Skip to main content Accessibility help
×
Hostname: page-component-76fb5796d-x4r87 Total loading time: 0 Render date: 2024-04-26T17:06:50.254Z Has data issue: false hasContentIssue false

2 - Transceiver challenges for white space radio

from Part I - White space technology signal processing and digital design

Published online by Cambridge University Press:  05 October 2014

Kevin Gard
Affiliation:
Analog Devices, USA
Nuno Borges Carvalho
Affiliation:
Universidade de Aveiro, Portugal
Alessandro Cidronali
Affiliation:
Università degli Studi di Firenze, Italy
Roberto Gómez-García
Affiliation:
Universidad de Alcalá, Madrid
Get access

Summary

Introduction

The availability of white space spectrum offers many new opportunities to provide the public with abundant access to broadband data services and enable communications between remote equipment and sensors. However, every new technology opportunity also carries with it new challenges that must be addressed to realize the benefits. The challenge for white space radio applications is that the receiver must be tolerant to the high levels of interfering signals that may be present and the restriction that the transmitter may not interfere with existing services. These two challenges impose heavy restrictions on the radio architectures used to meet white space radio system performance expectations. This chapter quantifies several of the restrictive transceiver requirements that a white space radio must meet. In the US, white space radio applications are permitted to use broadcast television spectrum that is not being used by broadcast television or other local services. The white space spectrum is divided into different parts according to the allocation of broadcast television channels: 2, 5–6, 7–13, 14–36, and 38–51. Channels excluded from white space use include channels 3 and 4 that are protected for video RF modulators commonly used to upconvert DVD, video tape, and video game signals for use with a television tuner, and channel 37 as it is reserved for radio astronomy applications. Each white space channel has an available bandwidth of 6 MHz.

Type
Chapter
Information
Publisher: Cambridge University Press
Print publication year: 2014

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

References

[1] http://reboot.fcc.gov/reform/systems/spectrum-dashboard
[2] C. E., ShannonCommunication in the Presence of noise,” Proceedings of the IRE, vol. 37, no. 1, pp. 10, 21, January 1949.Google Scholar

Save book to Kindle

To save this book to your Kindle, first ensure coreplatform@cambridge.org is added to your Approved Personal Document E-mail List under your Personal Document Settings on the Manage Your Content and Devices page of your Amazon account. Then enter the ‘name’ part of your Kindle email address below. Find out more about saving to your Kindle.

Note you can select to save to either the @free.kindle.com or @kindle.com variations. ‘@free.kindle.com’ emails are free but can only be saved to your device when it is connected to wi-fi. ‘@kindle.com’ emails can be delivered even when you are not connected to wi-fi, but note that service fees apply.

Find out more about the Kindle Personal Document Service.

Available formats
×

Save book to Dropbox

To save content items to your account, please confirm that you agree to abide by our usage policies. If this is the first time you use this feature, you will be asked to authorise Cambridge Core to connect with your account. Find out more about saving content to Dropbox.

Available formats
×

Save book to Google Drive

To save content items to your account, please confirm that you agree to abide by our usage policies. If this is the first time you use this feature, you will be asked to authorise Cambridge Core to connect with your account. Find out more about saving content to Google Drive.

Available formats
×