Difference between revisions of "Checking dust decorrelation in Raphael MHD based dust sim"

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(Created page with "Sept 8 2017, Clem Pryke Raphael has recently placed files on NERSC for dust and sync maps derived from MHD sims of the galactic magnetic field. Here I show a plot showing the...")
 
 
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Sept 8 2017, Clem Pryke
 
Sept 8 2017, Clem Pryke
  
Raphael has recently placed files on NERSC for dust and sync maps derived from MHD sims of the galactic magnetic field.
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Raphael has recently placed files on NERSC for dust and sync maps derived from MHD sims of the galactic magnetic field - these
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have been declared Sky Model 6.
 
Here I show a plot showing the spectra of the dust component in this sim and the degree of decorrelation.
 
Here I show a plot showing the spectra of the dust component in this sim and the degree of decorrelation.
 
These can be compared to the plots for the PySM models previously posted  at [[Checking dust decorrelation in models d1/d4/d7 and hipdt]].
 
These can be compared to the plots for the PySM models previously posted  at [[Checking dust decorrelation in models d1/d4/d7 and hipdt]].
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As for the PySM models the degree of decorrelation is extremely small.
  
 
[[File:170908_f1.gif]]
 
[[File:170908_f1.gif]]

Latest revision as of 09:45, 8 September 2017

Sept 8 2017, Clem Pryke

Raphael has recently placed files on NERSC for dust and sync maps derived from MHD sims of the galactic magnetic field - these have been declared Sky Model 6. Here I show a plot showing the spectra of the dust component in this sim and the degree of decorrelation. These can be compared to the plots for the PySM models previously posted at Checking dust decorrelation in models d1/d4/d7 and hipdt.

As for the PySM models the degree of decorrelation is extremely small.

170908 f1.gif