Astronomy and Astrophysics – Astrophysics
Scientific paper
Oct 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992apj...398..177i&link_type=abstract
Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 398, no. 1, p. 177-183.
Astronomy and Astrophysics
Astrophysics
6
Energy Transfer, Plasma Diffusion, Plasma Heating, Thermal Conductivity, Thermal Stability, Transport Properties, Heat Balance, Plasma Temperature, Temperature Distribution
Scientific paper
The range of values of the parameters characterizing the energy transport mechanisms and boundary conditions, for which slablike, cylindrical, and spherical structures are thermally stable, are determined. The configurations are assumed to be heated at a rate about T exp m cooled at a rate about T exp n and with a thermal conductivity coefficient about Tk. The linear stability of the trivial solution of the steady heat balance equation was carried out analytically. The remaining families of solutions were obtained numerically. They were classified, the minimal boundary temperature for steady solutions obtained, their stability analyzed, and their general properties depending on the indexes nu (symmetry), m, n, and k were outlined.
Iba~nez Miguel H. S.
Mendoza Cesar A. B.
Parravano Antonio
No associations
LandOfFree
On the thermal structure and stability of configurations with heat diffusion and a gain-loss function. I - General results 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 On the thermal structure and stability of configurations with heat diffusion and a gain-loss function. I - General results, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and On the thermal structure and stability of configurations with heat diffusion and a gain-loss function. I - General results will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1869599