RFI Subtraction with a reference horn - PowerPoint PPT Presentation

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RFI Subtraction with a reference horn

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RFI Subtraction with a reference horn... F. Briggs & M. Kesteven ... RFI not in reference horn. is NOT subtracted ! Non-Toxic. to celestial signals ... – PowerPoint PPT presentation

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Title: RFI Subtraction with a reference horn


1
RFI Subtraction with a reference hornF.
Briggs M. Kesteven
  • illustrations from Parkes Telescope (Jon Bell et
    al.)
  • origins in Int-Mit group at CSIRO ATNF

2
gAS
g1I
Rx
Cross Correlation
3
R F I
4
Reference Antenna
I(t) S ha(t) io(t-ta)
5
Reference Antenna
I
I(f) (S Ga(f) e-i2p taf ) Io(f)
G(f) Io(f)
6
Cross correlation single polarization feed with
2 reference signals
1. Pol A
G1 G4 Io2
3. Ref 1
G3 G4 Io2
4. Ref 2
7
Cross correlation single polarization feed with
2 reference signals
1. Pol A
G1 G4 Io2
C14
3. Ref 1
C34
G3 G4 Io2
4. Ref 2
G1
G1 G4 Io2

G3
G3 G4 Io2
8
Practical Application Auto-Correlation
Spectrometer
Power Spectrum P(f)
S
gA2S2
g12 I2
A/C spectrometer
I
g12 I2
9
Cross correlation single polarization feed with
2 reference signals
1. Pol A
G1 G3 Io2
C13
G1 G4 Io2
C14
3. Ref 1
C34
G3 G4 Io2
4. Ref 2
C13(f) C14(f) C34(f)
A/C Spectrum Contamination
g12 I2
10
Cross correlation dual polarization feed with 2
reference signals
1. Pol A
C13
G1 G3 Io2
2. Pol B
C14
G1 G4 Io2
C23
G2 G3 Io2
C24
G2 G4 Io2
3. Ref 1
C34
G3 G4 Io2
4. Ref 2
11
Raw Dynamic Spectra
Time
12
Pol A
Pol B
frequency
Canceled Dynamic Spectra
Time
Non-Toxic to celestial signals
13
Spectral Domain Contamination the VOLTAGE
spectrum
Estimate g1(f) I(f) X13(f) g3(f) I(f)
Time Domain Contamination
Effectively FIR filter coefficients
14
FIR Coefficients
Delay 0.1ms steps

Time 0.1 sec steps
15
Pol A
Pol B
using Ref. 3
16
Dynamic Pulsar Spectra
Pol. B
Pol. A
Phase
Frequency
17
Cancellation Applied
Dynamic Pulsar Spectra
Pol. B
Pol. A
Phase
Frequency
18
INTEGRATED PULSE PROFILES
Pulse Phase
19
Self-Normalized by Total Power Spectra
Dynamic Pulsar Spectra
Pol. B
Pol. A
Phase
Average Spectra
Frequency
20
VLBI
21
VLBI
Jodrell Bank
Westerbork
22
Power Spectrum at 840 MHz at Jodrell Bank
Cross Correlation Spectrum Jodrell Bank x
Westerbork
1504377
23
Celestial Signal
post- correlation processing .
24
Conclusions
  • complications of multi-path are contained in
  • complex gains G(f)
  • adaptive filtering with correlation functions
  • preserves phase information.
  • equivalent to subtraction of the
    voltage waveform
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