coupled escape probabilities - gives implementation details (trac #249)

[cloudy-bot]

reported by: @CloudyLex

Title:  
    Coupled Escape Probability for an Asymmetric Spherical Case: Modeling Optically Thick Comets
Authors:    
    Gersch, Alan M.; A'Hearn, Michael F.
Publication:    
    eprint arXiv:1212.1226
Publication Date:   
    12/2012
Origin: 
    ARXIV
Keywords:   
    Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Instrumentation and Methods for Astrophysics
Comment:    
    18 pages 22 figures
Bibliographic Code: 
    2012arXiv1212.1226G
Abstract
We have adapted Coupled Escape Probability, a new exact method of 
solving radiative transfer problems, for use in asymmetrical 
spherical situations. Our model is intended specifically for use in 
modeling optically thick cometary comae, although not limited to 
such use. This method enables the accurate modeling of comets' 
spectra even in the potentially optically thick regions nearest the 
nucleus, such as those seen in Deep Impact observations of 
9P/Tempel 1 and EPOXI observations of 103P/Hartley 2. 

Migrated from https://www.nublado.org/ticket/249

{
    "status": "new",
    "changetime": "2019-02-04T13:07:06Z",
    "_ts": "1549285626580696",
    "description": "{{{\nTitle:\t\n\tCoupled Escape Probability for an Asymmetric Spherical Case: Modeling Optically Thick Comets\nAuthors:\t\n\tGersch, Alan M.; A'Hearn, Michael F.\nPublication:\t\n\teprint arXiv:1212.1226\nPublication Date:\t\n\t12/2012\nOrigin:\t\n\tARXIV\nKeywords:\t\n\tAstrophysics - Earth and Planetary Astrophysics, Astrophysics - Instrumentation and Methods for Astrophysics\nComment:\t\n\t18 pages 22 figures\nBibliographic Code:\t\n\t2012arXiv1212.1226G\nAbstract\nWe have adapted Coupled Escape Probability, a new exact method of \nsolving radiative transfer problems, for use in asymmetrical \nspherical situations. Our model is intended specifically for use in \nmodeling optically thick cometary comae, although not limited to \nsuch use. This method enables the accurate modeling of comets' \nspectra even in the potentially optically thick regions nearest the \nnucleus, such as those seen in Deep Impact observations of \n9P/Tempel 1 and EPOXI observations of 103P/Hartley 2. \n}}}",
    "reporter": "gary",
    "cc": "",
    "resolution": "",
    "time": "2012-12-07T14:42:14Z",
    "component": "radiative transfer",
    "summary": "coupled escape probabilities - gives implementation details",
    "priority": "good to do",
    "keywords": "",
    "version": "trunk",
    "milestone": "no milestone",
    "owner": "nobody",
    "type": "enhancement"
}

[cloudy-bot]

@peter-van-hoof-noaccount changed milestone from "" to "no milestone"