Preliminary indirect measurement of cosmic-ray proton spectrum using Earth's γ-ray data from fermi large area telescope
Cosmic rays (CRs) are high-energy particles, mostly protons, propagating in space. The rigidity (momentum per charge) spectrum of CRs is well described by a power law for which the spectral index is approximately 2.8 around 30 - 1000 GV. Recent measurements by PAMELA and AMS-02 indicate an abrupt ch...
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th-mahidol.790182022-08-04T18:28:19Z Preliminary indirect measurement of cosmic-ray proton spectrum using Earth's γ-ray data from fermi large area telescope Patomporn Payoungkhamdee Mahidol University Physics and Astronomy Cosmic rays (CRs) are high-energy particles, mostly protons, propagating in space. The rigidity (momentum per charge) spectrum of CRs is well described by a power law for which the spectral index is approximately 2.8 around 30 - 1000 GV. Recent measurements by PAMELA and AMS-02 indicate an abrupt change of the CR proton spectral index at about 340 GV. When CRs interact with the Earth's upper atmosphere, γ rays can be produced and detected by space-based detectors. Here we use the Earth's γ-ray data collected by the Fermi Large Area Telescope along with a proton-air interaction model to indirectly determine the CR proton spectral index and compare against observations by other instruments. 2022-08-04T11:28:19Z 2022-08-04T11:28:19Z 2021-01-28 Conference Paper Journal of Physics: Conference Series. Vol.1719, No.1 (2021) 10.1088/1742-6596/1719/1/012016 17426596 17426588 2-s2.0-85100777218 https://repository.li.mahidol.ac.th/handle/123456789/79018 Mahidol University SCOPUS https://www.scopus.com/inward/record.uri?partnerID=HzOxMe3b&scp=85100777218&origin=inward |
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Physics and Astronomy Patomporn Payoungkhamdee Preliminary indirect measurement of cosmic-ray proton spectrum using Earth's γ-ray data from fermi large area telescope |
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Cosmic rays (CRs) are high-energy particles, mostly protons, propagating in space. The rigidity (momentum per charge) spectrum of CRs is well described by a power law for which the spectral index is approximately 2.8 around 30 - 1000 GV. Recent measurements by PAMELA and AMS-02 indicate an abrupt change of the CR proton spectral index at about 340 GV. When CRs interact with the Earth's upper atmosphere, γ rays can be produced and detected by space-based detectors. Here we use the Earth's γ-ray data collected by the Fermi Large Area Telescope along with a proton-air interaction model to indirectly determine the CR proton spectral index and compare against observations by other instruments. |
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Mahidol University |
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Mahidol University Patomporn Payoungkhamdee |
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Conference or Workshop Item |
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Patomporn Payoungkhamdee |
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Patomporn Payoungkhamdee |
title |
Preliminary indirect measurement of cosmic-ray proton spectrum using Earth's γ-ray data from fermi large area telescope |
title_short |
Preliminary indirect measurement of cosmic-ray proton spectrum using Earth's γ-ray data from fermi large area telescope |
title_full |
Preliminary indirect measurement of cosmic-ray proton spectrum using Earth's γ-ray data from fermi large area telescope |
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Preliminary indirect measurement of cosmic-ray proton spectrum using Earth's γ-ray data from fermi large area telescope |
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Preliminary indirect measurement of cosmic-ray proton spectrum using Earth's γ-ray data from fermi large area telescope |
title_sort |
preliminary indirect measurement of cosmic-ray proton spectrum using earth's γ-ray data from fermi large area telescope |
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2022 |
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https://repository.li.mahidol.ac.th/handle/123456789/79018 |
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1763490437943787520 |