Can the Superposition of Evaporative Flows Explain Broad Fe XXI Profiles during Solar Flares?

Can the Superposition of Evaporative Flows Explain Broad Fe XXI Profiles during Solar Flares?DOI: info:10.3847/2041-8213/ab290bv. 879L17
Polito, Vanessa, Testa, Paola, and De Pontieu, Bart. 2019. "Can the Superposition of Evaporative Flows Explain Broad Fe XXI Profiles during Solar Flares?" The Astrophysical Journal, 879 L17. https://doi.org/10.3847/2041-8213/ab290b.
ID: 154175
Type: article
Keywords: SAO