wfis
uni lodz
Uniwersytet Łódzki
Wydział Fizyki i Informatyki Stosowanej
Katedra Astrofizyki Wysokich Energii
90-236 Łódź, Pomorska 149, Polska
uni lodz

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Zarejestruj

Prof. UŁ dr hab. Zbigniew Szadkowski


Dyżur: poniedzialek 10.00 - 11.00, czwartek 13.00 - 14.00
Pok: 401 B

Tel: (42)635-56-59
E-mail: zszadkow@kfd2.phys.uni.lodz.pl
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Konferencje

PROGRESS IN ELECTROMAGNETIC RESEARCHES, 22-25 May 2017, St. Petersburg (Russia)

1. RFI filtering in AERA radio-detection of cosmic rays
2. Two-dimensional multiplier-less wavelet trigger for a radio-detection of cosmic rays
3. Optimization of the neural network trigger for a detection of cosmic rays in surface detectors of the Pierre Auger Observatory


PROGRESS IN ELECTROMAGNETIC RESEARCHES, 8-11 August 2016, Shanghai (China)

1. Detection of Neutrino-Induced Air Showers by the Artificial Neural Network FPGA Trigger
2. DCT trigger in a high-resolution test platform for a detection of very inclined showers in the Pierre Auger surface detectors


IEEE REAL TIME CONFERENCE, 5-10 June 2016, Padova (Italy)

1. A hardware implementation of the Levinson routine in a radio detector of cosmic rays to improve a suppression of the non-stationary RFI
2. The Least Mean Squares Adaptive FIR Filter for RFI Suppression in Radio Detectors of Cosmic Rays
3. Detection of Neutrino-Induced Air Showers by the Artificial Neural Network FPGA Trigger
4. Engineering Array Tests of High-Resolution Front End Electronics for Water Cherenkov Air Shower Detectors equipped with Cyclone V
5. DCT trigger in a high-resolution test platform for a detection of very inclined showers in the Pierre Auger surface detectors
6. Adaptive IIR-notch filter for RFI suppression in a radio detection of cosmic rays
7. Two-dimensional wavelet trigger in radio detection of cosmic rays


PIERRE AUGER COLLABORATION MEETING, 6-11 March 2016, Malargüe (Argentina)

1. A hardware implementation of the Levinson routine in a radio detector of cosmic rays to improve a suppression of the non-stationary RFI
2. Adaptive FIR filter using linear prediction implemented in the FPGA with HPS to reduce narrow-Band RFI for radio detection of cosmic rays in the AERA radio stations
3. Adaptive FIR filter using LMS algorithm in a radio detector of cosmic rays to improve a RFI suppression
4. An adaptive IIR filter for RFI suppression in radio detection of cosmic rays


AERA MEETING, 26-27 January 2016, Aachen (Germany)

1. A hardware implementation of the Levinson routine in a radio detector of cosmic rays to improve a suppression of the non-stationary RFI
2. Adaptive FIR filter using linear prediction implemented in the FPGA with HPS to reduce narrow-Band RFI for radio detection of cosmic rays in the AERA radio stations
3. Adaptive FIR filter using LMS algorithm in a radio detector of cosmic rays to improve a RFI suppression
4. An adaptive IIR filter for RFI suppression in radio detection of cosmic rays


PIERRE AUGER COLLABORATION MEETING, 11-17 November 2015, Malargüe (Argentina)

1. Field results from Front-End Board with Cyclone V
2. Technical Board - Discussion / decision on installing extra solar panel on EA tanks


AUGERPRIME WORKSHOP, 24-25 September 2015, Karlsruhe (Germany)

Tests with Lodz FE,


FEDERATED CONFERENCE ON COMPUTER SCIENCE AND INFORMATION SYSTEMS, Sept. 13-16, Lodz (Poland)

1. Artificial Neural Network as the FPGA trigger in the Cyclone V based Front-End for a Detection of Neutrino-Origin Air Showers in the Pierre Auger Engineering Array
2. First results from the spectral DCT trigger implemented in the Cyclone V Front-End Board used for a detection of very inclined showers in the Pierre Auger surface detector Engineering Array


