Signal processing algorithms
Signal Processing for
communications and array processing
This program has two related tracks:
- Signal processing for communications
- Array signal processing
Program chairmen: Alle-Jan van der Veen, Geert Leus
Researchers: Alon Amar, Shahzad Gishkori, Hadi Jamali Rad, Sina Maleki,
Raj Thilak Rajan, Yiyin Wang, Tao Wang, Tao Xu, Siamak Yousefi,
Mu Zhou, Dyonisius Ariananda.
Visitors: prof. Ubli Mitra, prof. Amir Leshem.
Mission
Signal processing for communications is an important area within
signal prodcessing, as it covers around 20% of research.
Among many questions, an important one is, how can multiple overlapping
signals be separated? This problem is very relevant in wireless
communications, where signals are overlapping in time, space and
frequency (the 'cocktail party problem'). With multiple antennas and
advanced separation techniques, the capacity and robustness of wireless
links can greatly be improved.
Similar problems are relevant in radio
astronomy, where the sky signals of interest are contaminated by
man-made interference (e.g., communication signals), which need to be
estimated and suppressed. The resulting algorithms are formulated in
terms of linear algebra operations and provide interesting test cases
for embedded system design.
Array signal processing refers both to parallel signal processing of an
array of signals as it occurs in a multiple antennas/receivers
situation, and to the mapping of such algorithms onto parallel hardware
platforms. This topic has great relevance in a number of contexts: the
mobile communication context, separation of airplane transponder
signals using phased antenna arrays, and spatial filtering for radio
telescope arrays.
Topics studied can be classified under "techniques" and "applications".
Techniques
- Estimation and detection theory; statistical signal processing
- Array calibration and beamforming algorithms; source localization
- Performance analysis and bounds
- Distributed processing; optimization techniques
- Sampling and reconstruction theory
- Adaptive signal processing
- Space-time coding; modulation; acquisition, synchronization, tracking
Applications
- CDMA and spread spectrum; multicarrier and OFDM; UWB
- Sensor networks
- MIMO communication; wireless networks
- Radar and sonar signal processing; radio astronomy; geophysics;
remote sensing
Research
In our work, we combine "techniques" with "applications". We work on a
variety of applications, such as sensor networks for the process industry,
a distributed radio telescope in space, an underwater communication system.
Typically, there is a receiver (antenna array) which receives a collection
of transmitted signals, perturbed by a multipath channel that may even be
highly time-varying. The challenge then is to derive algorithms that
estimate the channel and detect the transmitted data.
Our work is theoretical: the development
of new algorithms and the derivation of their performance, as well as
practical: the development of experimental phased array measurement
systems and the verification of the algorithms on the obtained data.
The focus of our work is as follows:
- Smart antenna technology for wireless communications:
This includes research on algorithms for source separation,
equalization and parameter estimation of communication signals,
and application of blind source separation/equalization techniques
to W-CDMA and OFDM.
- Signal processing over time-varying channels:
If the transmitter and/or receiver is moving fast, a large Doppler spread
makes the communication channel time-varying. This occurs in DVB-T
systems (e.g., digital television received in high-speed trains), but
is even more pronounced in acoustic underwater
communication channels. The challenge is to estimate and compensate for
these effects, especially for wideband (OFDM) signals.
- Signal processing for sensor networks:
Distributed sensor systems consist of a large number of nodes with only
local communication capabilities. Challenges include localization of the
nodes, low-power communication protocols, and distributed estimation
algorithms, where local estimates are combined to form global parameters
estimates.
- Signal processing for radio astronomy:
The trend in radio astronomy is to construct large arrays of small
antennas. An example is the LOFAR system, where 13,000 antennas are
distributed over 100 stations in The Netherlands and Germany. In the
future, we will have SKA (square kilometer array, consisting of 1 million
antennas) and OLFAR, a distributed radio telescope in space.
Central issues for us are array calibration, interference cancellation,
and image formation using array processing techniques.
