EPJ Web of Conferences
Volume 89, 2015AtmoHEAD 2014: Atmospheric Monitoring for High Energy AstroParticle Detectors
|Number of page(s)||3|
|Section||Poster and Companies|
|Published online||26 March 2015|
Pilot study of ultra-high energy Cosmic rays through their Space – Atmospheric interactions – COSAT
1 Institute of Space Science, Atomistilor Street 409, Magurele 077125, Romania
2 Institute of Research and Development for Optoelectronics, Atomistilor 409, Magurele 077125, Romania
a e-mail: firstname.lastname@example.org
Published online: 26 March 2015
One hundred years after the discovery of cosmic rays, the study of charged ultra-high energy cosmic rays remains a vital activity in fundamental physics. While primary cosmic rays could not be measured directly until it was possible to get the detectors high in the atmosphere using balloons or spacecraft, nowadays very energetic cosmic rays are detected indirectly by ground-based experiments measuring their Extensive Air Showers (EAS) induced Cherenkov and fluorescent light, or radio waves. Moreover, all cosmic ray measurements (performed either from space or ground) rely on accurate understandings of atmospheric phenomena. The concept of the COSAT project is the inter-link between Astroparticle Physics, Remote Sensing and Atmospheric Environment, willing to investigate the energetic cosmic rays physical processes using the atmosphere as a detector in order to identify potential scientific niches in the field of space sciences. A short introduction on the current status and perspectives of the national partnership COSAT project will be given.
© Owned by the authors, published by EDP Sciences, 2015
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