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OECD and Radio Astronomy Spectrum

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Title: OECD and Radio Astronomy Spectrum


1
OECD and Radio Astronomy Spectrum
  • Tasso Tzioumis
  • Australia Telescope National Facility
  • 10 June 2002

2
OECD
  • ORGANISATION FOR ECONOMIC CO-OPERATION AND
    DEVELOPMENT
  • International organisation
  • 30 Members mainly western countries i.e. USA,
    Japan, European countries, Australia, Canada,
  • Heads of government interactions

3
OECD and Science
  • Meetings of Science Ministers
  • Megascience Forum ? Global Science Forum
  • Considers multi-national large science projects
  • E.g. Structural Genomics, Proton beams, Laser
    pulses

4
OECD and Radio Astronomy
  • Working Group on Radio Astronomy
  • Report in 1998 adopted by ministers 1999
  • Large new facilities mm arrays (ALMA?) and cm
    large array (SKA?)
  • Identified threat to RAS from satellite
    down-links
  • ? New task force to address this issue

5
Task Force on Radio Astronomy and the Radio
Spectrum
  • High level informal group
  • Satellite people Radio Astronomers Spectrum
    management
  • Terms of reference document
  • Ron Ekers, Harvey Butcher, Tom Gergely,

6
Objectives
  • The Task Force should produce a brief,
    policy-level report that contains findings and
    action-oriented recommendations.
  • It is recognised that the ultimate resolution of
    this difficult problem could take many years, but
    the deliberations of the Task Force should lead
    to the initiation of appropriate activities in
    the near future.

7
Scope
  •  Technological solutions Radio astronomers and
    industry representatives could identify and
    jointly implement interference mitigation
    schemes.
  • Regulation If new, innovative ways of sharing
    the radio spectrum are to be found, the
    appropriate discussions must begin soon within
    national agencies and the ITU, as the
    implementation of new regulations usually
    requires a considerable amount of effort over
    several years.
  • Radio-quiet zones Remote areas on the Earth's
    surface could be designated where future radio
    observatories could be located, and where radio
    emissions, especially from spaceborne and
    airborne sources, would be restricted in
    frequency and time. The technical, regulatory,
    and legal dimensions of this concept would have
    to be carefully examined.

8
Work Program
  • A.     To investigate in detail the three-pronged
    approach indicated above, and to propose specific
    programs that will constitute a balanced,
    co-ordinated strategy. B.     To sound out
    members of their respective spheres of interest
    about the elements of acceptable regulatory and
    other solutions, and about their willingness to
    participate in achieving those solutions.C.    
    To develop a road map of long-term solutions,
    with a time schedule and milestones, for
    consideration by the relevant national and
    international bodies. Special attention should be
    given to taking advantage of (and strengthening)
    the procedures of the ITU.

9
Possible SKA configuration
10
SKA LocationWA Radio Quiet Reserve
  • RFI measurement system
  • Funded by WA state government
  • First results march-April 2001
  • 30-150 MHz
  • 1060-1800 MHz
  • Site comparison 2002
  • Noise floor gt 30db ITU
  • IMS under construction

11
Task Force outcomes?
  • Draft report NOT public
  • Will be presented to ministers in near future
  • Expectations
  • - some mechanisms for quiet zones
  • - proposals to go to ITU (WRC06?) via IUCAF
    or administrations
  • - NO weakening of current ITU protection for
    RAS.
  • - mitigation effort?
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