_151.gif Tangential velocity with velocity vectors (Model IIIC: No subgrid accretion, M2 = 0.25 Msun)]\\
    5050
    51 == Movies corresponding to figures in paper 2 ==
    52 Movies are in the lab (~system CM) reference frame with the CM of the particles located at the center of the frame.
    53 
    54 '''Figure 3 top row---face-on normalized gas binding energy (red means unbound, blue means bound, yellow is density contours, vectors show velocity):'''\\
    55 [http://www.pas.rochester.edu/~lchamandy/Graphics/RGB/Post-sink_particle/Post-modified_Lane_Emden/Run143/E_bind_normalized_vVec_rho_sliceP2_faceon_lview_500Rsun_P1dir_box_-1_1_RdBu_143.gif Face-on normalized energy (Model A: No subgrid accretion, M2 = 1 Msun)]\\
    56 
    57 [http://www.pas.rochester.edu/~lchamandy/Graphics/RGB/Post-sink_particle/Post-modified_Lane_Emden/Run149/E_bind_normalized_vVec_rho_sliceP2_faceon_lview_500Rsun_P1dir_box_-1_1_RdBu_149.gif Face-on normalized energy (Model IIIB: No subgrid accretion, M2 = 0.5 Msun)]\\
    58 
    59 [http://www.pas.rochester.edu/~lchamandy/Graphics/RGB/Post-sink_particle/Post-modified_Lane_Emden/Run151/E_bind_normalized_vVec_rho_sliceP2_faceon_lview_500Rsun_P1dir_box_-1_1_RdBu_151.gif Face-on normalized energy (Model IIIC: No subgrid accretion, M2 = 0.25 Msun)]\\
    60 
    61 '''Figure 3 second from top row---face-on normalized gas kinetic energy (magenta means thermal energy dominates, green means bulk KE dominates, yellow is density contours, vectors show velocity):'''\\
    62 [http://www.pas.rochester.edu/~lchamandy/Graphics/RGB/Post-sink_particle/Post-modified_Lane_Emden/Run143/E_int_kin_normalized_vVec_rho_sliceP2_faceon_lview_500Rsun_P1dir_box_-1_1_PiYG_143.gif Face-on normalized kinetic energy (Model A: No subgrid accretion, M2 = 1 Msun)]\\
    63 
    64 [http://www.pas.rochester.edu/~lchamandy/Graphics/RGB/Post-sink_particle/Post-modified_Lane_Emden/Run149/E_int_kin_normalized_vVec_rho_sliceP2_faceon_lview_500Rsun_P1dir_box_-1_1_PiYG_149.gif Face-on normalized kinetic energy (Model IIIB: No subgrid accretion, M2 = 0.5 Msun)]\\
    65 
    66 [http://www.pas.rochester.edu/~lchamandy/Graphics/RGB/Post-sink_particle/Post-modified_Lane_Emden/Run151/E_int_kin_normalized_vVec_rho_sliceP2_faceon_lview_500Rsun_P1dir_box_-1_1_PiYG_151.gif Face-on normalized kinetic energy (Model IIIC: No subgrid accretion, M2 = 0.25 Msun)]\\
    67 
    68 == Extra Movies ==
     51=== Extra Movies ===
    6952[http://www.pas.rochester.edu/~lchamandy/Graphics/RGB/Post-sink_particle/Post-modified_Lane_Emden/Run143/Paper1/Temperature/Temperature___sliceP2_faceon_lview_250.0Rsun_P1dir_left_1000.0_10000000.0_viridis_143.gif Temperature (Model A: No subgrid accretion, M2 = 1 Msun)]\\
    7053
    … …  
    8770[http://www.pas.rochester.edu/~lchamandy/Graphics/RGB/Post-sink_particle/Post-modified_Lane_Emden/Damp132/Paper1/Mach/Mach_corot_rel_2___sliceP2_faceon_lview_250.0Rsun_P1dir_left_0.01_100_difference_132.gif Mach, frame corotating about secondary (Model IB: Subgrid accretion, M2 = 1 Msun)]\\
    8871
    89 == Side-by-side comparison of Model A (left) and Model IB (right) from Paper I ==
     72=== Side-by-side comparison of Model A (left) and Model IB (right) from Paper I ===
    9073[http://www.pas.rochester.edu/~lchamandy/Graphics/RGB/Post-sink_particle/Post-modified_Lane_Emden/Compare_143_132/Figures1-2_rho.gif Face-on density in cgs]\\
    9174[http://www.pas.rochester.edu/~lchamandy/Graphics/RGB/Post-sink_particle/Post-modified_Lane_Emden/Compare_143_132/Figures4top_rho.gif Edge-on density in cgs]\\
    … …  
    9780[http://www.pas.rochester.edu/~lchamandy/Graphics/RGB/Post-sink_particle/Post-modified_Lane_Emden/Compare_143_132/Mach_corot_rel_2.gif Mach number in frame corotating about secondary]\\
    9881
     82== Movies corresponding to figures in Paper II ==
     83Movies are in the lab (~system CM) reference frame with the CM of the particles located at the center of the frame.
