Building on an exponential model for disk lifetimes, this dissertation presents analytic models for disk-array lifetime, evaluates these against event-drived simulation, and applies them to an example redundant disk array.
It has been shown for flake iron that the Young's modulus is in close agreement with the models for disk-shaped inclusions, and with models for spherical inclusions for the spheroidal iron.
The structures of the outer segment membranes support a model for disk morphogenesis in which basal disks are enveloped by the plasma membrane.
Our results obtained with pharmacological drug treatments suggest that the current animal model for disk degeneration-initiated pain recapitulates responses to human symptoms.
The coupled gyroscopic system equations are formulated using a Kirchhoff plate model for the disk, and the wave equation for the compressible fluid.
As before, we re-load a model from disk.
In this paper, I first introduce a model for gaseous disks such as protoplanetary and circumplanetary disks, and then, I revisit the derivation of Adachi et al. (1976) for the analytic formulae of (dot a), (dot e), and (dot i).
Several studies[15 18] were dedicated to devise models for individual hard disks, where the power consumption of a disk is predicted based on its states such as seek, rotation, reads, writes and idle.
Namely, they constructed their thermal models for passive protoplanetary disks without regard to the fact that T Tauri stars would be accompanied by a stellar wind.
Our technique opens up a path to explore other binary systems, providing an independent estimate of distance and the flaring angle, a crucial parameter for disk modelling.
Wood K, Crosas M, Ghez A. GG Tauri's Circumbinary Disk: Models for Near-Infrared Scattered-Light Images and 13CO (J= 1→ 0) Line Profiles.
