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Spectrum Strategy Committee Final Report

Announcements · Board and Committee Reports

Document 26

Spectrum Strategy Committee Final Report
To the
ARRL 2002 Annual Meeting
The Spectrum Strategy Committee has continued achieving its objectives as previously outline by the Board. Routine monitoring and documentation activity is continuing. The most notable accomplishment during the past 6 months has been the start of our own noise study named ARIA (Amateur Radio Interference Assessment). Attached to this report is a copy of the ARIA Test Plan. Test Method 1 is operational and our volunteers are currently collecting data. The ARRL Lab has completed initial work on a calibrated noise source procedure that will be implemented in Test Method 2 to follow in the coming months.

The Committee has also spent a considerable amount of time fostering an excellent working relationship with the FCC's Technological Advisory Council. Mr. Rinaldo was invited to present details of our noise study to the TAC last year. The presentation is attached.

As the committee has continued its work in evaluating the impact of various devices on the amateur service, the work is becoming more and more in line with that of the current RFI Task Force.

In order to provide a more efficient means of addressing these issues, we make the following recommendations:

  1. The Amateur Radio Interference Assessment continue as planned under the guidance of an ad hoc committee named "ARIA Steering Group" to be appointed by the President.

  1. The monitoring work in progress and the remaining objectives of the Spectrum Strategy Committee be transferred to the RFI Task Force.

  1. The RFI Task Force is renamed to the "Electromagnetic Compatibility Committee". The make up of the committee shall include the current member of the RFI Task Force plus additional members as deemed necessary by the President.

I want to thank the members of the committee, especially Chris Imlay, Paul Rinaldo, and Jim Maxwell for their very hard work and dedication to this effort.

Respectfully Submitted,

Joel Harrison, W5ZN
Chairman

DRAFT PR 12/10/2001

AMATEUR RADIO INTERFERENCE ASSESSMENT (aRIA)

Test Plan

(Revision 1)

1. PURPOSE

To assess radio noise levels and statistics in certain amateur bands and to determine any changes over time resulting from unlicensed devices.[1]

2. SCOPE

This study is related to a broader program initiated by the Federal Communication Commission (FCC) Technological Advisory Council (TAC) http://www.fcc.gov/oet/tac/ and its Spectrum Working Group, http://www.jacksons.net/tac/. The FCC/TAC program is to be implemented in three parts:

a) Literature survey: Using funds contributed by TAC members, the survey is to be conducted by:

Prof. Richard W. Adler, K6RWA, US Naval Postgraduate School, rwa@attglobal.net.

George H. Hagn, PE, Engineering Consultant, Annandale, VA, ghagn@erols.com

Adjunct Prof. Wilbur R. Vincent, W6PUX, US Naval Postgraduate School, wrvincent@urcad.org

George F. Munsch, W5VPQ, Consultant, munsch@attglobal.net

b) Simulation: This phase of the FCC TAC study is not yet funded.

c) Real-world noise measurements: This is where amateurs can make a substantial contribution by supplying radio noise data for the amateur bands in which unlicensed devices operate. As of this writing, there are no funds available to carry out these measurements. It is anticipated that radio amateurs will perform the measurements on a voluntary basis under technical guidance of the ARRL to help ensure standardized results to facilitate data comparisons.

2.1 Frequencies of Interest

While it is desirable to understand the noise levels of all amateur bands, resource limitations make it necessary to focus on certain bands. The bands of interest are those in which unlicensed devices typically operate and are growing in numbers:

420-450 MHz

902-928 MHz

1240-1300 MHz

2300-2310 MHz

2400-2450 MHz

3300-3500 MHz

5650-5925 MHz

Of these, the band 2400-2450 MHz should have priority because of the current influx of unlicensed devices such as cordless phones, Bluetooth devices and IEEE 802.11b local area networks.

2.2 Environments

International Telecommunication Union (ITU) Recommendation ITU-R PI.372, based on ITU-R Report 258-5 (1990), shows median values of man-made noise power in the frequency range 300 kHz to 250 MHz for the following environmental categories:

A: Business

B: Residential

C: Rural

D: Quiet rural

E: Galactic

The information is given in terms of the effective antenna noise figure, Fa, in dB above kT0B, where k = 1.38 x 10-24 (Boltzmann's constant T0 = 288 K, room temperature) and B = noise power in Hz. The antenna noise level is referenced to the noise power available from a resistor at room temperature (-204 dBW + 10 log10 B).

