Active Standard

IEEE 187-2018

IEEE Standard for Measurement of Emissions from FM and Television Broadcast Receivers in the Frequency Range of 9 kHz to 40 GHz

Spurious radiation from sound and television broadcast receivers are possible sources of interference with other radio services. This standard describes the potential sources of spurious radiation from receivers intended for the reception of sound and television broadcast, and the measurement methods for them.

Standard Committee
EMC/SDCom - Standards Development Committee
Status
Active Standard
PAR Approval
2014-10-27
Superseding
187-2003
Board Approval
2018-02-15
History
Published:
2018-05-31

Working Group Details

Society
IEEE Electromagnetic Compatibility Society
Standard Committee
EMC/SDCom - Standards Development Committee
Working Group
P187 Working Group - IEEE Standard for Measurement Methods of Emissions from FM and Television Broadcast Receivers in the Frequency Range of 9kHz to 40GHz
IEEE Program Manager
Jennifer Santulli
Contact Jennifer Santulli
Working Group Chair
David Traver

Other Activities From This Working Group

Current projects that have been authorized by the IEEE SA Standards Board to develop a standard.


No Active Projects

Standards approved by the IEEE SA Standards Board that are within the 10-year lifecycle.


No Active Standards

These standards have been replaced with a revised version of the standard, or by a compilation of the original active standard and all its existing amendments, corrigenda, and errata.


No Superseded Standards

These standards have been removed from active status through a ballot where the standard is made inactive as a consensus decision of a balloting group.


No Inactive-Withdrawn Standards

These standards are removed from active status through an administrative process for standards that have not undergone a revision process within 10 years.


No Inactive-Reserved Standards
Subscribe to our Newsletter

Sign up for our monthly newsletter to learn about new developments, including resources, insights and more.