Multi wavelength spectropolarimetric observations to understand the solar magnetic activity
by Guillaume Molodij
at Astrophysics and Cosmology Seminar
Wed, 03 Jun 2015, 11:15
Physics building (#54) room 207
Abstract
Violent phenomena resulting from the magnetic activity of the Sun are responsible for non recurrent disturbances in the interplanetary medium To understand the underlying processes a multi wavelength analysis is performed to precisely identify the solar sources of coronal mass ejections and magnetic clouds and to derive the continuous emerging magnetic flux coming from the active region In order to estimate the magnitude and the time duration of the energy released
Created on 25-03-2015 by Bar Lev, Yevgeny (ybarlev)
Updaded on 25-03-2015 by Bar Lev, Yevgeny (ybarlev)