Abstract
We report phase-difference and travel-time analyses of propagating chromospheric oscillations in and around an equatorial coronal hole as observed by TRACE. Our results suggest a significant change in atmospheric conditions at the base of the chromosphere inside the coronal hole relative to its boundary and quiet-Sun regions.
| Original language | English |
|---|---|
| Pages (from-to) | L95-L98 |
| Journal | Astrophysical Journal |
| Volume | 609 |
| Issue number | 2 II |
| DOIs | |
| State | Published - Jul 10 2004 |
| Externally published | Yes |
Keywords
- Sun: atmospheric motions
- Sun: chromosphere