Abstract

We will present and discuss results of the WHI Quiet Sun Characterization Campaign of April 10 - 16, 2008. Using high spatial and temporal resolution multi-wavelength observations from a broad suite of observatories we made a detailed study of the response of the quiet solar chromosphere, transit... Show moreWe will present and discuss results of the WHI Quiet Sun Characterization Campaign of April 10 - 16, 2008. Using high spatial and temporal resolution multi-wavelength observations from a broad suite of observatories we made a detailed study of the response of the quiet solar chromosphere, transition region and corona to the constantly evolving photospheric magnetic field. These joint observations show that there is no place in the solar atmosphere that is magnetically or dynamically "quiet". Show less