The Solar Corona – contd. We discussed: Physical properties of the corona We will now discuss: Coronal scale height Ionization equilibrium Coronal heating.
Charge-Exchange Mechanism of X-ray Emission V. Kharchenko ITAMP, Harvard-Smithsonian Center for Astrophysics, Cambridge 1. Introduction - interaction between.
Neutrino mass spectroscopy with atoms-- experimental status-- N. Sasao and M. Yoshimura (Okayama U.) for SPAN collaboration 2015/8/2117th Lomonosov1.
