To approach the study of the cosmic rays in the energy range E > 10 20 eV, the upper end of the spectrum observed to date, with a large statistical significance (103 events/year), and hence address the solution of several astrophysical and cosmological problems related to their existence and behaviour, a new generation of experiments will probably have to be conceived and realised. They will be based on the observation and measurements of cosmic rays from space. The extremely low rate of these events (∼ 1 event/(century × km2 × sr)) imposes a very large effective area to be monitored, of the order of 105km2, as an observational requirement to meet the target statistics. The Extreme Universe Space Observatory (EUSO) mission has been proposed as the precursor of this new generation of experiments. Its approach consists in fact in looking downwards to the Earth atmosphere by means of a large field-of-view telescope accommodated aboard an orbiting satellite. The fluorescence strike produced by a cosmic ray through the atmosphere will be recorded by the detector, which will reconstruct the kinematical and dynamical features of the primary cosmic ray. The atmosphere acts therefore as an active target for the detectable event. A strategic tool for the success of EUSO as well as for all the experiments of its category will be a correct and detailed atmospheric sounding system, in order to monitor the atmospheric parameters within the field-of-view of the telescope. Beside an on-board measurement by means of dedicated devices such an infrared camera (IR) and possibly a LIDAR (Light Detection And Ranging) coupled to the main instrument, the Atmosphere Sounding will take advantage from the continuous observation of the atmospheric parameters given by the orbiting meteorological satellites. Their databases have thus to be interfaced to the experimental data and used picking-up the relevant data according to the space and time coordinates corresponding to each triggered event. The present work outlines a software module (MARVIN-Multiparametric Advanced Research tool for Visualisation In the Network) able to build-up such an interface, and shows a preliminary implementation of it, using a sample of existing satellites and ISCCP meteorological data collection. It has been developed during the phase A study of the EUSO mission but is general enough to be adapted to different missions observing the Earth atmosphere from space.
Aanzalone, ., D'Ali'Staiti, G., Raimondi, F., M., C., & V., R. (2006). Multi Parametric Advanced Research tool for meteo satellite data interfacing with space observation of Ultra High Energy Cosmic Rays. IL NUOVO CIMENTO DELLA SOCIETÀ ITALIANA DI FISICA. C, GEOPHYSICS AND SPACE PHYSICS, 29(5), 519-528.
|Data di pubblicazione:||2006|
|Titolo:||Multi Parametric Advanced Research tool for meteo satellite data interfacing with space observation of Ultra High Energy Cosmic Rays.|
|Citazione:||Aanzalone, ., D'Ali'Staiti, G., Raimondi, F., M., C., & V., R. (2006). Multi Parametric Advanced Research tool for meteo satellite data interfacing with space observation of Ultra High Energy Cosmic Rays. IL NUOVO CIMENTO DELLA SOCIETÀ ITALIANA DI FISICA. C, GEOPHYSICS AND SPACE PHYSICS, 29(5), 519-528.|
|Digital Object Identifier (DOI):||http://dx.doi.org/10.1393/ncc/i2006-10010-6|
|Appare nelle tipologie:||1.01 Articolo in rivista|