Документ взят из кэша поисковой машины. Адрес
оригинального документа
: http://www.sao.ru/precise/Midas_doc/doc/94NOV/vol2/node193.html
Дата изменения: Fri Feb 23 14:01:56 1996 Дата индексирования: Tue Oct 2 18:34:59 2012 Кодировка: Поисковые слова: http astrokuban.info astrokuban |
After having crossed an absorbing cloud, the intensity of a source,
I,
is received by the observer as I(
) = I
, where
is the optical depth of the cloud.
Let's connect to the physical parameters.
N : column densitya(
: line absorption coefficient
: broadening function
a0 =
![]()
![]()
l : lower level of the atomic transition
k : upper level of the atomic transition
: rest wavelength of the transition
g
: statistical weight of the lower level
g
: statistical weight of the upper level
a
: spontaneous transition probability
f= upward oscillator strength