📣 Try out the NEW Gateway to Research and let us know what you think.

We're looking for users to test the new service during August and September and share their feedback. Express your interest by completing this short form.

Evolution of the transverse density structure of oscillating coronal loops inferred by forward modelling of EUV intensity (2018)

First Author: Goddard C

Attributed to: The Cool Alter-Ego of the Hot Solar Corona funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.48550/arxiv.1808.03476

Publication URI: https://arxiv.org/abs/1808.03476

Type: Preprint