Cosmic Rays
Cosmic Rays are high-energy particles originating from outer space that strike Earth’s atmosphere. They consist mainly of protons, atomic nuclei, and a small fraction of electrons and antiparticles. Cosmic rays are produced by energetic astrophysical processes such as supernova explosions and active galactic nuclei. Studying cosmic rays provides insight into particle acceleration mechanisms and extreme environments in the universe. When cosmic rays interact with the atmosphere, they generate cascades of secondary particles. Detection methods include ground-based detectors and satellite experiments. Cosmic ray research connects astrophysics, particle physics, and atmospheric science. It also helps probe fundamental interactions at energies beyond current accelerators.
Thomas F Ramos
Lawrence Livermore National Laboratory, United States
Ephraim Suhir
Portland State University, United States
Alexander Unzicker
Pestalozzi Gymnasium Munchen, Germany
Thomas J Webster
Brown University, United States
Jon H Brasher
Stelleo Scientific Foundation, United States
Jason Liu
West Windsor-Plainsboro High School North, United States
Tom Lawrence
Ronin Institute of Independent Scholarship 2.0, United KingdomSubmit your abstract Today
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Vladimir Chigrinov, Hong Kong University of Science and Technology, Hong Kong
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Thomas J Webster, Brown University, United States
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Thomas F Ramos, Lawrence Livermore National Laboratory, United States
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Omar Mohammed Daud Shakarneh, Novosibirsk State University of Architecture and Civil Engineering, Russian Federation
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Alexei Krivolutsky, Central Aerological Observatory (CAO), Russian Federation
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Paulo Cesar De Morais, University of Brasilia, Brazil