Portal:Radiation astronomy/Resource/8

Subatomics edit

 
A mechanism is suggested for anomalous cosmic rays (ACRs) of the acceleration of pick-up ions at the solar wind termination shock. Credit: Eric R. Christian.{{fairuse}}

An "analysis of the energy-loss distributions in the GRS HEM during the impulsive phase of this event indicates that γ-rays from the decay of π0 mesons were detected [...] The production of pions, which is accompanied (on average) by neutrons, has an energy threshold of ~290 MeV for p-p and ~180 MeV for p-α interactions, giving, therefore, a lower limit to the maximum energy of the particles accelerated at the Sun."[1]

References edit

  1. E. L. Chupp, H. Debrunner, E. Flueckiger, D. J. Forrest, F. Golliez, G. Kanbach, W. T. Vestrand, J. Cooper, G. Share (July 15, 1987). "Solar neutron emissivity during the large flare on 1982 June 3". The Astrophysical Journal 318 (7): 913-25. doi:10.1086/165423. http://adsabs.harvard.edu/abs/1987ApJ...318..913C. Retrieved 2014-04-08.