Документ взят из кэша поисковой машины. Адрес оригинального документа : http://xmm.vilspa.esa.es/sas/8.0.0/doc/ssclib/node39.html
Дата изменения: Wed Jul 2 03:52:39 2008
Дата индексирования: Fri Sep 5 18:38:20 2008
Кодировка:
Поисковые слова: наблюдения метеорных потоков

XMM-Newton Science Analysis System


ssclib (ssclib-3.33.4) [xmmsas_20080701_1801-8.0.0]

Meta Index / Home Page / A module which contains

Black Body routines

These subroutines calculate the power (in watts) radiated per unit surface area (m2) per unit solid angle (sr) by a black body at temperature='kelvin'. The power can be calculated either per unit frequency, at a given frequency (both in hertz), or per unit wavelength (in metres) at a given supplied wavelength (in angstroms).

The subroutines are designed to be portable and as fast yet as accurate as possible.