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authorjaseg <git-bigdata-wsl-arch@jaseg.de>2020-05-13 13:22:17 +0200
committerjaseg <git-bigdata-wsl-arch@jaseg.de>2020-05-13 13:22:17 +0200
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modulation, freq estimation: add some blurb, citations
-rw-r--r--ma/safety_reset.tex71
1 files changed, 48 insertions, 23 deletions
diff --git a/ma/safety_reset.tex b/ma/safety_reset.tex
index 3462740..303b519 100644
--- a/ma/safety_reset.tex
+++ b/ma/safety_reset.tex
@@ -1011,30 +1011,45 @@ controllable load:
\item[Modulation amplitude] proportionally related to modulation power. In a practical setup we might realize a
modulation power up to a few hundred \si{\mega\watt} which would yield maybe a few tens of \si{\milli\hertz} of
frequency amplitude.
- \item[Modulation pre-emphasis and slew-rate control]. Pre-emphasis might be necessary to ensure an adequate SNR at
- the receiver. Slew-rate control and other shaping measures might be necessary to reduce the impact of these
- sudden load changes on the transmitter's primary function (say, aluminium smelting) and to prevent disturbances
- to grid components.
+ \item[Modulation pre-emphasis and slew-rate control]. Pre-emphasis might be necessary to ensure an adequate
+ Signal-to-Noise ratio (SNR) at the receiver. Slew-rate control and other shaping measures might be necessary to
+ reduce the impact of these sudden load changes on the transmitter's primary function (say, aluminium smelting)
+ and to prevent disturbances to grid components.
\item[Modulation frequency]. For a practical implementation a careful study would be necessary to determine an
optimal frequency band for operation. On one hand we need to prevent disturbances to the grid such as through
- excitation of some local or inter-area modes. On the other hand we need to optimize SNR and data rate to achieve
- optimal latency between transmission start and successful reception and to reduce the overall burden on
- transmitter and grid.
+ excitation of some local or inter-area modes. On the other hand we need to optimize Signal-to-Noise ratio (SNR)
+ and data rate to achieve optimal latency between transmission start and successful reception and to reduce the
+ overall burden on transmitter and grid.
\item[Further modulation parameters]. The modulation itself has numerous parameters that are discussed in sec.\
\ref{mod_params} below.
\end{description}
-\section{From grid frequency to a reliable communications channel}
-% FIXME
+\section{From grid frequency to a reliable communication channel}
\subsection{Channel properties}
-% FIXME
+In this section we will explore how we can construct a reliable communication channel from the analog primitive we
+outline in the previous section. Our load control approach to grid frequency modulation leads to a channel with the
+following properties.
+\begin{description}
+ \item[Slow-changing.] Accurate grid frequency measurements need several periods of the mains sine wave. Faster
+ sampling rates can be achieved with more complex specialized synchrophasor estimation algorithms but this will
+ result in a tradeoff between sampling rate and accuracy\cite{belega01}.
+ \item[Analog.] Grid frequency is an analog signal.
+ \item[Noisy.] While stable over long periods of time thanks to Load-Frequency Control\cite{entsoe04} it shows
+ considerable random short-term variations. In addition our modulation amplitude is limited by technical and
+ economic constraints so we have to find a system that will work at poor SNRs.
+ \item[Polarized.] Grid frequency measurements have an inherent sense of \emph{up} (higher frequencies). We can use
+ this in a polarized modulation scheme to encode information without first transmitting some reference signal to
+ establish this polarization.
+\end{description}
\subsection{Modulation and its parameters}
-
\label{mod_params}
+In this section we will consider how to select a good set of parameters for a modulation scheme fitting grid frequency
+modulation.
+
The sensitivity of the grid to oscillation at particular frequencies described above means we should avoid any
modulation technique that would concentrate a lot of energy in a small bandwidth. Taking this principle to its extreme
provides us with a useful pointer towards techniques that might work well: Spread-spectrum techniques. By employing
@@ -1285,12 +1300,12 @@ required precision for manageable averaging times--we would need either a ADC sa
for a reconstruction through interpolated readings an impractically high ADC resolution.
