Pamela Measurements of Galactic and Solar Cosmic Rays in the 23rd Solar Minimum (Invited)

Astronomy and Astrophysics – Astrophysics

Scientific paper

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[7500] Solar Physics, Astrophysics, And Astronomy, [7513] Solar Physics, Astrophysics, And Astronomy / Coronal Mass Ejections, [7536] Solar Physics, Astrophysics, And Astronomy / Solar Activity Cycle

Scientific paper

We will discuss the measurements of protons and helium of galactic, solar and trapped origin taken with PAMELA detector in the period 2006-2010. PAMELA was launched in 2006 and is currently orbiting the Earth in a 350*600 km, 70 degree inclination polar orbit in a pressurized container located on one side of the Russian Resurs-DK1 satellite. Data were acquired at solar minimum, but show the effect of solar modulation on p and he low energy spectra (about 100 MeV/n - 1 GeV/n). Galactic protons and helium particles are measured up to 1 TV. Trapped and secondary proton component will be compared with existing models; the spectra of solar particle events of 13 and 14 December 2006 will also be discussed.

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