PI.372 also provides values of decile deviations of man-made noise, i.e., the 90% and 10% values of variations from the medians. Unfortunately, very little documented information is available on man-made noise levels in band above 250 MHz. Thus, there is a need to establish man-made noise levels and related statistics for UHF (300-3000 MHz) and SHF (3-30 GHz) bands and to determine whether the above environmental categories are appropriate.

Of the above categories, assuming they are found to be valid, "residential" and "rural" environments should be of primary interest because they indicate the locations of most amateur stations.

2.3 Duration of Tests

The tests should be conducted over a sufficient period of time to indicate a trend in noise levels and related statistics. Three years is considered a minimum to establish changes in the radio noise environment at a given location.

Within this time frame, daily, weekly and seasonal noise patterns should be determined. Additional short-term tests will be performed using portable/mobile equipment.

3. OBJECTIVES

The goals of this noise study test plan are to:

¨ characterize the types, numbers and signal levels of unlicensed devices operating in amateur bands of interest;

¨ sample residential and rural areas on a long-term basis;

¨ determine trends over a 3-year period, noting variations throughout the day, week and year;

¨ publish the results of these studies for League membership, and for the FCC, National Telecommunications and Information Administration (NTIA), ITU and CISPR, as appropriate;

¨ involve League volunteers in the planning, collection and analysis of test data;

¨ cooperate with, and contribute to, the TAC noise study being conducted for the FCC by the Naval Postgraduate School;

¨ on the basis of analysis of test results, estimate the potential for harmful interference to amateur operations in these bands due to a proliferation of unlicensed devices;

¨ where discovered, identify any uses of these bands not in conformance with FCC regulations or the NTIA Manual and share these results with the appropriate government agencies.

4. OPERATOR REQUIREMENTS

4.1 Availability

Test participants should be willing to make at least a three-year commitment to collect and report noise observations. More specifically, the individual or group would be willing to install a monitoring station, operate it on a semi-automatic basis, send data collected routinely and write reports of significant activity. Periods that the equipment is turned off, such as during vacations, should not normally exceed 3 weeks.

Operators should be available to exchange email correspondence in relation to the tests and participate in telephone conferences if necessary.

4.2 Qualifications

Participation is open to all League members having an understanding of radio theory and some practical experience with bands above 400 MHz. Participants should have the ability to recognize different types of signals that may be encountered in the bands of interest. Further, they should be willing to follow the ARRL test plan. ARRL will provide technical support needed to ensure that the results are uniform and credible.

4.3 Geographical Location

It is desirable to select participants in major metropolitan, suburban and rural areas so there is a diversity of noise environments. Participants should also be geographically dispersed throughout the United States.

5. HARDWARE AND SOFTWARE REQUIREMENTS

5.1 Antennas

Stations at fixed locations participating in the test plan should have both an omnidirectional antenna and a directional antenna of at least 10 dB dBi gain with a short run of low-loss transmission line.

Walk/drive-around stations should have both standard vertical monopole and directional antennas.

5.2 Receivers

Receivers should be of the type normally used by amateurs for weak-signal operation, and should be selected for high sensitivity, low noise figure and large spurious-free dynamic range (SFDR).

WINRADIO model 3700e (approximately $3 k) has a frequency range up to 4 GHz, which covers all the bands of interest. George Hagn recently purchased one and is evaluating it.

Inexpensive hand-held receivers may have some utility in drive/walk-around tests to locate and identify noise sources. The ICOM IC-R3 that covers frequencies up to 2.5 GHz is one example that has been tested by the ARRL lab. Initial tests indicate that it can receive IEEE 802.11b signals at short distances using a loop-Yagi antenna.

5.3 Black Boxes

Participants will be supplied with three "black boxes," as follows:

5.3.1 Noise Source Box

This "black box" will be mounted near to, and a standard distance from, the station receiving antenna, and will include a noise source and a remotely controlled switch to turn on the noise source to calibrate the receiving system. A noise source box may be needed for each band tested. The noise sources will be calibrated by the ARRL Laboratory and will comply with FCC Part 15 limitations.

5.3.2 RF Filter/LNA Box

An RF band-pass filter will be used to protect the broadband low-noise amplifier (LNA), which will be used to increase the sensitivity of the noise measurement receiver. These two components may be housed in the same box.