ADVANCEMENTS IN NUCLEAR INSTRUMENTATION MEASUREMENT METHOTHS AND THEIR APPLICATIONS, Apr. 20-24, Lisbon Congress Center (Portugal)

1. Adaptive FIR Filter Using Linear Prediction Implemented in the FPGA with HPS to Reduce Narrow-Band RFI for Radio Detection of Cosmic Rays in the AERA radio stations
2. DCT trigger for horizontal old showers + Neural network trigger for young showers + Front-End for Auger-Beyond-2015


PIERRE AUGER UPGRADE MEETING, IPN-Orsay, 3-6 February 2015, Salle des conseils, IPN, Bat. 100 (France)

Cyclone V Front-End for SDE-Upgrade


PIERRE AUGER COLLABORATION MEETING 2014, Nov. 16-21, Malargüe (Argentina)

1. An optimization of the FPGA based wavelet trigger in radio detection of cosmic rays
2. Prototype of the Front-End Board with Cyclone V as a Test High-Resolution Platform for the Auger_Beyond_2015 Front End Electronics
3. FPGA/NIOS Adaptive FIR Filter Using Linear Prediction Implemented in the AERA Radio Stations to Reduce Narrow-Band RFI for Radio Detection of Cosmic Rays
4. FE with high frequency readout (Technical Board)


AERA MEETING 2014, Sep. 18-19, Wuppertal (Germany)

First results from the FPGA/NIOS Adaptive FIR Filter Using Linear Prediction Implemented in the AERA Radio Stations to Reduce Narrow Band RFI for Radio Detection of Cosmic Rays


IEEE REAL-TIME CONFERENCE 2014, May 26-30, Nara (Japan)

1. First results from the FPGA/NIOS Adaptive FIR Filter Using Linear Prediction Implemented in the AERA Radio Stations to Reduce Narrow Band RFI for Radio Detection of Cosmic Rays
2. Front-End Board with Cyclone V as a Test High-Resolution Platform for the Auger_Beyond_2015 Front End Electronics
3. Artificial Neural Network as a FPGA Trigger for a Detection of Very Inclined Air Showers
4. An Optimization of the FPGA Based Wavelet Trigger in Radio Detection of Cosmic Rays


33rd INTERNATIONAL COSMIC RAY CONFERENCE 2013, July 01-10, Rio de Janeiro (Brazil)

1. Analysis of the efficiency of the spectral DCT trigger in arrays of surface detectors
2. Analysis of the efficiency of the filters suppressing the RFI being developed for the extension of AERA
3. FPGA Based Wavelet Trigger in Radio Detection of Cosmic Rays


AERA++ Meeting, 2013, Feb. 01-02, Nijmegen (Holland)

1. The new Front-End Board for AERA++ based on the Cyclone V SoC FPGA
2. Cooperation of the FPGA FIR filter with the external ARM microcontroller in the AERA radio stations


ASPERA AugerNext Progress Meeting, 2013, Jan. 29-30, Karlsruhe (Germany)

1. Adaptive FIR Filter Using Linear Prediction Implemented in the AERA Radio Stations
2. FPGA Based Wavelet Trigger in Radio Detection of Cosmic Rays


SURFACE DETECTOR ELECTRONICS WORKSHOP 2013, Jan. 21-22, Orsay (France)

The new Front-End Board for the surface detector based on the Cyclone V for the Auger-Beyond-2015


AERA MEETING 2012, Oct. 10-11, Paris (France)

1. FPGA/NIOS Implementation of an Adaptive FIR Filter Using Linear Prediction to Reduce Narrow-Band RFI for Radio Detection of Cosmic Rays
2. FPGA implementation of the 32-point DFT for a wavelet trigger in cosmic rays experiments


SURFACE DETECTOR ELECTRONICS WORKSHOP 2012, Oct. 8-9, Paris (France)

