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Designing Proton and Electron Detector for Monitoring Solar Cosmic Rays

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Abstract

The project of the compact space detector for measuring proton (10–100 MeV) and electron (to 10 MeV) energy spectra in solar cosmic rays is presented. The detector can operate in two modes: differential (each event is reconstructed) and integral (only energy spectrum and radiation composition are reconstructed at a high loading).

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References

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Authors and Affiliations

  1. Moscow Institute of Physics and Technology, Institutskii per. 9, Dolgoprudnyi, Moscow oblast, 141701, Russia

    M. E. Zelenyi, E. M. Stadnichuk, A. A. Nozik, A. G. Kudinov & I. K. Reznikov

  2. Institute for Nuclear Research, Russian Academy of Sciences, pr. 60-letiya Octyabrya 7a, Moscow, 117312, Russia

    E. M. Stadnichuk & A. A. Nozik

  3. Space Research Institute, Russian Academy of Sciences, Profsoyuznaya ul. 84/32, Moscow, 117810, Russia

    I. V. Zimovec

Authors
  1. M. E. Zelenyi
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  2. E. M. Stadnichuk
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  3. A. A. Nozik
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  4. I. V. Zimovec
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  5. A. G. Kudinov
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  6. I. K. Reznikov
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Corresponding author

Correspondence to M. E. Zelenyi.

Additional information

Russian Text © M.E. Zelenyi, E.M. Stadnichuk, A.A. Nozik, I.V. Zimovec, A.G. Kudinov, I.K. Reznikov, 2019, published in Kratkie Soobshcheniya po Fizike, 2019, Vol. 46, No. 1, pp. 3–7.

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Zelenyi, M.E., Stadnichuk, E.M., Nozik, A.A. et al. Designing Proton and Electron Detector for Monitoring Solar Cosmic Rays. Bull. Lebedev Phys. Inst. 46, 23–25 (2019). https://doi.org/10.3103/S106833561901007X

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  • DOI: https://doi.org/10.3103/S106833561901007X

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