5.3.3 Anti-Aliasing Filter and A/D Box

This "black box" takes the intermediate-frequency (IF) output of a receiver, filters it to eliminate aliasing, converts the signal from analog to digital form and outputs the digital signal to a personal computer. These boxes will be checked by the ARRL Laboratory and provided to the participants.

5.4 Computer

Any personal computer may be used. However, participants should run tests to verify that the computer does not add to the received noise. If computer-generated noise is a problem, then a Faraday shield may be required around the computer and the cables may require filtering. Instructions on the fabrication of the shield and cable filtering will be provided.

Software to acquire the time samples will be supplied. This software will perform the following functions:

6. TEST OPERATIONS

6.1 Test Method #1

This test method involves driving/walking around to receive signals of interest, identify them by type, determine the origins of the signals (e.g., residential, commercial, etc.), and prepare a report characterizing the radio environment in the bands of interest. Participants using this method should carry a GPS receiver to determine the exact locations and times. This is a short-term test method that may take only one day but which should be repeated about every six months or when significant changes in the environment are observed (e.g., a new building or roadway). The results may be anecdotal and somewhat subjective but they are useful as indications of the types and locations of various emitters.

6.1.1 Test Method #1 Reporting Format

1) Latitude of the test site,

2) Longitude of the test site,

3) Date of test (format YY/MM/DD),

4) Time of test in UTC,

5) Name and of observer (i.e. Paul Rinaldo),

6) Call sign of observer (i.e. W4RI),

7) Center frequency in GHz (Fo),

8) Span Bandwidth in MHz (BW),

9) Resolution Bandwidth in (kHz),

10) Video Bandwidth in (kHz),

11) Manufacture of test instrument,

12) Model number of test instrument,

13) Serial number of test instrument,

14) Calibration due date of test instrument,

15) Diagram of test setup (this will require some thought as to format i.e., AutoCAD drawing etc.),

16) Power measurements in dBm,

17) Spectrum analyzer plot from the actual test (windows metafile or a bit mapped image of some standard format),

18) Observer's receiving setup (brief narrative description such as: vertical LP antenna /antenna oriented toward source/2 dB NF preamp/XYZ1234 receiver),

19) Mobility (examples: fixed location/driving/walking),

20) Distance between source and observer (km),

21) Assumed location of noise source (location name and grid square),

22) Measured polarization of noise source,

23) Description of observed noise (narrative), description of the location. Possibly words like "Rural," "Residential," "Industrial," "Business," "Campus," etc would do.

24) Remarks (narrative. Could include information about whether the use

appears to be within FCC Rules or exceeding limits.)

6.2 Test Method #2

This test method consists of receiving from a fixed location to determine noise levels and statistics and the types of signals of interest and their characteristics over time. The current literature on noise trends with time for a given band and type of noise environment (excepting the Japanese) is almost nonexistent. This is an area where radio amateurs can make a major contribution.

6.2.1 Receiving System Block Diagram

Noise

Source

RF Filter

LNA

RX

Anti-alias

Filter, A/D

Internet

ARIA Web site

Software


Note: The above diagram shows the Noise Source Box connected to an antenna. An alternative is to have the receiver switch between its antenna and a direct connection to the noise source.


6.2.2 Data Elements

6.2.3 Outputs

6.3 Test Method #3

This method is self directed and is based on the assumption that there are a number of participants who are expert at devising test plans and who have access to laboratory quality/traceable test equipment.

Participants volunteering to use this test method should document a specific test plan and share it with the ARIA team prior to implementation. Some consideration should be given to studying the effects of certain types of noise on the bit error rate (BER) of amateur digital communications. Polarization and direction of arrival of signals should be noted to the extent practicable.

7. REPORTS AND ANALYSES

The test data will be sent to a central Web site for analysis. The results will be made available to participants on an ongoing basis. The results of the analysis of individual contributions will be shared with the contributors. Results will be analyzed further on a noise-environment category basis and provided to the TAC noise study.

8. SCHEDULE

(Time line of events in test plan to be developed.)

9. FUNDING

While the tests are largely self-funded, we should consider preparing a list of any items that should be centrally funded, and develop sources such as the ARRL laboratory budget and the ARRL Foundation.

