๐”– Bobbio Scriptorium
โœฆ   LIBER   โœฆ

A spectral meteorological model on the ICL DAP

โœ Scribed by Glenn Carver


Publisher
Elsevier Science
Year
1988
Tongue
English
Weight
436 KB
Volume
8
Category
Article
ISSN
0167-8191

No coin nor oath required. For personal study only.


๐Ÿ“œ SIMILAR VOLUMES


Monte Carlo calculations of neutron diff
โœ L.M. Delves ๐Ÿ“‚ Article ๐Ÿ“… 1985 ๐Ÿ› Elsevier Science ๐ŸŒ English โš– 658 KB

Monte Carlo techniques are potentially well suited to SIMD architectures, provided that the samples used can be treated in parallel. The standard sampling schemes used for the simulation of neutron diffusion make this impossible; we describe here a revised scheme which has been implemented on the IC

Particle simulation of 3D galactic hydro
โœ T.C. Johns; A.H. Nelson ๐Ÿ“‚ Article ๐Ÿ“… 1985 ๐Ÿ› Elsevier Science ๐ŸŒ English โš– 756 KB

A non-self-gravitating galactic hydrodynamics code based on a quasi-particle technique and making use of a mesh for force evaluation and sorting purposes is described. The short-range nature of the interparticle pressure forces, coupled with the use of a mesh allows a particularly fast algorithm. Th

A prominence model based on spectral obs
โœ J. M. Fontenla ๐Ÿ“‚ Article ๐Ÿ“… 1979 ๐Ÿ› Springer ๐ŸŒ English โš– 359 KB

Intensities and profiles of the Ha, H/3, H3,, K, and D3 lines are measured in a solar prominence. From the profiles of these lines we estimate T = 6400 K and vt = 5.7 km s -1. We construct a simple isothermal model which explains the Ha intensity and profile for an assumed total particle density nT