Abstract
Comparing high spatial resolution (∼ 1″) images observed in Lyα with the Transition Region Camera (TRC) and in Hα at Sacramento Peak and Meudon Observatories, we notice that some structures are well correlated in the two lines (plages), while others are less correlated (chromospheric network, filaments). This is an indication of the inhomogeneous distribution of physical parameters in these structures.
| Original language | English |
|---|---|
| Pages (from-to) | 105-109 |
| Number of pages | 5 |
| Journal | Advances in Space Research |
| Volume | 17 |
| Issue number | 4-5 |
| DOIs | |
| Publication status | Published - 1996 |
| Externally published | Yes |
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