Giant Solar Flare Neutrons |
Contents
the measurements at Climax | 6 |
the spectrum | 9 |
the choice of two spectra | 12 |
10 other sections not shown
Common terms and phrases
abundant assume average energy beam calculated cascade cavity model center of mass Chapter chromosphere cm² Column CORNELL CORNELL CORNELL UNIVERSITY counting rate increase cross section curve cutoff energy detectable neutron spectrum differential spectrum energy in Bev estimate extrapolate factor flare particles flare protons fraction Function of Proton gives gr/cm² helium Hence high energy particles hydrogen hydrogen reaction impact zones inelastic integral intensity isotropic kinetic energy lab system laboratory system leaving the sun LIBRARY CORNELL low energy cutoff mass system mean energy mean free path measurements at Climax mechanism meson monitors Neutron Density neutron detection neutron emitted neutron energy neutron flux neutron yield neutrons produced nuclear number of neutrons number of protons obtained ordinary cosmic ray primary intensity primary neutrons proton spectrum ratio rest mass Sacramento Peak secondary nucleons solar flare solar neutrons specific yield Spectra of Flare steep Table target total energy total number Wellington