# Are constant loop widths an artifact of the background and the spatial   resolution?

**Authors:** M.C. Lopez Fuentes, P. Demoulin, J.A. Klimchuk

arXiv: 0704.0637 · 2009-11-13

## TL;DR

This study investigates how background and resolution affect measurements of EUV loop widths, demonstrating that constant widths are often artifacts, and provides a reliable method to distinguish true expansion from measurement errors.

## Contribution

The paper introduces a procedure to accurately determine EUV loop expansion properties despite background and resolution limitations, validating its effectiveness with synthetic and real data.

## Key findings

- Constant loop widths can be distinguished from expanding loops even near resolution limits.
- Background subtraction imperfections mainly cause small-scale width variations.
- Observed loops do not systematically expand with height, confirming previous predictions.

## Abstract

We study the effect of the coronal background in the determination of the diameter of EUV loops, and we analyze the suitability of the procedure followed in a previous paper (L\'opez Fuentes, Klimchuk & D\'emoulin 2006) for characterizing their expansion properties. For the analysis we create different synthetic loops and we place them on real backgrounds from data obtained with the Transition Region and Coronal Explorer (\textit{TRACE}). We apply to these loops the same procedure followed in our previous works, and we compare the results with real loop observations. We demonstrate that the procedure allows us to distinguish constant width loops from loops that expand appreciably with height, as predicted by simple force-free field models. This holds even for loops near the resolution limit. The procedure can easily determine when loops are below resolution limit and therefore not reliably measured. We find that small-scale variations in the measured loop width are likely due to imperfections in the background subtraction. The greatest errors occur in especially narrow loops and in places where the background is especially bright relative to the loop. We stress, however, that these effects do not impact the ability to measure large-scale variations. The result that observed loops do not expand systematically with height is robust.

## Full text

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## Figures

11 figures with captions in the complete paper: https://tomesphere.com/paper/0704.0637/full.md

## References

18 references — full list in the complete paper: https://tomesphere.com/paper/0704.0637/full.md

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Source: https://tomesphere.com/paper/0704.0637