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Energetic particles in spaceA review is presented of observations of suprathermal particles in the interplanetary medium along with new data on low energy particles from experiments aboard the ISEE spacecraft. Energy spectra of protons in the near earth atmosphere are plotted in the rest frame of the solar wind noting that at energies above 10 to the 9th eV, the galactic cosmic ray electron component has an unattenuated access into the heliosphere. Solar transient events such as flares accelerate and release energetic particles into the interplanetary medium; flare particle fluxes generate shock waves propagating past 1 AU following the event. It is concluded that the energy spectra for shock wave accelerations show a characteristic shape in accordance with the power law with a rapid steepening at high energies.
Document ID
19810026384
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Lin, R. P.
(California, University Berkeley, Calif., United States)
Date Acquired
August 11, 2013
Publication Date
September 1, 1980
Publication Information
Publication: Solar Physics
Volume: 67
Subject Category
Astrophysics
Accession Number
81A10788
Funding Number(s)
CONTRACT_GRANT: NAS5-22307
CONTRACT_GRANT: NGL-05-003-017
Distribution Limits
Public
Copyright
Other

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