Proposal of the new Front-End Board


FEDERATED CONFERENCE ON COMPUTER SCIENCE AND INFORMATION SYSTEMS 2012, Sept. 9-12, Wrocław (Poland)

An Optimization of the FPGA Based Wavelet Trigger in Radio Detection of Cosmic Rays


IEEE REAL-TIME CONFERENCE 2012, June 11-15, Berkeley (California)

1. Prototype trigger and readout-electronics built on unified Altera® platform for underground muon counters triggered by surface detectors
2. Optimization of the Detection of Very Inclined Showers Using a Spectral Trigger Based on the Discrete Cosine Transform in Arrays of Surface Detectors
3. FPGA/NIOS implementation of an adaptive FIR filter using linear prediction to reduce narrow-band RFI for radio detection of cosmic rays


PIERRE AUGER COLLABORATION MEETING 2011, Nov. 13-18, Malargüe (Argentina)

1. Proposal of the spectral trigger based on the Discrete Cosine Transform
2. AMIGA – Altera® platform


32nd INTERNATIONAL COSMIC RAY CONFERENCE 2011, Aug. 11-18, Beijing (China)

Trigger based on the Discrete Cosine Transform for new ground EAS arrays


PIERRE AUGER COLLABORATION MEETING, 2011, March 6 – 11, Malargüe (Argentina)

Proposal of the spectral trigger based on the Discrete Cosine Transform


17th IEEE REAL TIME CONFERENCE 2010, May 24-28, Lisbon (Portugal)

1. The prototype of 4th generation single FPGA Front-End Boards with 100 MHz sampling for Auger surface detectors
2. Triggers, data flow and the synchronization between the Auger surface detector and the AMIGA underground muon counters
3. An FPGA based trigger and RFI filter for radio detection of cosmic rays


AERA MEETING 2010, Feb. 2-3, Groningen (Holland)

Prototype for a real time digital self trigger for radio detection


31st INTERNATIONAL COSMIC RAY CONFERENCE 2009, July 7-15, Łódź (Poland)

1. Spectral FPGA triggers for detection of very inclined showers in the surface detectors of the Pierre Auger Observatory
2. A prototype of 100 MHz sampling 1st level surface detector trigger based on a single Cyclone™ III FPGA
3. Triggers, data flow and the synchronization between the Auger surface detector and the AMIGA underground muon counters


AUGER RADIO WORKSHOP 2009, Jan. 27-28, Nijmegen (Holland)

Prototype for a real time digital self trigger for radio detection


IEEE NUCLEAR SCIENCE SYMPOZIUM 2008, Oct. 19-25, Dresden (Germany)

An optimization of 16-point Discrete Cosine Transform implemented into a FPGA as s design for a spectral 1st level surface detector trigger in the Pierre Auger Observatory


PIERRE AUGER COLLABORATION MEETING 2008, May 10-16, Lamar (Colorado)

1. Discrete Cosine Transform as the spectral 1st level surface detector trigger in the Pierre Auger Observatory
2. Pedestal processing


AUGER NORTH MEETING 2008, March 13-18, Paris, France

4th generation of the 1st level trigger with 100 MHz sampling


30th INTERNATIONAL COSMIC RAY CONFERENCE 2007, July 3-11, Merida (Mexico)

1. 16-point DCT as the spectral 1st level SD trigger in the Pierre Auger Observatory
2. 4th generation of the 1st level surface detector trigger in the Pierre Auger Observatory
3. Sigma – Delta compensation of pedestals in the 1st level surface detector trigger of the Pierre Auger Observatory


XXth IEEE-SPIE JOINT SYMPOZIUM ON PHOTONICS, WEB MASTERING, ELECTRONICS FOR ASTRONOMY AND HIGH ENERGY PHYSICS EXPERIMENTS 2007, May 21-27, Wilga (Poland)

Triggers for the Pierre Auger Observatory


PIERRE AUGER COLLABORATION MEETING 2007, April 22-28, Malargüe (Argentina)

A single FPGA 100 MHz sampling Front End for Infill Array


AUGER NORTH DESIGN REPORT MEETING 2007, February 26 – 28, Karlsruhe (Germany)

