Radiative stability of interstellar masers - A variational technique

Details Radiative stability of interstellar masers - A variational technique Radiative stability of interstellar masers - A variational technique

Sep 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982ap%26ss..86..477s&link_type=abstract

Astrophysics and Space Science, vol. 86, no. 2, Sept. 1982, p. 477-484.

Astronomy and Astrophysics

Astrophysics

4

Flow Stability, Interstellar Masers, Radiation Distribution, Radiative Transfer, Variational Principles, Dispersing, Pumping, Steady State, Time Dependence

Scientific paper

A variational technique has been developed to study the stability of the radiation field in a cylindrical homogeneous interstellar maser with steady state pumping. A dynamical potential has been constructed, the extremal of which gives the radiative transfer equations and rate equations. The dispersion equations and the stability criteria are determined from the potential for specific natures of perturbations.

Affiliated with

Also associated with

No associations

Rating

Radiative stability of interstellar masers - A variational technique 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 Radiative stability of interstellar masers - A variational technique, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Radiative stability of interstellar masers - A variational technique will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1256861