Ãùöù Blockinþ³× Ó× Ùòòòö Aeí¹ääòùü
نویسنده
چکیده
We report on the latest version of our GNU-Linux port of the ATLAS – SYNTHE – WIDTH suite of codes for the stellar atmosphere modeling. The latest version (8.1 at the time of the workshop) of the Intel Fortran Compiler allowed for a significantly better backward compatibility with the VMS version of the code, thus allowing us to remove almost all the modifications we initially introduced in order to compile the code under IFC. We now provide ported versions both of ATLAS 9 (the ODF version of ATLAS) and ATLAS 12 (the opacity sampling version). A comprehensive website has been created to host the ported codes, along with a growing body of documentation and resources. Also, three mailing lists have been created at the university of Ljubljana in order to cover general usage, code development and ATLAS-related announcements.
منابع مشابه
Çò Ëô Blockinð Óöñ× Ó Êê×øøöøøò Ùøóññøø * º Åöþ´ñöþ×úºñ׺ñº Blockinùòº Blockinþµ¸åº Èððø´ôððø×ºñ׺ñº Blockinùòº Blockinþµ Ò Åº Èöó Blockinþ
متن کامل
Èööññøøö Óòøöóð Ò Úóðùøøóòòöý Ððóööøøñ× Ó×øóò º Ò Êóóöø Ààòøøöööòò Òò Òòòû Åå Blockinððûû Blockinþ
متن کامل
Èöóóöö×× Ò Ùòòòö×øøòòòòò Òò Üôðóóøøòò ×øøðððö Ó× Blockin Blockinðððøøóò ×ô Blockinøöö
Rich oscillation spectra of dwarf-like pulsators contain a wealth of information about the object interiors and, in particular, about macroscopic transport processes, which is the most difficult aspect of stellar physics. Examples of extracting such information from data on solar-like and opacity driven pulsators are given. Problems in understanding new oscillation spectra are discussed. Import...
متن کاملذخیره در منابع من
با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید
عنوان ژورنال:
دوره شماره
صفحات -
تاریخ انتشار 2005