A single chip 100 MHz sampling Front End for Auger North


DEUTSCHE PHYSIKALISCHE GESELLSCHAFT 2006, March 28-31, Dortmund (Germany)

Implementation of a FPGA based 16-point Discrete Fourier Transform (Radix-2 FFT) as UHECR trigger for horizontal air showers in the Pierre Auger Observatory surface detector


AUGER NORTH MEETING 2006, February 9 – 10, Boulder (Colorado - USA)

Front End and Triggers in Auger North


29th INTERNATIONAL COSMIC RAY CONFERENCE 2005, August 3 – 10, Pune (India)

16-point Discrete Fourier Transform based on the Radix-2 FFT algorithm implemented into Cyclone FPGA as the UHECR trigger for horizontal air showers


CRITICAL DESIGN REVIEW OF THE CYCLONE DESIGN 2005, June 9, Orsay (France)

3rd generation of the 1st level SD trigger based on the Altera Cyclone FPGA


DEUTSCHE PHYSIKALISCHE GESELLSCHAFT 2005, March 4-9, Berlin (Germany)

First Level Surface Detector Trigger in the Pierre Auger Observatory


AUGER UPGRADE MEETING 2005, February 25 – 27, Karlsruhe (Germany)

Cyclone for Auger North


PIERRE AUGER COLLABORATION MEETING 2004, July 21-25, Leeds (UK)

Cyclone status - updated


AUGER NORTH MEETING 2004, June 20, Orsay (France)

Cyclone status


DEUTSCHE PHYSIKALISCHE GESELLSCHAFT 2004, March 29 – April 4, Mainz (Germany)

A Proposal Of A Single Chip Surface Detector Trigger Based On Altera Cyclone Family


PIERRE AUGER COLLABORATION MEETING 2003, Nov. 14 – 19, Malargüe (Argentina)

Proposal of the 3rd generation of the 1st level SD trigger


IEEE NUCLEAR SCIENCE SYMPOSIUM 2003, Oct. 21 – 28, Portland (Oregon – USA)

The PLD First Level Surface Detector Trigger for the Pierre Auger Observatory


28th INTERNATIONAL COSMIC RAY CONFERENCE 2003, July 31 – August 7, Tsukuba (Japan)

The Surface Detector Trigger for the Pierre Auger Observatory


PIERRE AUGER COLLABORATION MEETING 2002, April 19-24, Malargüe (Argentina)

ACEX cost-effective 1st level SD trigger


SURFACE DETECTOR ELECTRONIC WORKSHOP 2001, March 21-23, FermiLab (USA)

PLD vs. ASIC - 1st level SD trigger


SURFACE DETECTOR ELECTRONIC CRITICAL DESIGN REVIEW 2001, Dec 13-14, Orsay (France)

Cost-effective ACEX PLD 1st level SD trigger”


PIERRE AUGER COLLABORATION MEETING 2001, Nov. 12-17, Malargüe (Argentina)

PLD 1st level SD trigger


SURFACE DETECTOR ELECTRONIC WORKSHOP 2001, Sept. 17-19, Orsay (France)

PLD 1st level SD trigger


PIERRE AUGER COLLABORATION MEETING 2000, Nov. 13-18, Malargüe (Argentina)

Proposal of the PLD 1st level SD trigger


SURFACE DETECTOR ELECTRONIC WORKSHOP 2000, April 21 – 22, FermiLab, Batavia (Illinois – USA)

Proposal of the 1st level trigger based on the Altera APEX PLD chip


SPECIAL MINI-REVIEW IN MICHIGAN TECH 2000, March 17, Houghton (Michigan - USA)

1st level SD trigger


PIERRE AUGER COLLABORATION MEETING 1999, Nov. 14-19, Malargüe (Argentina)

1st level SD trigger


MORELIA PIERRE AUGER COLLABORATION MEETING 1999, Jan. 15 – 25, Morelia (Mexico)

2nd level trigger in the fluorescence detector