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Technical RFI Mitigation

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Radio service separation better done as a broader design problem ... Radio Science has outgrown its cm-wave frequency allocations ... – PowerPoint PPT presentation

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Title: Technical RFI Mitigation


1
Technical RFI MitigationSpectrum Management
  • Rick Fisher
  • NRAO

2
RFI Mitigation Research StatusDemonstration
Projects
  • Array Image Processing
  • local interference VLA
  • Parametric Subtraction
  • GLONASS - ATCA Radar - Arecibo
  • Pulse Blanking
  • Radar - Arecibo, GBT, Nancay DME - GBT
  • Post-correlation Subtraction
  • TV repeater - ATCA Sun - Parkes
  • Multi-station Coincidence
  • Various 1200-1800 MHz signals - Arecibo/GBT
  • Adaptive Filtering/Nulling
  • individual satellites - ATA, GBT, ATCA TV
    repeater - Parkes

3
NGC6251, 333 MHz, VLACornwell, Perley, Golap,
Bhatnagar RFI2004
RFI from ABQ glide slope transmitter
Mitigated with all-sky self-cal
4
RFI Mitigation Research StatusDemonstration
Projects
  • Array Image Processing
  • local interference VLA
  • Parametric Subtraction
  • GLONASS - ATCA Radar - Arecibo
  • Pulse Blanking
  • Radar - Arecibo, GBT, Nancay DME - GBT
  • Post-correlation Subtraction
  • TV repeater - ATCA Sun - Parkes
  • Multi-station Coincidence
  • Various 1200-1800 MHz signals - Arecibo/GBT
  • Adaptive Filtering/Nulling
  • individual satellites - ATA, GBT, ATCA TV
    repeater - Parkes

5
RFI Mitigation Research StatusDemonstration
Projects
  • Array Image Processing
  • local interference VLA
  • Parametric Subtraction
  • GLONASS - ATCA Radar - Arecibo
  • Pulse Blanking
  • Radar - Arecibo, GBT, Nancay DME - GBT
  • Post-correlation Subtraction
  • TV repeater - ATCA Sun - Parkes
  • Multi-station Coincidence
  • Various 1200-1800 MHz signals - Arecibo/GBT
  • Adaptive Filtering/Nulling
  • individual satellites - ATA, GBT, ATCA TV
    repeater - Parkes

6
Top Half of Aircraft Navigation Band (DME)
7
Two-hour Integration on GBT, Quasar 0952176with
and without Pulse Blanking
8
RFI Mitigation Research StatusDemonstration
Projects
  • Array Image Processing
  • local interference VLA
  • Parametric Subtraction
  • GLONASS - ATCA Radar - Arecibo
  • Pulse Blanking
  • Radar - Arecibo, GBT, Nancay DME - GBT
  • Post-correlation Subtraction
  • TV repeater - ATCA Sun - Parkes
  • Multi-station Coincidence
  • Various 1200-1800 MHz signals - Arecibo/GBT
  • Adaptive Filtering/Nulling
  • individual satellites - ATA, GBT, ATCA TV
    repeater - Parkes

9
RFI Mitigation Research StatusDemonstration
Projects
  • Array Image Processing
  • local interference VLA
  • Parametric Subtraction
  • GLONASS - ATCA Radar - Arecibo
  • Pulse Blanking
  • Radar - Arecibo, GBT, Nancay DME - GBT
  • Post-correlation Subtraction
  • TV repeater - ATCA Sun - Parkes
  • Multi-station Coincidence
  • Various 1200-1800 MHz signals - Arecibo/GBT
  • Adaptive Filtering/Nulling
  • individual satellites - ATA, GBT, ATCA TV
    repeater - Parkes

10
Adaptive Filtering on TV RFI to Pulsar at Parkes,
680 MHzKesteven, Hobbs, Clement
11
Lessons Learned So Far
  • Considerable processing power required
  • 2x to 10x of no-RFI processing (cost)
  • Greater than 20 dB suppression gets rapidly
    tougher
  • Currently an enthusiasts game
  • Case-by-case solutions
  • Non-expert use will require considerable
    development
  • Observer demand so far is soft
  • Lots of other science to do
  • RFI mitigation requires effort and resources
  • Development ahead of the perceived need
  • Common situation in spectrum management

12
Derivative Thoughts
  • Some types of signals are more harmful than
    others
  • ITU-R R.A.769 is too simplistic, even with
    de-correlation caveats
  • Radio service separation better done as a broader
    design problem
  • Include transmitter, receiver, and temporal
    requirements adaptively
  • Transmitters can know where they are
  • Receivers and transmitters from all services can
    communicate
  • Some types of signals are easier to excise than
    others
  • Radio Science has outgrown its cm-wave frequency
    allocations
  • Much wider bandwidths than R.A. bands below 30
    GHz
  • Need to optimize our protection requirements with
    trade-offs
  • Geography, time, frequency, signal compatibility,
    etc.
  • We dont need or want narrow bands all the time,
    everywhere
  • New set of rules and protocols need to be
    developed
  • Both risks and rewards, but status quo is highest
    long term risk
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