Astrophysical Opacities

LEDCOP® Astrophysical Opacities mixed by TOPS®
Calculated by
Los Alamos National Laboratory
Group T-4, Atomic and Optical Theory

This web page was created on April 4, 2000
Materials on this page were last updated on April 4, 2000




Introduction

Welcome to the Los Alamos astrophysical opacity page. This page will enable users to select and view precalculated opacity tables for a selection of standard astrophysical mixtures as well as providing several widely accepted variations in the Z composition for some of these mixtures. The web page provides a broad range in X, Y and Z for each mixture. Individual X-Y-Z tables or the entire set of X-Y-Z tables for each mixture may be downloaded by the user for use in their model calculations. There are more than 1500 Rosseland opacity tables available to the user on this web page, which should satisfy most astrophysical models. Tables not available on this web page can be calculated on the main opacity web page. Requests for nominating new mixtures to be added to this astrophysical opacity page should be sent to the E-mail address given at the bottom of the page.

General Information

New users should examine the information provided in the links given below before proceeding. These links will list the paramater spaces for the tables, give detailed information on all current materials and discuss the advantages and limitations of using this web page instead of the main opacity web page.

There is one limitation for these tables that must be realized by users and this limitation is so important that you will see it listed on all of the Web pages. These tables were calculated with atomic models and have no molecular species in the equation of state and no molecular cross sections in the opacity calculation. Users must provide their own tables below 12,000 oK if they wish to include these important molecular contributions.


Mixture Selection

This Web page is set up to allow users to examine or download a maximum of one mixture at a time. Since this file can be over 1 megabyte in size, it was felt that this is the practical upper limit for file transfers at the present time. It is also possible for the user to download a selected subset of the X-Y-Z tables. The options are given below:

1. (1+ megabytes)  Full mixture with all X-Y-Z tables.
                   NOTE:  Some mixtures are smaller.


2. (10+ kilobytes) Single X-Y-Z table for specified mixture. Individual tables may be displayed and plotted and then downloaded.

3. (10+ kb/table) Depending on your browser and/or platform, users can download a group or block of individual X-Y-Z tables.

These options can be exercised from the next Web Page after the mixture is selected. This page will default to the standard Anders-Grevesse-Noels mixture.

Ross-Aller (standard mix)
Anders-Grevesse-Noels (standard mix)
Anders-Grevesse-Noels (alpha enhance I)
Anders-Grevesse-Noels (alpha enhance II)
Anders-Grevesse-Noels (Na,Mg,Ti enhance)
Anders-Grevesse-Noels (V - Zn reduced)
Anders-Grevesse-Noels (N enhanced 2x)
Anders-Grevesse-Noels (N enhanced 4x)
Anders-Grevesse-Noels (N enhanced 8x)
Anders-Grevesse-Noels (N enhanced 16x)
Grevesse-Sauval (standard mix)
Grevesse-Sauval (Ne decreased by 15%)
Grevesse-Sauval (Ne increased by 15%)


May take up to 30 seconds to set up the tables for your mixture.


Useful Links

Return to t-4 home page.......... Main Opacity Web Page.


Please mail questions or comments to:
LANL T-4 Opacities <opacity@t4.lanl.gov>

Hits since April 4, 2000: 11850 by 2887 users

Los Alamos Report No. LA-UR-01-1258

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