Injection of Relativistic Solar Cosmic Rays into Interplanetary Space

We assume that during the generation of solar cosmic rays in gradual events, the solar atmosphere has a limited spatial size due to the inhomogeneous distribution of the magnetic field turbulence level. For a limited solar atmosphere, the flux of relativistic particles injected into interplanetary s...

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Bibliographic Details
Published inBulletin of the Russian Academy of Sciences. Physics Vol. 87; no. 7; pp. 1071 - 1073
Main Authors Petukhov, I. S., Petukhova, A. S., Petukhov, S. I.
Format Journal Article
LanguageEnglish
Published Moscow Pleiades Publishing 01.07.2023
Springer Nature B.V
Subjects
Hadrons
Heavy Ions
Interplanetary space
Mathematical analysis
Nuclear Physics
Physics
Physics and Astronomy
Relativistic effects
Relativistic particles
Solar atmosphere
Solar cosmic rays
Solar magnetic field
solar cosmic rays
injection
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Summary:We assume that during the generation of solar cosmic rays in gradual events, the solar atmosphere has a limited spatial size due to the inhomogeneous distribution of the magnetic field turbulence level. For a limited solar atmosphere, the flux of relativistic particles injected into interplanetary space is calculated. The calculated flux is compared with the solar cosmic ray flux determined from the measurements of the worldwide network of ground-based neutron monitors on the April 15, 2001 event.
ISSN:1062-8738
1934-9432
DOI:10.3103/S1062873823702441