30TH INTERNATIONAL COSMIC RAY CONFERENCE Experimental Details and Calibration of The FLASH Thin Target Experiment
نویسنده
چکیده
The thin target mode of the FLASH (Fluorescence in Air from Showers) experiment was conducted at SLAC. The aim was to measure the total and spectrally resolved fluorescence yield of charged particles traveling through air to better than 10%. The setup consisted of a 15.24 cm thick gas volume which was viewed by two PMT detectors each equipped with 15 remotely interchangeable narrow band filters to measure the fluorescence spectrum between 300 and 430 nm. Final results of the FLASH experiment will be presented in a talk at this conference. The calibration of the experimental setup is crucial in minimizing the systematic uncertainty of the measurement. We will describe how the physics of Rayleigh scattering is used to derive an absolute end-to-end calibration of the experiment from first principles. In addition, a method for a relative calibration is presented using a setup with a mercury lamp, a monochromator and a NIST calibrated photo diode in a light sealed black box. Finally, the toroid measuring the beam charge had to be calibrated. The combination of all three measurement uncertainties provided an absolute calibration of the FLASH experiment.
منابع مشابه
30TH INTERNATIONAL COSMIC RAY CONFERENCE Calibration and monitoring of the air fluorescence detector for the Telescope Array experiment
The air fluorescence detectors (FDs) of the Telescope Array (TA) experiment have been constructed in a dessert of Utah, USA. We can measure the longitudinal developments of EASs directly with the FDs by detecting air fluorescence lights and determine the primary energies of ultra-high energy cosmic rays. In order for accurate observation and measurements of EASs, elaborate detector calibrations...
متن کامل30TH INTERNATIONAL COSMIC RAY CONFERENCE Direct Measurements, Acceleration and Propagation of Cosmic Rays
This paper summarizes highlights of the OG1 session of the 30th International Cosmic Ray Conference, held in Merida (Yucatan, Mexico). The subsessions (OG1.1, OG1.2, OG1.3, OG1.4 and OG1.5) summarized here were mainly devoted to direct measurements, acceleration and propagation of cosmic rays.
متن کامل30TH INTERNATIONAL COSMIC RAY CONFERENCE CODALEMA : A Cosmic Ray Radio Detection Array
Extensive air showers are associated with transient radio emission, which could provide a new mode of detection of UHECR with an important target volume and a high duty cycle. The Codalema experiment has been set up and is running in the Radio Observatory in Nancay, France, to investigate this possibility. The apparatus is composed of an antenna array overlapped by a ground particle array. A se...
متن کامل30TH INTERNATIONAL COSMIC RAY CONFERENCE The end of the Galactic spectrum
We use a diffusion galactic model to analyze the end of the Galactic cosmic ray spectrum and its mixing with the extragalactic cosmic ray flux. We analyze the transition between Galactic and extragalactic components using two different extragalactic models. We compare the sum of the diffusive galactic spectrum and extragalactic spectrum with the available experimental data.
متن کامل30TH INTERNATIONAL COSMIC RAY CONFERENCE Study of the performance and capability of the new ultra-fast 2 GSample/s FADC data acquisition system of the MAGIC telescope
In February 2007 the MAGIC Air Cherenkov Telescope for gamma-ray astronomy was fully upgraded with an ultra fast 2 GSamples/s digitization system. Since the Cherenkov light flashes are very short, a fast readout can minimize the influence of the background from the light of the night sky. Also, the time structure of the event is an additional parameter to reduce the background from unwanted had...
متن کاملذخیره در منابع من
با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید
عنوان ژورنال:
دوره شماره
صفحات -
تاریخ انتشار 2008