Abstract
The introduction to this review summarizes chromosphere observation with two
figures. The first part showcases the historical emphasis on the eclipse chromosphere in the
development of NLTE line formation theory and criticizes 1D modeling. The second part
advertises recent breakthroughs after many decades of standstill. The third part discusses
what may or should come next.
| Original language | English |
|---|---|
| Pages (from-to) | 565-575 |
| Number of pages | 11 |
| Journal | Memorie della Societa Astronomica Italiana |
| Volume | 81 |
| Publication status | Published - 2010 |