Electronics for Calorimeters at LHC

Some principal design features of front-end electronics for calorimeters in experiments at the LHC will be highlighted. Some concerns arising in the transition from the research and development and design phase to the construction will be discussed. Future challenges will be indicated. (4 refs)

Strontium and calcium in foodstuffs

U referatu je dat općeniti pregled načina kontaminacije biljaka radioaktivnim elementima. Posebna pažnja posvećena je kontaminaciji biljaka radioaktivnim stroncijem. Interpretirani su rezultati analize nekih prehrambenih artikala biljnog porijekla i stočne hrane.In 1962 and 1963 determination of Sr-90 and Ca in some foodstuffs and fodder of vegetable origin was carried out. Analysis of the results obtained has led to the following conclusions: 1. Grass (hay, lucerne) is for the most part contaminated by surface contamination. 2. The degree of surface contamination of hay and lucerne is comparatively higher in spring than in summer vegetation owing to a higher radioactive fallout in spring. 3. The activity of lucerne is somewhat lower than the activity of hay because the roots of lucerne go deeper into the soil and are therefore less exposed to indirect contamination. 4. The plants with a lower Ca content take a proportionately lower content of Sr-90 from the soil. This is extremely important for the articles contaminated through the soil, because the amount of strontium and calcium taken by the plant from the soil is in an approximate relation to the amount of these elements dissolved in the soil

Sensor Development for the Large Synoptic Survey Telescope.

The Large Synoptic Survey project proposes to build an 8m-class ground-based telescope with a dedicated wide field camera. The camera consists of a large focal plane mosaic composed of multi-output CCDs with extended red response. Design considerations and preliminary characterization results for the sensors are presented in this contribution to the Workshop

Towards Precision LSST Weak-Lensing Measurement - I: Impacts of Atmospheric Turbulence and Optical Aberration

The weak-lensing science of the LSST project drives the need to carefully model and separate the instrumental artifacts from the intrinsic lensing signal. The dominant source of the systematics for all ground based telescopes is the spatial correlation of the PSF modulated by both atmospheric turbulence and optical aberrations. In this paper, we present a full FOV simulation of the LSST images by modeling both the atmosphere and the telescope optics with the most current data for the telescope specifications and the environment. To simulate the effects of atmospheric turbulence, we generated six-layer phase screens with the parameters estimated from the on-site measurements. For the optics, we combined the ray-tracing tool ZEMAX and our simulated focal plane data to introduce realistic aberrations and focal plane height fluctuations. Although this expected flatness deviation for LSST is small compared with that of other existing cameras, the fast f-ratio of the LSST optics makes this focal plane flatness variation and the resulting PSF discontinuities across the CCD boundaries significant challenges in our removal of the systematics. We resolve this complication by performing PCA CCD-by-CCD, and interpolating the basis functions using conventional polynomials. We demonstrate that this PSF correction scheme reduces the residual PSF ellipticity correlation below 10^-7 over the cosmologically interesting scale. From a null test using HST/UDF galaxy images without input shear, we verify that the amplitude of the galaxy ellipticity correlation function, after the PSF correction, is consistent with the shot noise set by the finite number of objects. Therefore, we conclude that the current optical design and specification for the accuracy in the focal plane assembly are sufficient to enable the control of the PSF systematics required for weak-lensing science with the LSST.Comment: Accepted to PASP. High-resolution version is available at http://dls.physics.ucdavis.edu/~mkjee/LSST_weak_lensing_simulation.pd

Monolithic front-end preamplifiers for a broad range of calorimetry applications

The present paper summarizes the salient results of a research and development activity in the area of low noise preamplifiers for different applications in calorimetry. Design target for all circuits considered here are low noise, ability to cope with broad energy ranges and radiation hardness

Determination of the apparent age of nuclear explosions

Određena je prividna dob nuklearne eksplozije pretpostavljajući da se izmjerena aktivnost od više eksplozija može uzeti kao da je nastala samo od jedne nuklearne eksplozije.The apparent age of a nuclear explosion is determined by a well known formula, assuming the observed activity can be characterized as that resulting from a single nuclear detonation

Optically Based Charge Injection System for Ionization Detectors

An optically coupled charge injection system for ionization based radiation detectors which allows a test charge to be injected without the creation of ground loops has been developed. An ionization like signal from an external source is brought into the detector through an optical fiber and injected into the electrodes by means of a photodiode. As an application example, crosstalk measurements on a liquid Argon electromagnetic calorimeter readout electrodes were performed

Developments of a 2D Position Sensitive Neutron Detector

Chinese Spallation Neutron Source (CSNS), one project of the 12th five-year-plan scheme of China, is under construction in Guangdong province. Three neutron spectrometers will be installed at the first phase of the project, where two-dimensional position sensitive thermal neutron detectors are required. Before the construction of the neutron detector, a prototype of two-dimensional 200 mmx200 mm Multi-wire Proportional Chamber (MWPC) with the flowing gas of Ar/CO2 (90/10) has been constructed and tested with the 55Fe X-Ray using part of the electronics in 2009, which showed a good performance. Following the test in 2009, the neutron detector has been constructed with the complete electronics and filled with the 6atm.3He + 2.5atm.C3H8 gas mixture in 2010. The neutron detector has been primarily tested with an Am/Be source. In this paper, some new developments of the neutron detector including the design of the high pressure chamber, the optimization of the gas purifying system and the gas filling process will be reported. The results and discussion are also presented in this paper.Comment: 5 page