Abstract
We determine the three-dimensional topography of the magnetic canopy in and around active regions by mapping the propagation behavior of high-frequency acoustic waves in the solar chromosphere.
| Original language | English |
|---|---|
| Pages (from-to) | L185-L188 |
| Journal | Astrophysical Journal |
| Volume | 613 |
| Issue number | 2 II |
| DOIs | |
| State | Published - Oct 1 2004 |
| Externally published | Yes |
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