The recovery of the cosmic ray flux from maximum solar modulation at IMP-8 (1 AU) and at Pioneer (R 30 AU)

Details The recovery of the cosmic ray flux from maximum solar modulation at IMP-8 (1 AU) and at Pioneer (R 30 AU) The recovery of the cosmic ray flux from maximum solar modulation at IMP-8 (1 AU) and at Pioneer (R 30 AU)

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....5..206m&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 5 p 206-209 (SEE N85-34991 23-93)

Physics

Cosmic Rays, Heliosphere, Propagation Velocity, Solar Activity, Solar Wind Velocity, Energy Spectra, Explorer 50 Satellite, Helium, Protons, Voyager 1 Spacecraft, Voyager 2 Spacecraft

Scientific paper

In the period 1980 - 84, observations of relativistic and low energy (30
⪉ E ⪉ 70 MeV/n) cosmic ray nuclei from Pioneer 10 in the outer
heliosphere and from IMP-8 at 1 AU show that increases as well as
decreases in intensity propagate outward at velocities equal to or
greater than the average solar wind velocity.

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