Currently Running Projects
Current multi-AUV systems are far from being capable of fully
autonomously taking over real-life complex situation-awareness
operations. For this, significant advances are
required, involving cooperative and cognitive-based
communications and sonars (low level), Gaussian Process-based
estimation as well as perceptual sensory-motor and learning
motion control (medium level), and learning/cognitive-based
situation understanding and motion strategies (high level).
In the design of the NOPTILUS underwater system, robustness,
dependability, adaptability and flexibility will be emphasised,
especially when it deals with completely unknown underwater
environments and situations "never taught before".
The world radio astronomical community is planning some major new
radio facilities. Foremost among these is LOFAR, constructed largely
within the Netherlands. It is considered THE pathfinder for the
SKA, the Square Kilometre Array, a project supported and led by the
world radio community.
New, larger and more complex radio telescopes
bring new challenges. Foremost among these is the calibration of the
data in order to remove atmospheric and instrumental effects which
corrupt the exceedingly faint signals from cosmic sources. Indeed,
the scientific success of the new generation of radio telescopes will
depend critically on the ability to calibrate the data, and to deliver
'thermal-noise-limited' performance. This project will study signal
processing challenges in calibration, imaging and RFI mitigation,
all tightly related.
The goal of this project is to shift from centralized communication
networks to distributed self-organizing networks where nodes adapt their
procedures (related to spectrum utilization, sensing, information
processing, and localization) based on only local information. To
develop large self-organizing networks we need cognitive radio devices
that are capable of sensing the radio spectrum and adapt accordingly. We
further require energy efficient distributed information processing and
localization algorithms for large sensor networks. The mathematical
tools we want to build on are compressed sampling, convex optimization,
game theory, and linear algebra.
Lithography machines have a fast-moving waferstage; also the mask
is moving. These stages have many sensors used for accurate
positioning. It is desired to connect these sensors wirelessly to
a central controller. However, the aggregate data rate is very
high (over 1 Gbps), and the latency requirements are very tight.
Currently, there are no wireless standards that can accomodate
this.
The D2S2 project aims at developing a framework for programming and
operating distributed sensor systems that can be depended on in
practical application scenarios. To make an experimental approach
feasible, the project focuses on localization and tracking systems in
two scenarios that are very relevant to the Dutch society: traffic
monitoring and control (static setup) and rescue operations by
firefighters and policemen (dynamic setup). A key, innovative feature
of the project is the development and use of an advanced miniaturized
radar sensor that can operate under a wide range of "difficult"
environmental conditions (smoke, fog, etc.) that cannot be handled by
typical localization systems in operation today.
This project will develop and demonstrate the capability to establish an
underwater ad hoc robust acoustic network for multiple purposes with
moving and stationary nodes.
Applications are e.g. surveillance and mine
reconnaissance using autonomous underwater vehicles (AUVs).
A network of underwater nodes should rapidly be deployed in littoral
waters. In this project, we will develop modulation and receiver
techniques for communication over highly time-varying channels.
One of the last unexplored frequency ranges in radio astronomy is the
frequency band below 30 MHz.
Because these frequencies are blocked by the ionosphere,
earth-bound observations would be be severely limited or
impossible. A radio telescope in space would not be hampered
by the earth's ionosphere.
In this project, we aim to design a distributed radio telescope in
space, consisting of a swarm of about 50 nano-satellites flying in a
cloud of 10 to 100 km.
The quality of chemical reactions inside a tank can be improved if we can measure locally parameters such as temperature and flow. To do this, the idea is to throw small (tennis-ball size) units called PEAS into the tank, that make the observations and communicate their findings using UWB (either RF or acoustic) communication. Also the locations of the PEAS need to be measured.
Recently Ended Projects
This SenterNovem project studied how MIMO technology can be employed in
WLAN equipment, now that the 802.11n standard makes WLAN with multiple
antennas ubiquitous. We took an interdisciplinary approach: the multiple
RF chains and ADC chains can become costly and power-hungry.
Using feedback from the digital receiver part, can we design an analog
preprocessing unit to compress the number of antenna signals into fewer
receiver chains? The aim is to obtain better performance than simple
antenna selection.
