UNLIMITED FREE
ACCESS
TO THE WORLD'S BEST IDEAS

SUBMIT
Already a GlobalSpec user? Log in.

This is embarrasing...

An error occurred while processing the form. Please try again in a few minutes.

Customize Your GlobalSpec Experience

Finish!
Privacy Policy

This is embarrasing...

An error occurred while processing the form. Please try again in a few minutes.

NASA-LLIS-1595

Lessons Learned - Interferometer Design

active, Most Current
Organization: NASA
Publication Date: 10 February 2005
Status: active
Page Count: 3
scope:

Abstract:

The Focal Plane Arrays (FPAs)-to-Read-Only Integrated Circuits (ROICs) timing and frame synchronization for imaging interferometers are significantly different than those typically used in radiometric cameras and other similar FPA applications. Because the Michelson interferometer used on GIFTS utilizes a translating end mirror to change and continuously scan the optical path, the frames of FPA are collected at constant Optical Path Difference (OPD) intervals over the entire scan. The interferometer mirror»s translation rate and its corresponding OPD change rate are not perfectly linear. Thus, the FPA collection frame rate will vary with time.

Document History

NASA-LLIS-1595
February 10, 2005
Lessons Learned - Interferometer Design
Abstract: The Focal Plane Arrays (FPAs)-to-Read-Only Integrated Circuits (ROICs) timing and frame synchronization for imaging interferometers are significantly different than those typically used in...
Advertisement