|
|
|
|
|
|
|
|
|
|
|
|
|
Jorit Leenaarts, Mr. - PhD |
|
Institute for Solar Physics, Stockholm University, Stockholm, Sweden |
|
|
|
|
|
|
|
Session 3 - Invited Speaker |
|
Modeling the Mg II h & k lines observed by IRIS and the Ca II H & K lines observed from the ground |
|
J. Leenaarts, Institute for Solar Physics, Stockholm University, Stockholm, Sweden |
|
|
|
The Mg II h & k and Ca II H & K lines have similar formation properties.
Their main difference is the 18 times larger abundance of Mg compared to Ca. This
leads to a significant height difference of the line-core
optical-depth-unity-heights. I will review the formation of the Ca and Mg lines, and
discuss their diagnostic potential, in particular if observed simultaneously. |
|
|
|
|
|
|
|
 
 |
