Abstract
The recent launch of the High resolution Coronal imager (Hi-C) provided a unique opportunity of studying the EUV corona with unprecedented spatial resolution. We utilize these observations to investigate the properties of low-frequency (50−200 s) active region transverse waves, whose omnipresence had been suggested previously. The five-fold improvement in spatial resolution over SDO/AIA reveals coronal loops with widths 150−310 km and that these loops support transverse waves with displacement amplitudes
Original language | English |
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Pages (from-to) | L10 |
Journal | Astronomy & Astrophysics |
Volume | 553 |
DOIs | |
Publication status | Published - 22 May 2013 |
Keywords
- Sun: corona
- Sun: chromosphere
- waves
- magnetohydrodynamics (MHD)