A comparative study of gamma-ray spectrometers with LaBr3(Ce3+) and CeBr3 scintillation crystals for planetary remote sensing applications.
Alexander Kozyrev(Space Research Institute), S. Pospı́šil(Czech Technical University in Prague), В. Н. Швецов(Joint Institute for Nuclear Research), V. I. Tretyakov(Space Research Institute), F. Quarati(Delft University of Technology), Carlos Granja(Czech Technical University in Prague), A.R. Owens, M. L. Litvak(Space Research Institute), A. Malakhov(Space Research Institute), A. Vostrukhin(Space Research Institute), И. Г. Митрофанов(Space Research Institute), Г. Н. Тимошенко(Joint Institute for Nuclear Research), J. Benkhoff(University of Münster), Tomáš Slavíček, Maxim Mokrousov(Space Research Institute), B. N. Bakhtin(Space Research Institute), А. Б. Санин(Space Research Institute), D. V. Golovin(Space Research Institute)
EGUGA
April 1, 2016
Cited by 0
Related Papers
Distribution of Hydrogen in the Near Surface of Mars: Evidence for Subsurface Ice Deposits
|Science|2002|921
Mars Science Laboratory Mission and Science Investigation
|Space Science Reviews|2012|819
An exceptionally bright flare from SGR 1806–20 and the origins of short-duration γ-ray bursts
|Nature|2005|602
Habitability on Early Mars and the Search for Biosignatures with the ExoMars Rover
|Astrobiology|2017|481
Lunar Reconnaissance Orbiter Overview: The Instrument Suite and Mission
|Space Science Reviews|2007|402