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This content will become publicly available on September 18, 2026

Title: Measurements of the Perpendicular Correlation Length of Coronal Alfvénic Waves with DKIST
Abstract We have measured the perpendicular correlation lengthLof Alfvénic waves in the corona using data from the Daniel K. Inouye Solar Telescope (DKIST) Cryogenic Near Infrared Spectropolarimeter (Cryo-NIRSP) instrument. These data have high spatial resolution and were collected using a raster, enabling us to unambiguously identify the parallel and perpendicular directions with respect to the wave propagation. We find that the measured medianL ≈ 3.5 Mm, which is about half the value found by previous measurements. We ascribe the smaller value measured here to the improved spatial resolution of DKIST. There is a gradual decrease ofLas a function of frequency. We also computed the spatial correlation length of the observed static density structures and found that their typical correlation lengths of ≈8.4 Mm were significantly larger than those of the waves.  more » « less
Award ID(s):
2229100 2005887
PAR ID:
10651266
Author(s) / Creator(s):
; ; ;
Publisher / Repository:
Astrophysical Journal
Date Published:
Journal Name:
The Astrophysical Journal
Volume:
991
Issue:
1
ISSN:
0004-637X
Page Range / eLocation ID:
97
Format(s):
Medium: X
Sponsoring Org:
National Science Foundation
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