VICI: Signal processing for communications [2003-2009]
This NWO-sponsored VICI project studied
multi-user, multi-antenna
receiver algorithms for future generation communication systems,
in particular multi-user CDMA (used in UMTS), OFDM (used in WLAN)
and UWB radio. Specific topics are multi-antenna transmission and
space-time coding, and advanced modulation techniques that
facilitate multi-user detection. Applications to radio astronomy
(the LOFAR telescope) were also studied.
VIDI: Communication over time-varying channels [2005-2009]
The NWO-sponsored
VIDI
project considers the problem that Doppler shifts due to
mobility and carrier frequency offsets introduce channel
time-variations.
As a result, some wireless systems can only provide low data rates at
high mobility, e.g., the third generation wireless system UMTS, or
even break down completely at high speeds, e.g., digital video
broadcasting (DVB-T) applications.
To solve these problems, the project proposes an
innovative wireless system design that takes the
time-varying nature of the channel
explicitly into account.
AIR-LINK: UWB impulse-radio communication system [2002-2008]
The objective of AIR-LINK was to design a
communication system using Ultra-Wideband (UWB) technology, which
is using narrow radar-like pulses to transmit data. The advantage
of this is that no carrier modulation/demodulation is needed,
which enables cheaper single-chip solutions. Data rates are
promised to be very high. Another feature is that a large part of
the frequency spectrum below 10 GHz is used, on top of existing
allocations. This is possible because the transmitted energy is
very small. Key issues in the design are synchronization
algorithms, source separation and multi-access interference
mitigation. Our interest is specifically in signal processing for
the physical layer of ad hoc networks that can be constructed
using UWB devices.
UBROAD: Ultra wideband communication and ad hoc networks
[2002-2004]
The U-BROAD project was a 6-th framework EU "STREP" project, on
Ultra High bit rate over copper technologies for broadband
multiservice access (VDSL). The main objective was to develop and
integrate advanced access technologies of true broadband content
over Ethernet based networks to the customer premises. It aimed at
quadrupling the total bandwidth available to the end user. Project
partners were
Metalink,
France Telecom, OTE, Bar-Ilan University (Amir Leshem), and the
University of Crete (Nicholas Sidiropoulos).
Separation of airplane transponder signals [1999-2003]
The goal in this project was to separate
received airplane transponder signals (secondary surveillance
radar or SSR). Especially in Europe, the crowded airspace can lead
to the reception of multiple return frames from different
airplanes, partially overlapping in time and frequency. By
employing a phased antenna array, these frames can be separated
and the information detected. In addition, the direction of the
airplanes can be estimated.
Apart from the derivation of new signal processing
algorithms for this application, we have also developed a
4-channel recording system to obtain actual measurements
using a small phased array mounted on the roof of the EWI
department building.
NOEMI: Nulling obstructing interferers in radio astronomy [1998-2003]
Radio-astronomical observations are increasingly
corrupted by RF interference, and online detection and filtering
algorithms are becoming essential. Examples of interferers are GSM
mobile phones, GPS satellites, and TV signals. In the STW project
NOEMI (with ASTRON), we considered interference mitigation techniques
for the Westerbork Synthesis Radio Telescope array. The approach is
to formulate the astronomical problem in an array signal processing
language, so that elementary algorithms from that field can be
applied. Two topics are considered in detail: calibration of
polarized telescope arrays using new signal processing techniques, and
spatial filtering by subspace estimation and projection. This can be
used to filter out continuously present interferers such as TV
stations. Spatial filtering works better if a good estimate of the
interfering signal is available. Although the telescopes themselves can
be used for this, it is attractive to use a separate antenna for this.
However, a simple omni-directional antenna will not have a sufficiently
good signal to noise power ratio. To improve on this, we have started
to use a 64-element adaptive phased array developed by ASTRON as
reference antenna. The output of the array is a weighted sum of the
elements. By adapting the weights (beamforming), the array can be
pointed at any direction in the sky and give a much better reference
signal.
| 30 Apr 2010 |