# Hinode EIS line widths in the quiet corona up to 1.5 Rsun

## TL;DR

This study analyzes Hinode EIS observations of coronal line widths in the quiet Sun up to 1.5 solar radii, finding no significant wave damping but highlighting instrumental uncertainties affecting measurements.

## Contribution

It identifies instrumental issues in EIS data, especially for strong lines, and emphasizes the reliability of weaker lines for coronal diagnostics.

## Key findings

- No significant variation in line widths up to 1.5 Rsun
- Instrumental uncertainties affect line width measurements
- Weak lines provide more reliable data

## Abstract

We present an analysis of several Hinode EIS observations of coronal line widths in the quiet Sun, up to 1.5 Rsun radial distances. No significant variations are found, which indicates no damping of Alfv\'en waves in the quiescent corona. However, the uncertainties in estimating the instrumental width mean that a firm conclusion cannot be reached. We present a discussion of various EIS instrumental issues and suggest that the strongest lines, from Fe XII at 193.5 and 195.1 A, have anomalous instrumental widths. We show how line widths in EIS are uncertain when the signal is low, and that the instrumental variation along the slit is also uncertain. We also found an anomalous decrease (up to 40%) in the intensities of these lines in many off-limb and active region observations, and suggest that this is due to opacity effects. We find that the most reliable measurements are obtained from the weaker lines.