Radiative power loss from laboratory and astrophysical plasmas. I - Power loss from plasmas in steady-state ionisation balance

Details Radiative power loss from laboratory and astrophysical plasmas. I - Power loss from plasmas in steady-state ionisation balance Radiative power loss from laboratory and astrophysical plasmas. I - Power loss from plasmas in steady-state ionisation balance

Jul 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979jphb...12.2387s&link_type=abstract

Journal of Physics B - Atomic and Molecular Physics, vol. 12, July 28, 1979, p. 2387-2412. Research supported by the U.K. Atomic

Physics

82

Bremsstrahlung, Deuterium Plasma, Energy Dissipation, Plasma Radiation, Rarefied Plasmas, Steady State, Continuous Radiation, Optical Thickness, Radiative Transfer, Solar Atmosphere, Tritium

Scientific paper

The power radiated by an optically thin low-density plasma in steady state ionization balance is calculated taking into account spectral lines, recombination continuum and bremsstrahlung. Calculations were performed in the temperature range 10 to the 4th to 10 to the 10th K for all ions of carbon, oxygen, silicon and argon and for all ions of iron and molybdenum of charge greater than 7 and 23, respectively. The role of impurity radiation loss for a D-T power-producing plasma is investigated and a composite calculation of the radiated power loss from the solar atmosphere is also presented.

Affiliated with

Also associated with

No associations

Rating

Radiative power loss from laboratory and astrophysical plasmas. I - Power loss from plasmas in steady-state ionisation balance 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 power loss from laboratory and astrophysical plasmas. I - Power loss from plasmas in steady-state ionisation balance, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Radiative power loss from laboratory and astrophysical plasmas. I - Power loss from plasmas in steady-state ionisation balance will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1557228