    9984
     85'''Figure 3 top row---face-on normalized gas binding energy (red means unbound, blue means bound, yellow is density contours, vectors show velocity):'''\\
     86[http://www.pas.rochester.edu/~lchamandy/Graphics/RGB/Post-sink_particle/Post-modified_Lane_Emden/Run143/E_bind_normalized_vVec_rho_sliceP2_faceon_lview_500Rsun_P1dir_box_-1_1_RdBu_143.gif Face-on normalized energy (Model A: No subgrid accretion, M2 = 1 Msun)]\\
     87
     88[http://www.pas.rochester.edu/~lchamandy/Graphics/RGB/Post-sink_particle/Post-modified_Lane_Emden/Run149/E_bind_normalized_vVec_rho_sliceP2_faceon_lview_500Rsun_P1dir_box_-1_1_RdBu_149.gif Face-on normalized energy (Model IIIB: No subgrid accretion, M2 = 0.5 Msun)]\\
     89
     90[http://www.pas.rochester.edu/~lchamandy/Graphics/RGB/Post-sink_particle/Post-modified_Lane_Emden/Run151/E_bind_normalized_vVec_rho_sliceP2_faceon_lview_500Rsun_P1dir_box_-1_1_RdBu_151.gif Face-on normalized energy (Model IIIC: No subgrid accretion, M2 = 0.25 Msun)]\\
     91
     92'''Figure 3 second from top row---face-on normalized gas kinetic energy (magenta means thermal energy dominates, green means bulk KE dominates, yellow is density contours, vectors show velocity):'''\\
     93[http://www.pas.rochester.edu/~lchamandy/Graphics/RGB/Post-sink_particle/Post-modified_Lane_Emden/Run143/E_int_kin_normalized_vVec_rho_sliceP2_faceon_lview_500Rsun_P1dir_box_-1_1_PiYG_143.gif Face-on normalized kinetic energy (Model A: No subgrid accretion, M2 = 1 Msun)]\\
     94
     95[http://www.pas.rochester.edu/~lchamandy/Graphics/RGB/Post-sink_particle/Post-modified_Lane_Emden/Run149/E_int_kin_normalized_vVec_rho_sliceP2_faceon_lview_500Rsun_P1dir_box_-1_1_PiYG_149.gif Face-on normalized kinetic energy (Model IIIB: No subgrid accretion, M2 = 0.5 Msun)]\\
     96
     97[http://www.pas.rochester.edu/~lchamandy/Graphics/RGB/Post-sink_particle/Post-modified_Lane_Emden/Run151/E_int_kin_normalized_vVec_rho_sliceP2_faceon_lview_500Rsun_P1dir_box_-1_1_PiYG_151.gif Face-on normalized kinetic energy (Model IIIC: No subgrid accretion, M2 = 0.25 Msun)]\\
     98
     99== Movies corresponding to figures in Paper III ==