ÚTEFČVUT Ústav technické a experimentální fyziky ČVUT v PrazeInstitute of Experimental and Applied Physics, CTU in Prague

Coralco: Cosmic rays - light, compact & low-cost device for the real-time radiation environment measurement in the atmosphere and stratosphere

NázevTitle
Coralco: Cosmic rays - light, compact & low-cost device for the real-time radiation environment measurement in the atmosphere and stratosphereCoralco: Cosmic rays - light, compact & low-cost device for the real-time radiation environment measurement in the atmosphere and stratosphere
Druh výsledkuResult type
Příspěvek ve sborníkuProceedings paper
AutořiAuthors
J. Urbář, J. Scheirich, J. Jakůbek, R. Švarc, K. Doubner
Klíčová slovaKeywords
cosmic ray, Medipix, space weather, atmospheric phenomena, stratospheric balloon platform, BEXUS (Balloon Experiments for University Students)
KonferenceConference
61st International Astronautical Congress 2010 (IAC 2010) (Praha, 2010-09-27)
Časopis / citaceJournal / citation
In: 61<sup>st</sup> International Astronautical Congress 2010. Paris: International Astronautical Federation (IAF), 2010, pp. 3781-3786. ISBN 978-1-61782-368-8. Available from: http://iafastro.directory/iac/archive/browse/IAC-10/E2/3/8918/
RokYear
2010
JazykLanguage
eng
ZáznamyRecords
ProjektProject
Fundamentální experimenty ve fyzice mikrosvětaFundamental Experiments in Physics of Microworld; Spolupráce ČR s CERNCollaboration of the Czech Republic with CERN; Využití radionuklidů a ionizujícího zářeníApplication of radionuclides and ionising radiation
Citace ke staženíDownload citation
TXT · BibTeX

AbstraktAbstract

We present the platform for the on-line Cosmic Ray measurement in the atmosphere and stratosphere, along with the results of our previous stratospheric balloon experiments already undertaken using the semiconductor pixel detectors of the Medipix family for energetic particle imaging. The original detecting device was the hybrid pixel detector Medipix-2 & Timepix developed at CERN, with USB interface developed at Institute of Experimental and Applied Physics of Czech Technical University in Prague. Terrestrial Cosmic Ray (CR) Flux is generally considered as a possible important agent influencing various atmospheric phenomena that range from Global Atmospheric Electric Circuit, dust concentrations, to cloud properties. Therefore, better experimental data on specific atmospheric fluxes along with particle types and energies present are an important input into various models. According to many scientists it will be very important to develop fully automatic, small, and light CR stations for regular ship and aircraft lines for continuous planetary surveys. Such an extended network of both stationary and moving CR stations will be much more effective also for problems related to space weather (e.g., forecasting of dangerous magnetic storms by analyzing galactic CR distribution and great radiation hazards from solar CRs). Therefore we argue that such a CR station could be readily available in our low-cost setup, providing all the required measurements. More advanced setup was flown twice on the stratospheric balloon platform, which is the optimal realization for in-situ measurements of atmospheric electricity. Not only because of the high altitudes reached, but also due to its slow ascent velocity for statistically relevant sampling of the ambient environment for improving cosmic ray induced ionisation rate model inputs. Our devices were flown on the BEXUS-7 and in modified setup on BEXUS-9 campaign from Swedish Space Corporation's ESRANGE center north of the arctic circle.

We present the platform for the on-line Cosmic Ray measurement in the atmosphere and stratosphere, along with the results of our previous stratospheric balloon experiments already undertaken using the semiconductor pixel detectors of the Medipix family for energetic particle imaging. The original detecting device was the hybrid pixel detector Medipix-2 & Timepix developed at CERN, with USB interface developed at Institute of Experimental and Applied Physics of Czech Technical University in Prague. Terrestrial Cosmic Ray (CR) Flux is generally considered as a possible important agent influencing various atmospheric phenomena that range from Global Atmospheric Electric Circuit, dust concentrations, to cloud properties. Therefore, better experimental data on specific atmospheric fluxes along with particle types and energies present are an important input into various models. According to many scientists it will be very important to develop fully automatic, small, and light CR stations for regular ship and aircraft lines for continuous planetary surveys. Such an extended network of both stationary and moving CR stations will be much more effective also for problems related to space weather (e.g., forecasting of dangerous magnetic storms by analyzing galactic CR distribution and great radiation hazards from solar CRs). Therefore we argue that such a CR station could be readily available in our low-cost setup, providing all the required measurements. More advanced setup was flown twice on the stratospheric balloon platform, which is the optimal realization for in-situ measurements of atmospheric electricity. Not only because of the high altitudes reached, but also due to its slow ascent velocity for statistically relevant sampling of the ambient environment for improving cosmic ray induced ionisation rate model inputs. Our devices were flown on the BEXUS-7 and in modified setup on BEXUS-9 campaign from Swedish Space Corporation's ESRANGE center north of the arctic circle.

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