The Solar Corona – contd. We discussed: Physical properties of the corona We will now discuss: Coronal scale height Ionization equilibrium Coronal heating.
Radio Astronomy and Amateur Radio Glenn MacDonell VE3XRA 3 August 2010.
Solar Spectral Irradiance (SSI) changes, atmospheric effects? J. Fontenla NorthWest Research Associates and LASP-University of Colorado.
Thyrso Villela Instituto Nacional de Pesquisas Espaciais – INPE Divisão de Astrofísica Prêmio Nobel de Física 2006.
Candels the correlation_between_galaxy_morphology_and_star_formation_activity_at_z2
Vellinga joe
Evidence for a_complex_enrichment_history_of_the_stream_from_fairall_9_sightline
One tenth solar_abundances_along_the_body_of-the_stream
Xiaohu Wang, Abraham Loeb and Eli Waxman- Stability of the Forward/Reverse-Shock System Formed by the Impact of a Relativistic Fireball on an Ambient Medium
Gravitational lensing characteristics of the transparent sun
Microstructures in planetary_nebulae
Infrared transmission spectroscopy_of_the_exoplanets
