Changes between Version 57 and Version 58 of u/ehansen


Ignore:
Timestamp:
06/20/12 09:15:00 (12 years ago)
Author:
ehansen
Comment:

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  • u/ehansen

    v57 v58  
     1[[PageOutline]]
     2[[BackLinksMenu]]
     3
    14= Useful Links =
    25* [http://www.pas.rochester.edu/~ehansen home page on pas server]
    … …  
    58= Projects =
    69[[BR]]
    7 
    8 === My Library ===
     10=== [wiki:u/ehansen/EddiesLibrary My Library] ===
    911Here I have been collecting the important literature relative to my research.  Most of these papers are about or related to radiative, magnetized jets and shocks.  I will also include notes/summary for each paper.
    1012
    11 [wiki:u/ehansen/EddiesLibrary Eddie's Library]
    1213[[BR]]
    1314
    14 === 3D Cooling Jets ===
     15=== [wiki:3dcoolingjets 3D Cooling Jets] ===
    1516Using Martin's CRL618 jet module, I have been testing 3D jets with different cooling strengths.
    1617
    17 [wiki:3dcoolingjets]
    1818[[BR]]
    1919
    20 === 1D Radiative Shocks ===
     20=== [wiki:1dradshocks 1D Radiative Shocks] ===
    2121This is the problem of setting up a semi-analytic solution for a steady, 1D, radiative shock.  It was mainly used to test the implementation of NEQ and Z cooling.
    2222
    2323[[Image(allcool_temp.png,width=300)]]
    2424
    25 [wiki:1dradshocks]
    2625[[BR]]
    2726
    28 === Z Cooling ===
     27=== [wiki:zcooling Z Cooling] ===
    2928The 5th type of cooling implemented in astrobear.  This includes forbidden line emission, and uses Pat Hartigan's tables.
    3029
    31 [wiki:zcooling]
    3230[[BR]]
    3331
    34 === Non-equilibrium Cooling ===
     32=== [wiki:neqcooling Non-equilibrium Cooling] ===
    3533The 4th type of cooling implemented in astrobear.  This includes effects of ionization and recombination.
    3634
    37 [wiki:neqcooling]
    3835[[BR]]
    3936
    40 === Building a 1D Hydro Code ===
    41 The best way to learn how to write a hydro code is to build your own.  I've created a separate page on the wiki to document the important aspects of fluid dynamics and numerical methods as I learn how to build my own 1D hydro code: [wiki:ehansen/buildcode Building a 1D Hydro Code]
     37=== [wiki:ehansen/buildcode Building a 1D Hydro Code] ===
     38The best way to learn how to write a hydro code is to build your own.  I've created a separate page on the wiki to document the important aspects of fluid dynamics and numerical methods as I learn how to build my own 1D hydro code.
    4239[[BR]]
    4340
    44 === Rayleigh-Taylor Instability ===
    45 The RT Instability...a dense fluid sitting on top of a light fluid.  When slightly perturbed the light fluid rises upwards, and the heavy fluid sinks downwards.  See this page for more details on the problem analysis and simulations: [wiki:ehansen/RT My Rayleigh-Taylor Page]
     41=== [wiki:ehansen/RT Rayleigh-Taylor Instability] ===
     42The RT Instability...a dense fluid sitting on top of a light fluid.  When slightly perturbed the light fluid rises upwards, and the heavy fluid sinks downwards.  This page contains more details on the problem analysis and simulations.
     43
    4644|| [[Image(density_image0000.png, height=400, width=300)]] || [[Image(density_image0040.png, height=400, width=300)]] || [[Image(density_image0125.png, height=400, width=300)]] ||
    4745[[BR]]
    4846
    4947=== Field Loop Advection ===
    50 This is from when I was first learning how to run AstroBEAR.
     48My very first simulation.  I had just joined the group, and this was from when I was first learning how to compile and run AstroBEAR.
    5149* [attachment:Bvec_movie.gif Bvec Movie]
    5250----