# Signal Monitoring and Analysis

## Monday, February 12, 2018

### Kalman filter position solution for the KiwiSDR

This is work in progress, updates can be found
here on GitHub.

## Wednesday, January 24, 2018

### Using an extended Kalman filter for TDoA HF geo-location

In this post the precision of geo-location using TDoA on shortwave is explored using the data shown here before.

The idea is to feed the time series of time differences into an extended Kalman filter (EKF) using two models for the propagation time from the transmitter to the receiver:

1) Simple ray-geometry for oblique propagation in the ionosphere:

All receiver coordinates are assumed to be in WGS84, however in practice it is suspected that there are deviations from the true locations of up to 20 km, as the KiwiSDR positions are provided by the KiwiSDR owners and are not taken from the GPS position solutions used for time synchronization.

The plot below shows the output of the EKF

The simple ionosphere propagation model improves the match to the known position but there is still a remaining bias of about 30km North, 4km West. Clearly, more studies are needed in order to find out if this improvement is by chance or real.

The idea is to feed the time series of time differences into an extended Kalman filter (EKF) using two models for the propagation time from the transmitter to the receiver:

1) Simple ray-geometry for oblique propagation in the ionosphere:

- based on arXiv:1104.2248 which uses the Breit and Tuve + Martyn theorems to convert vertical to oblique incidence
- using vertical electron density profiles from the IRI2016 model as an input
- group refractive index: 1/sqrt(1-f
_{N}^{2}/f^{2}), i.e., no magentoionic effects are taken into account - when integrating over the group refractive index in the vertical direction, analytic integration of 1/sqrt(f(h)) is performed in each height interval in order to avoid the spurious numerical singularity at the reflection point
- spherical coordinates are used (r
_{E}=6371km)

2) Alternatively, great-circle distances on the WGS84 ellipsoid are used:

- geographiclib adapted for octave

All receiver coordinates are assumed to be in WGS84, however in practice it is suspected that there are deviations from the true locations of up to 20 km, as the KiwiSDR positions are provided by the KiwiSDR owners and are not taken from the GPS position solutions used for time synchronization.

The plot below shows the output of the EKF

- implementation in octave following ADA285972
- state = [lat, lon] of the unknown position
- measurements = time differences between pairs of KiwiSDRs
- the measurements covariance matrix (constant) is build from the covariances of time differences (and is set to zero for time differences not sharing a common receiver)
- state covariance matrix = diag(0.01, 0.01)
^{2}deg^{2}(constant) - start covariance = diag(0.1, 0.1)
^{2}deg^{2} - there are about 60 measurements which are run 5 times sequentially through the EKF

Extended Kalman Filter (EKF) output; note that the range of the x(y) axis corresponds to approximately 17(67)km. |

The simple ionosphere propagation model improves the match to the known position but there is still a remaining bias of about 30km North, 4km West. Clearly, more studies are needed in order to find out if this improvement is by chance or real.

## Thursday, January 18, 2018

### Cyprus OTHR

Yesterday I found the OTHR from Cyprus operating with 25 Hz pulse repetition rate and μ=500kHz/s sweep rate. The most likely geo-location is just north of the known location:

I was thinking about an alternative way of geo-location using an extended Kalman filter, and found this reference: www.dtic.mil/dtic/tr/fulltext/u2/a285972.pdf. It is written very well and I was able to implement it quickly in octave using dfpdp from the optim toolbox for the Jacobian. More on this later.

TDoA plots 17030 kHz 20180113T1126Z |

Cross-correlations 173030 kHz 20180113T1126Z |

## Wednesday, January 17, 2018

### OTHR on 6950 kHz

TDoA maps 6950 KHz 20180112T2138Z |

Cross-correlations 6950 kHz 20180112T2138Z |

abs(z) vs. time 6950 kHz 20180112T2138Z |

## Friday, January 5, 2018

### De-chirping applied to a HF over the horizon radar signal (2)

This is a follow up to this blog post. Again the signals of the OTHR in Cyprus were analyzed using GPS time-stamped IQ samples from several KiwiSDRs.

In this case the OTHR signal was found between 13965 and 13985 kHz. The slope of the FMCW signal is μ=1MHz/s, and there are 50 sweeps per second. This results in a bandwidth of about 20kHz.

