Long-duration cosmic ray modulation from a Sun-Earth L1 orbit

Details Long-duration cosmic ray modulation from a Sun-Earth L1 orbit Long-duration cosmic ray modulation from a Sun-Earth L1 orbit

Oct 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000a%26a...362l..21p&link_type=abstract

Astronomy and Astrophysics, v.362, p.L21-L24 (2000)

Astronomy and Astrophysics

Astrophysics

1

Sun: Activity, Sun: Atmosphere, Sun: Uv Radiation, Ism: Cosmic Rays

Scientific paper

We analyse cosmic ray hits impacting the detector system of the Coronal Diagnostic Spectrometer aboard the Solar and Heliospheric Observatory spacecraft. These observations allow us to study the modulation of cosmic rays over a 4 year period (1996-2000) running from solar minimum to maximum, from a Sun-Earth L1 Lagrangian orbit. The modulation, at the 45-50% level is consistent with cosmic rays of energy 1 GeV.

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