scispace - formally typeset
S

Sabino Piazzolla

Researcher at University of Southern California

Publications -  6
Citations -  250

Sabino Piazzolla is an academic researcher from University of Southern California. The author has contributed to research in topics: Holography & Holographic grating. The author has an hindex of 5, co-authored 6 publications receiving 244 citations.

Papers
More filters
Journal ArticleDOI

First-harmonic diffusion model for holographic grating formation in photopolymers

TL;DR: In this article, a model with which to describe and predict the formation of gratings during exposure in holographic photopolymers is presented, which combines the action of photopolymerization and of free-monomer diffusion during holographic exposures.
Journal ArticleDOI

Holographic grating formation in photopolymers

TL;DR: This model, which combines polymerization kinetics with results from coupled-wave theory, indicates that the grating formation time depends sublinearly on the average holographic recording intensity, and the beam intensity ratio controls thegrating index modulation at saturation.
Journal ArticleDOI

Dynamics during holographic exposure in photopolymers for single and multiplexed gratings

TL;DR: In this paper, the authors present a model that describes the dynamics of the holographic grating formation in photopolymers under the assumption that at low recording intensity the grating forming process is much slower than the free monomer diffusion, while the average recording intensity is related in a nonlinear fashion to the process time.
Journal ArticleDOI

Single-step copying process for multiplexed volume holograms.

TL;DR: A technique for copying the index or absorption modulation of a multiplexed volume holographic element into a secondVolume holographic medium is presented and can perform the copy process in a single exposure step.
Proceedings ArticleDOI

Statistics of link blockage due to cloud cover for free-space optical communications using NCDC surface weather observation data

TL;DR: In this paper, the site location chosen for a telescope used for optical communications must rely on knowledge of weather and cloud cover statistics for the geographical area where the telescope itself is located.