Coherent receiver components for high frequency astrophysics applications

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Abstract/Contents

Abstract
Coherent receivers for electromagnetic radiation in the frequency band from 120 - 180 GHz and higher have many important applications for ground-based astronomy and millimeter-wave imaging, such as security screening and imaging from aircraft. This thesis reviews the development and testing of new receiver components that have enabled the design of compact and mass-producible receiver modules for instruments that require high sensitivity in this frequency band. A genetic algorithm was used to optimize a smooth-walled feedhorn antenna, which will be presented along with analysis of feedhorn efficiencies. Record low noise measurements for Monolithic Millimeter-wave Integrated Circuit (MMIC) Low Noise Amplifiers (LNAs) in this band, made possible by recent advances in High Electron Mobility Transistors (HEMTs), are also included. These devices are now being incorporated into complete receiver modules that will be used in instruments for astrophysics applications.

Description

Type of resource text
Form electronic; electronic resource; remote
Extent 1 online resource.
Publication date 2013
Issuance monographic
Language English

Creators/Contributors

Associated with Larkoski, Patricia Elaine Voll
Associated with Stanford University, Department of Applied Physics.
Primary advisor Church, Sarah
Primary advisor Petrosian, Vahe
Thesis advisor Church, Sarah
Thesis advisor Petrosian, Vahe
Thesis advisor Cabrera, Blas
Advisor Cabrera, Blas

Subjects

Genre Theses

Bibliographic information

Statement of responsibility Patricia Elaine Voll Larkoski.
Note Submitted to the Department of Applied Physics.
Thesis Thesis (Ph.D.)--Stanford University, 2013.
Location electronic resource

Access conditions

Copyright
© 2013 by Patricia Elaine Voll Larkoski
License
This work is licensed under a Creative Commons Attribution Non Commercial 3.0 Unported license (CC BY-NC).

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