نتایج جستجو برای: gamma ray spectrometer

تعداد نتایج: 424287  

Journal: :Science 1998
D J Lawrence W C Feldman B L Barraclough A B Binder R C Elphic S Maurice D R Thomsen

Lunar Prospector gamma-ray spectrometer spectra along with counting rate maps of thorium, potassium, and iron delineate large compositional variations over the lunar surface. Thorium and potassium are highly concentrated in and around the nearside western maria and less so in the South Pole-Aitken basin. Counting rate maps of iron gamma-rays show a surface iron distribution that is in general a...

Journal: :Osmaniye Korkut Ata Üniversitesi Fen Bilimleri Enstitüsü dergisi 2023

In the present work, gamma-ray linear attenuation coefficients (µ) and transmission factors (TF) were measured for Erzurum Ispir dry bean (IDB) Ankara Kızılcahamam (KDB). Photons of Am-241 point source with an energy 59.54 keV, Energy Dispersive X-Ray Fluorescence Spectrometer (EDXRFS), a Si (Li) detector used in experiment. As result, it was observed that average factor İspir dried beans highe...

1999
D. S. McGregor M. Blakely

A new detector geometry is described with relatively high gamma ray energy resolution at room temperature. The device uses the geometric weighting effect, the small pixel effect and the Frisch grid effect to produce high gamma ray energy resolution. The design is simple and easy to construct. The device performs as a gamma ray spectrometer without the need for pulse shape rejection or correctio...

2001
Larry G. Evans Richard D. Starr Johannes Brückner Robert C. Reedy William. V. Boynton Jacob I. Trombka John O. Goldsten Jozef Masarik Larry R. Nittler Timothy J. McCoy

Elemental composition and composition ratios derived from gamma-ray measurements collected by the NEAR-Shoemaker spacecraft while on the surface of 433 Eros are reported. Performance of the gamma-ray spectrometer (GRS) during cruise and orbit is reviewed. The best gamma-ray data were collected on the surface of Eros after the spacecraft’s controlled descent on 12 February 2001. Methods used in ...

2008
R. Murphy

Gamma-ray and neutron emissions from solar flares carry information about the flaring process and conditions within the flaring magnetic loop. Extraction of this information from solar flare measurements requires an ionacceleration, transport, and interaction model with parameters directly related to those physical processes. In this paper we describe such a magnetic-loop model. Each of the gam...

2000
C. J. Lister

This paper presents new results obtained using the U.S. national gamma-ray facility Gammasphere, which has been operating at the ATLAS accelerator at Argonne National Laboratory since January 1998. Gammasphere was built at Lawrence Berkeley Laboratory and used primarily as a powerful spectrometer for studying nuclei at the highest spins [1].

1999
P. Jean J. Gómez - Gomar M. Hernanz J. José J. Isern G. Vedrenne P. Mandrou V. Schönfelder G. G. Lichti R. Georgii

The shield of the INTEGRAL spectrometer provides a large detection area with a wide field-of-view. Calculations have been performed to check whether the temporal analysis of the counting rate of the SPI anticoincidence allows the detection of explosions of novae. The background rate of the shield as well as its response to gamma-ray have been modelled with

Journal: :Geology, Geophysics and Environment 2021

Portable EDXRF (Energy Dispersive X-Ray Fluorescence) spectrometer with the ability to perform rock tests in a helium atmosphere was applied prepare unique calibration coefficients and mineralogical models. These data could be used for chemical profiling, chemostratigraphy, gamma-ray, TOC lithological interpretation of borehole geological profile. The measurements were conducted on 19 samples s...

2003
P. Jean J. Knödlseder V. Lonjou M. Allain J. - P. Roques G. K. Skinner B. J. Teegarden G. Vedrenne P. von Ballmoos B. Cordier R. Diehl Ph. Durouchoux P. Mandrou J. Matteson N. Gehrels V. Schönfelder A. W. Strong P. Ubertini G. Weidenspointner C. Winkler

We report the first measurements of the 511 keV line emission from the Galactic Centre (GC) region performed with the spectrometer SPI on the space observatory INTEGRAL (International Gamma-Ray Astrophysics Laboratory). Taking into account the range of spatial distribution models which are consistent with the data, we derive a flux of 9.9

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