As is well known, the frequencies Δf of the spectrum of the de-chirped signal correspond to time delays τ=-Δf/μ in the case of a stationary target.

Plots for 5 KiwiSDR are shown below. The splitting of the ionospheric reflection is most likely due to O- and X-mode propagation in the F layer.

Thanks to all KiwiSDR owners who make their receivers available and do connect a GPS antenna.

In this case the OTHR signal was found between 13965 and 13985 kHz. The slope of the FMCW signal is μ=1MHz/s, and there are 50 sweeps per second. This results in a bandwidth of about 20kHz.

As is well known, the frequencies Δf of the spectrum of the de-chirped signal correspond to time delays τ=-Δf/μ in the case of a stationary target.

- for this one has to multiply the received signal with the original waveform
- tuning offsets w.r.t. center frequency of the OTHR signal correspond to a time delay of the original waveform
- when Δf is positive the delay corresponds to the frequency Δf-f
_{s}(f_{s}is the sampling frequency), i.e. the ranges wrap around the x-axis.

_{d}vs. Δf where f_{d}= v•λ/2 (for velocity v and wavelength λ). Here one has to be careful to adjust the phases in each bin to correct for the fact that the sampling times are not exactly aligned to multiples of 0.02 seconds.Plots for 5 KiwiSDR are shown below. The splitting of the ionospheric reflection is most likely due to O- and X-mode propagation in the F layer.

13975 kHz 20180105T1114Z @CS5SEL; the band at f_{d}=0 is caused by an interference |

13975 kHz 20180105T1114Z @DF0KL |

13975 kHz 20180105T1114Z @G8JNJ |

13975 kHz 20180105T1114Z @Izhvesk |

13975 kHz 20180105T1114Z @Julisdalen |

## Sunday, December 17, 2017

### TDoA measurements using GPS time-stamped IQ samples from KiwiSDRs (8)

Today I picked up a HF radar signal on 13500+-20 kHz. These are the time-differences between four KiwiSDRs:

This is most likely the Calypso CODAR radar system:

Within the TDoA resolution the three sites in Ta'Sopu (Gozo), Ta'Barkat (Malta) and Pozzallo Harbour (Sicily) cannot be distinguished.

It is still puzzling for me that the TDoA maps seem to provide reasonable results, as for now great-circle distances are used, i.e., delays due to skywave propagation are not taken into account.

TDoA 13490 kHz |

This is most likely the Calypso CODAR radar system:

TDoA maps for 14390 kHz |

It is still puzzling for me that the TDoA maps seem to provide reasonable results, as for now great-circle distances are used, i.e., delays due to skywave propagation are not taken into account.

## Thursday, December 14, 2017

### De-chirping applied to a HF over the horizon radar signal

Here is another look at the HF OTHR signal from Cyprus already mentioned in this blog post.

This OTHR signal is (at least to 1st order) FMCW modulated (period 0.02 sec, bandwidth 20kHz), as can be seen in the FM demodulated phase which follows a sawtooth pattern with period 0.02 sec.

Although the bandwidth of the KiwiSDR IQ data stream is smaller than the bandwidth of the OTHR signal it turns out that de-chirping can be done: using KiwiSDR GPS time-stamps t, de-chirping can be implemented by multiplying the IQ samples by exp(-2i*pi*f(t)) with f=@(x) 0.5*1e6*(mod(x,0.02)-0.01).**2-50; (this is octave notation)

The de-chirped signal looks like in the bottom panel below and is flat as expected:

OTHR FM demodulated phase; bottom: de-chirped |

The relative range (which includes a contribution from the doppler effect, see, e.g., here) is then obtained by performing a FFT transformation on the de-chirped signal in each 0.02 sec period (~240 samples):

OTHR de-chirped spectrum vs. time |

- There is a main reflection in the ionosphere which has an interesting, time-varying structure to the left of it, i.e., towards smaller ranges
- In the light blue regions there is a kind of digital pattern visible; this might be due to the signal processing and limited bandwidth of the KiwiSDR but it could also be caused by some additional modulation of the radar signal

Subscribe to:
Posts (Atom)