You are viewing an old version of this page. View the current version.

Compare with Current View Page History

« Previous Version 4 Next »

LAT CU Heavy Ion Beam Test at GSI - Run Plan

Motivations

The CU Beam Test at GSI is part of the general beam test program of the GLAST LAT CU.
The main goal of the program is to support the LAT Instrument Calibration by providing direct measurements of the physical processes taking place in the CU detector when exposed to different beams, by comparing the obtained measurements with Monte Carlo predictions and by eventually validating the full LAT MC code used to provide instrument calibrations and background rejection strategies.

The first part of the program took place at CERN using a variety of different particle beams (e, e+, p, pions, photons) and ranging in energies from tens of MeV up to hundreds of GeV.
The second part of the program exploits the high energy heavy ion beams available at GSI to measure the response of the CU to such radiation. Heavy ions are an important component of primary cosmic rays, and the LAT plans to use them to calibrate the CAL and ACD subsystems during flight operations. Therefore the GSI test is primarily meant to verify the on-orbit calibration procedure for the CAL, which uses also the ACD and TKR subsystems for triggering and tracking.
The CU beam test at GSI is also a first test with heavy ions for the TKR subsystem.

List of topics

Below is a list of specific topics of intereset for the subsystems

TKR: saturation effects from heavy ions on ToT signal, tracking performance, instrument deadtime
CAL: verification of quenching factors (measured at GSI 2003), test on-orbit calibration procedure and code
ACD: verification of CNO trigger, verify ACD dynamic range

General overview of the run

The run at GSI is scheduled between november 15 and november 20, with beam avaialble between november 18 8AM and november 20 8AM.
Installation and debug will take place on november 15, 16, 17.

Below is a table summarizing the standard operating mode agreed with GSI. Specific run conditions can be agreed and must be defined beforehand (see detailed run schedule)

Run period

Operation mode

Ions

Energy

Rate

18/11-8AM 19/11-8PM

daytime, parasitic mode to therapy (approx 20 min irradiation with 20 min break)

C, Xe (few hours overnight, TBC)

1.5GeV/n

O(100)Hz/cm^2

The beam focus can be moved from a few meters upstream the detector down to the CU location, in order to enlarge or squeeze the beam spot. This feature can also be used to decrease/increase particle density.

Trigger considerations

Beam configuration

List of runs

Below is a list of specific run requests. Plese update the table and notify Luca Latronico

Purpose

preferred schedule

Ion

Energy

Rate on CU

Beam focus

CU configuration

Trigger

notes

contact

Test multiple trigger engines prior to beam

nov 16-17

NA

NA

NA

NA

enable multiple trigger engines

CNO, periodic, internal trigger

take runs at different CNO thresholds, periodic trigger frequency

luca

Test multiple trigger engines w beam

nov 18

C

1.5Gev/n

100Hz

any

enable multiple trigger engines

CNO, periodic, internal trigger

take runs at different CNO thresholds, periodic trigger frequency

luca

  • No labels