Can superposition of evaporative flows explain broad IRIS Fe XXI line profiles during flares?
Vanessa Polito, Bay Area Environmental Research Institute Moffett Field, Moffett Field, CA, United States, Paola Testa, Harvard-Smithsonian Center for Astrophysics, Cambridge, MA, United States and Bart De Pontieu, Lockheed Martin Solar and Astrophysics Laboratory, Palo Alto, CA, United States