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Solar Cosmic Rays

  • Book
  • © 2001

Overview

Authors:
  1. Leonty I. Miroshnichenko

    1. IZMIRAN, Troitsk, Moscow Region, Russia
      UNAM, Mexico

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Part of the book series: Astrophysics and Space Science Library (ASSL, volume 260)

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Table of contents (12 chapters)

  1. Front Matter

    Pages i-xi
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  2. Solar Cosmic Rays — Object and Tool for Space Research

    • Leonty I. Miroshnichenko
    Pages 1-21

  3. Observational Features and Databases of Solar Cosmic Rays

    • Leonty I. Miroshnichenko
    Pages 23-64

  4. Energetic Particles and High-Energy Solar Phenomena

    • Leonty I. Miroshnichenko
    Pages 65-90

  5. Solar Cosmic Rays at High Energies

    • Leonty I. Miroshnichenko
    Pages 91-117

  6. Particle Acceleration at the Sun

    • Leonty I. Miroshnichenko
    Pages 119-170

  7. Interactions of Accelerated Particles with the Solar Atmosphere

    • Leonty I. Miroshnichenko
    Pages 171-204

  8. Acceleration and Release of Particles from the Corona

    • Leonty I. Miroshnichenko
    Pages 205-256

  9. Solar Cosmic Rays in the Interplanetary Space

    • Leonty I. Miroshnichenko
    Pages 257-296

  10. Spectrum of Solar Cosmic Rays Near the Earth

    • Leonty I. Miroshnichenko
    Pages 297-329

  11. Solar Cosmic Rays in the Geosphere

    • Leonty I. Miroshnichenko
    Pages 331-366

  12. Energetic Solar Particles and Radiation Hazard in Space

    • Leonty I. Miroshnichenko
    Pages 367-406

  13. Summary and Conclusions: Problems and Prospects

    • Leonty I. Miroshnichenko
    Pages 407-420

  14. Back Matter

    Pages 421-480
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Keywords

About this book

It turned out to be really a rare and happy occasion that we know exact1y when and how a new branch of space physics was born, namely, a physics of solar cosmic rays. It happened on February 28 and March 7, 1942 when the fIrst "cosmic ray bursts" were recorded on the Earth, and the Sun was unambiguously identifIed for the fIrst time as the source of high-velocity 10 particles with energies up to > 10 eV. Just due to such a high energy these relativistic particles have been called "solar cosmic rays" (SCR), in distinction from the "true" cosmic rays of galactic origin. Between 1942 and the beginning ofthe space era in 1957 only extremely high energy solar particle events could be occasionally recorded by cosmic ray ground-Ievel detectors and balloon borne sensors. Since then the detection techniques varied considerably and the study of SCR turned into essential part of solar and solar-terrestrial physics.

Authors and Affiliations

  • IZMIRAN, Troitsk, Moscow Region, Russia

    Leonty I. Miroshnichenko

  • UNAM, Mexico

    Leonty I. Miroshnichenko

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