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Searching for Sources of Solar Cosmic Rays in Weak Events

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Bulletin of the Russian Academy of Sciences: Physics Aims and scope

Abstract

Some of the weak solar proton events in which protons with energies E ≥ 10 MeV are registered by observers on the Earth are particles accelerated by shock waves in interplanetary space. They can be associated with flares and coronal mass ejections tens of hours before an observed increase in proton fluxes that inject particles into the process of subsequent acceleration in interplanetary space.

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CONFLICT OF INTEREST

The authors declare that they have no conflicts of interest.

Author information

Authors and Affiliations

  1. Lebedev Physical Institute, Russian Academy of Sciences, 119991, Moscow, Russia

    G. A. Bazilevskaya

  2. Skobeltsyn Institute of Nuclear Physics, Moscow State University, 119991, Moscow, Russia

    E. I. Daibog & Yu. I. Logachev

Authors
  1. G. A. Bazilevskaya
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  2. E. I. Daibog
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  3. Yu. I. Logachev
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Corresponding author

Correspondence to E. I. Daibog.

Ethics declarations

The authors thank all researchers who submitted data on SCRs (https://satdat.ngdc.noaa.gov/sem/goes/data/ avg/1999/06/goes08/csv/), flares (https://www .ngdc.noaa. gov/stp/space-weather/solar-data/solar-features/solar-flares/ x-rays/goes/ xrs/); CMEs (https://cdaw.gsfc.nasa. gov/CME_list/), and parameters of the interplanetary medium (https://omniweb.gsfc.nasa.gov/form/omni_ min.html/; https://www.obsebre.es/en/rapid#ssc/; http:/ipshocks.fi/database/) over the Internet.

Additional information

Translated by T. Sokolova

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Bazilevskaya, G.A., Daibog, E.I. & Logachev, Y.I. Searching for Sources of Solar Cosmic Rays in Weak Events. Bull. Russ. Acad. Sci. Phys. 87, 935–937 (2023). https://doi.org/10.3103/S1062873823702787

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  • DOI: https://doi.org/10.3103/S1062873823702787

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