Effects of partial frequency redistribution functions R(II), R(III) and R(V) on source functions

Details Effects of partial frequency redistribution functions R(II), R(III) and R(V) on source functions Effects of partial frequency redistribution functions R(II), R(III) and R(V) on source functions

Jun 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984japa....5..169m&link_type=abstract

Journal of Astrophysics and Astronomy (ISSN 0250-6335), vol. 5, June 1984, p. 169-180.

Astronomy and Astrophysics

Astrophysics

4

Atmospheric Models, Frequency Distribution, Line Spectra, Radiative Transfer, Stellar Atmospheres

Scientific paper

The effects of partial frequency redistribution on the formation of spectral lines have been studied. The angle-averaged R(II), R(III) and R(V) types of redistribution with isotropic phase function have been considered. Transfer equation with plane-parallel geometry is solved in isothermal atmospheres. For an atmosphere with constant thermal sources, the frequency-dependent source function S/L/(R/V/) lies below S/L/(R/III/) but above S/L/(R/II/) in the line wings.

Affiliated with

Also associated with

No associations

Rating

Effects of partial frequency redistribution functions R(II), R(III) and R(V) on source functions does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Effects of partial frequency redistribution functions R(II), R(III) and R(V) on source functions, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Effects of partial frequency redistribution functions R(II), R(III) and R(V) on source functions will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1854882