INTRODUCTION
CERN is European Organization
for Nuclear Research and it is located near the Geneva, Switzerland.
I've been participating in two neutrino experiments from 1995 till 1999:
NOMAD and
NOMAD-STAR.
NOMAD-STAR experiment
ENVIRONMENT
- 13 institution, over 20 people, 8 countries.
- OSF/1 DEC/alpha workstations, SunOS, Solaris, PC/Linux RedHat 4.2 &
Slackware 3.2.
- 2 working langugages (English & French).
- Duration of experiment: ~2 years,
~14 monthes data taking (day/night shifts),
data analyses 2 years.
SYSTEM ADMINISTRATION
- Installation, support and deployment of NOMAD-STAR software.
Transfering, troubleshooting, debugging of NOMAD/NOMAD-STAR software on
OSF/1 main cluster and RedHat farm. Client support for Linux machines
(environment, library support, graphics, software management).
- Web-support:
An automatic update of internal NOMAD-STAR
Web-site was performed during a full period of time. Update of data samples,
software and access to internal data base were established.
- Data management:
During a whole year data were transfered between
DLT robot storage farm to a local cluster. Approximately 20 Gb/day
were analysed, sorted and transfered (see example of
source code).
- Software support:
Automatic update of NOMAD-STAR software on RedHat Linux client boxes.
Development and support of NOMAD-STAR software. As an example below
you can see one of the modules of installation package for
NOMAD-STAR experiment which was
written in Tcl/Tk:

The code can be found here.
OFF-LINE SOFTWARE
- As of leader of off-line software development group of NOMAD-STAR
experiment I was responsible for data digitization,
hit, track and vertex reconstruction. I was developing
all individual parts of the off-line software. Among them:
- design and implementation of track reconstruction algorithm;
- data decoding and hit digitization;
- track reconstruction and extrapolation;
- developing of 2D Kalman filter for NOMAD-STAR;
- track matching between DC and STAR;
- vertex reconstruction;
- event display for NOMAD-STAR;
- data visualization and analysis.
The code was developed and tested under Unix operation system using
C language and gcc/gdb tools, shell scripting (sh, Tcl/Tk, awk/sed). Event display
was based on OnX/Motif interface and Ci interpreter
(LAL software).
ON-LINE SOFTWARE
- On-line software was developed for direct digitization
of incoming signal from detector in readable format and on-line
data analysis. The stand alone event display was also provided.
My contribution included:
- data decoding;
- setup on-line event display using direct stream of data
from working sub-detectors;
- data analysis.
DATA MANAGEMENT
- I was responsible for transfer, analyse, triggering and backup
of NOMAD-STAR data. My responsibilities included:
- automatic data transfer from central CERN storage facility
(DLT robot tapes) through LAN network;
- data triggering (only 0.5-1% of incoming data where usefull
during a run). Out of 1,000,000 triggers only 10,000 real
events where recordered and analysed;
- pedestals and noise calculation were established automatically
and written to another tapes;
- data access for local users was performed.
PICTURE GALERY
NOMAD EXPERIMENT
ENVIRONMENT
- 13 institutions, over 100 people, over 10 countries.
- OSF/1 DEC/alpha, SunOS, Solaris workstations, PC/Linux RedHat 4.2 &
Slackware 3.2.
- Duration of experiment: ~5 years, ~4 years data taking (day/night shifts).
OFF-LINE SOFTWARE
- I was responsible for track reconstruction. I was developing
some individual parts of the off-line software. Among them:
- track reconstruction in NOMAD-STAR detector;
- track matching and extrapolation among Drift Chambers and STAR detectors;
- developing of 2D Kalman filter for NOMAD-STAR sub-detecotr;
- vertex reconstruction in NOMAD-STAR sub-detector;
- event display for NOMAD-STAR sub-detector;
- data visualization and analysis.
The code was developed and tested under Unix operation system using
C language, shell scripting (sh, Tcl/Tk, awk/sed). Event display
was created using OnX/Motif interface and Ci interpreter
(LAL software). I also performed a MC simulation of passive (Pb) target
for neutrino trident production.
PICTURE GALERY