Examples of potential items for this list include the following black boxes:

¨ Noise Source

¨ RF Filter LNA

¨ Anti-alias Filter, A/D


Appendix A

Bibliography

American Radio Relay League, Report of the Ad Hoc Spectrum Strategy Committee, http://www.arrl.org/announce/reports-01/ss.html, January 2001

Anderson, David S., et al, Assessment of Compatibility Between Ultrawideband (UWB) Systems and Global Positioning System (GPS) Receivers, Report No. 01-45, National Telecommunications and Information Administration, 1995, http://www.ntia.doc.gov/osmhome/reports/UwbGps/NTIASP_01_45.pdf

Biggs, Michael, et al, Measurements to Characterize Aggregate Signal Emissions in the 2400-2500 MHz Frequency Range, Report No. 95-323, National Telecommunications and Information Administration, 1995

Dalke, Roger, "Effects of Noise on VHF Satellite Communications," Proc. of International Symposium on Advanced Radio Technologies, Institute for Telecommunication Sciences, NTIA, 1999, http://www.its.bldrdoc.gov/isart/art99/slides99/dal/dal_s.pdf

Dalke, Roger, et al, Spectrum Measurements for an RF-driven Lighting Device, Report No. 99-365, National Telecommunications and Information Administration, May 1999, http://www.its.bldrdoc.gov/pub/all_pubs/1990.html

Federal Communications Commission DA 99-2743, Memorandum Opinion and Order, In the Matter of Amendment of Part 2 of the Commission's Rules to Make Non-Substantive Revisions to the Table of Frequency Allocations, December 1999

Federal Communications Commission, 47 CFR 15 Part 15--Radio Frequency Devices, http://www.fcc.gov/Bureaus/Engineering_Technology/Documents/cfr/1998/47cfr15.pdf

Federal Communications Commission, 47 CFR 18 Part 18--Industrial, Scientific and Medical Equipment, http://www.fcc.gov/Bureaus/Engineering_Technology/Documents/cfr/1998/47cfr18.pdf

Gawthrop, P., et al, Radio Spectrum Measurements of Individual Microwave Ovens, Vols 1 and 2, TR94-303-1 and --2, National Telecommunications and Information Administration, 1994

Hoffman, J. Randy, Measurements to Determine Potential Interference to GPS Receivers from Ultrawideband Transmission Systems, Report No 01-384, National Telecommunications and Information Administration, February 2001, http://www.its.bldrdoc.gov/pub/ntia-rpt/01-384/

International Special Committee on Radio Interference (CISPR), Measurement of Radio Disturbance Characteristics of Industrial, Scientific and Medical R/F Equipment, CISPR11.

International Telecommunication Union, Recommendation ITU-R F.758-1, Considerations in the development of criteria for sharing between the terrestrial fixed service and other services,1997.

International Telecommunication Union, Recommendation ITU-R P.372-6, Radio Noise, 1993.

International Telecommunication Union, Report ITU-R 258-5, Man-Made Radio Noise, 1990.

International Telecommunication Union, Recommendation ITU-R SM.182-4, Automatic Monitoring of Occupancy of the Radio-Frequency Spectrum, 1992

International Telecommunication Union, Recommendation ITU-R SM.337-4, Frequency and Distance Separations, 1997

International Telecommunication Union, Recommendation ITU-R SM.378-6, Field-Strength Measurements at Monitoring Stations, 1955.

Parker, Andrew A., et al, Spectrum Signatures of Man-Made Noise, paper presented at the Conference on Factors Affecting the Reception of Radio Signals, Naval Post Graduate School, March 2001.

Roosa, Paul C, Jr., et al, Assessment of Compatibility Between Ultrawideband Devices and Selected Federal Systems, Report No. 01-43, National Telecommunications and Information Administration, 2001, http://www.ntia.doc.gov/osmhome/reports/uwb/uwb.pdf

Sanders, Frank, et al, Broadband Spectrum Survey at Denver, Colorado 1995, Report No. 95-321, National Telecommunications and Information Administration, 1999, http://www.its.bldrdoc.gov/pub/surv_dnv/

Sanders, Frank, et al, Broadband Spectrum Survey at Los Angles, California May 1997, Report No. 99-336, National Telecommunications and Information Administration, 1999, http://www.its.bldrdoc.gov/pub/ntia-rpt/97-336/97-336_complete_rpt.pdf

Sanders, Frank, et al, Broadband Spectrum Survey at San Diego, California, Dec 1996, Report No. 99-334, National Telecommunications and Information Administration, 1999, http://www.its.bldrdoc.gov/pub/surv_sdg/sdg_ab.html

Sanders, Frank, et al, Broadband Spectrum Survey at San Francisco, California May-June 1995, Report No. 99-367, National Telecommunications and Information Administration, July 1999, http://www.its.bldrdoc.gov/pub/ntia-rpt/99-367/abstract.html

Skomal, Edward N., Man-Made Radio Noise, Van Nostrand Reinhold Company, ISBN 0-442-27648-6, 1978.

