Environment
13 institutions, over 100 people, over 10 contries.
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 DC & STAR detectors;
developing 2D Kalman filter for NOMAD-STAR;
vertex reconstruction in NOMAD-STAR detector;
event display for NOMAD-STAR;
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 based interface and Ci interpreter (
LAL software). I also performed a MC simulation of passive (Pb) target for neutrino trident production.
Notes
I was worked in large international collaboration (over 100 people were involved in this project). Source code was developed on different platforms, then tested and updated on main server using CVS system.
Automatic update of NOMAD database and source code on local client site was established.
A local Linux cluster at JINR was used for code development, run production and data analysis.
Picture gallery


NOMAD detector 3D view NOMAD detector top view NOMAD-STAR prototype

NOMAD detector NOMAD numu event NOMAD event (3D view)



1999 © Designed by
V.E.Kuznetsov