Detail on the inner workings of commercial phasor measurement units is scarce but given their essential role to SCADA
-systems there is a large amount of academic research on such algorithms\cite{narduzzi01,derviskadic01}. A popular
-approach to these systems is to perform a Short-Time Fourier Transform (STFT) on ADC data sampled at high sampling rate
-(e.g. \SI{10}{\kilo\hertz}) and then perform some analysis on the frequency-domain data to precisely locate the strong peak
-around \SI{50}{\hertz}. A key observation here is that FFT bin size is going to be much larger than required frequency
-resolution. This fundamental limitiation follows from the nyquist criterion %FIXME maybe cite? and if we had to process
-an \emph{arbitrary} signal this would highly limit our practical measurement accuracy
+systems there is a large amount of academic research on such algorithms\cite{narduzzi01,derviskadic01,belega01}. A
+popular approach to these systems is to perform a Short-Time Fourier Transform (STFT) on ADC data sampled at high
+sampling rate (e.g. \SI{10}{\kilo\hertz}) and then perform some analysis on the frequency-domain data to precisely
+locate the strong peak around \SI{50}{\hertz}. A key observation here is that FFT bin size is going to be much larger
+than required frequency resolution. This fundamental limitiation follows from the nyquist criterion %FIXME maybe cite?
+and if we had to process an \emph{arbitrary} signal this would highly limit our practical measurement accuracy
\footnote{
Some software packages providing FFT or STFT primitives such as scipy\cite{virtanen01} allow the user to
super-sample FFT output by specifying an FFT width larger than input data length, padding the input data with zeros
@@ -1351,12 +1366,22 @@ resolution and despite numerous distortions.
Published grid frequency estimation algorithms such as \textcite{narduzzi01} or \textcite{derviskadic01} are rather
sophisticated and use a combination of techniques to reduce numerical errors in FFT calculation and peak fitting. Given
that we do not need reference standard-grade accuracy for our application we chose to start with a very basic algorithm
-instead. We chose to use a general approach developed by experimental physicists at CERN that is described by
-\textcite{gasior01}. This approach assumes a general sinusoidal signal superimposed with harmonics and broadband noise.
-Applicable to a wide spectrum of practical signal analysis tasks it is a reasonable first-degree approximation of the
-much more sophisticated estimation algorithms developed specifically for power systems. Some algorithms have components
-such as kalman filters\cite{narduzzi01} that require a phyiscal model. As a general algorithm from \textcite{gasior01}
-does not require this kind of application-specific tuning, eliminating one source of error.
+instead. We chose to use a general approach to estimate the precise fundamental frequency of an arbitrary signal that
+was developed by experimental physicists at CERN and that is described by \textcite{gasior01}. This approach assumes a
+general sinusoidal signal superimposed with harmonics and broadband noise. Applicable to a wide spectrum of practical
+signal analysis tasks it is a reasonable first-degree approximation of the much more sophisticated estimation algorithms
+developed specifically for power systems. Some algorithms have components such as kalman filters\cite{narduzzi01} that
+require a phyiscal model. As a general algorithm from \textcite{gasior01} does not require this kind of
+application-specific tuning, eliminating one source of error.
+
+The \textcite{gasior01} algorithm passes the windowed input signal through a DFT, then interpolates the signal's
+fundamental frequency by fitting a wavelet such as a gaussian to the largest peak in the DFT results. The bias parameter
+of this curve fit is an accurate estimation of the signal's fundamental frequency. This algorithm is similar to the
+simpler interpolated DFT algorithm used as a reference in much of the synchrophasor estimation
+literature\cite{borkowski01}. The three-term variant of the maximum sidelobe decay window often used there is a blackman
+window with parameter $\alpha = \frac{1}{4}$. Analysis has shown\cite{belega01} that the interpolated DFT algorithm is
+worse than algorithms involving more complex models under some conditions but that there is \emph{no free lunch} meaning
+that more complex perform worse when the input signal deviates from their models.
\subsection{Frequency sensor hardware design}
\label{sec-fsensor}