Vincent, Wilbur R., et al, Ambient Signals and Noise in the 915-MHz ISM Band, paper presented at the Conference on Factors Affecting the Reception of Radio Signals, Naval Post Graduate School, March 2001.

Vincent, Wilbur R., et al, A Review of Man-Made Radio Noise at 37 HF Receiving Site, paper presented at the Conference on Factors Affecting the Reception of Radio Signals, Naval Post Graduate School, March 2001.

Vincent, Wilbur R., et al, The Temporal and Spectral Structure of 2.4 GHz Radio Noise from a Microwave Oven, paper presented at the Conference on Factors Affecting the Reception of Radio Signals, Naval Post Graduate School, March 2001.


Appendix B

Domestic Allocations and Band Usage

United States Table

Federal Government

Non-Federal Government

FCC §§

Non-Amateur Usage

420-450

RADIOLOCATION G2

S5.286 US7 US87 US217

US228 US230 G8

420-450

Amateur

S5.28 S5.286 US7 US87

US217 US228 US230

NG135

90

97

15.209

Intentional radiators-general limits.

902-928

RADIOLOCATION G59

S5.150 US215 US218

US267 US275 G11

902-928

ISM

PRIVATE LAND MOBILE

Amateur

18.107

90

97

15.245

15.247

Location and Monitoring Service

High-power spread spectrum (cordless telephones)

High-power intentional radiators

Field-disturbance sensors/perimeter protection

Periodic radiators

Material measurement systems

1240-1300

RADIOLOCATION S5.333

G56

S5.334

1240-1300

Amateur

S5.282 S5.333 S5.334

97

15.209

Intentional radiators-general limits

Periodic radiators

LPI voice/data

2300-2305

G123

2300-2305

Amateur

97

15.209

Intentional radiators-general limits

2305-2310

G123

2305-2310

FIXED

MOBILE (except aero)

RADIOLOCATION

Amateur

US338

27

97

15.209

Wireless Communications Service

Intentional radiators-general limits

2390-2400

G122

2390-2400

AMATEUR

97

15.209

15.321

Intentional radiators-general limits

Asynchronous unlicensed personal communications service devices

2400-2402

S5.150 G123

2400-2402

ISM S5.150

Amateur

Amateur-Satellite S5.282

18.107

097

15.247

Microwave ovens

High-power digital cordless telephones

High-power IEEE 802.11b local area networks

Bluetooth

Field disturbance sensors

Unlicensed Personal Communications Service

Intentional radiators-general limits

Periodic radiators

2402-2417

S5.150 G122

2402-2417

ISM S5.150

AMATEUR

Amateur-Satellite S5.282

18

97

15.247

2417-2450

Radiolocation G2

S5.150 G124

2417-2450

ISM S5.150

Amateur

Amateur-Satellite S5.282

18

97

15.245

15.247


United States Table (continued)

Federal Government

Non-Federal Government

FCC §§

Non-Amateur Usage

3300-3500

RADIOLOCATION US108

G31

S5.149

3300-3500

Amateur

Amateur-Satellite S5.282

Radiolocation US108

S5.149

97

15.205

15.251

3300-3332 MHz, 3339-3345.8 MHz and 3358-3500 MHz Intentional radiators-general limits.

3332-3339 MHz and 3345.8-3358 MHz are restricted.

5650-5925

RADIOLOCATION G2

S5.150 US245

5650-5830

ISM S5.150

Amateur

18.107

97

15.245

15.247

15.249

5725-5825 Unlicensed NII

Field-disturbance sensors, perimeter protection

High-power Intentional radiators

High-power intentional radiators-spread spectrum

5830-5850

ISM S5.150

Amateur

Amateur-satellite

(space-to-Earth) S5.282

18

97

15.247

15.249

High-power intentional radiators

High-power intentional radiators-spread spectrum

5850-5925

ISM S5.150

FIXED-SATELLITE

(Earth-to-space) US245

MOBILE NG160

Amateur

18

90

97

15.249

Intelligent Transportation DRCS

High-power intentional radiators



[1] For the purposes of this paper, "noise" includes all manmade radio signals whether intentional or incidental.



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